Radio Boulevard - Western Historic Radio Museum
Vintage Longwave Receivers
Restoration and Performance Testing the Following Longwave Receivers
~ IP-501-A - Radiomarine Corp. of America - 1923 ~
~ Type 105-A - Mackay Radio & Telegraph Co. - 1932 ~
~ RIO - National Co.,Inc. - 1933 ~
~ RAZ-1, CRM-46092 - Radiomarine Corp. of America - 1941 ~
~ RAK-7, CND-46155 - RCA-Andrea Radio Co. - 1944 ~
~ BC-344-D - Farnsworth Television and Radio Corp. - 1944 ~
~ AR-8510 - Radiomarine Corp. of America - 1944 ~
~ RBL-5, CNA-46161-B - National Co., Inc. - 1945 ~
~ RBA-1, CFT-46154, RBA-6 CFT-46300 - RCA-Federal Tele.&Radio Corp - 1941-45 ~
~ Type 3001-A - Mackay Radio & Telegraph Co. - 1948 ~
~ R-389/URR - Collins Radio Co. - 1951 ~
- Hammarlund Mfg Co., Inc.- 1955 ~
Operating Vintage Gear on the 630M
(472 khz) Band
NBD Stations in Nevada & NDB Station Log
photo above: These massive towers dwarf the two-story station house in the foreground. This is the VLF station at Arlington. The photo is from the early-1920s when Arlington's time signals were on 10kc. photo from: Radio Broadcast 1922
"Longwave" is an unofficial but commonly used term that refers to all frequencies below the AM BC band. These frequencies are properly known as Medium Wave (MW, 300kc to 3000kc,) Low Frequency (LF, 300kc to 30kc) and Very Low Frequency (VLF, 30kc to 10kc.) A Long Wave Receiver would be a receiver specifically designed for a frequency coverage of 600kc down to 15kc but also can be any receiver that has significant LW coverage.
Vintage Longwave Receivers
Testing Classic Vintage Longwave
Radiomarine Corporation of
IP-501-A - MW & LF Receiver-Amplifier
Commercial Shipboard Receiver from 1923
40kc to 1000kc
"Listening on longwave with a 1923, battery operated, regenerative receiver? You gotta be kidding!"
One has to remember, the IP-501-A was the commercial shipboard receiver that was built to the highest standards of the day. It was well-known for its superior performance and reliability. It is the "R-390" of the 1920s.
The initial versions of this receiver were built at Wireless Specialty Apparatus, a company that was part of the cross-licensing "Radio Group" headed by General Electric and included Westinghouse, AT&T, RCA and the United Fruit Company (who owned Wireless Specialty Apparatus (WSA.) WSA built a few broadcast radios for RCA in 1921 and 1922 but by 1923 they had become part of RCA. Soon WSA became Radiomarine Corporation of America and was building shipboard radio gear for RCA.
This three tube receiver uses a three-circuit tuner with a regenerative detector and two transformer coupled audio frequency amplifier stages - not exactly the norm for a lot of radio receivers in 1923. What really sets the IP-501-A apart from the other three-circuit tuner regen sets is its incredible Antenna Tuner section that is entirely shielded from the main part of the receiver (which is also entirely shielded.) The Antenna Tuner allows exact tuning of the antenna's impedance so the load remains the same on the Secondary circuit. It's like having a built-in pre-selector. The only transference of signal happens by way of the small variable coupling coil located inside the Antenna coil. The fact that the receiver cabinet and front panel are entirely shielded results in no hand-capacity effects when the receiver is operated as an autodyne detector. This makes tuning CW super-easy. The Secondary Tuner has six frequency ranges from 1000kc down to 40kc and the dial is calibrated in meters. The Tickler coil is actually a variometer built into the Secondary coil form and includes load windings from the Secondary inductance to improve regeneration on the lower frequencies. The audio amplifier section is standard and uses two RCA interstage transformers. The audio gain is more-or-less controlled by the filament voltage and the operator can also select how much gain is required by using one of the phone jack outputs. The phone jacks also control the filament voltage to the tubes and only the tubes needed are in operation when that jack is selected. Maximum audio is from the AF2 jack which provides Det + 2 AF stages. In high noise level conditions or for very loud signals, AF1 saves the operator's ears by using just one audio amplifier. If the DET jack is used, only the detector tube is in operation - this would be for receiving local transmissions. Intended audio output is to Hi-Z earphones but the IP-501-A will drive a horn speaker loudly from the AF2 jack. To power the receiver up requires 6vdc at .75A for the filaments, 45vdc and 90vdc for the B+ requirements and -4.5 for C bias. The filament adjustment pot controls the A battery into the receiver and is used to turn off the receiver. Pulling the phone plug from one of the jacks will turn off the tubes but the meter will still show A battery voltage unless the filament pot is turned off. The tubes normally used in the IP-501-A were UX/UV-201A triodes. Operating any radio receiver that uses batteries for its power source can be a hassle and expensive unless you are all ready set-up to run battery receivers. Usually highly-filtered power supplies provide "close to pure" DC voltages to operate these types of receivers. I use a Lambda 6vdc 4A power supply for the A supply, a 1920s RCA Rectron B Eliminator for the B supply and a 4.5vdc battery for the C bias. Hi-Z earphones are necessary for the audio output and I generally us a set of 2200 ohms dc, Western Electric 518W 'phones. The IP-501-A also requires a fairly large antenna worked against a true earth ground for best performance.
||In operation, the filaments are set to about 4.5 to 5.0vdc using the panel meter as reference. Tuning is accomplished with the Secondary Condenser and then "peaking" the signal with the Antenna Condenser. Sensitivity is controlled by use of the Tickler. Since an adjustable resonance and load can be controlled by the Antenna Condenser control, the Tickler control can be set to one position and doesn't require too much adjustment per each tuning range. Selectivity is controlled by the Coupling control. Changing the settings of any of the controls will always cause an interaction in any regen set when it is used as an Autodyne Detector (oscillating regenerative detector.) When the IP-501-A is used as a three-circuit tuner with Autodyne Detector, the Coupling control must be set to "Critical Coupling" for best performance. This requires the operator to tune through the Antenna Condenser's resonance while listening for a "double-click" (and for the oscillating to stop.) If the clicks are heard, this indicates too much coupling. Continue to loosen the coupling and retune the Antenna Condenser until no clicks are heard at resonance. Now the Coupling is set properly. Large changes in tuned frequency will require minor adjustments to the Coupling setting. All tuning can usually be accomplished using just the Secondary Condenser control for tuning stations and then using the Antenna Condenser for adjusting the signal to maximum. Now and again you will have to slightly re-adjust the Tickler. For tuning in NDBs, the IP-501-A should be operated as an Autodyne Detector receiver. This provides a heterodyne so the NDB carrier can be easily heard. Regenerative detectors can become unstable at the oscillation point and good construction helps to stabilize the regeneration. The IP-501-A is very stable and easy to operate in the Autodyne set-up since that was one of its intended uses - to copy the CW from arc transmitters.|
I have had this IP-501-A since 1979. A ham friend sold it to me after he had traded a telephone pole for it. I have performed three restorations on the set over the years. The last one in 1984 brought the IP-501A back to full original configuration and appearance internally and very good restored condition externally. I used the receiver back in the 1980s with a 125' EFW antenna and tuned in all the normal AM BC stations one would expect. As far as Airport Non-Directional Beacons (NDB,) the only one I remember tuning in was SPK 251kc, located at the old Reno-Cannon AP. I remember SPK because they used to transmit voice weather with the MCW ID "SPK" in the background. I really didn't know how to get a lot of performance out of the IP-501-A back then. The AM BC performance was fine but listening to AM BC over a horn speaker gets boring after awhile. When I opened the museum in 1994, the IP-501-A was installed in a display case and it stayed in the case for almost 15 years. Lately, I had been thinking about trying something different, as a challenge to the performance capabilities of early regenerative receivers. Since the IP-501-A was the commercial receiver of choice in difficult environments and it had every indication of being the "best" of its day, I decided to give it a try. I used my ham antenna, a 135' tuned dipole, but with the feedline shorted. This would provide a vertical with large capacity hat configuration similar to the large "T" antennas of the twenties. Our initial tests turned up a small problem with the IP-501-A's circuit selector switch. We had no detector plate voltage but it was just a bad contact that needed a bit of cleaning and we were up and operating,...sort of. Lack of audio output was another easy fix. The bias SS power supply had failed and was at -25vdc, definitely in the cut-off region for UX-201As! I sub'd a battery for the bias and then the IP-501-A sprang to life. Before power-up, I had tuned the receiver to around 800 meters as a pre-set and, to my complete surprise, SX 367kc in Cranbrook, BC, Canada was coming in (this was at about 5PM local time in December.) I tuned in a few more NDBs and then decided to wait until about 10PM and try again. At 10PM, I received around 25 more NDBs tuning from 326kc up to 414kc. Best DX was the 2KW transatlantic beacon DDP 391kc in San Juan, Puerto Rico.
|IP-501-A NDB Log - 2009 - The following is the log of the NDBs copied using just the IP-501-A receiver and the 135' tuned dipole antenna with the feedline shorted. NDB location, frequency and power (if know) are listed. Total was 103 NDBs copied in a three-week period in January 2009.|
|AA - 365kc - Fargo, ND - 100W
AEC - 209kc - Base Camp, NV
AOP - 290kc - Rock Springs, WY
AP - 260kc - Denver, CO - 100W
AZC - 403kc - Colorado City, AZ
BKU - 344kc - Baker, MT - 80W
BO- 359kc - Bosie, ID - 400W
CII - 269kc - Choteau, MT - 50W
CNP - 383kc - Chappell, NE - 25W
CSB - 389kc - Cambridge, NE - 25W*
CVP - 335kc - St. Helena, MT - 150W
DC - 326kc - Princeton, BC, CAN
DDP - 391kc - San Juan, Puerto Rico - 2KW
DPG - 284kc - Dugway Proving Gnds, UT
DQ - 394kc - Dawson Creek, BC, CAN
EUR - 392kc - Eureka, MT - 100W
EX - 374kc - Kelowna, BC, CAN
FCH - 344kc - Fresno, CA - 400W
FN - 400kc - Ft. Collins, CO
FO - 250kc - Flin Flon, MB, CAN
GLS - 206kc - Galveston, TX - 2KW
GUY - 275kc - Guymon, OK - 25W
GW - 371kc - Kuujjuarapik, QC, CAN
HQG - 365kc - Hugoton, KS - 25W
IOM - 363kc - McCall, ID - 25W
ITU - 371kc - Great Falls, MT - 100W
IY - 417kc - Charles City, IA - 25W
JW - 388kc - Pigeon Lake, AB, CAN
LBH - 332kc - Portland, OR - 150W
LFA - 347kc - Klamath Falls, OR
LV - 374kc - Livermore, CA - 25W
LW - 257kc - Kelowna, BC, CAN
LYI - 414kc - Libby, MT - 25W
MA - 326kc - Midland, TX - 400W
MEF - 373kc - Medford, OR
MF - 373kc - Rogue Valley, OR
MKR - 339kc - Glascow, MT - 50W
MLK - 272kc - Malta, MT - 25W
|MO - 367kc - Modesto, CA - 25W
MOG - 404kc - Montegue, CA - 150W
MR - 385kc - Monterey, CA
NO - 351kc - Reno, NV - 25W
NY - 350kc - Enderby, BC, CAN
ON - 356kc - Okanagan, Penticton, BC, CAN*
OT - 378kc - Bend, OR
PBT - 338kc - Red Bluff, CA - 400W
PI - 383kc - Tyhee, ID
PN - 360kc - Port Menier, Anticosti Is., QC, CAN*
PTT - 356kc - Pratt, KS - 25W*
QD - 284kc - The Pas, MB, CAN
QQ - 400kc - Comox, BC, CAN
QT - 332kc - Thunder Bay, ON, CAN
RD - 411kc - Redmond, OR - 400W
RPB - 414kc - Belleville, KS
RPX - 362kc - Roundup, MT - 25W
RYN - 338kc - Tucson, AZ - 400W
SAA - 266kc - Saratoga, WY - 25W
SB - 397kc - San Bernardino, CA - 25W
SBX - 347kc - Shelby, MT - 25W
SIR - 368kc - Sinclair, WY
SX - 367kc - Cranbrook, BC, CAN
SYF - 386kc - St. Francis, KS - 25W
TAD - 329kc - Trinidad, CO
TV - 299kc - Turner Valley, AB, CAN
TVY - 371kc - Tooele, UT - 25W
ULS - 395kc - Ulysses, KS - 25W
VQ - 400kc - Alamosa, CO
VR - 266kc - Vancouver, BC, CAN
WG - 248kc - Winnepeg, MN, CAN
WL - 385kc - Williams Lake, BC, CAN
XD - 266kc - Edmonton, AB, CAN
XH - 332kc - Medicine Hat, AB, CAN
XS - 272kc - Prince George, BC, CAN
XX - 344kc - Abbotsford, BC, CAN
YAZ - 359kc - Tofino, Vancouver Is., BC, CAN
YBE - 379kc - Uranium City, SK, CAN
|YCD - 251kc - Nanaimo, BC, CAN
YHD - 413kc - Dryden, ON, CAN
YJQ - 325kc - Bella Bella, BC, CAN
YK - 269kc - Castlegar, BC, CAN
YKQ - 351kc - Waskaganish, QC, CAN*
YL - 395kc - Lynn Lake, MN, CAN
YLB - 272kc - Lac La Biche, AB, CAN
YLD - 335kc - Chapleau, ON, CAN
YLJ - 405kc - Meadow Lake, SK, CAN
YMW - 366kc - Maniwaki, QC, CAN*
YPH - 396kc - Inukjauk, QC, CAN
YPL - 382kc - Pickle Lake, ON, CAN
YPO - 401kc - Peawanuck, ON, CAN
YPW - 382kc - Powell River, BC, CAN
YQZ - 359kc - Quesnel, BC, CAN
YTL - 328kc - Big Trout Lake, ON, CAN
YWB - 389kc - West Bank, BC, CAN
YWP - 355kc - Webequie, ON, CAN
YY - 340kc - Mont Joli, QC, CAN
YYF - 290kc - Penticton, BC, CAN
YZH - 343kc - Slave Lake, AB, CAN
ZP - 368kc - Sandspit, QC IS., BC, CAN
ZSJ - 258kc - Sandy Lake, ON, CAN
ZSS - 397kc Yellowhead/Saskatoon, SK, CAN
ZU - 338kc - Whitecourt, BC, CAN
Z7 - 408kc - Claresholm, AB, CAN
3Z - 388kc - Taber, AL, CAN*
* = New NDB heard
Mackay Radio & Telegraph Company
MW, LF & VLF Radio Receiver Type 105-A
Serial No. 32081
Commercial Shipboard Receiver from 1932
16kc to 1500kc
built by: Federal Telegraph Company
Mackay Radio & Telegraph Company was founded by Clarence Mackay, son of John W. Mackay, one of the "Big Four of the Comstock" fame in Virginia City, Nevada. John Mackay initially made his fortune in Comstock silver but he later (1883) moved into telegraphic communications. Mackay, along with J. Gordon Bennett Jr., formed several telegraph communications companies to compete with Jay Gould's Western Union. Postal Telegraph Company (1886) was the best known, along with Commercial Cable Company (1884). Eventually, these companies, along with other Mackay-Bennett telegraph companies, had transoceanic cables across both major oceans. When John Mackay died in 1902, Clarence inherited the businesses. Clarence Mackay saw to the completion of the transpacific cable in 1904. Radio was added to the business end of things in 1925 to provide "radiogram" service to every area of the world. Mackay Radio was mainly interested in maritime communications which went along with the maritime radio-telegraph business. By 1928, ITT had merged with most of Mackay's business interests but the Mackay name continued on for several decades. Mackay Communications is still in business, located in North Carolina.
photo above: The chassis of the Mackay 105-A. The rectangular box on the right side of the chassis contains the power input filters. The right side cylinder contains the RF choke while the remaining cylinders contain the AF interstage coupling transformers.
photo right: The underside of the Mackay 105-A. The lower coils are the Antenna Tuning coils and the upper coils are the Detector Tuning coils.
|The Type 105-A is a pre-WWII commercial shipboard receiver that dates from after the Federal Telegraph move to New Jersey since the ID tag lists Newark, N.J. as FTC's location. Later Mackay radios incorporate the year of manufacture into the first two digits of the serial number. It looks like this is also the case with the Type 105-A and, with the serial number 32081, this receiver was built in 1932. The circuit uses four tubes that are five-pin cathode-type tubes. It is possible to use type 27 or type 56 tubes and with an increase in the filament voltage, type 76 tubes could also be used. The frequency coverage is 1500kc down to 16kc in seven tuning ranges. Power is supplied by batteries. Like earlier designs for shipboard receivers, the Mackay 105-A utilizes an LC Antenna tuner ahead of the regenerative detector to increase gain and selectivity. An Antenna Series Condenser switch selects various value capacitors to match the ship antenna to the receiver input and a stepped Tone control provides some relief from static. The panel meter is a dual meter that normally reads filament voltage but B+ voltage can also be monitored by activating a panel switch. The left large tuning knob tunes the Antenna Condenser, the middle large knob controls the Regeneration Condenser and the right large knob tunes the Detector Condenser. The Mackay 105-A is built for shipboard use being physically stout and very heavy. Originally the receiver was probably in a metal cabinet but later it could also have been panel mounted in one of the Mackay Marine Radio Units that would have housed the majority of the radio gear for the ship.|
photo above: This is the radio room onboard the S.S. Manhattan, ca. 1938, entirely equipped with Mackay Radio and Telegraph Company gear. The Type 105-A receivers are flanking the central transmitter in the photo. The receiver to the right of the "right-side" Type-105-A is a shortwave receiver, the Type 104-B. This photo is from the frontispiece of Sterling's THE RADIO MANUAL, 3rd Edition, 1938.
|This Type 105-A was an eBay find that was purchased in October 2009. The receiver has vintage modifications that were probably installed during its life as a "shipboard receiver." The original concept appears to have been designed for exclusive DC operation. The Filament control has been bypassed since cathode tubes were now being used and since cathode type tubes are used, AC could be supplied to the tube heaters. However, AC voltage won't read on the panel meter since it doesn't have an internal rectifier - also the internal series resistor is burnt out for the B+ section of the meter. Additionally, there was a DC voltage input filter on the filament line that has been bypassed. I have examined this Type 105-A carefully and it appears that the five pin tube sockets are not original but the rework looks vintage. It could be that the receiver was rebuilt at the factory sometime in its past resulting in professional looking rework and the patina of age appearing on the solder joints. The good news is that this Type 105-A is a working receiver. It operates very much like the IP-501-A in that the position of the regeneration control is dependent on how you set-up the Antenna Tuning. Though there is no coupling control, the interaction between the Antenna Tuning and Regeneration does about the same thing as setting the "Critical Coupling" on the earlier IP-501-A. The Antenna Series Condenser switch compensates for use of a single antenna length and adds to the range of the Antenna Tuning. The Tone Control knocks down the static noise on the LF and VLF ranges. At first, I used an old Signal Corps power supply that provides 6.3vac and regulated 135vdc to power up the Type 105-A. Using the 135' Tuned Dipole antenna with the feed line shorted at the receiver antenna terminal, I was able to easily receive all of the usual longwave signals using WE 509W 'phones for the audio output. Some of the NDBs tuned in were MM 388kc from Fort McMurray, Alberta, ZP 368kc Sandspit, BC for best DX but also consider SYF 386kc, a 25W marker beacon in St. Francis, KS. The VLF reception included the Navy NSRTTY stations in Jim Creek, WA (24.8kc) and Cutler Maine (24.0kc.)|
Update on Mackay Type 105-A Performance: The high noise level of the Type 105-A seemed to be limiting the reception of very weak signals. I finally decided to run the heaters on DC voltage which was a subtle change and hardly noticeable but very weak signal detection was improved. I was able to receive WG 248kc in Winnepeg, MB and RL 218kc in Red Lake, ON. Note that both of these NDBs are in the 200kc - 250kc part of the spectrum - a particularly noisy area. DC voltage on heaters does help on weak signal detection.
Additional Note on Set-up and Performance: I decided to try an entirely different DC power supply set up using a 6vdc 4A Lambda power supply for the tube heaters and a vintage B eliminator, the RCA Rectron, to test if the noise would be further reduced. The change was amazing! Apparently the old Signal Corps power supply wasn't filtered as well as the Rectron because now the MCW signals from NDBs have no distortion and the tone sounds like a good sine wave. Luckily, there happened to be a true CW station operating on 425kc during my test. This was probably an "events" type of operation of one of the old Point Reyes stations since the signal was very strong and was only "on the air" for about one hour. This CW also was very pure in tone. The operation and performance of the Mackay Type 105-A only seems to improve that closer one gets to operating it on pure DC (as original.) November 21, 2009
National Company, Inc.
Intermediate Frequency Receiver (LF and MW)
Serial Number: 3
160kc to 630kc
- National Co., Inc. built their first contracted "airport" receivers in
1932. The first superheterodyne was designated as "RHM" and was part of a contract with the Department of Commerce, Aeronautics
Branch, Airways Division & Lighthouse Service. The DOC wanted to upgrade
all radio communications and navigation equipment at the many airports
that were already servicing Air Mail routes and were beginning to provide air travel and
other types of air services throughout
the USA. General Electric was contracted to build the ground
transmitters and Aircraft Radio Corp built the airborne equipment. National
was contracted to build the ground receivers. The RHM was a nine tube,
superhet with plug-in coils that covered 2.3mc to 14.8mc, a micrometer
Type-N tuning dial and all aluminum construction. The circuit used single preselection
and two IF amplifiers operating at 500kc. Three plug-in coils were
necessary for each of the five bands thus totaling 15 coils. Each
installation also included a Model 58C Monitor receiver, a GRDPU dual
power supply, coil rack and rack speaker all mounted in an open frame
About 100 RHM receivers were built to fulfill the initial contract. National wanted to benefit from the prestige of the government contract by selling these types of receivers to the ham and shortwave listener market. After installing a few upgrades the new receiver was released as the "AGS" in 1933. Frequency coverage of the AGS was from 1.5mc to 20.0mc. The IF remained at 500kc. In late-1933, the "Single Signal" AGS-X was introduced. This version had the Lamb Crystal Filter installed and also moved the BFO frequency adjustment to the front panel. >>>
|>>> The "Single Signal" AGS-X had other accessories
such as band spread coil sets for 160, 80, 40 and 20 meters. By
late-1934, 10 meter coil sets were also available. The high price of the
AGS-X limited its market and National never produced any of the RHM-AGS
line in any significantly large quantities.
As airport communications and airways navigation requirements evolved so did the National receivers that were being supplied for these services. The RHM was upgraded to the RHQ, a receiver that ganged the three plug-in coils into one assembly that allowed plugging in all three coils at once. In other services the RHQ was designated as the AGU. The RHQ-AGU frequency coverage was greatly reduced to specifically what the airports needed, 2.5mc to 6.5mc (only two coil sets were supplied.)
Not all airport operations were on HF and much of the airways navigation radio needs were on lower frequencies. National also provided an Intermediate Frequency receiver that covered 160kc up to 630kc and was designated as the RIO. The RIO wasn't a superhet, however. This receiver was three stages of TRF amplification followed by a detector and single stage audio amplifier. The circuit also provided a "tracking BFO" that utilized a section of the five-gang tuning condenser to allow the BFO to always track at the tuned frequency. An AVC tube controlled the TRF amplifiers grid bias dependent on signal strength from the detector tube. Only two tuning ranges are provided with the higher frequency range A covering 275kc up to 630kc and the lower frequency range B covering 160kc up to 330kc. The tuning ranges were selected by a panel switch. The RIO was powered by the same type GRDPU rack power supply that the RHM used or it could also be powered by the 5886 "dog house" power pack (as could all of the other receivers in the RHM/AGS family.). Like the RHQ/AGU receivers, the RIO used a Type BX tuning dial (an illuminated SW-3-style dial.) In some National advertising the RIO was also identified as the AGL receiver.
|Serial Number 3
- Details - This RIO receiver is virtually "all
original." Only one resistor, a cathode resistor on the second TRF
amplifier, had been replaced and one paper capacitor was changed. Both changes
were performed decades ago
based on the resistor style and the orange paper capacitor used for the repairs. As standard for the RHM/AGS
receivers, the original capacitors were built by Sprague in the black "postage stamp" style along with a few metal tub capacitors. Resistors are the standard
National-made types with the white ceramic body and hand-written values
(in blue ink ).
Tubes used are as follows: 1RF = 78, 2RF = 78, 3RF = 78, Det = 37, Audio Output = 89, AVC = 36, BFO = 36. The power pack will also account for a type 80 rectifier tube.
Unlike later USN longwave TRF receivers with a tracking BFO, rather than have the BFO set slightly higher than the tuned frequency (usually 1kc,) the RIO alignment instructions have the user set the BFO frequency to "zero beat" with the tuned frequency. This allowed the user to tune a ICW (Interrupted CW used a rotating chopper wheel to "break" the continuous wave at an audio frequency rate resulting in a modulated CW signal) or "true" MCW signal. The user would then zero the carrier frequency and the modulated CW would be heard somewhat normally. With this method of tuning it was much easier to find weak signals since the carrier was usually easily heard. The RIO uses an output transformer that is a fairly high impedance indicating that hi-z 'phones were probably the intended audio reproducers. If a loudspeaker was needed then either a hi-z armature-pin loudspeaker or a voice coil-type speaker with a matching transformer could be used.
When testing the tubes it was noted that every tube was a "U.S.N." tube.
The tubes had not been out of their sockets in many decades. This could
imply that this RIO was used by the Navy. Not surprisingly, all
of the tubes tested good. I also tested a few important components for
shorts or continuity and didn't find any problems. I used a National
5886 Dog House power pack (6.3vac and +180vdc) as a voltage source. I
connected a set of Navy Baldwin Type C 'phones for audio reproducers.
With power applied, the dial lamp came on and within about 20 seconds
audio was being received. I had the RIO on Band B at the top end so KPLY
on 630kc in Reno was coming in strong. All switches were noisy or
expected) but AM BC signals were being received. I later tried Band A with the BFO on and tuned in the DGPS
node on 314kc and it was coming in fairly
strong. Any switching to either Band A or B resulted in extreme "static"
in the 'phones. If the BFO is on then the AVC
must be turned off so any noisy contacts are routed thru the audio
system unattenuated - ouch!
Even through the RIO seemed to function, it really needed a thorough servicing, especially contact cleaning and alignment. To clean the tuning condenser and the bandswitch required removal of the tuning condenser shield and the bandswitch shield. DeOxit was brushed onto the contact surfaces and the component operated to work out the corrosion. I also lubricated the bearings on the tuning condenser to reduce the drag on the BX dial as much as possible. The improvement was dramatic. The bandswitch could be now operated without severe noise being generated and the BFO operation was stable. Tuning was light and didn't slip. The SPKR-TEL switch needed contact adjustment since in the SPKR position there was no connection to the output terminals. The switch was a cam-operated finger-contact type of switch that needed cleaning and a slight adjustment for a positive contact.
|photo left: The tuning condenser shield removed to show the
five-gang air variable tuning capacitor. The rear-most section is the
tracking BFO capacitor.
photo right: The bandswitch shield removed to show the five section, two position bandswitch.
- Alignment is very easy since the RIO is a TRF receiver. Peaking the RF
coil trimmers and aligning the BFO are all that's required. The
procedure starts with Band A and finishes with Band B. There is a pencil
notation (see photo right) on the back of the front panel indicating "Realigned 9/12/35
FHS Tubes OK" and that probably was the last time this RIO
was aligned. Alignment provided a major improvement on both tuning
ranges. The trimmers on most of the RF coils needed considerable
adjustment to "peak" the test signal. After alignment the MVC gain could
be reduced to only 20% advanced for headset listening. BFO has adjustments
on both bands since it has to track the tuned signal. Band A BFO was
slightly off but Band B BFO was so far off that several turns were required
on the trimmer to get the BFO in tune with the signal. After alignment
was complete the RIO was connected to a the 135' CF Inv-vee with 96' of
ladder line that was shorted together. This antenna, although not designed
as a LF antenna, does a good job as a sort of "T" antenna. During
test-listening I heard KPH on 400kc running true CW at 25WPM to honor Memorial
Day. This was at 1100 PDT 5/26/18. Strong signal with clear note. Easy
The fact that the RIO does function on almost all original parts after many decades of idle storage and static display is an indication that National used the very best components available in 1933 for the construction of the receiver. Of course, the circuit is fairly simple and that also might account for the reliability.
Performance - The first thing to remember when listening on the RIO is that there isn't any type of noise limiter or bandpass filters or output limiters,...nothing to suppress noise. Any pulse-amplitude noise is going to disrupt your hearing when using 'phones for audio reproduction. The old radio ops always kept the 'phone cups slightly in front of their ears to avoid painful discomfort when listening in a noisy environment.
The RIO is very sensitive with the manual specs indications as low as 1uv. But at MW and LF that level of sensitivity is usually lost in the ambient noise. Using a low-noise antenna is a real benefit. The remotely tuned loop antenna provides the low noise necessary to take advantage of the receiver's sensitivity. Of course, late-spring isn't the best time of the year for testing a longwave receiver but some regional NDBs can be heard. Listening at 10PM on 5/27/2018 using the wire antenna I heard, MOG 404kc, XX 344kc, ZP 367kc, NY 350kc and DC 326kc. Except for MOG, the remaining NDBs heard were all Canadian beacons that tend to run more power. Conditions were terrible with high static levels that sometimes bordered on painful. The next test will be with the loop but the best test results will be those conducted during November through January. This performance information will be updated when better listening conditions allow for a more thorough test.
Radiomarine Corporation of America
U.S. NAVY - RAZ-1
MW, LF & VLF Radio Receiver - 1941
Serial Number: 65
CRM-46092, CRM-50092, CRM-20096
aka: AR-8503, AR-8503-P, RM-6
15kc to 600kc
The Radiomarine Corporation of America was a division of RCA that specialized in the operation of RCA's Communications Stations and sold RCA-built equipment for both major communications stations and for shipboard installations. The AR-8503 was introduced around 1938 and was designed mainly for shipboard installations. A matching pre-selector was also included, designated as the AR-8503-P. Additionally, an AC power supply was offered, the RM-6. Although in an emergency, the AR-8503 could be operated from a battery pack the preferred method of operation used the RM-6 to supply the required 6 volts for tube heaters, +22 vdc for the detector B+ and +90 vdc for the amplifier plates. Sometime around 1941, the US Navy wanted to install the AR-8503 on some of their smaller ships and a contract was issued for a small number of receivers. "RAZ-1" designated a complete set of equipment that included the CRM-46092 Receiver (AR-8503) with the matching CRM-50092 Pre-selector (AR-8503-P) and the CRM-20096 Power Supply (RM-6.) The contract date was just five days before the attack on Pearl Harbor, Dec 2, 1941.
The CRM-46092 receiver uses four metal octal tubes in its regenerative circuit. The RF amplifier, detector and first audio are all 6K7 metal octal tubes while the audio output tube is a 6F6. The CRM-50092 preselector uses a single 6SG7 metal octal tube as a tuned RF amplifier. The CRM-20096 uses a 5Z4 metal octal tube for the rectifier. The CRM-50092 pre-selector receives power from the CRM-20096 power supply via a three foot long, three conductor cable that is connected to the power supply ground terminal along with the 6vac terminal and the +90vdc terminal. The CRM-46092 receiver has four tuning ranges covering 15 KC up to 600 KC. Three bandswitches - two on the receiver and one on the preselector - have to be utilized for changing tuning ranges. The National Type-N dials are scaled 0 to 100 and have a 180 degree layout. A tuning chart is provided in the manual to correlate the dial reading to tuned frequency. Coupling, Regeneration and Volume controls are on the front panel and the preselector also has an RF Gain control. Audio output is provided for a single audio stage or for full audio output via two telephone jacks on the front panel. Output is designed for the Western Electric 509W earphones and, although any Hi-Z 'phones will work, the 509W phones seem to give the best immunity to noise. The receiver case is shock mounted and is made of copper plated steel painted a grayish-brown color. The preselector case is made of aluminum and painted to match the receiver although it is not shock mounted. The power supply is a standard steel box painted gray. The front panels of the receiver and the preselector are machine textured aluminum that has been matte chromium plated.
|Left photo: The CRM-46092 chassis showing the large bee's
wax dipped coils and the sparse layout of components. The tuning
condenser is inside the shielded box in the center of the chassis.
Right photo: The CRM-50092 preselector chassis showing the tuning condenser and the 6SG7 RF amplifier tube. The RF coils are under the chassis.
I first saw this RAZ-1 in 1997 at the home of W3ON, John Ridgway. It was setting next to the SX-28 he was going to sell me (if I could lift it off of the table.) I asked John if he wanted to sell the RAZ-1, to which he replied, "You wouldn't take a longwave receiver away from an old Navy radioman, would you?" John was living in Galena, Nevada at the time but since he was 85 and now alone, he was moving back to Maryland. John lived to the age of 93, becoming an SK in January 2006. To my surprise, in the summer of 2006, I got a 'phone call from an estate agent who said that they had found a letter among John's papers that stated that he wanted his radios and parts to be sent to the "Radio Museum in Virginia City, Nevada." The agent was calling me to see if I really wanted any of "this junk." I told them I did. The estate paid to ship the parts and equipment back out west. The shipping of the 22 boxes was spaced out over about a six week period. In the 21st box was the RAZ-1. Shipping had caused one small problem, one of the largest coils had broken from its mount. The large buss wiring had kept it in place and all that was required was to glue the mount back together and screw the coil form back in place. I acquired the correct shock mounts from N7ID. I did have to replace the filter capacitors in the power supply for quiet reception.
The RAZ-1 is very sensitive and almost any station on LW can be tuned in however the lack of a calibrated dial makes this somewhat difficult if looking for a specific frequency just using the RAZ-1 dial alone for reference. Though I could use a heterodyne frequency meter if it is important to determine the exact frequency being received, I find it is easier to know approximately where I am tuning by listening to known adjacent signals. In other words, if the NDB MOG is zero beat (or being heard in the background) and I'm trying to copy another weaker signal partially obscured by MOG, I know that weak NDB is on 404kc or very close to it, since that is MOG's frequency. I can usually determine an unknown NDB's frequency within 1 or 2 kc by this method. The lack of any kind of limiter is sometimes a problem if local noise is present, however switching to the loop antenna has greatly reduced local noise. To reduce noise to a minimum, the Coupling is set very close to zero (0 to 25% maximum,) the Volume about 25% to 60% advanced, Regeneration right on the oscillation point (autodyne detection) and then signals are peaked with the the Preselector and then slightly manipulated with the Trimmer control. The Preselector gain is usually set to about 85%. These settings usually result in the best response of signal to noise along with the greatest selectivity. Although very strong signals are encountered from local or powerful stations, very weak MCW signals are the norm when searching for DX NDB stations. Usually, with several NDBs on the same frequency it is possible to slightly de-tune the loop antenna to one side or the other of the frequency and enhance one or more of the NDB signals for successful copy. I have probably logged more NDBs with the RAZ-1 than any other LW receiver. However, that might be because it was one of the first LW receivers that I used when I started logging NDB stations. But, it can always be relied upon to pickup whatever is out there as long as reasonable conditions are present.
Radiomarine Corporation of America
MW, LF & VLF Shipboard Receiver - 1944
15kc to 600kc
|The AR-8510 was the replacement receiver for the AR-8503 (aka RAZ-1 for
the USN - profiled in a section above) and is a five tube regenerative
receiver that tunes from 15kc up to 650kc in four tuning ranges. Two TRF amplifiers
are used with a Regenerative Detector and two stages of audio
amplification. The RF amplifiers use a combination of tuned grid input
and tuned plate output using a three-section ganged tuning capacitor.
The antenna switch allows the user to select which receiver will be
connected to the antenna - either the AR-8510 or an emergency receiver. The audio output can drive the panel mounted loud speaker or headsets
either simultaneously or, using the Loudspeaker switch, the panel
speaker can be turned off. The receiver requires a separate power source of which many
types were available. Various types of battery combinations could be
utilized with either the RM-2 or the RM-4 Battery Control panels. These
functioned on ships that provided 115vdc or 230vdc power. If 115vac was
to be used then the RM-23 Rectifier (power supply) was used. There was
also an RM-37A unit that provided 90vdc B+ output with a 115vdc input
from the ship's power. This
was to be used if it was necessary to conserve the B batteries that
normally provided the +90vdc. The AR-8510 requires 6.3 volts at 1.8A (AC
or DC) and 90vdc at 15mA. The vacuum tubes used are four 6SK7 tubes
and one 6V6G or GT.
photo right: Top of the chassis showing the antenna connections (far left front of chassis) and the power input connections (far right back of chassis.) The tuning condenser is under the central cover.
The AR-8510 could be provided with a cabinet and shock mounts if it was to be used as a "stand alone" receiver. However, if it was going to be installed into a shipboard communications console (as most were) then the cabinet and shock mounts were not provided. Many AR-8510 receivers were part of the shipboard 3U transmitter console that included a 200W transmitter, an emergency crystal receiver, battery charger switching, clocks and more. The 4U console used the RMCA AR-8506 MW-SW receiver with a larger transmitter. The 5U console had both receivers installed along with transmitters and auxiliary equipment. Mackay Radio and Telegraph Company also supplied Marine Radio Consoles MRU-19 or 20 that had their equipment installed.
The AR-8510 was approved by the FCC for shipboard use in 1942 (concerning minimum radiation from the antenna.) The schematic drawings are dated 1943. It's likely that it was at least 1944 before any AR-8510s were in use and this particular AR-8510 is dated NOV. 1944 (with a serial number of 2774) making it an early example. It seems that most of the installations during WWII were onboard Liberty ships. Post-WWII installations were generally on commercial ships. The AR-8510 found a lot of use and longevity with some receivers still in use onboard some old oil tankers as late as the 1980s.
Unfortunately, most AR-8510 receivers led a pretty hard life
and the sea environment didn't help preservation. Most examples have
been worked on or have missing parts (or non-original parts.) The
AR-8510 shown in the header photo is cosmetically restored with nearly all original parts. The
exception is one capacitor under the chassis, the speaker grille and the RCA pointer knobs. The
paint job on the front panel is VHT Gray wrinkle finish which is
slightly darker than the original RMCA gray.
|Later manuals and some Internet sites will show a slightly
different AR-8510 that has silk-screened nomenclature on the panel
including the information on the data plate silk-screened onto the
panel in the upper right part of the panel. The B&W photo (shown
right) in the 1950 manual shows this later version with a date on
the panel of 1947. It's probable that the WWII version (early
version) used the easy-to-replace nomenclature tags as an
ease-of-maintenance function. Later post-war receivers were probably
not going to be subjected to the rigors that the wartime versions
experienced so the silk-screened panels could be used and provided
an excellent appearance.
I was given the AR-8510 shown in the photos as payment for some radio repair work. It probably was taken off of one of the Liberty ships that were part of the "moth-balled" fleet that was moored outside of Benicia, California since the receiver originally was obtained from the SF Bay Area. The "as received" condition was fairly good considering how the ships were taken care of - they weren't. Of course, the front panel has been repainted in the past - probably with a brush. The perf-metal grille had more than its share of paint applied (and it wasn't original either.) The receiver came without any type of power supply (the RAZ-1 power unit RM-6 can be used as a power source.)
|This AR-8510 required a little bit of work to get it
operational. Bands 1 and 2 functioned okay but needed alignment.
Band 3 and 4 were non-functional due to broken leads from the coils
that are in the plate circuit. The open coils resulted in an
absence of plate voltage to the first RF amplifier when bands 3 or 4
were selected. I had to remove the coils and rebuild them then finishing them
off with a re-waxing job. After reinstalling, bands 3 and 4 had to
Performance using a "T" antenna of 98 vertical feet running to a 135 foot horizontal section was very good. Since the AR-8510 was the replacement for the AR-8503, it's fair to compare the two receivers. First, with a direct readout dial there's no need for the charts and graphs necessary for finding where you're tuned on the AR-8503. The preselector is built-in with the AR-8510. Also, only a single band switch is necessary on the AR-8510 while two band switches are used on the AR-8503 plus a band switch on the preselector. Sensitivity on the AR-8510 is about the same as the AR-8503 with preselector. Regeneration action is very similar in that it's a very sharp adjustment between maximum sensitivity (either non-oscillating or oscillating) and any adjustment below either point greatly reduces sensitivity (this is typical of regenerative detectors though.) The AR-8510 seems to hold its adjustments better across the band especially the Trimmers that only require a slight adjustment from one band end to the other. This is expected since it's part of the alignment process. I find that the loudspeaker is actually pretty good for some reception. If you want to use Hi-Z phones, it's better if you leave the loudspeaker on. Without the speaker load the 'phones seem to respond to more noise than signal.
Andrea Radio Co. CND-46155,RAK-7 - 1944
Andrea Radio Co. CND-46156,RAL -7 - 1944
The Navy wanted more modern LF, MW and SW receivers in the mid-thirties so RCA provided the Navy with the RAK/RAL series. The RAK/RAL were to replace the aging RAG and RAH receivers built in 1933. The RAG/RAH were TRF receivers with non-regenerative detectors and tracking BFOs built by Sylvania. There was an early version of the RAL that was supplied to users other than the USN that was designated as the TBR.
Any receiver built for shipboard use had to be "bullet and bomb" proof, in other words, the ship had to take a couple of torpedoes, be sinking fast and the radio gear would still be working. Additionally, steel and iron was kept to a minimum in shipboard radio construction to reduce corrosion problems that were common on marine equipment. The RAK/RAL series were built like the battleships they served on. The construction is something to marvel at - so over-built, so heavy-duty with no expense spared - it's no wonder that most RAK or RAL receivers still function with all original parts even though they are pushing seventy years old. The design concept was to provide maximum reliability in severe service by simplicity of design - and it paid off since the receivers were in use up until the end of WWII with their last service on board submarines.
RCA was the primary designer and builder of the first contracts of RAK and RAL receivers. During WWII, Andrea Radio Corp. became another contractor building RAK and RAL receivers. The RAK, (aka CND-46155 by its Andrea/Navy designation, substitute "R" for the "N" for the RCA /Navy designation) covers 15kc up to 600kc in six tuning ranges. There was a RAK-8 and RAL-8 produced with Magnavox as the contractor.
The RAK and the RAL used glass tubes that were large six-pin type, 6D6 tubes for the two RF amplifiers, a 6D6 for the regenerative detector, a 6D6 for the first audio amplifier, a 41 for the audio avc amplifier and another 41 for the audio output. The power supply, CNV-20131, was a separate unit that used a 5Z3 rectifier, an 874 regulator tube and an optional 876 ballast tube. The 876 can be left out of the power supply if the AC power is stable and noise free. An internally mounted switch routes the 120vac to a different tap on the power transformer if the ballast is not required. If the ballast tube is installed it will be on regardless if it is used or not although less current is flowing through it when it is switched out of the circuit. When switched in, the 120vac actually is dropped through the ballast and a different tap on the power transformer is used (~70vac) thus providing the regulation of the AC to the transformer if the line voltage is not stable. Since the ship had to generate its own power and most of the equipment onboard (including motors to rotate gun turrets) ran on this power, the varying switching loads are what caused the line voltage fluctuations that required using the ballast regulators. In shore set-ups, on standard AC line power, ballast regulators were not required.
The RAK is designed for CW or MCW only. The receiver has a low pass filter that is permanently connected in the audio circuit to roll off the upper audio frequency at about 1200 hz. An elaborate audio avc circuit allows the user to limit the audio or noise peaks at an adjustable level. This was to allow the receiver to be used in heavy static conditions. Also a selectable audio bandpass filter was provided to enhance CW reception in noisy conditions. Voice can be received but it is severely limited on the higher audio frequencies making copy difficult. The manual states that another receiver should be used if voice reception is required - like the RAL. The tuning of the RAK is heavy duty, gear driven and the tuning dial readout is shown on two circular dial scales of 0 to 10 and 0 to 100. The actual tuned frequency has to be correlated with a graph that is in the manual. The receiver does provide a logging chart on the front panel for a "most used frequencies" reference. A frequency trimmer, an antenna trimmer, sensitivity and regeneration controls on on the lower panel of the receiver. The meters monitor audio output level in db and tube heater voltage. The RAL receiver is almost identical construction but has nine bands covering 300kc to 23mc. Additionally, the low pass filter can be switched out of the circuit for voice reception and a vernier frequency control is provided. Most of the concern about a stable AC line voltage was directed at the RAL receiver which itself can become unstable at high frequencies if the line input varies. Normally, the two receivers operated together through a control box (CND-23073) that allowed the radio op to monitor two frequencies simultaneously. The control box also could be used to switch the AC to the receivers on or off.
photo left: The RAK and RAL in use aboard a US Navy ship. Also, National RBL and RAO receivers far left, the LM-type frequency meter by the telephone handset and a Scott SLR-type receiver below the order binders.
|Nowadays, a RAK and RAL set up will require an ample and heavy-duty
table for the complete set-up.
In my installation I had the power supplies for the RAK/RAL receivers
bolted to the underside of the table. I provided for a space of about
3.5" above the supplies to allow good ventilation for the ballast tubes.
I ran the power supplies with their ballasts even though wasn't
necessary. The actual difference in power consumption is significant -
the ballast dissipates about 140 watts. I had run the receivers
both with and without ballasts and I noticed that the received noise seemed to be
slightly less with the ballast in use.
In actual operation, the RAK is a very sensitive receiver that spreads the LF tuning range over several bands. This bandspread action is nice for tuning in weak stations or trying to separate several stations that are on the same frequency - as many NDBs are. The major problem is that calibration is relying on the readout versus a graph and that graph is in the manual. The first thing to do is make a copy of the frequency graph to keep with the receiver. Next is to calibrate the RAK so the readout is fairly close to the graph. Then it is easy to keep track of where you are in the LF spectrum. If it is important to know the exact frequency, I use a heterodyne freq-meter set up. The Audio AVC will help with static crashes and to a certain extent, noisy conditions but, like most output limiters, if it is advanced too far it severely clips the audio with high distortion. The adjustable bandpass filters are almost useless. This is due to the high frequency chosen for the first audio frequency cut-off - 450hz. This may have been fine for true CW but that is seldom encountered anymore in the LF bands. All NDBs use MCW with a 400hz tone. The lowest setting of the filter works okay on NDBs but the other bandpass frequencies are even higher in frequency and so are not very useful.
The tuned loop antenna, with its high Q, really helps reduce the noise and increase the signal to noise ratio. The audio output is taken from the front phone jack. It's 600Z ohms and, while the RAK will easily drive a 600 ohm speaker, many more weak signals can be copied using earphones rather than a speaker. I have tuned in all of the normal LF signals with my RAK-7. The best NDB DX were several in North-Eastern Canada and Puerto Rico's powerhouse transatlantic beacon, DDP. At lower frequencies, the RAK seems to get better and better with JJY at 40kc a fairly regular copy. The Navy MSK-RTTY signals from 19.8kc up to 25.2kc are always present.
Army Signal Corps
BC-344-D - LF/MW Radio Receiver - 1944
150kc to 1500kc
SN: 5 Contractor: CFN (Farnsworth)
Order No. 10651-PHILA-44
|The BC-344 belongs to a family of radio receivers that were designed by the U.S. Army Signal Corps at Fort Monmouth, New Jersey in the late-thirties. The early versions of the receiver used more aluminum in the chassis and some early versions were painted with a "leatherette" finish paint (properly called "Crackle Finish.") By the time WWII contractor manufacturing had started, the receiver used an all-steel chassis and the paint used was the standard black wrinkle finish. Farnsworth Television & Radio Corporation built the AC operated versions, those being the BC-342 and the BC-344. RCA Manufacturing Co., Inc. built the DC operated versions, those being the BC-312 and BC-314. The BC-312 and BC-342 are shortwave receivers with six frequency ranges that cover 1.5mc up to 18.0mc. The BC-314 and BC-344 are LF (low frequency) and MW (medium wave) receivers with four frequency ranges the cover 150kc up to 1500kc. The BC-344 has two RF amplifiers and two IF amplifiers (four 6K7 tubes.) A separate Mixer (6L7) and LO (6C5) are used. The BFO uses a 6C5 triode, the detector-AVC-first AF is a 6R7 and the AF Output tube is a 6F6. There are ten tubes used in the BC-344 including the 5W4 rectifier tube used in the RA-20 power pack that mounts internally. No selectivity filter is used in the BC-344. Audio output is generally 4000Z ohms but may be set to 250Z ohms by moving a jumper inside later versions of the receiver. The LS-3 loudspeaker was commonly used with the BC-344 receiver although a headset would allow copy of weaker signals.|
||The Signal Corps utilized the BC-312/314/342/344 receivers in many
applications. Fixed stations generally used two or more receivers paired
with at least one BC-191 transmitter. A typical Army station is shown in
the photo to the left. Note that three BC-342 receivers are utilized
with an AC operated BC-191 transmitter (the RA-34 power supply is
barely visible under the transmitter table.) Mobile stations ranged from small
vehicle set-ups to the SCR-299 that used a BC-342 and BC-344 set up with
a BC-610 transmitter, all powered by an AC generator towed in a trailer.
Most DC set-ups operated on 12vdc from vehicle battery-charger systems.
There was a 28vdc BC-312 version, the BC-312-NX.
BC-344-N on Long Wave? - I've been interested in how well the BC-344 would perform on MW and LF reception for some time. I have a "rough-condition" receiver that had been painted "metallic" green. I even had it on the work bench once but I lost interest when I saw some "hamster" rework inside. Recently (2016,) I obtained another BC-344 receiver that happened to have the scarce shock mount installed. This receiver seemed to be pretty original and virtually complete. Replacements for the few missing or poor condition parts were easily located in my BC-312/314/342/344 junk box.
Reworking the BC-344-D - Since the BC-312/314/342/344 were essentially "workhorses" for the Army, many are in rough condition today. All will require some work and many require a full restoration in order to function correctly. The receiver is difficult to disassemble and this has saved many BC-344s (and 342s) from being modified too much by hams. Most hams preferred to modify the easy-to-work-on BC-348-Q. Most 344/342 receivers will be very close in alignment because all of the adjustments were "locked" if they were easy to access, like the IF transformers, or hidden by covers or plugs in the case of the RF adjustments. Most receivers will be missing the dial lock since this piece often times interfered with the rotation of the vernier knob. It's not unusual to do mostly a cosmetic restoration and have the receiver work with all original parts with the exception of the dual electrolytic filter capacitor located in the RA-20 power pack.
Dismounting - One of the common problems with any of this
series of receivers was present on this BC-344. That is, the plastic dial
index that always seems to have warped, cracked and discolored to the
point where it's no longer even transparent. Luckily, I had an excellent
condition replacement. Unfortunately, to install the index requires
completely dismounting the front panel.
I say "unfortunately" because this task is unbelievably complicated by the Army's mechanical design that never seemed to even consider the possibility that the receiver might need to be disassembled someday. Besides the abnormal amount of front accessed screws there are three screws that mount from the backside of the panel that must be removed. The two fuse holders must be unsoldered and removed. All of the phone jacks and controls must have their mounting nuts removed. The wires to the dial lamps have to be unsoldered. All of the wires going to the front panel "trunk" connector have to be unsoldered. The power input terminal strip has to be dismounted. All screw connections to Antenna and Ground connections have to be dismounted. Knobs and control nuts must be removed. At this point, you'd think the front panel would easily come off, but not yet! The Fast Tuning gear has a pinned shaft that is flanged. You can't remove the front panel unless the gear and shaft are taken apart and that requires driving out the pin. However, once the gear and flanged shaft are apart, the front panel finally can be dismounted.
photo right: A rear view of the chassis showing the stout construction of these receivers
|At this point, installing the replacement dial index is easy (it's
mounted with eight screws!) Since the front panel is off, now is the time for a thorough cleaning
and touch-up. I use jet black nitrocellulose lacquer that is thinned
about 3:1 for touch-ups. After the lacquer has set for a while, I rub
down the panel with light weight machine oil. Usually, this will blend
the color of the touch-ups with the original black wrinkle paint making
the touch-ups invisible.
When remounting the front panel, it will be noted that all of the 6-32 screws are the same length. However, there are three different length 4-40 screws. The four long 4-40s are for the wire mounts. There are two short 4-40s and the rest are all the same length. The two short 4-40s are very important. There are two places where, if long 4-40 screws are used, they will protrude far enough thru the rear panel mounted nut to contact the dial mask with possible scratching of the mask when the band switch is operated. The "short" 4-40 screws must be mounted as follows: One "short" screws is by the band change switch and is the screw nearest the "G" in "CHANGE" in the nomenclature of that switch. The other "short" 4-40 is used near the lower left side of the data plate (the screw head almost is contacting the data plate edge.)
The other observation is the small component board that is mounted to the back of the front panel uses two different length stand-offs. The reason is that the lower screw must past thru a part of the chassis mounting flange and the top screw doesn't. The longer stand-off is the upper one.
Patience is required in any BC-321,314,342,344 rework. The work is tedious and none of the component parts are easy to access without removing another part or assembly first.
Capacitor - Most military gear used oil-filled paper
dielectric capacitors as the filters. The disadvantage of this type of
capacitor was its large size but the advantage was long-term reliability.
Since space was at a premium in the RA-20 power supply, a dual
electrolytic filter capacitor was used. The advantage was a small
size for two 8uf 450vdc caps but the disadvantage now is, after 75
years, the dielectric paste has dried up and drastically reduced the value of
There's ample room to mount new electrolytic capacitors inside the old capacitor can. There are many methods to accomplish this "re-stuffing." I cut the cap in two and remove the old cap and black wax using a heat gun to soften the wax. This allows the old capacitor to be easily pulled out of the can. I install new capacitors connecting them to the correct terminals and then epoxy the can back together. I remount the rebuilt cap and connect it into the circuit.
The photo to the left shows the underside of the BC-344 and in particular the RA-20 power pack. Note that the RA-20 is "swung out" on the right side hinge mount. Also note the wiring harness that is connected to the power terminal strip.
|Miscellaneous Rework - Sometimes the OFF-MVC-AVC switch contacts don't allow the operator the ability to turn the receiver on. These are special build, stacked switches that have the MVC and AVC switches enclosed. Luckily, the AC on/off switch is only covered with a fiber disk that can be bent to allow access to the arm and contacts. It's usually only dirt or maybe minor corrosion that is causing the problem. This can be cleaned off using a small piece of Alu-Ox paper or a very small wire brush. It might be necessary to bend the arm slightly to have better contact. If the AC contacts are damaged beyond reconditioning then the entire switch has to be replaced with a used-good original. These are sometimes difficult to find except from parts sets. The same switch is used on all of the versions of the BC-312, 314, 342 and 344.||Alignment Notes - IF is 92.5kc. Note in the photo above left that the large LO box (far left) has four plugs that are covering access to the trimmers for each band. Also note the shield cover over the two RF amp boxes and the Mixer box that is preventing easy access to these trimmers. Each IF transformer adjustment has a lock nut on the threaded shaft to prevent tampering (see photo above right showing top of chassis.) Other than the lower frequencies involved, the BC-344 is straight forward in its alignment procedure.|
a Wire Antenna - The antenna used was my 135' CF
Inv'd Vee with 96' of ladder line with the two feed line wires tied
together. This is something like a "T" antenna and it performs fairly
well on LF. The test listening was on January 29, 2018 from 1915 to 1945
PST. I only tuned the BC-344-D from 405kc down to 300kc. Within the
frequency span and time period I tuned in 25 NDBs. Greatest USA DX was
IN 353kc in International Falls, MN. Greatest DX was YMW 366kc in
Manawaki, Quebec, CANADA. Another Canadian NDB tuned was YXL 346kc in
Sioux Lookout, Ontario. Listening QTH was Dayton in Western Nevada.
All signals were heard over a headset, not by loudspeaker. BFO was on and stations generally tuned for zero beat of carrier to then hear the MCW tone correctly. The AVC was off. Noise level wasn't too bad and I'd rate the conditions as "very good."
The BC-344-D is a capable LW receiver that has ample sensitivity in the medium wave portion of the spectrum using a wire antenna. There is no crystal filter or any other method to reduce IF bandwidth so many signals are "heard" over what seems to be a fairly wide IF passband. It's easy to select one particular signal and then concentrate on that tone or sound of the signal to then successfully copy the call. Most of the time this process will be with very, very weak signals that are within the passband with stronger signals. If the received noise seems to be covering up some weaker signals it's possible to slightly "detune" the antenna trim (ALIGN INPUT control) to reduce the noise while not affecting signal copy.
While the BC-344-D is kind of a "basic" superhet with no fancy filters or output limiters, it does a good job with the few controls provided. It's certainly sensitive enough and the reduction of the VERNIER tuning mechanism allows for easy tuning of all stations, including NDBs. Without an output limiter though there isn't any way to reduce "pops and clicks" or heavy static. Wearing the 'phones just ahead of the ears is recommended. I'm sure if the BC-344-D was used with a wire antenna in a modern RFI-noisy, urban-type location the weak signal DX reception would be terrible. But, in the rural RFI-quite area here in Dayton, NV, the BC-344-D does a very good job of pulling in NDB DX using just a wire antenna.
|Performance on a Tuned Loop
Antenna - The remotely tuned loop is six feet "point to
point" of its diamond-shape and tuned using varactor diodes with a
variable bias voltage source. The receiver is connected to a pick-up
loop that is mounted within the main loop. Test listening was on
February 1, 2018 from 1930 to 2000 PST. I only tuned the BC-344 from
325kc up to about 390kc. 23 NDB stations were tuned in during that time.
Conditions were very good. Greatest USA DX was FIS 332kc in Key West,
FL. Greatest Canadian DX was GW 371kc in Kuujjuarapik, Quebec, CAN.
All signals were heard over a headset, not by loudspeaker. BFO was on, AVC was off. Loop Antenna was pointing NE/SW for the entire test listening period.
The BC-344-D running with the tuned loop antenna is a surprisingly good performer. Without any bandwidth controls, one would expect noise to be a problem but the loop does keep the noise level somewhat lower than the wire antenna. Additionally, the "loop tuning" provided the ability to slightly detune the peak adjustment which lowered the noise without causing loss of the signal. This was a nice advantage for signals that were "in the noise." Also, the ALIGN INPUT (antenna trimmer) could be used to slightly detune the antenna and reduce the noise peaks allowing some weaker signals to be copied. These two features, loop tuning and antenna trimmer, do a lot to make up for the "wide open" IF bandwidth which does have a tendency to be somewhat noisy.
As mentioned in the "wire antenna test" section, the BC-344-D is a pretty basic receiver with no filters or no bandwidth control. Yet, I was still able to copy NDBs all the way to the east coast and Canadian NDBs out to Quebec. I don't think any vintage LW receiver enthusiasts will be going out to purchase a BC-344-D to use as their main LW receiver, but I was impressed with its performance and would rate the receiver as one of the better medium wave and low frequency receivers. It is fully capable of receiving DX LW signals and, with its incredible "WWII Military" appearance, makes a fine addition to any collection of vintage LW receivers. Additionally, if you get tired of listening to MCW signals on 'phones, you can always tune in almost the entire AM BC band and listen on an LS-3 loudspeaker - very cool.
National Co., Inc.
RBL-5, CNA-46161-B - MW, LF & VLF Radio Receiver - 1945
15kc to 600kc
|National Company also provided a great LW receiver for the Navy in WWII - the RBL series of regenerative receivers. Following the long Navy tradition of National providing NC-100A types of receivers - like the RAOs and similar HF receivers, the RBL series uses the same general appearance with a similar dial layout and a familiar band switching feel. Though the bandswitch looks like the RAO catacomb system, it isn't. The mechanism uses several large gears to simultaneously actuate two large ceramic switches to provide band changes. The RBL is the same approximate size as the RAO receivers so it was probably intended that they be paired up for coverage from 15kc to 600kc on the RBLs and 540kc to 30mc on the RAOs. Unlike the earlier LW receivers described above, the RBL has a built in power supply and has direct frequency readout on the illuminated dial. Like the RAO receivers, Wells-Gardner Company was a second contractor and built the RBL-3 and RBL-4 versions under contract using many National parts for assembly (see RBL-3 at the bottom of this write-up.)|
|The circuit uses a cascade of three 6SK7 RF amplifier stages. The detector is a 6SG7 regenerative autodyne detector
followed by a 6H6 audio limiter circuit followed by a
6K6G audio tube. The power supply rectifier is a 5U4 in early RBLs but later was
changed to a 5Y3G. Like the RAO, some RBL receivers were built by Wells-Gardner
Company. Heavy duty construction, ample shielding, copper-plated cabinet under
the black wrinkle paint are standard construction used in the RBL receivers.
They were normally bolted to a cushioned mount that attached to the holes in
the lower front and rear corners of the cabinet. Nowadays these mounts are
usually missing. Included in the circuit is an audio filter for wide or narrow
bandwidths (switch on left side of escutcheon below ON-OFF switch) and an adjustable audio limiter
(switch and control on right side of escutcheon.) The limiter is very well designed
and works wonders in reducing the static crashes while not distorting the audio
signal. The direct frequency readout on the dial is the major advantage of using
the RBL receivers and the accuracy is impressive considering the receiver's age.
The illuminated dial is quite a departure from the usual military LF
receiver. The lower controls (l to r) are gain, regeneration, bandswitch, antenna trim,
oscillation push button
and frequency trim.
This RBL-5 was acquired from a ham neighbor here in Virginia City. It required a little work before it was functioning to its specifications. The tubular antenna connection input that attaches to the box that bolts to the back of the cabinet was shorted internally so essentially whatever antenna was connected was shorted to chassis. Removal of the tubular connector and just running the coax through the box directly to the antenna and ground terminals fixed the problem. Also, there was a soldering job at the audio output transformer that was poorly done. Exactly what the object of the solder job was is not known but it probably was in search of the lack of output that was really caused by the shorted antenna input. Fortunately, no original parts were removed and only the connections to the audio output transformer were moved to incorrect terminals. We just returned everything to the original connections and then the receiver output returned to normal.
photo left: The chassis on this RBL-5 is immaculate and all original. RF section is on the right side of the chassis and the power supply, limiter and audio sections are on the left side.
I have logged a lot of NDBs using this RBL-5 receiver, primarily because the RBL-5 is easy to use, very sensitive, has direct frequency readout and the limiter functions quite well. The limiter makes long sessions of receiving comfortable since the static crashes are reduced to the point where they aren't causing headaches anymore. I take the audio output right from the earphone jack on the front panel running 600 ohm 'phones for best copy on weak signals. The NBDs normally copied are multiple stations operating on the same frequency, with two and sometimes three different CW identifications being heard simultaneously. Using the RF trimmer and the Antenna Compensator controls, it is usually possible to enhance one or the other of the MCW signals and identify the particular NDB, (the RAK and RAZ LW receivers also have this ability to manipulate the signal a little to enhance copy.) The RBL works particularly well with the tuned loop antenna and this provides the ability to add some directional characteristics to the reception. Additionally, the loop can be slightly de-tuned to allow enhancing NDBs that are on one side or the other of antenna resonance which can sometimes help with copy.
photo right: The underside of the RBL-5 is also immaculate and all original. The photo shows the multiple gears that drive the two ceramic bandswitches. Construction is first rate as expected from National Company. Note that the alignment trimmers are all clustered together. The bottom cover has a sliding access panel that allows the receiver to be aligned with the bottom cover installed - probably why the RBL-5 has such an accurate dial readout.
|Shown in the photos right and left is the Wells-Gardner Co. version, the RBL-3. This receiver is also in excellent condition. Note the difference in the transformers and chokes used in the W-G version compared to the National RBL-5. Typically, W-G used mostly National parts but did use their own transformers, chokes and smaller components. Note the rectifier tube in the upper left corner is a 5U4G rather than the 5Y3GT used in later versions of the RBL. Performance of the W-G RBL-3 is the same as the National RBL-5.|
RCA-Federal Telephone & Radio Corporation
U. S. NAVY
15kc to 600kc
1943 RBA-1 CFT-46154
In the late thirties, it was becoming apparent that a replacement receiver was going to be necessary for the aging series of longwave receivers used by the Navy at that time. The receivers included the RAA superhet from 1931, the RAG TRF from 1933, the RAK TRF with regenerative detector from 1935 and the various upgraded versions of these receivers that were built on later contracts. The new LW receiver design was going to blend the advantages of the TRF plus tracking BFO design of the RAG receiver but built with modern circuits. Using a TRF with tracking BFO was advantageous in keeping the leakage radiation on the antenna to a very low level that prevented enemy direction finding equipment from determining the location of the receiver. Additionally, the low-level of radiation allowed the receiver to operate in the presence of other receiving and transmitting equipment along with radar equipment without interference. The tracking BFO design utilized a section of the main tuning condenser so the BFO tuning condenser was ganged to the main tuning. Since the new receiver was not a superheterodyne, the BFO had to track at 1kc above the tuned frequency allowing a 1kc heterodyne to be heard thus allowing CW to be readily copied. There were a couple of very good reasons for not designing the new LF receiver as a superheterodyne. First, was to provide complete coverage of the tuning range of 15kc to 600kc. Most IF amplifier sections utilized around 400kc to 500kc for the intermediate frequency, right in the middle of the most used portion of the medium wave band (as far as the Navy was concerned.) Operation of the IF amplifier at, for example 455kc, would eliminate a section of frequency coverage of about 20kc either side of the intermediate frequency. Some superhet LW receivers moved the IF above the intended tuning range (15kc to 600kc) but there were disadvantages to this solution to the problem. For example, the RBH receiver uses an IF of 1500kc but any transmitting activity around 1500kc will "leak into" the IF section of the receiver and cause heterodynes throughout the tuning ranges.
The separate power supply is the CRV-20130, which is the same power supply used for the 15 tube RBB and RBC superheterodyne receivers. The CRV-20130 provides the filament voltage and B+ requirements via an armored cable with heavy-duty connectors. The power supply will easily operate two RBA receivers for emergency conditions and two separate connectors are provided. The power supply has a cold-cathode regulator tube (OC3) and a HV rectifier (5U4.) The RBA uses eight tubes, three 6SK7 RF amplifiers, one 6J5 Triode Detector, one 6SK7 BFO, two 6SJ7 AF amplifiers and one 6K6 AF Output. Table top versions of the RBA receiver were identified as C(FT)-46154 (FT would indicate that Federal Tele. & Radio Corp. was the contractor) and CFT-46154-A (RBA-5) while the rack mount versions are identified as CFT-46300. Internally, all versions of the RBA receiver circuit are the same.
| photo left: Inside the RBA-6 receiver showing the top of the
chassis. All of the TRF coils are in the cylindrical shielded cans to
the left. The moveable covers on top of the cans allow access to the trimmers for
alignment. The two front coils are for the tracking BFO. Note the
gear-driven potentiometer coupled to the main tuning. This is the
auxiliary gain control that allows for constant gain across the tuning
ranges. Also note the shielded meters. The blue "dots" on the tops of
the tubes are my indicators that I have tested these tubes and they are
in good operational condition.
photo right: The underside of the RBA-6 chassis. Full shielding of each RF section is provided when the bottom cover is installed. The heavy-duty band switch uses ceramic mounts with .25" silver-plated contact buttons. All components are mounted on terminal boards or are mounted directly to the chassis. Tracking BFO is the front section of coils. RF3, RF2 and RF1 are next going towards the rear. The rear-most set of coils are the Antenna Input coils.
Mackay Radio & Telegraph Company
Marine Radio Receiver Type 3001-A
Commercial MW, LF & VLF Shipboard Receiver
15kc to 635kc
Model Introduced in 1948 SN: 52-M-070 from 1952
Mackay Radio & Telegraph Company was founded by Clarence Mackay, son of John W. Mackay, one of the "Big Four of the Comstock" fame in Virginia City, Nevada. However, by the time this Mackay Radio receiver Type 3001-A was produced, International Telephone & Telegraph Co. had owned Mackay Radio for a couple of decades. ITT continued to use the Mackay name in their marine radio equipment up until just recently, 2006.
The 3001-A is a Longwave regenerative receiver covering 15kc to 635kc in four bands and although the design dates from around 1948 this receiver was built in 1952. The 3001-A is an updated version of the WWII Mackay Type 128-A receiver. The 3001-A was mainly for commercial shipboard (non-military) use where it could be set up as the main receiver or as the emergency receiver. These receivers were sometimes installed into Mackay MRU-19/20 shipboard radio consoles - two 3001-A receivers were normally used in these set-ups along with transmitters and other auxiliary equipment. The 3001-As were panel mounted when installed in the MRU set-ups. The receiver uses an AC-DC circuit and can operate on 115vac or on batteries. Various filament battery options were available with 6vdc, 12vdc and 24vdc being the most popular. B+ was supplied by standard dry cell B batteries when used. The receiver uses a four pin Amperite ballast tube along with six octal tubes. The cabinet has "knock-outs" all along the back and the bottom-rear to allow routing the various cables necessary for the installation. These would consist of the Main Antenna and Auxillary Antenna, the AC power connections, the DC power connections and an external earphone connection. A small built-in speaker provides for radio room monitoring but earphones would normally have been used by the shipboard radio operator. These type of Mackay receivers were used onboard ship for decades (a few reports indicate that some may still be in use.)
|photo left: Top of the chassis showing the Jones plugs that are for
the power and signal inputs to the receiver. The large resistor is for operation on
12vdc for the filaments.
photo right: The under side of the chassis showing the various coils and other components. This receiver was partially re-capped sometime in the past.
|This Mackay 3001-A was a ham swap meet find purchased in October, 2009. The design and construction of the Mackay 3001-A is obviously commercial and is no where near the "cost-no-object" designs and "over-built" construction that were used by the Navy. Still, the receiver is an impressive performer and has some interesting designs in the circuitry. Tubes used are 1 - 6SK7 RF Amplifier, 1-6J5 Detector, 2 - 6SJ7 AF Amplifiers, 1 - 6G6G Audio Output, 1 -35Z5GT Rectifier and 1 Amperite Ballast Tube. Interestingly, the detector input is also directly connected to the first AF amplifier since the 6J5 is acting like a diode. Each Detector coil has its own "tickler" winding which is routed back to the RF Amplifier's screen and is controlled by a 50K Regeneration pot. Selectivity is controlled by a combination of the RF Gain setting and the setting of the Regeneration - too much RF Gain results in very broad signals. Best performance is achieved using earphones with the AF Gain fully advanced and using only what RF Gain is necessary to hear the signal. Regeneration should be set just at the oscillation point or slightly into the oscillation range - which ever gives the best signal. The Antenna Trim will somewhat manipulate the signal tuning and can contribute to successful copy on very weak signals. The vernier reduction action of the main tuning dial seems a bit fast at first but in actual use the bandspread is wide enough that the tuning rate works out just fine. The 3001-A is a great little receiver (weight is only about 35 lbs) with excellent sensitivity and it is capable of receiving just about anything in the LW spectrum. Besides all of the normal NDBs, this 3001-A also has received the LW BC station from Sakhalin Island on 279kc and also JJY 's pulse-coded time signals from Japan on 40kc. The Navy NSRTTY station from Hawaii on 21kc and from Cutler, Maine on 24kc both can received quite well. An impressive receiver that doesn't challenge your back to move.|
Army Signal Corps
MW, LF, VLF Double Conversion Superheterodyne
15kc to 1500kc
SN: 268 from 1951 Contract (1955 build date)
1955 R-389 SN: 268 installed in CY-979A Mobile Table Cabinet
Description - Electronics - Built along some of the same lines as the famous R-390 receiver,
the Collins R-389 is essentially the LF companion to the R-390 receiver, covering 15kc to 500kc in one
tuning range and 500kc to 1500kc in the second tuning range. The R-389
uses very complex methods, both electronic and mechanical, to achieve its complete MW, LF and VLF coverage while still
utilizing a 455kc IF. The receiver uses 36 tubes within five modules
that interconnect and are mounted within the main frame. The 15kc to 500kc
tuning range utilizes five permeability-tuned RF bands. The 500kc to 1500kc tuning range
utilizes two permeability-tuned RF bands. The band switching is
motor-driven and occurs
seamlessly as the receiver is tuned from the lowest to the highest
frequency within the two tuning ranges.
Two RF amplifiers are used and the first conversion mixes the incoming RF signal frequency with the VFO (470kc to 1955kc output f) plus the 10.455mc Crystal Oscillator (8.5mc to 9.985mc resulting f) to achieve a 10mc IF. The second conversion mixes the 10mc IF with the same 10.455mc Crystal Oscillator to achieve the 455kc IF. This double conversion scheme was to allow complete coverage from 15kc to 1500kc with no gaps in the frequency coverage. Additionally, since the two mixer stages are 180 degrees out of phase, any drift within the conversion mixers is cancelled leaving only the VFO drift. This is similar to how the "drift-cancelling" Wadley Loop operates.
From the second mixer circuit on, the R-389 utilizes the same modules that are found in the R-390. That would be the six-stage IF module, the two channel audio and electronic voltage regulator circuit module and the power supply module. Although the PTO (VFO) looks exactly like that found in the R-390, it's very different inside and tunes from 470kc to 1955kc.
- The manual tuning of the receiver RF front end uses clutch-coupled gears to rotate
the main RF tuning shaft that has worm gears that perpendicularly engage and
rotate the gear-driven front and rear line shafts
that have worm gears that in turn engage gear-driven vertical
screw-shafts (cut with forward and reverse threads) that raise and lower the various slug racks.
gear-driven system is correctly adjusted and lubricated sparingly with
light-weight oil it will be easy to manipulate and have the feel of a
good condition R-390A gearbox. Since the two tuning ranges cover so much
clutch-coupled, motor-drive tuning system is
provided. A separate motor-drive band switching system is also provided
to select the proper band (one of seven) to allow seamless bandswitching
as the receiver is tuned throughout it ranges.
The Veeder-Root counter is somewhat different than that used in the R-390 and provides two sets of digits, one for 15kc to 500kc (lower set) and the other for 500kc to 1500kc (upper set.) The resolution of the digits (tuned f) is to the tenth of a kilocycle (which are the red background digit wheels.) Neither a calibration oscillator or an antenna trimmer are provided (or needed.)
Most of the controls are the same as those found on the R-390. The BFO controls, the Noise Limiter, the Local Gain, Line Gain, Line meter range switch, RF Gain, AGC switch, Break-in switch, Audio Response switch and Function switch. The controls that are unique to the R-389 are Motor Drive, IF Bandwidth (five ranges instead of six,) RF bandwidth KC indicator and the single tuning knob. The two meters perform the same functions as the R-390 meters, that is, Carrier Level and Line Level.
- Physically, the R-389 is the same dimensions as the R-390 and will fit
into the CY-917 or CY-979 table cabinets. If installed into a table
cabinet, the top and bottom covers should be removed. The receiver
weighs 82 pounds but, for easier moving (e.g., up or down stairs,) the
power supply and AF module can easily be removed and then the receiver
weighs around 65 pounds.
Two antenna connectors are available. Balanced input for 125 ohms input impedance from dipoles or other balanced antennae. Balanced is connected to the primary winding of each antenna coil. Unbalanced input is for random length wire antennae. This input is capacitively-coupled through a .01uf capacitor to the RF amplifier coils. The Unbalanced input impedance is not specified but is probably fairly high assuming that end-fed wires were probably the design target Z. The Balanced input utilizes a "Twin-ax" two-pin coaxial connector and the Unbalanced input utilizes a "C-type" coaxial connector. As mentioned, no antenna trimmer is provided so the antenna impedance should be somewhat matched to the particular antenna input used.
Both audio outputs, Local Audio and Line Audio, are 600 Z ohm outputs
and can provide about 500mW on Local and about 10mW on Line. The phone
jack doesn't disconnect the audio output (LOCAL) from its respective load. There is a series resistor
and a load resistor to the PHONES jack to keep the audio level (5mW) from
over-driving the headset if the proper 600 Z phones are used.
|>>> The AC power connector is a four-pin military connector that is keyed
and held in place with a central screw that has a fold-down, wing-type handle.
There are at least two different types that fit,...sort of. The original
(CX-1358/U cable + connector PN) connector has a small round cylinder-shaped housing with
a cable exit tube on the side. This type will fit in almost any
orientation and can be used if the receiver is installed into a table
cabinet. There is also a large square housing with the triangular top
type that will only fit in one orientation that won't interfere with the
terminal strip or the fuse housing. With the larger connector installed
the receiver must have spacers to elevate the bottom enough for the
connector body (if the receiver is setting on a table) to clear the
table. Also, with this larger connector, the
receiver won't fit into the table cabinets.
Unlike most other LF and VLF receivers, the R-389 doesn't have any fixed-circuit audio restrictions within the audio module other than the switch-selected Broad-Medium-Narrow. Selecting Broad results in a fairly wide audio bandwidth. Medium is shaped for voice with noisy conditions and Narrow is a bandpass filter at 800hz for CW. The IF bandwidth can be restricted down to 100hz. Both 100hz and 1000hz IF bandwidths use a crystal filter that's onboard the IF module. The 2kc, 4kc and 8kc IF bandwidths are determined by the IF transformers and Q-resistor set-up. For static bursts and other types of atmospheric noise, the dual positive-negative noise limiter is available. When tuning in the AM BC range, the receiver's bandwidth can be increased to 8kc and BROAD and, with no other specific audio restrictions, the resulting audio isn't too bad. However, the audio is more-or-less communications-grade audio so don't expect high fidelity because it isn't. Most listening on LW will usually be using a headset. Most listening on the AM-BC band will be on loudspeaker.
The R-389 is a "top notch" MW, LF and VLF receiver but
using it today can result in user frustration due the very high noise
levels that plague LF enthusiasts in many locations. The R-389 does cope
with significant noise levels very well. It can do a good job with a
wire antenna (probably what it was designed for anyway) especially if
the user is located in a RFI-quiet area. Using a loop antenna may help
in extremely noisy areas. Of course, like any LW receiver, best results
will be experienced when listening "at night" during the "LW Season"
(Oct thru Jan.)
|The R-389 receiver is a marvelous combination of
electronic and mechanical complexity. Completely permeability-tuned with
a mechanical-digital readout. To say that it operates
differently from all of the other LW receivers profiled in this write-up
is an understatement. The tuning manipulation is very light and easy but
it can also take quite a lot of turns of the tuning knob to span just
100kc. The motor drive is handy if you find yourself at one end of the
tuning range and want to go to the other. Complete travel from one end
to the other takes less than 30 seconds.
The tuning reduction on average, at 300kc for example, is one turn of the Tuning knob changes the frequency by 2.5kc. With that amount reduction it's easy to listen carefully between signals as you're tuning the receiver.
The Problems and Repairs - The performance of this R-389 when first acquired was terrible - it barely worked! The mechanical sections, this is, the gearbox, the RF module line shafts and slug rack lifters were all victims of years of "slathering" grease on everything that rotated. As the grease aged it hardened and made mechanical operation more difficult. To compensate, the motor-drive clutch had been adjusted to "full engagement." This then had the manual tuning working against the motor drive through the clutch. The effort required to manually turn the tuning knob was extreme. Even the slip-clutch in the tuning knob was adjusted to "not slip" in order to operate the manual tuning at all.
Major disassembly and cleaning was required to remove all old grease from all gears, worm gears, threaded shafts and to remove old grease where it had been deposited after being "flung off" of the gears as they rotated. A real messy job but the transformation of the manual tuning into a very light and easy to manipulate mechanism was incredible. The motor-drive operation was greatly improved also with it now running very fast with no bogging-down because of excessive loads of grease. >>>
>>> The next problem was the modification of the power supply module to solid state diodes to replace the 26Z5 rectifier tubes. The modification removed the four 47 ohm 2W CC plate resistors. Apparently, this modification would blow the B+ fuse since the output of the rectifiers is routed directly thru the 3/8A fuse to the electronic voltage regulator. It seemed the electronic regulator presented an increased load to the "instant on" characteristics of solid state diodes and this would blow the fuse. To "modify the mod," the wires were removed from the fuse holder and soldered together thus eliminating the fuse at the input to the electronic voltage regulator. Instead, the CT of the power transformer was disconnected from chassis ground and wired to pin 15 of J115. The wiring of the CT was routed to the B+ fuse and then to a chassis connection nearby. The fuse was increased to 3/4A. I don't know whether this was a military field mod or just some hamster mod. It didn't seem to help receiver performance.
I rewired the power supply back to CT going directly to chassis. The B+ fuse was rewired to be inline with the input to the electronic voltage regulator and the fuse returned to 3/8A value. The diodes were removed from the power supply and the four 47 ohm 2W CC resistors were added to the power supply. Two good 26Z5 rectifiers were installed. This was the original configuration.
Another minor problem was with one of the coaxial cables from the Antenna Relay box. P110 had a deformed pin in the BNC male connector on the end of the cable. It was also noted the J110 also had a problem with the mating pin on the BNC receptacle. These pins were bent back to their normal shape to allow proper mating of the connection.
Both the Carrier Level meter and the Line Level meter were non-original types that were similar in appearance but internally were not correct movements. I obtained two original "R-390" (early style) Carrier Level and Line Level meters and these were installed into the R-389.
|Alignment - When
the R-389 was reassembled it was tested and seemed to function much better.
It had much more audio now. AM-BC signals were moving the Carrier
Level meter but not as much as expected. I knew the receiver had never
been aligned in at least the thirty years the former owner had it. I
suspected some parts of the receiver hadn't been touched since it was
retired from military service. A complete and thorough alignment was
going to be
The first check actually was performed before reassembly. That was the mechanical alignment of the slug racks in the RF module. This operation can only be performed with the RF module on the bench out of the receiver. The check requires that specific slug racks have to be at their maximum height at a specific measured distance at specific frequency readouts on the Veeder-Root counter. This check assures that the slug racks are traveling correctly as the receiver is tuned throughout its two ranges. The measured distances index lines are silk-screened on the rear panel of the RF module along with the specified frequencies.
Upon reassembly and power up, the receiver was then ready for electronic alignment after a 30 minute warm-up. The IF module is aligned first. This is six stages of IF amplification at 455kc. There is a Crystal Filter for the 100hz and 1000hz bandwidths that must also be adjusted. Also, the Amplified AGC has to be adjusted for maximum voltage at the AGC terminals.
Next, the First and Second Mixer transformers and the 10.455kc Crystal Oscillator output stage are aligned. An RF VTVM is required since the 10.455kc oscillator is used as the signal source.
The left-most slug racks are the VFO output stage, the Injection Mixer and the Output Coupler. These are aligned at opposite ends of the tuning ranges. This is a good test for the motor-drive tuning since the entire span of both ranges must be aligned. The remaining seven slug racks cover the seven tuning bands. These are aligned for 15kc-26kc, 26kc-55kc, 55kc-126kc, 126kc-250kc, 250kc-500kc, 500kc to 850kc and 850kc-1500kc. Each band has four RF transformers or 28 total with two adjustments each for 56 adjustments. The VFO has two coils and four adjustments and the Mixers have four coils and eight adjustments. The total number of adjustments is 68. >>>
>>> After the RF tracking is finished then the balance for the first Mixer has to be set using potentiometer R-260. This minimizes any Mixer noise. Overall IF gain and BFO adjustment finish up the alignment procedure. Although I took about four days to complete the alignment, total time for the alignment was probably around two hours or so.
|Performance - After
the alignment, local AM BC stations that before had pushed the Carrier
Level meter to about +20db now sent the meter up to +75db. That was
using the Unbalanced input. Where before, Balanced Antenna input didn't
respond at all, now the same local AM BC station showed +72db on the CL
meter. Using a 135' CF Inv Vee with 96' of ladder line with the feed
wires shorted as an antenna all of the usual NDBs were tuned in. The
testing was performed in late-April and conditions were poor (as
expected.) Still, NDBs from all over the Western USA and Canada were
received. Performance on the remotely tuned loop was not as well as
expected. I had modified the loop to work with the SP-600VLF receiver.
Perhaps I'll have to do some additional changes to the loop for best
performance with the R-389. Just as an additional test I connected the
HP 606B RF Signal Generator to the Balanced Antenna input of the R-389
using a coaxial cable. I tested the response at 200kc, 300kc and 700kc.
A 100mv RMS signal "pegged" the CL meter. A 10mv RMS signal showed about
90db. Reducing the signal down to 10uv RMS barely showed any reading on
the CL meter. At 1uv RMS the signal was easily audible on loudspeaker.
Although this isn't really how you measure sensitivity in a receiver, it
was a "quickie test" that showed the R-389 would respond to very weak
signals. A comparison test with the SP-600VLF using the same antenna and
test frequencies showed that both receiver's had nearly identical
performance characteristics and sensitivity.
More details and photos on "going thru" the R-389 (in the form of a Rework Log) are in the web-article "Rebuilding the R-390A Receivers," use navigation index at the bottom of this page.
|PERFORMANCE UPDATE: September 24, 2018
- Finally the Autumnal Equinox has arrived and conditions on LW,
especially in the early mornings are improving dramatically. All
summer-long, I'd perform tests on the R-389 trying various LW signals using combinations
of antennae from loops to wires. Barely any signals were audible. Once
in a while, the carrier of MOG 402kc in Montegue, California could be heard
but usually the MCW was not audible. At night, the static crashes and other atmospherics
seemed to mask all of the LW signals except for the DGPS nodes which
were about the only thing that assured me the R-389 was at least receiving
some types of LW signals.
With the Autumnal Equinox approaching, I began by listening in the early evening on 9/21/18, which was the day before the Equinox. Only two NDBs were heard, MOG and ULS (392kc, Ulysses, KS) and the noise was still pretty severe. I decided that in the next couple of days I would have to try early morning to see if the noise was down and maybe the signals would be up.
At 0530 on 9/24/18 I started listening using the 100'x135' "T" antenna. Right off, I tuned in ZZP 248kc from Queen Charlotte Islands, BC. Multiple NBDs were heard on many frequencies. I tuned around 390kc and heard what sounded like a voice transmission. I widened the bandwidth to 4kc (from 2kc) and at 394kc I easily copied voice weather being transmitted. With BFO turned off, I could hear in the background RWO being sent in MCW. This was the NDB on Kodiak Island that transmits TWEB or Voice Weather. In about 30 minutes of listening, I had tuned in about 30 NDBs, three of which were newly heard NDBs, ZZP 248kc, RWO 394kc and POY 344kc (#328, #329 and #330, respectively.)
I guess this illustrates that besides a quiet location, a large antenna and a superb receiver, good receiving conditions are absolutely necessary for successful LW DX copy and that my concerns about the R-389's abilities to cope with the modern LW reception issues were unfounded. As conditions continue to improve, I'm looking forward to the "peak LW reception" which will be from mid-November thru mid-January.
UPDATE: Oct. 1, 2018 - Tuned in LLD 353kc in Hawaii at 0545 this morning using 100'x135' "T" wire antenna. Also, tuned in JJY on 40kc, pulse-encoded time signal from Japan at 0615.
|The CY-979A/URR Cabinet
- This cabinet was included in a donation of old parts and parts sets.
The CY-979A was in very poor condition with a very severe bend in the
top where something very heavy had been setting for a very long time. At
one time, someone had thought about a repaint job and had sanded the
exterior. The shock mounts and skids were also in pretty sorry
condition. But,...that's why it was free.
The restoration consisted of first disassembling the shock mounts and skids to remove them from the cabinet. Then the cabinet was cleaned. I used some "body work" tricks (mainly wooden blocks and a 2 pound hammer) to straighten the cabinet. I did a little more sanding to even out the prep-work. The shock mounts were cleaned and measured for height. This is to make sure the cabinet sets straight. The shocks and skids were installed onto the cabinet before it was painted. I then painted the entire cabinet and shocks-skids with Rustoleum "Machine Gray" paint as this seemed to be the closest match from "off-the-shelf" paint. I knew I wanted to save the CY-979A for use with a R-389 if I ever located one. So, the cabinet was just going to be setting around for quite a while which gave the "shelf-type" paint plenty of time to harden.
When painting I had masked the cabinet contractor ID that on this particular example was silk-screened on the inside bottom. Taffet Electronics was the contactor and the cabinet was built in the early-sixties.
Hammarlund Manufacturing Company, Inc.
SN: 20101 from 1955
|When the first paragraph of the SP-600VLF-31
manual states that the receiver is unique because the tuning "extends to
audio frequency 10kc" one wonders whether the writer of the manual
understood the difference between 10kc of varying air pressure (sound-audio) and 10kc of radio frequency oscillation (a varying electromagnetic
field.) Of course, the writer may have just been thinking of an RMS
voltage varying at 10kc. The SP-600VLF is not just an HF SP-600
with LF coils in the turret. It's a very different receiver that was
designed specifically for longwave reception. The SP-600VLF-31 was first offered in 1954. It
was the first VLF version of the SP-600 series with a later SP-600VLF-38
for 25 to 60~ AC operation being the only other version produced. The
receiver shown here is from 1955 (ink-stamped June 27, 1955 on backside
of the front panel.)
Hammarlund also produced several SP-600VLF receivers for the Dero
Company and these receviers will have the Dero name on the front panel.
The 1950s was a time when the radio frequency spectrum below 500kc was brimming with signals that included many voice transmissions and lots of true CW transmissions. Signals that could be tuned included airport beacons (many with voice weather reports,) maritime weather and navigation signals, ship to ship traffic, ship to shore traffic, long wave AM broadcasting from foreign lands to name just a few. Nothing like today's almost entirely data-driven transmissions that defy decoding, unidentifiable signals of all varieties and the rapidly diminishing and displaced airport beacons (Non-Direction Beacons or NDBs.) In the 1950s, the SP-600VLF would have been used in the laboratory, in commercial coastal stations or perhaps onboard ship. It was an expensive receiver that probably wouldn't have interested the average radio amateur or average radio listener. It was mainly for laboratory, commercial or military users.
|Comparison to the HF SP-600s - One notices the although the receiver is obviously a "600" it has several minor physical differences. One first sees that the chassis and most of the sheet metal is gold iridite finish. Also apparent are the quite different side panels used on the VLF (similar to R-390A panels.) Another difference is the "X" option that on the HF 600 has six positions and uses HC-6 crystals but on the VLF has only four positions and uses FT-243 crystals. The Carrier Level meter is also only a single scale, bakelite case unit reading "db over 50uV" while the HF 600 meter is usually a metal-cased, dual scale unit. With the dual scale meter, a switch for RF-AF is on the HF 600 that is not necessary on the VLF. A "warning" tag is mounted between the tuning dial and the logging dial There are two additional IF cans that are smaller than the standard IF cans that are for the AVC and for the IF output. The "X" option oscillator uses a different tube. Antenna input is not on the RF platform but is terminals on a rear bracket.||
photo above: Note that most of the coupling and decoupling capacitors are ceramic disks on this 1955-built SP-600VLF.
|VLF Circuit - The SP-600VLF is not just an HF SP-600 with LF coils in the turret. It's a very different receiver. First, it's not a double conversion receiver (like the HF version) but it is double preselection in that two RF amplifiers are used on all bands. The frequency coverage is from 540kc down to 10kc in six bands. 21 tubes are used in the circuit (20 tubes are used in the HF version.) The IF is 705kc and a dual crystal filter is used for selectivity. One crystal filter is ahead of the first IF amplifier and the other crystal filter is ahead of the second IF amplifier. Five different IF bandwidths are available and all positions utilize the crystal filter (the HF version uses three of the six positions for the crystal filter.) There is a 1160kc crystal oscillator circuit in the receiver but this is to heterodyne with the 705kc IF to provide a fixed 455kc IF OUTPUT to drive RTTY devices or other types of equipment that require a 455kc input signal derived from the last IF amplifier stage (full selectivity.) The audio output uses a 600Z ohm transformer that's very similar to the HF version. AVC is provided as is a BFO and there is a Noise Limiter circuit. As expected for the vintage, the 600VLF uses a standard envelope detector circuit so the RF Gain has to be reduced for proper signal to BFO injection ratio (also the AVC should be off.) The "X" function provides for only four crystal channels using FT-243 type crystals. This "X" function provides a crystal controlled oscillator in place of the LO for increased stability. With two RF amplifers and four IF amplifiers provided the SP-600VLF has a lot of sensitivity and a lot of gain - but does that really help in today's noisy LF region of the spectrum?|
- Noise versus gain - that's the problem. Certainly the number of times
that the SP-600VLF receiver will be tuned to a voice modulated carrier
signal, with AVC on and the BFO off,
will be very limited. AM BC at 540kc and public information BC at 530kc
will be about the only AM voice signals easily received. The only other
voice modulated carrier signals will be from LW BC stations. Of the LW
BC stations that can be heard in the western USA only Radio Rossii was
an easy station to receive. Other LW BC were extremely weak so the
tuning is done with the BFO on and tune to zero beat. This is called an
"exalted carrier" type of reception of AM and it sometimes helps with
weak signals. Unfortunately, all I could ever hear was the carrier and
the modulation wasn't detectable.
It's worth noting that, in 2014, I haven't been able to reliably receive Radio Rossii 279kc from Sakhalin Island due to a digital-data beacon also on 279kc. In late November 2013 I was able to hear Radio Rossii somewhat using the 6' loop antenna but the beacon severely limits intelligibility. Radio Rossii was the only LWBC station that could be received in the west and it now appears to have a case of "chronic QRM." (Radio Rossii LW BC shutdown Jan. 9, 2014)
Although NDBs are MCW signals, all "NDB-chasers" use a BFO (tuned to the exact IF) to help locate the NDB carrier and then tune to zero beat to copy the MCW (this method results in a nice sounding 400~ note.) Best results for NDBs has the AVC off, BFO on and riding the RF Gain control.
Nearly all operation of the SP-600VLF will be with the RF gain throttled back to 5 or 6, Audio gain at about 5 to 7, with the AVC turned off and the BFO on (I've started having the AVC on in an effort to help reduce "pops and crashes" - it helps a little bit is all.) I've found that Selectivity at 1.3kc gives the best signal to noise ratio. The Crystal Filter should be set for narrowest bandwidth (about 8 or 9 on the dial scale.) With high noise it's sometimes better to reduce the Selectivity to the narrowest bandwidth while keeping the Crystal Filter at about 8 or 9. A 600Z ohm headset connected to the 600 Z ohm audio output (not the phone jack) gives the best results for weak signal detection. The Noise Limiter and AVC circuits are not very effective on static bursts or electrical "pops" so keeping the 'phones in front of the ears is necessary during these types of conditions. I'm using a six foot remotely tuned loop antenna. Nearly all of the NDBs tuned in seem to have two or three signals on each frequency. Stations below about 100kc will probably require an outdoor wire antenna for best reception. Stations like JJY (40kc) or WWVB (60kc) can be received with the AVC on and with the BFO off which lets the Carrier Level meter function. In this set-up you can watch the meter respond to the pulse-encoded signal that either station sends out. USN Submarine Fleet comm stations NAA, HOLT, NPM and NLK are very strong MSK Navy VLF stations in the 19kc to 25kc region of the spectrum. MSK stations will require the BFO to be on. No information can be decoded from these stations and their usefulness to LW enthusiasts is that their exact frequency is known along with their location so they provide excellent test signals for the VLF region of the spectrum.
My first serious listening session was using my 80M Inverted Vee antenna with the feed line shorted. I logged two newly-heard NDB stations. Not that they were any great DX, being PND 356kc in Portland, OR and BF 362kc in Seattle, WA, but they were new ones (#259 and #260, respectively.) Super smooth tuning with oversize controls only adds to the pleasure of using the SP-600VLF.
Chronic Dial Slippage - All SP-600 receivers mechanically drive the tuning using the same set up. A brass drive wheel is rotated with the Tuning knob. This wheel in turn drives, by friction, a brass reduction wheel that is spring-loaded against the drive wheel. The reduction wheel is grooved and mates with the Logging dial driving it, by friction, at its perimeter. If contaminates are allowed to accumulate on the friction drive surfaces eventually dial slippage will be the result. Although some SP-600 enthusiasts believe that the "S" spring used for loading the reduction wheel causes the slipping, I've seldom had just the spring be responsible for dial slippage. Almost always, dirt and grease will have collected on the friction surfaces of the brass wheels or on the rim of the Logging dial and this is what is causing the slippage. Thorough cleaning is necessary to correct the problem. Fortunately, all parts are accessible without any disassembly. The brass wheels and be accessed with the receiver on its side and the Logging dial rim can be accessed from the top. Clean all friction surfaces with denatured alcohol. I use several Q-tips to clean the brass wheel surfaces. Repeat the cleaning until the Q-tips don't turn black. On the rim of the Logging dial, I use a small piece of paper towel that is dampened with denatured alcohol. Again, clean until the towels don't turn black. Remove and check the "S" spring. It should be straight or slightly bent out. If it's bent inwards then the spring load will be somewhat reduced. You can expand the "S" spring by just bending it outwards with your fingers. Reinstall the "S" spring. As an added help, lubricate all of the bearings with a drop of 10W machine oil. Also, check that the Dial Lock is completely open and not "dragging" on the Logging dial. Check the SP-600 tuning now. It should not slip and should be "velvet smooth."
I had the SP-600VLF for three years before I finally performed this procedure. Last year the dial slippage was really getting bad. So this year, before the LW season gets going, I decided to fix some of the minor problems with the receiver, like the dial slippage. I guess I didn't check the tubes very well, I found V12 was a 6AU6 instead of a 6BA6. That got the AVC working better. Thorough cleaning and complete (and hopefully accurate) tube testing and location check. October 2017
Nov. 22, 2017 - Well, it's
only been about a month and the tuning dial is again slipping. It's a
receiver out of the cabinet job to check the problem to see what's
happened. Will update.
UPDATE: Jan. 1, 2018 - The slipping dial is back. Although I haven't pulled the receiver out of the cabinet I can see what I think is the problem. The logging dial rim has a small gouge that I think is causing the slippage since this "dent or gouge" changes the dial friction in the drive wheel groove when the gouge comes around. I also noticed that the logging dial has a significant bend so it isn't really engaging into the drive wheel groove with the same "fit" each revolution of the drive wheel. To repair this will be a receiver out of the cabinet and front panel off since I'll have to dismount the logging dial for straightening and repair of the gouge. I'll do this after the Longwave season is over - probably around March.
UPDATE: May 1, 2018 - Slipping dial issue required pulling the receiver out of the cabinet and then disassembling to the point where the front panel could be removed. The dial lamp assembly over the logging dial has to be removed. Then the three screw mounting plate is removed and the logging dial can be removed. Close inspection revealed that near "45" on the dial rim there was a deformation that had a "lumpy" feel to it. Also, between "50" and "55" was another rough area. I carefully dressed these areas with a fine file. The dial also had a warp that was easy to take out with minor flexing of the dial. Upon reinstalling the dial on the hub, I found that the slipping was still happening in the same areas. I readjusted the "S" spring for a greater load against the drive wheel. No improvement. I thought about how improve the "grip" of the brass against brass surfaces and came up with using rosin. I dissolved some powdered rosin in some denatured alcohol to make a thin (viscosity like water) mixture. I used a small paint brush to apply the rosin mixture into the drive wheel groove. Then I rotated the logging dial to transfer some of the rosin mix to the rim of the dial. I let the mix dry (alcohol evaporates.) That did it. No more slipping - at all! I didn't need much rosin-mix, just a little brushed just into the drive wheel groove worked great. If the rosin somehow disappears from the drive wheel groove in the future, it's very easy to reapply the rosin-mix. Hopefully, the "grip" will last for quite awhile.
Also, during this rework that required removing the front panel, I noticed that the gray rubber boots over the toggle switches had deteriorated to the point where two of them ripped and came apart. Fortunately these rubber boots are still being made by the same manufacturer and using the same part number. I ordered a new set of four gray boots from Grainger via their eBay listings. The price was $4.50 per boot. The boots are for 15/32"-32 toggle switches and are manufactured by APM HEXSEAL (part number is IN1030.) I know these aren't original,...neither are the grab handles nor the fillister-head slotted screws used in each corner for the panel mounting,...but I think that these additions improve the front panel appearance and aren't serious deviations from originality.
photo above: The carrier level meter is unique to the SP-600VLF
photo above: Only four crystal positions are offered in the X option
photo above: Tag between the tuning and logging dials
||Conclusions - Medium Wave
Amateur Operation - NDBs are going "off
the air" in droves. LW BC stations are almost totally gone. Loran-C is "long-gone." The spectrum below 500kc
is rapidly becoming exclusively data transmissions that require special
equipment or computer programs to decode. Nowadays, the SP-600VLF might
have become a high-quality receiver that could be used to hear just a few
interesting signals. Fortunately, now there are some MW and LF amateur bands
that can present a real challenge for the SP-600VLF.
Amateur operation on 472kc to 479kc (630M band) requires UTC approval for ham operations. Regulations allow CW and data with 5 watts EIRP. As of March 2018, I've been successfully using the SP-600VLF as the receiver in my 630M station. I'm using a six-foot remotely tuned loop antenna for reception. The station is described in detail with photo in the section "Operating Vintage Gear on 630 Meters" further down this webpage.
The SP-600VLF is a "top notch" LW receiver but using it today can be frustrating in some locations due to the very high noise levels that plague many LF enthusiasts. Special antennas are necessary for practically any receiver that tunes below 500kc and the SP-600VLF is no exception. The user's ability to hear LF signals will benefit greatly by employing a noise-reducing antenna system which generally means using a tuned loop of some kind.
Using the Remote Tuned Loop Antenna
- I decided to try the six foot remote-tuned loop antenna with the SP-600VLF-31
receiver. The loop suffered a bit during the move down here to Dayton. I
had it stored in one the shop garages. I brought the loop out for
inspection and found that the wire had come out of the grooves in the
combs in several places and there was wire hanging and getting tangled.
All that was needed was to straighten out the wire and get it back into
the grooves of the combs to get everything looking okay again. During
the move I discarded the loop's stand because it was beginning to fall
apart. So now I'm without a stand for the antenna but it can set on one
of its corners and be propped up against the wall - at least for
testing. A new 9vdc battery was installed to get the bias and remote
tuning working again.
With the tuned loop upstairs and propped up so it was pointing sort of north-south, I tuned in FCH 342kc and peaked the signal using the remote tuner. What I noticed was the gain peak was not as pronounced as it seemed to be with other receivers. Still, there was a peak, so I figured the loop was working. I waited until dark and then positioned the loop east-west. In tuning from around 325kc up to 400kc several NDBs from the US mid-west were received and several Canadian NDBs from Manitoba and Ontario were also received. The improvement over the "ham antenna" with the feed line shorted was dramatic. The only thing noticed was the "peak tuning" of the loop is very broad and not all that much gain change is noticed. I suspect that there may be an impedance mismatch between the loop and the SP-600VLF-31 that will require a little more tweaking. But, for now, I have a nice improvement in signals and some directivity. - November 15, 2014 Removing one turn on the pick-up loop, which had three turns and is now two turns, has improved the loop performance with the 600VLF. Sharper tuning (higher Q) and seems to have better gain. - November 17, 2014
UPDATE: For December 17, 2014 - I've been using the SP-600VLF-31 for about a month now (with the loop) and have logged over 100 NDBs, ten of which are newly heard NDBs. The greatest DX is the not-unexpected DDP in San Juan, Puerto Rico - over 3000 miles away, although DDP is not too difficult to hear since it's a 2KW transatlantic beacon. Performance of the SP-600VLF is exceptional and using only 600 Z ohm 'phones for the audio output and running the bandwidth selectivity at 1.3kc or narrower (and with manipulation of the crystal filter phasing) the ability to copy two or three different NBDs on the same frequency is impressive. The six foot loop has certainly made the difference in the ability to copy very weak signals.
NOTE: As of JAN 31, 2015 - 23 "newly heard" NDBs with the SP-600VLF so far with well-over 200 NDBs logged. Also, the Hawaiian LLD 353kc has been copied more than once - a distance of over 2500miles. The recommended "arrow" placement (position 5) of the Crystal Filter isn't particularly good for NBDs. I find that around position 8 gives better noise reduction and allows weaker signal copy. Once in a while, adjusting to 2 or 3 will increase the bandwidth and the "highs" and sometimes this helps with multiple signals on the same frequency. Feb 4, 2015 - Newly heard NDB is another Hawaiian NDB, POA 332kc copied at 0550PST.
UPDATE: October 2, 2017 - Out of curiosity, I decided to connect the SP-600VLF to my 135' CF Inv-Vee with the feedline shorted and see what was on the frequencies below 200kc (the lowest that the loop will tune is 200kc.) Lots of various types of beacons and data signals of unknown origin everywhere. I think some of these are harmonics from various power line data or other switching or data sources that don't care what they are radiating. At 51kc there was a strong MSK station, probably USN. At 60kc was WWVB with its pulse-encoded signal. Jim Creek NLK USN MSK was very strong at 24.8kc followed by NAA in Cuttler, ME at 24.0kc and two other MSK stations, 21.4kc NPM in Hawaii and 19.8kc Holt in Australia. All of these USN stations were strong but NLK was very strong. Below 17kc there isn't much. A few signals that are unidentifiable. 12kc had some type of signal there (Russian?). Nothing was heard between 132kc to 136kc (a supposed ham band.) Nothing was heard between 160kc and 190kc (the Lowfer band.) Nothing was heard between 472kc and 479kc (supposed 630M ham band.) This was at 4PM local so JJY at 40kc wasn't received. Checked a few days later at 06:15PDT and heard JJY on 40kc with their CW ID. Also heard POA 332kc. Also checked 630M supposed ham band and heard nothing except DGPS signals (or harmonics of them.)
Regenerative TRF Receivers versus Superheterodynes on Longwave
In the early days of wireless communications, all transmissions were on longwave. After the signing of the Alexander Bill in 1912 moved the amateur
operation to 200 meters or below, experimentation into the shorter wavelengths
began. Ships and navigation remained in the longwave region, (even today most
navigation and submarine communications remain in the LW spectrum.) After
WWI, most receivers used were regenerative detectors with two-stage audio
amplifiers. Later, TRF stages were added ahead of the detector to further
improve weak signal reception. As designs
progressed, the superheterodyne did not immediately replace the TRF regenerative receivers on LW. At first, superheterodyne designs used rather low intermediate
frequencies that limited coverage of certain segments of the LF bands. The USN
RAA LW superhet receiver from the early 1930s used four different IF
stage frequencies to optimize performance and provide complete tuned
frequency coverage (10kc to 1000kc.) For full LW (typically 15kc to 600kc) coverage, the regenerative receiver had no such limitations. Later
designs moved the intermediate frequency above the LW bands to give complete
Regenerative receivers have some advantages over the typical superhet receiver on LW. For example, receiver internal noise - regen sets are quiet and don't add much noise to an already noisy part of the spectrum. The frequency conversion required in the superheterodyne can create substantial internal noise in the receiver that limits its weak signal ability on longwave. Also, since a minimal number of tubes are used in regen sets, thermal noise is at a low when compared to a large tube-count superhet. The regen set's ability to be set-up as an Autodyne Detector, that is to produce an oscillating condition without a BFO, is also an advantage. With a superhet it is necessary to use the BFO to set-up a condition where the carrier can be heard however the BFO in a superheterodyne can sometimes mask weak signals. Though most BFOs are very lightly coupled in early superhet receivers to prevent "masking" this is not always the case in modern receivers. Additionally, when the regenerative set is oscillating, it is doing so at the tuned frequency while a superhet, using a BFO, is actually providing an audible heterodyne by injecting an oscillator signal at the detector that is somewhere near the intermediate frequency. It is the level of the injection that is important to weak signal copy. >>>
|>>> Lack of Automatic Volume Control (AVC) in the regen sets is also an
advantage as a high noise level can capture the AVC and decrease sensitivity.
Normally, with vintage superhet receivers, most CW listening is done with the AVC off
for that very reason. Most superhet communications receivers will provide switchable AVC. However,
some modern receivers, especially SWL portable types, do not have a switchable
AVC provision leaving the listener at the mercy of atmospheric noise. Selectivity can
be be achieved by use of audio filters in later sets or by advancing the
regeneration control to the point where oscillation just begins in earlier
receivers. Many early receivers also provide a coupling control for
selectivity (and for setting "critical coupling" for optimizing the ratio of
signal to regeneration at the detector.) By using the ear and listening for a particular tone frequency our
own brain can be a very effective filter although this does require some
practice to become proficient at. Another habit that old radio ops had was to copy
using earphones. This will allow hearing weak signals that are at the
"noise level" - of course static bursts can be almost painful at times when
using early sets without limiters. Most WWII USN LW receivers will have audio
output limiters that function very well at keeping static bursts at a
manageable level. More common (and modern) "clipping" noise limiters
don't seem to work as well as Output Limiters and will allow "pops" and
static bursts through. This is because the clipping noise limiter works
on repeating pulse patterns - like auto ignition noise - rather than
acting on a single, quick, intense pulse. An easy method to preserve
your hearing is to keep the 'phones slightly in front of the
ears. Notice in vintage photos of USN radio ops that the phones are always in front of
the ops ears. This method has been used by experienced CW ops since the
wireless days (when static bursts were just about the only loud signals.)
Mentioned above, the RCA-built USN RAA longwave superheterodyne receiver was a gigantic, 465 pound receiver that used 14 tubes and had four different IFs that were individually selected by the bandswitch(s.) Four specifically tuned BFOs were also needed in the RAA. The four different IFs allowed for uninterrupted coverage from 10kc to 1000kc. The complexity and expense of the RAA forced the Navy to reconsider earlier, less complicated and less expensive longwave receivers. After the RAA, all Navy longwave receivers were either TRF with regenerative detector or TRF with tracking BFO. Of the latter catagory is the RBA series built for the Navy during WWII. These receivers use three cascade TRF amplifiers feeding a non-regenerative triode detector followed by three audio amplifiers - in essence, the typical TRF receiver of the late twenties. However, that's where the similarity ends. The RBA also uses a "tracking" BFO that tunes via an additional ganged section of the five-gang tuning condenser. This allowed the BFO to always be 1kc above the tuned frequency and provide the heterodyne necessary to demodulate CW. Also, the RBA featured a "tracking" auxiliary gain control that was gear-driven from the tuning mechanism and kept the gain level constant throughout the tuning range. The RBA was used by the Navy for about two decades after WWII ended and its superior performance illustrates what can be accomplished in TRF design when cost was not an issue - the RBAs sold to the Navy for $3000 a piece in the 1940s.
Now, all of the above isn't saying that a vintage superheterodyne can't do a good job on LW reception. When specifically designed for LW, with low noise tubes and circuits, a superhet can perform quite well on LW when used with the proper antenna. However, many superhets just added a portion of a LW band to a receiver that was really designed for HF. These types of superhets are common and their LW performance is usually rather poor. There are exceptions with the National HROs (using G, H and J coil sets,) the Hammarlund SP-200LX (aka BC-779) and the RCA AR-88LF (aka CR-91) being noteworthy as high performance superhets that do a fine job on their limited coverage LW bands.
Also, there are two well-known, vintage, ultra high-end, designed specifically for LW, receivers that were made for the military and for the laboratory. The Hammarlund SP-600VLF is a top performer with continuous coverage from 10kc up to 540kc and the familiar "SP-600" appearance. However, it isn't just an SP-600 with LW coils installed in the turret but rather it's a completely "designed for LW" receiver that uses the basic SP-600 physical appearance and mechanical features. Unfortunately, the "VLF" is a rather rare and usually expensive version of the SP-600 and, while the SP-600VLF is an exceptional performer, it does require a low-noise antenna and, for LW DX reception, it's really helps to have a low-noise location. The other "high-end" LW receiver is the Collins R-389 LW receiver but it's so rare (856 built) and so expensive that it has become better known as an ultimate "Collins Collector's receiver" than known for its incredible LW performance. The R-389 is a mechanically and electronically complex, double conversion receiver that mixes the incoming RF LF frequency with a VFO plus crystal oscillator to convert the frequency to an IF of 10mc which is then mixed with the same crystal oscillator to achieve the 455kc IF. This signal is then routed thru six IF stages using the same type of IF module used in the R-390 receiver. The remaining circuits and modules are the same as the R-390 receiver. The R-389 is another exceptional receiver but many times, its performance is reported as "adequate but not phenomenal." It's likely that many of the R-389 receivers in collections would benefit from a complete servicing. These complex receivers generally don't attain their high-performance capability unless they are maintained and aligned by competent techs. As with any LF receiver, a low-noise location is necessary for LW DX reception.
Many casual LW listeners aren't aware that all of the "top performing" LW receivers must be operated with a low-noise loop antenna, even in a RFI-quiet location, to achieve DX reception on LW. In reality, most "high-end" LW receivers have about the same abilities and superior performance is more dependent on the operator's experience, the antenna type used and the receiving location rather than on the type of receiver being used. If the LW superhet user runs his receiver with a tuned loop antenna (especially a shielded, magnetic loop in urban noisy areas,) he will find the signal to noise ratio is greatly improved and, in a quiet location, he should be able to receive ample LW DX.
Selective Level Meters and Wave Analyzers as Longwave Receivers
Selective Level Meters and Wave Analyzers are test instruments that incorporate a tunable sensitive receiver with selectable filters and attenuators to drive a calibrated analog meter. These instruments are used for a variety of purposes such as measuring leakage or unwanted signal levels on transmission lines, testing response of various kinds of amplifiers, some types even provide a built-in signal generator for test signals. None of these type of instruments are designed specifically as Longwave receivers, however, some of them actually perform quite well in that function. I have used two Selective Level Meters as LW receivers, a Sierra Model 125B and a model made by Cushman. The Sierra 125B was a vacuum tube model and was fully operational with a good set of tubes and I had performed a full alignment. However, that particular model did not have a BFO to help locate weak NDBs. This made the Sierra 125B very limited in its usefulness as a LW receiver. I also had loan of another selective level meter made by Cushman. This was a solid-state model that did have an on-board BFO with USB and LSB capabilities. It didn't matter, I couldn't pick up any signals using it. The set's owner was also disappointed with the Cushman's performance as a LW receiver and he eventually sold it on eBay. By far, the best instruments for use as longwave receivers are some of the Hewlett-Packard Wave Analyzers.
I happen to have the HP 310-A version in which the receiver tunes from 1kc up to 1500kc. The 310-A also has selectable USB or LSB and AM detection along with 200Hz, 1000Hz and 3000Hz selectable bandwidths. Lowest scale sensitivity is 10uv FS meter reading (maximum signal level) although using this sensitivity depends on how much atmospheric noise is present. With a tuned loop antenna, 10uv FS meter can almost always be used. During high noise periods with a wire antenna, 30uv FS provides better noise immunity. In the "Relative" measurement position the sensitivity is adjustable for best response versus noise. The HP 310-A is a late sixties to early seventies vintage instrument with a mechanical counter providing the digital frequency readout.
|photo left: The
Hewlett-Packard 310-A Wave Analyzer. The mechanical digital readout is
for receiver frequency while the long horizontal scale illuminates a red
numeral depending on the sensitivity (max. signal) selected. The tags
above the meter switch are USAF property identification tags.
photo right: The Sierra Model 125B Frequency Selective Voltmeter. The drum dial scale is at a "slant" because it is continuous tuning that has the scale spiral up as the drum is turned about four turns to go from 1kc up to 620kc. Lack of a BFO on the Sierra is a severe limitation for using it as a LW receiver
|I find that the performance of the HP 310-A is very favorably compared with any of the vintage longwave receivers profiled in this web-article. The 310-A doesn't have a noise limiter - mainly, because noise was one of the things the instrument was designed to measure. However, manipulation of the sensitivity versus the atmospheric noise seems to do pretty well for coping with the lack of a limiter. Since this is a measurement instrument, no AVC is provided, so strong signals will over-drive the 310-A, especially when using a tuned loop antenna. Watch the meter and keep the measured signal level at about 75% to 95% of FS with the Relative Gain control. I have received hundreds of NDBs from all over North America on my HP 310-A, from DDP 391kc in Puerto Rico to LLD 353kc in Hawaii. My conclusion is that Selective Level Meters and Wave Analyzers are designed for finding and measuring leakage in systems, measuring frequency response or measuring unwanted signals on transmission lines and other similar applications. Some of these instruments are useless as longwave receivers. Read up on any instrument you intend to purchase for longwave reception and make sure others have had success using it for that purpose. The first two instruments I tried were of the "useless" variety, however the HP 310-A performs very well as a longwave receiver.|
Other Vintage Receivers with Some Medium Wave and Low Frequency Coverage
All but one of the receivers profiled above were specifically designed for MW, LF and VLF coverage - generally 600kc down to 15kc. Many other receivers were offered in versions that covered a portion of either the MF or the LF spectrum. During the 1930s, many "All Wave" radios for the home tuned down to 150kc because there was so much to listen to then in that part of the spectrum. Also, a few models of communication receivers were offered with limited MW/LF coverage. Some of these versions were excellent performers while others were barely adequate. The following is a short list of some of the more common types of receivers. None of the receivers listed below cover the entire "longwave" spectrum of 600kc down to 15kc.
|National Co., Inc. - HRO -
using coil sets G - 420kc to 200kc,
H - 200kc to
100kc, J - 100kc to 50kc - Very good performer with long wire antenna or
loop. These coil sets were generally optional equipment but the military versions did
include a complete set of coils, including those for MF/LF coverage. Of these
military versions, the HRO-W and the RAS are
the most common. LF coil sets can be used in any of the HRO receivers
but alignment to the specific receiver is required for best performance.
Double preselection (two TRF amplifier stages) are used in all
coil sets for the HRO. IF is 456kc on almost all versions. Notice that
there is a gap in frequency coverage from 480kc to 420kc (coil set
F covers 920kc to 480kc.) This was
because of the HRO's IF of 456kc. The RAS used 175kc IF and that allowed
it to cover from 195kc up to 500kc without a gap in the frequency
coverage (the USN wanted complete coverage in the 400kc to 500kc range
which the standard HRO couldn't provide.) The RAS receiver must be used
with RAS coil sets identified as coil sets 1 through 7 on a metal tag on
the coil panel. Later HROs, like the HRO-50 and HRO-60, can also provide
excellent performance using the G,
J coil sets. The LW coil sets
for these later receivers are a bit more difficult to find and are
usually somewhat expensive because of that.
Hammarlund SP-200LX aka BC-779 - covers 400kc to 200kc and 200kc to 100kc - Excellent with loop antenna, a bit noisy with long wire antenna. Good dial accuracy. The BC-779 is probably the most popular of the military WWII versions of the SP-200 series. Some BC-779 receivers were built by Howard Radio Co. under contract. Band spread was not provided on the LF frequencies. SP-200LX is the designation used for any pre-WWII or non-military version of the "200 Series" receivers. IF is 465kc on all versions and double preselection is used on all bands. There was also a SP-100LX version that is an earlier version with the same frequency coverage but this version is rare.
RCA AR-88LF and CR-91/CR-91A - covers 550kc to 73kc (550kc to125kc on AR-88LF version) with SW coverage above 1.5mc - Excellent with long wire antenna or with a loop. Good dial accuracy. A heavy receiver weighing nearly 100 lbs in the cabinet. All steel construction is why. Stability was what RCA was trying to achieve and these receivers have virtually no drift. The AR-88LF versions were generally sent overseas during WWII and are somewhat difficult to find in the USA. The CR-91 is the USA-built replacement for the AR-88LF but it's very rare. Most CR-91s are actually the post-war CR-91A receivers that were built in Canada (RCA-Montreal.) IF is 735kc on all LF versions and double preselection is used on all bands.
|The Ultimate Vintage Long Wave
Receiver? - If you're looking to find the ultimate
receiver,...the one that's the most sensitive,...the one that can pick
up weak DX signals through any sort of noise,...the one that doesn't require
special antennas,...well,...unfortunately that receiver doesn't exist. There are
very good performers and there are
"not so good" performers
but there really isn't one receiver that "stands out" above the rest as the
ultimate LW receiver.
I've tested and used dozens of different kinds of vintage LW receivers and
in my opinion the "best" of the LW receivers all
perform at about the same level. While all of the receivers profiled above
can perform quite well on LW, there are a few that standout as my "favorites" to use. My first choice
would be the Hammarlund SP-600VLF-31 receiver. An extremely close "second" is
the US Navy RBA receiver. My third pick would be the Collins R-389. These three receivers are about the best of the
receivers because all three can detect very weak signals that are "in
the noise." All three have direct frequency readout with
illuminated dials, the RBA receivers have excellent Output Limiters that
are very effective noise limiters and
all three have excellent mechanical
construction. However, even these three top vintage LW receivers can't
perform well within certain environments or when LW receiving conditions
Regardless of the LW receiver used, for effective LW reception you absolutely need the following: First, a good receiving location that has very low RFI-noise levels (Radio Frequency Interference, e.g., manmade RF noise.) High RFI-noise areas will limit what even the best receiver can pick-up and separate from the interference. Second, a good low-noise antenna. An antenna that "picks up" a lot of RFI-noise will only compound a noisy location problem, making even the best LW receiver a poor performer. Even in RFI-quiet areas, using a low-noise antenna will benefit your reception. When you have a superb receiver operating in a quite receiving location with a good low-noise antenna then you absolutely must to use headphones for the audio output. Don't use the 'phones jack as the audio source. You must operate the 'phone directly from the 600Z ohm audio output of the receiver. You'll never hear the extremely weak signals using a loudspeaker. 'Phones are a must. Finally, you must do your LW listening during "the LW season." This would be late-Fall and Winter nights and early mornings (the "LW season" is usually between the Autumnal Equinox and the Vernal Equinox ). The following sub-articles detail some of these MW/LF reception problems and some of the solutions to noise and what types of antennas are best for successful LW reception.
What to Listen to using Vintage Long Wave Receivers
LW Propagation - The time of the year and hour of the day are important to successful DXing on LW. Although in theory LF and VLF propagation is generally considered to be mainly ground wave, most NDBs are actually in the medium wave band (MW) which is 300 kHz up to 3000 kHz. MW does have both ground wave and substantial sky wave propagation characteristics. About the only NDB DX reception is going to happen at night and up to just before local sunrise. Below 100 kHz, ground wave makes up the majority of the signal propagation, however losses due to absorption are highest during the daytime so best signals are usually a nighttime occurrence. Sometimes sky wave will still happen in the LF part of the spectrum and this also adds to nighttime's advantage for better reception. Although you can receive the Navy MSK VLF stations (19kc to 25kc) day or night, weaker LF stations, like JJY at 40 kHz, can only be received just before local sunrise and still nighttime west across the Pacific to Japan.
Due to the sun's position, its affect on the ionosphere and the intense noise generated by the sun's activity, winter nights are always best for reception on LF and MW (in the Northern Hemisphere.) Summer is plagued with countless thunderstorms that add intense noise to the LW spectrum - day and night. Usually by mid-September, the LW signals are getting better and the summer noise is becoming less bothersome. By mid-May, the noise is again increasing to the point where only the strongest signals can be heard. Therefore the LW listening "season" is usually considered to be between the Autumnal equinox and the Vernal equinox. Also, low noise LW conditions generally occur during sunspot minimum during the 11 year sunspot cycle. Increased solar activity, usually favored for HF DX, increases the band noise on LW. VLF is not usually affected by much of anything which is why it is used for 24 hour, worldwide USN communications. The US Navy MSK stations located around the world are always easy to receive with equipment that can tune low enough - 19kc up to 25kc.
Some of the Signals (Past and Present) below 500KC
Tuning around below 500kc offers some interesting challenges and a different kind of DXing. Nearly all signals encountered are either CW, MCW, RTTY or some kind of data transmission. There are virtually no voice transmissions except for a handful of foreign longwave BC stations. Here are some of the types of signals found below 500kc.
NDBs - An enjoyable part of listening below 500kc is receiving the many different Non-directional Beacon (NDB) stations that are located at many airports around the world. Airport NDBs operate continuously, 24 hours a day, seven days a week. The transmissions are nearly always in MCW using a 400hz tone (1020hz was popular in the USA but isn't used anymore.) The NDB station will transmit its assigned call letters in International Morse every few seconds. The NDB ID usually is a three-letter combination that often bears some resemblance to the airport location, e.g., CHD in CHanDler, Arizona. US NDBs that use only two letters for an ID are usually "marker beacons" located at the beginning of a runway. Often, marker beacons are not listed on NAV-AID websites and therefore are sometimes difficult to identify. NDB transmitter power is generally around 25 watts in the USA, however there are some US regional NDBs that run up to 400 watts and a few coastal "transoceanic" and Alaskan NDBs that run 1KW to 2KW.
Canadian NDBs will follow their station call with a "key-down" signal until the call is sent again. This makes all Canadian NBDs easy to identify. Also, most Canadian NDBs run substantially more power than the typical 25W US NDB, so their NDBs usually put out strong signals. Sometimes Mexican NDBs will proceed the ID with a "long dash" - not "key down," just a long dash, (I have heard this on GRN several times but not on other Mexican NDBs.) NDBs can be found from 190kc up to 529kc. Many NDBs are being "covered up" by powerful DGPS* signals within the same part of the spectrum (generally signals from 285kc up to 325kc are predominately DGPS signals in the Western USA.) Since the NDB signals are MCW, a carrier is always present on the assigned frequency. With the receiver BFO on, it is easy to locate the NDB carrier and then ID the station when the call is sent. Nearly always, there are multiple NDBs assigned to the same frequency so listening for different characteristics of the transmitted signal becomes part of the method of identification. Also, due to changing propagation, different DX NDBs assigned to the same frequency, will be heard during different listening sessions.
Once the NBD call letters are known, they can be checked against one of the NAV-AID websites. By entering the station ID, the websites will provide the NDB airport location, assigned frequency and sometimes the transmitter power. The best information source is www.classaxe.com/dx/ndb/rna where you'll have to load either the call of the NDB or the frequency into the search parameters and then the page will jump to the listing. You can also scroll down the entire page of NDBs listed by frequency. There are also notes regarding certain characteristics for some NDBs as reported by listeners. Classaxe provides the most up to date information on NDBs. Another navaid source for USA, Canadian and worldwide NDBs is www.worldaerodata.com . World Aero Data has almost all NDBs listed but you will have to click on the "Airport Call" to find the actual location. A lot of specific airport information can be gathered from worldaerodata. These two websites provide the "double-check" that is necessary to confirm the NDB ID heard on a specific frequency is the actual station received since there are usually several NDBs with the same call letters but never are identical IDs transmitting on the same frequency. Eventually, a list will have to be maintained in order to know when "new" NDBs are received.
Knowing International Morse - NDBs seldom send faster than 10 words per minute, so it's not really much of a challenge to copy their call letters, especially since the NDB call sign is sent "over and over and over." When the signal is strong and there's no interference, copy is easy, even if your Morse ability is limited. Can you still receive and identify NDBs if you can't copy Morse at all? More than likely the answer will be yes, mainly because NDBs send so slow and the NDB call is sent "over and over." Since many private pilots were barely Morse proficient (if at all) the intention was that NDBs would send slow enough that the "dots and dashes" comprising the NDB call sign could be written down, e.g.," _.. _.. ._ _. ," and then "translated" into the letters (DDP) that identify the beacon. Being fluent in International Morse is a major advantage when trying to copy several NDBs operating on the same frequency. It's also helpful when the signal is so weak that it's practically at the same level as the noise and is fading into oblivion. I'm not saying that you have to be able to copy 20WPM in your head while having a conversation with someone else on the telephone but a good code receiving ability will ultimately help fill your NDB log.
*DGPS - Differential GPS,...see section below.
||Other Beacons - There other kinds of beacon signals that will be received on LW.
Sometimes these are buoys that provide some navigation or hazard information in
bays, lakes and other waterways. Most of the time it's next to impossible to find
out the location of these particular signals that are obviously beacons
of some kind. If the MCW ID is not listed in the NAV-AID sites, it does
not mean that the signal received is not a legitimate beacon. Even
legitimate airport NDBs sometimes aren't listed in any of the NAV-AIDs,
like some "marker beacons."
This can be an oversight or sometimes it's a new NDB (yes, there are new ones
starting up with some regularity, even today - LYQ in Manchester, TN, for instance, just started up in
2008.) If the NDB heard is not listed in the NAV-AIDs, then try a web
search on the NDB ID or try some of the web NDB logs to see if other
listeners have heard the same station. Sometimes, though not too often,
complete information on the NDB is found by this method. Part of the interest in LW listening is receiving weird and
strange signals that are a challenge to identify.
On the future of NDBs - Current US regulations state that if an NDB transmitter fails, the airport is not required to repair or replace their NDB station. Every month, more and more US NDBs are "retired" as obsolete technology since there are other more modern navigation signals available that are more accurate. However, many airports do select to maintain their NDBs as the operation costs are negligible and it provides a safety backup if the pilot has problems with his other air navigation equipment. It's up to the airport to decide if they want to continue to provide their NDB signal as part of a tradition of air navigation. Remote airports, especially in Alaska and in the USA along the Canadian border, seem to be more inclined to keep their NDBs in operation.
|DGPS Signals - DGPS,
or Differential GPS, uses a somewhat local transmitter signal that works
with satellite GPS to correct intended errors in the GPS satellite information.
When GPS was being developed there was a concern that an enemy could use
the GPS satellite information to accurately aim and deploy various types
of weapons. To prevent accurate information from being available
directly from the satellite, errors were built-in. These errors could
then be corrected using local transmitters sending "correction" signals.
This initially was for military uses but eventually also was to allow civilians to utilize the
GPS information. GPS evolved over the years but still the DGPS
correction transmitters are being used. There are 85 DGPS transmitters
in the USA (some of which were converted from the 85 GWEN* nodes by the
USCG.) Most are located along coastlines and some major waterways.
Canada also uses DGPS along its coasts and along the St. Lawrence
Seaway. There is a specific frequency band where the DGPS signals are
located, 183.5kc up to 325kc. It depends where in the USA you are
located just how much interference the DGPS signals impose upon
reception of NDBs. Here in the Western USA, most DGPS signals are
concentrated from 285kc up to 325kc. There are a few in the lower part
of the DGPS band but the strongest signals are centered around 300kc (in
the West.) As more and more demand for civilian GPS uses increase,
expect to encounter more DGPS signals.
NOTE: Although I hate to admit it, I have used the DGPS signal on 314kc as a receive "test signal" many times. That node is located near Sacramento, California and is extremely strong here in Western Nevada. Since I know it's on 314kc and very strong, it makes an ideal "test signal" for the middle of the "NDB Band." When FCH 344kc in Fresno, California shut down (Jan 2018) I no longer had any NDB signal strong enough for daytime copy. Our strong local NDB, NO 351kc in Reno, Nevada, had shut down in August 2013 (and it's really missed.) DGPS 314kc is very strong and does provide a handy "test signal" for daytime use.
*GWEN, or Ground Wave Emergency Network, was a LF military communications network that utilized of 85 transmitter nodes located within the USA. Each node consisted of a high power LF transmitter in the 170kc to 190kc part of the spectrum, a 200 ft tall tower/antenna and all of the support gear for providing emergency communications post-nuclear attack. Supposedly, LF was not vulnerable to damage from the EMP of nuclear detonations and could theoretically survive as an operational system. Military and presidential comms to SAC were intended but the system had many problems and, by 1994, had lost funding. The system was eventually shutdown. Many of the nodes were converted to DGPS use.
More Longwave Signals
Longwave Broadcasting - In addition to NDBs, there are foreign longwave broadcasting stations. These are only located in Europe, Africa or Asia. The stations run incredible power levels. One million watts of carrier power is common for longwave broadcast stations. Even though their power levels are extremely high, the signal's propagation faces severe losses and most longwave broadcasting is intended for regional service only. Here in the western part of the USA, it is possible to receive a couple of LW BC stations but those stations are never strong signals and rarely can the program be enjoyed. The strongest and most often received station here is Radio Rossii, located on Sakhalin Island (North of Japan) broadcasting on 279kc at a power level of one million watts. During the winter months in the early morning (~5AM PST,) Radio Rossii is very strong (for LW BC) and can be heard playing Russian pop-jazz music and reading their news service. These are always reports in Russian read by alternating male and female announcers with a short musical interlude between stories. Other LW BC stations are very weak and many times only the carrier can be received, the modulated information being too weak to really understand or even identify. UPDATE 2017: Radio Rossii on LW is gone for good. In fact, all Russian Long Wave broadcasting has stopped as of January 9, 2014. Only a few LW BC stations are active in Asia. Turkey has one and one in Georgia. Apparently these LW stations are too expensive to operate and maintain along with enduring a continuing loss of listeners that have gone to satellite or Internet services.
Longwave Broadcasting's Future - It doesn't look good - Most of Asia no longer broadcasts on LW. Europe has about four stations still operating. The BBC-4 LW station is still running a vacuum tube transmitter and claims when the last tube goes, they are permanently off the air. They claim to have "bought up" all of the spare tubes available in world a few years ago,...and, apparently these tubes can't be rebuilt (more likely the BCC doesn't want to spend the money to have the tubes rebuilt.) When the Irish LW BC station, RTE-Radio One, shutdown a few years ago there was an enormous protest from the Irish in Britain that eventually got RTE-Radio One to reverse their decision to shutdown. The arguments to shutdown all LW BC are based on technology in that higher fidelity programming is available on Medium Wave (AM BC) or FM BC or Satellite or even the Internet. However, ardent LW listeners say "so what?" They don't want to change their listening habits. Even if the LW BC technology has its limitations it doesn't matter since most listeners aren't using new receivers anyway. Many are still using their old vacuum tube radio purchased decades ago. Expensive operation and maintenance cost when power level is at one million watts and the transmitter is of vacuum tube design seems to be the ever present threat that shuts down the LW BC station. At the present, the only thing keeping LW BC alive is their devoted listeners and those include still many maritime listeners. However, the end is probably "in sight" for LW BC. None of the stations want to upgrade their equipment since the future of LW BC is so bleak. Also, in many cases, the real estate that the massive antenna systems inhabit is probably worth more to the governments than maintaining "an obsolete technology" that benefits few and costs them so much to operate.
"Lowfer" is a nickname for the LF enthusiasts that transmit 1 watt signals to 50 foot antennas in the 190kc to 160kc part of the LF spectrum. A license is not required to operate these transmitters because their effective radiated power (EIRP) is so low. The limitations have resulted in very clever ways of extracting very weak signals out of the noise in that particular region of the spectrum. QRSS, or very very slow CW, is one method used. It is so slow that a computer usually monitors the signal for several hours (all night) to assure that copy is possible. Other computer programs are also used to make possible copy of these extremely weak signals. Sometimes, when conditions are favorable, two-way "human" CW contacts do occur. Those are usually referred to as "Real Morse Communications" since so much on this particular band is computer driven and monitored for transmission and reception.
Amateur LF Operations - In other countries, 136kc is an amateur frequency that can be used for fairly high power transmissions. The limitations are not nearly as strict as in the "Lowfer" band. In the USA, 22 experimental licenses have been issued under the call WD2XSH/xx. These are licensed individuals that are carrying out experimental transmissions around 500kc (usually 508kc.) The limitations are 20 watts EIRP. About half of the 22 licensees have not gotten "on the air" but some signals can usually be found. In the West, WD2XSH/22 in Sweethome, Oregon is very strong and easy to copy. These signals are CW, not MCW. UPDATE: I haven't heard any amateur activity on 508kc for some time now. It seems that the spectrum around 500kc is now being used by commercial or military users. - 2017 UPDATE: Further down this page are more details on the 630 meter and 2200 meter ham bands along with more information on FCC Experimental License Grants - 2017
Time and Navigation Signals - WWVB (60kc) and JJY (40kc) are both pulse encoded time transmissions. JJY will identify their transmissions in CW at 15 and 45 minutes after each hour. WWVB provides no identification. Both WWVB and JJY can be received better if the BFO is on to demodulate what is basically a CW-type signal. There should be no problem with WWVB as its signal is extremely strong anywhere in the USA. JJY is a relatively strong signal in the Western USA in the early morning hours.
Loran C - All Loran C stations used to transmit on 100kc. The Loran C signal consisted of a precisely timed series of rapid pulses that both identified the station (as Master or Slave) and also allowed all Loran transmitters to be on 100kc simultaneously. The timing was critical and controlled by cesium-atomic clocks at each station. The shipboard navigation receivers were capable of identifying Master from Slave stations and designed to time the propagation delay based on "knowing" precisely when the pulses were sent and "timing" when they were received. Using the Master signal plus one or more Slave signals allowed the ship's navigation receiver to triangulate the wave fronts and determine their intersection point and the ship's position with an accuracy of around 50 feet, which in the ocean was pretty close. All Loran-C stations were shutdown in 2010 in what was mainly a political move that eliminated the last terrestrial-based, long-distance navigation system in favor of satellite-based GPS navigation.
Computer Programs - There are several computer programs available that will demodulate many of the data transmission-type LF signals and allow the user to "view" what kind of information is being transmitted. In some cases, weather maps and weather reports can be printed out from NAVTEX. SeaTTY is one such computer program. USN MSK signals can't be decoded without special equipment, data reassembly programs, encoding data and other sophisticated encryption/decryption information.
Amateur Operation on 630 Meters and 2200 Meters in the USA
As usual,...there seems to be a lot of opposition to having US amateurs transmit below 1800kc. Here it is late-2017 and still getting on the 630M band requires a lot of "red tape" here in the US. The 2200M band is even worse. The ultimate factor in the decision for each individual ham operator will be his physical location and that decision will be up to the Utilities Technology Commission. Only time will tell how many hams will be approved by the UTC for 630M operation. The following was written over the time period beginning with the announcement in 2012 up to the present. I guess it illustrates my frustration with the lethargic pace of the entire approval process.
GOOD NEWS! - 630 Meter Amateur Band Proposal - As of February 2012, there is a proposal to create a world-wide amateur band dubbed "630 Meters." Actually, the proposal is for 7kc between 472kc and 479kc. Initially 1 watt effective radiated power was proposed but there is some indication that maybe that will be raised to 5 watts EIRP - essentially the effective power radiated from the antenna. Since nearly all of the antennas that would be possible for most amateurs to construct would be short in relation to the wavelength, the efficiency of those antennas would be compromised. Therefore, even though the EIRP might be 5 watts, because of antenna inefficiency it might take 100 watts of RF input to achieve 5 watts of EIRP. There are other restrictions that mostly involve other countries where interference with NDBs might be a problem. Also, at the moment there doesn't appear to be any details about the modes of transmission that can be used. Likely, due to the nature of the wavelength, transmissions will be restricted to CW or data transmissions - similar to the 30 meter amateur band in the HF range. The whole proposal has to still go through several steps to become official so it looks like the earliest that amateurs might be able to use "630 Meters" will be early 2013. (I was optimistic at this time.)
Finally,...five years later,...well,...maybe,...but,... probably NOT! - As of July 2017,....472kc to 479kc is now supposedly an amateur band in the USA with only a few "strings attached." Most modes are allowed at 5 watts EIRP. BUT,...don't get your hopes up. Here's the "hold-up." Because certain utility companies run test and troubleshooting data on some types of power transmission lines at some unspecified times and certain officials believe that there might be a possibility (not substantiated by any test evidence) that this utility test transmission could be corrupted by amateur interference, the FCC has left the ultimate decision of whether an individual amateur can use the 630M band up to a political lobby concern called the Utilities Technology Commission (the UTC.) The UTC's primary interest is to promote business and commerce for the various Utilities. The UTC is not interested in amateur radio operation unless it could adversely affect the operations and profits of the utility concerns they represent. A further indication that neither the FCC nor the UTC have any real interest in amateur operation on 472kc (or 136kc) is that fact that there is currently no methodology in place for the individual amateur to apply for UTC approval of operation (that was as of June 2017.) Supposedly, the UTC and the FCC are "working" on this problem but it's obvious that neither entity has any interests in permitting any regular amateur radio operation in this part of the spectrum. Essentially, this has effectively stopped amateurs from operating on 472kc. (SOS.) On 2200 meters, the EIRP is 1 watt. At present, in the USA, operation on 2200 meters requires a special experimental license from the FCC unless you operate with the same restrictions that apply to Lowfers (so, 2200 meters isn't really an amateur band then, is it?)
So, what about those amateurs who want to operate on LF legally, right now, without all of the red tape and hassle? The only option is to become a Lowfer.
This above data was from ARRL and Wikipedia - June 2017.
PROGRESS - Maybe - UPDATE: Dec 30, 2017: Thanks to information provided by Mel K6KBE, I've just submitted my request to the UTC for 472kc operation (December 30, 2017.) You can use an online form from the UTC that requests your physical location coordinates in degrees, minutes and seconds. I used an address to GPS converter that I found online that gives both the decimal coordinates and the degrees, minutes and seconds. If your location is more than 1km from a HV line that has controlled-carrier power company troubleshooting data on it, you will get approved for operation. It appears they contact via e-mail but also request your telephone number. I'll update as to what feedback I get.
Here's the link for the UTC online form: https://utc.org/plc-database-amateur-notification-process/
UPDATE: I've heard from two different hams that the UTC is very, very slow to send any e-mails. One ham had to call the UTC after six weeks to complain. He received his e-mail approval the next day. The other ham had read on the UTC site that if nothing is heard from the UTC within thirty days, you're approved. He went on to operate on 630M. In about two more weeks, he received his e-mail approval. Looks like the UTC is on a six week response time (or, maybe not at all.) Maybe they're only counting "work days" so six, five-day work weeks equals 30 days.
UPDATE: Feb 23, 2018 - Nothing heard from UTC yet. March 2, 2018 - Still nothing. Oct. 3, 2018 - Figure that the UTC won't contact you unless there's a problem with your QTH.
UPDATE: March 11, 2018 - Information provided by Mel K6KBE indicates that there are some plans for voice transmission with significant bandwidth reduction located somewhere in the middle of 630M (around 475kc.) Bandwidth approximately 1.8kc.
630M Success! - I set up a sked with Mel, K6KBE (QTH: Ione, CA) to see if he would be able to copy my station on 473.5kc. Our sked was for 0600 on March 15, 2018. I was to send CW consisting of "V", "TEST", "de WA7YBS" and QSL information. The transmission lasted about five minutes with all of the text repeated three times. Mel reported his reception to me via e-mail and indicated that he heard me "come on" at 0600 "straight up." RST was 419, which doesn't sound that great but, on 630 meters at a distance of just over 100 miles, that's success. Mel is working on his 630 meter antenna which still needs a loading coil to function correctly. Weather has been his hold up. When Mel is able to transmit we'll go for 2X Morse on 630M.
Successful two-way CW on 630 Meters! - Mel and I set up a CW sked for 0600 for April 2, 2018. Mel was using a homebrew transverter and a "loaded" 75 meter antenna. I called "K6KBE de WA7YBS" at 0600 and Mel came back with a RST 549 signal that sounded strong and in the clear. Conditions were good at this point. Mel gave me a RST 549 also. Next go 'round the QRN started up but copy was still solid. Mel's transmission was that "QRN got u" and he was missing quite a bit of what I sent. Our 73s completed the short QSO. Just over 100 miles and a two-way CW QSO on 473.5khz.
That night, at 2000 PDT, there was a West Coast 630M "get together" on CW 473.5kc. I heard W0YSE tuning up but he was too weak to copy. He was answered by K6KBE and Mel's signal was incredibly strong, 589 or better. I had the loop antenna pointing SW in Mel's direction which obviously helped his signal and was probably why W0YSE was too weak to copy (YSE's QTH is in Washington state, should have been pointing N.) I know,...why didn't I move the loop? A six-foot loop in the house is pretty difficult to reorient.
Effective Isotropic Radiated Power? - Why use Effective Isotropic Radiated Power to set the power limit of 5 watts? This regulation is a method to limit the EM radiation of the transmitted signal to a certain level by control of the relationship of the RF power input to the antenna versus the antenna's physical size. Consider that a full-size 630 meter half-wave antenna is over 1000 feet long. This type of "full-size" antenna might actually exhibit a slight gain when compared to an isotropic radiator (dependent on other losses.) Therefore, the power input would have to be < 5 watts to stay within the regulations (assuming no other losses.) With a full-size antenna, even just 5 watts input could result in a formidable signal on CW. However, an antenna that will fit onto a typical city lot will be very inefficient at 630 meters and therefore would exhibit a considerable loss rather than gain. That's how the RF power input to a "small" antenna can be fairly high and yet only result in 5 watts EIRP. Think of the small, inefficient antenna as being like a "dummy load." You can input lots of RF watts into a dummy load and the dummy load does radiate a few feet but it isn't an efficient radiator. So, to stay within the regulations, one has to know the efficiency of their antenna and then calculate RF power input to the antenna versus EIRP. The efficiency is primarily determined by antenna size, antenna height and antenna resistance. The best info I could find is at www.472kHz.org under "Antennas for 630 Meters" and "EIRP." The formulae are explained in detail and four "real antenna" examples are shown to help answer "the EIRP question" for your particular or proposed set up.
Dealing with LF RFI-Noise
The Longwave part of the RF spectrum can be very noisy with intense static making copy difficult. In an extreme RF noise generating environment maybe all that will be heard is intense "buzzing" any where you tune. These factors can pose anywhere from difficult to solve problems up to impossible to solve problems when using any type of equipment to tune in LW signals. So, does vintage LW gear respond any better or is it actually worse when used in a noisy environment? Most WWII LW equipment will have some kind of noise limiter and also some filtering though they may be of little use against the types of noise encountered today. Fortunately, most of the intense noise found on LW is originating from our own houses. Light dimmer switches are notorious for producing a loud "buzzing" RFI on LW. Certain kinds of controllers that have neon pilot lamps (the orange glowing light) can also create RFI noise. Florescent lighting, certain types of illuminated clocks, computers and monitors, burglar alarms, grow-lamps, "wired" smoke-detectors, switching power supplies including some types of "wall wart" power supplies and some types of CFI lamps - all of these (and probably more) can produce RFI noise. Additionally, modern efficient furnaces that are multi-stage and modulate the blower speed can cause some RFI. This generally is heard as a changing pitch to the RFI as the motor speed changes. The newer the furnace, generally the less RFI will be encountered. RFI is also dependent on how the thermostat controls the blower and burner modulation. Although the list of RFI appliances keeps increasing and sometimes it seems like an impossible challenge, cleaning up our own houses for RFI noise is the first step towards successful receiving of LW DX.
Another noise producer is street lamps - not when they are operating correctly but when they are malfunctioning. Usually before the street lamp goes out altogether it will cycle on and off with a time interval of about 30 seconds to one minute on the start-up cycle. During this time intense RFI is emitted. It's amazing how far away the malfunctioning street lamp can be and still create RFI at your location. Expect intense RFI from a street lamp within your block. Fairly intense RFI from two to three blocks away and nuisance RFI from four to five blocks away. Some receiver noise limiters can reduce the interference but early LW receivers with no filters are useless during the lamp's start-up cycle. Most of the time the failing street lamp will cycle on and off every couple of minutes, all night long. Normally, if you call the power company they will come out and replace the failing lamp. You will have to have the street lamp ID number that is located on the underside of the assembly by the lens and also the street location (the ID number is visible from the ground looking up.) Fortunately for LW listening, the most intense RFI from street lamps is located in the frequency range from about 450kc up to about 4000kc.
Some of the LF RFI noise is on the power lines. There is a tremendous amount of data that is "riding" on the AC power lines. This is in the form of some controlled-carrier information, test and troubleshooting data, time setting information and, in some areas, broadband on the power lines. Some of the data exchanging on the power line is via the "smart meter" that has replaced the old electro-mechanical power meters can also cause RFI. The quieter your receiving area is, the more likely it is that you'll notice some type of power line noise, especially if you use an end-fed wire antenna.
Since there are so many LF RFI noise sources today, especially within urban areas, just about the only practical relief will be by using a tuned-loop antenna. In extremely noisy locations the only solution is to use a shielded-magnetic loop antenna. The shielded-magnetic loop antenna will use a non-ferrous metal loop-tube that almost entirely encloses the loop antenna wires that are inside. Since the antenna is electrically "shielded" but not magnetically "shielded" it responds mostly to the magnetic portion of the electromagnetic signal. Since most man-made RFI is electrical in nature, that noise is shielded by the loop's enclosure. However, all shielded loops will have some kind of signal amplifier that is either "tuned" or is somewhat "broadband" due to the limited response because of the shielding that almost entirely encloses the antenna itself. In many urban areas, only these types of antennas can provide relief from RFI and allow reception on the lower frequencies. Unfortunately, most commercially-made shielded loops are fairly expensive (~$500 and up.) In less severe noise locations, a simple tuned loop will provide a major improvement over a wire antenna and allow reception of very weak signals. Remember, none of these loops will produce stronger signals at the receiver if compared to a large wire antenna. However, in a RFI-noisy area, the loops will provide a much lower noise level and allow you to hear weaker signals. In an RFI-quiet area, a large wire antenna will provide strong signals significantly above the noise and will probably out-perform the loop.
Tuned Loop Antennas versus End-Fed Wires or Other Wire Antennas
Though LW stations can be tuned in using almost any type of antenna, the "Tuned Loop" provides the user with low noise reception due to its high Q, high selectivity. Another advantage is the ability to null out noise if it is from a particular direction. Most man-made noise will be somewhat directional and possibly could be nulled out. The selectivity of the loop will help with atmospheric noise by increasing the receiver's response to the tuned frequency and increasing the signal to noise ratio.
The End-Fed Wire is generally any wire antenna that has no feed line - one end of the antenna connects directly to the receiver antenna input. Usually, EFW antennas are between 75 and 150 feet in length due to physical limitations of the user's property size. Much longer than 250 feet and the EFW might begin to exhibit "long wire" characteristics of improved directional gain off of the ends although this actually depends on the frequency that the antenna is being used to receive.
Below 500kc, most EFW antennas are going to be "short" and exhibit none of the advantages of typical "long wires" used on HF. However, long (that is, a few hundred feet long or more) EFW antennas do provide better signal to noise performance than the typical short EFW and in some quiet locations might out-perform a tuned loop that's used in a poor location. Extremely long, "Beverage antennas*" perform entirely different (much better) than the typical, short (for LW) End Fed Wire. The EFW's advantage is ease of installation and, even if the antenna is not tuned, it will still give a fairly consistent response throughout the receiver's tuning range. However, because of this wide response and lack of a feed line, it's susceptible to all kinds of noise - made man and atmospheric.
While it's interesting to compare the two antennas, I have found that almost without exception a well-designed tuned loop antenna will always outperform almost any end-fed wire when comparing signal to noise ratio (not necessarily signal strength.) This is especially true with more modern receivers - the newer the receiver's design, the better it usually works with a tuned loop antenna. Very early three-circuit tuner regenerative receivers (1920s) seem to be much happier with long wire antennas of various configurations rather than the relatively small tuned loop antennas. However when using WWII or later vintage receivers, either regenerative or superhet, the tuned loop antenna provides the low signal to noise ratio necessary for successful DX NDB station copy.
Be sure to read the next section, "270ft Long Center-Fed Wire Antenna," as this provides an example of what a sizeable wire antenna can do on LW in a RFI-quiet area.
*The Beverage antenna (developed by Harold H. Beverage of RCA) is a one to two wavelength long antenna that is terminated to ground on its far end with a 450 ohms non-inductive load resistor. The Beverage antenna is mounted fairly close to the ground with 3 meters specified, although not too much difference in performance is noted with heights from 6 to 15 feet above the ground. Any higher and the antenna will begin to pick up noise. Beverage antennas are directional off of the terminated end. If the 450 ohm resistor is removed the antenna will become bi-directional off of the ends. Beverage developed the antenna for low noise reception and competitive performance. Two wavelengths is the specified maximum length according to Harold Beverage.
270 ft. Long Center-Fed Wire Antenna
Last year (2016,) I put up a wire antenna that was primarily for 75 meter operation. I wanted to run "two half-waves in-phase" which is basically a 160M dipole antenna operating on 75M. I used 135 feet of wire on each side and fed the center with 77 feet of 450 ohm ladder line. The ends were supported by a counterweight and pulley system erected in some cottonwood trees. Most of the antenna was about 30 feet off the ground but to the south-east the height was up about 37 feet. The center support was 31 feet high. The entire antenna was matched to the transmitter using a Nye-Viking antenna coupler. This system worked great on 75M. I noticed that received signals were generally 20db stronger than with the previous wire antenna (135' Inv-Vee.)
I hadn't thought about using this 270' antenna on longwave until I started restoring a couple of low frequency receivers. The first LF receiver operational was a RBA-1. Since the only sizable antenna available was the 270' dipole, I connected this to the RBA-1. I disconnected the feed line from the Nye-Viking coupler and used a test lead to short the two ladder line wires together. This was then connected to the RBA-1 using a 14 gauge stranded hook-up wire going to the center conductor of the Navy coax fitting (antenna input.)
During the next few days, while I was repairing and aligning the RBA-1, I would test the results using this antenna system. I was completely surprised when I started receiving NDBs from Idaho during the day. The big surprise was the next afternoon (13:30) when I tuned in DC 326kc from Princeton, British Columbia. Finally, when I had the RBA-1 finished I ready to do a serious test the following morning. From 05:55 to 06:35 in the morning I tuned in 47 NDBs in about 40 minutes and five of those NDBs were newly heard ones (#305 to #309 for the total tuned NDBs.) Greatest DX was POA in Hawaii and DB in Burwash Landing in the Yukon. Almost all signals were quite strong and nearly all stations had one or two other NDBs on the same frequency. Another surprise was receiving the first ham signal I'd ever heard below 500kc. WH2XVN in Burbank, CA on 183kc.
To determine if this performance is a result of the antenna or the receiver will require another test. This time using the National RBL-5 receiver.
This antenna forms a "T" which might be considered a vertical with a large top hat. This is the typical antenna used at many NDB sites. Most antennas from the early radio days had a two to three wire horizontal separated with spreaders on each end. Then the center of the "flat top" was tied together and fed with a single wire dropping down to the radio building.
More testing is necessary to determine if this antenna configuration will continue to provide a relatively low-noise operation. Much of the RFI that plagues smaller outdoor antennae and even the tuned-loop (when used indoors) seems to be greatly reduced, especially in the 190kc to 300kc region. I also would like to check if the feed line is shorted at the feed point of the horizontal wires thus making the antenna a true "T" wire, if the performance remains unchanged.
This large wire antenna can be connected directly to a substantial earth ground when not in use. The counterweight system seems to keep the antenna stationary as the wind runs the weights up and down as the tree limbs move around.
More information will be added as I do more testing,... November 5, 2017
UPDATE: While this antenna does provide strong signals, there's been only a few times that conditions are quite. Most noise is in the form of static and bursts. This could be wind noise or nearby storm fronts. With quiet conditions, this antenna is great but those conditions seem to be rare. November 23, 2017
Had great conditions on Dec 23, 2017, 44 stations copied in 40 minutes, one newly heard NBD in LaSalle, MB, CAN, LF-336kc, on the RBA-1 receiver. Best DX - FIS 332kc Key West, FL
The upshot here is,...when conditions are great this 270' x 77' "T" antenna is unbeatable. BUT, if anything does "beat" this antenna, it's noise,...not RFI but atmospheric noise. This is mostly caused by the ionosphere but can also be weather-related.
Remotely Tuned Loop Antenna Design
My first tuned loop antenna was a ten foot in diameter octagon with 12 turns of 20 gauge stranded wire remotely tuned with variable bias supplied to MVAM-108 varactor tuning diodes. The bias control, or tuning, was located at the receiver position for ease of operation and the bias voltage ran to the antenna via RG-58U coax cable. Tuning range was from 135kHz to 400kHz and by shorting out a turn on the loop the upper end of the range was increased to 500kHz. A 9' diameter single turn pick-up loop was mounted inside the 10' loop and was fed directly to the receiver's antenna input via RG-58U coax. This antenna performed very well with WWII vintage regenerative TRF receivers. Though the 10' loop antenna provided great signals it had a couple of problems. First, due to its size it was non-directional. That might be considered an advantage since I didn't have to provide any method of changing where it pointed. Second, due to its size it had to be located outdoors where it was highly susceptible to strong wind damage. After repairing the wind-broken 10' loop several times, I decided to rebuild the loop into a smaller configuration. This would result in a stronger antenna and would also result in some directional characteristics.
The new loop is a square with four foot sides and six feet across the diagonal. 17 turns are used in the antenna portion of the loop. A separate pick-up loop couples the signal energy from the tuned antenna where it is then routed to the receiver. I initially tried a single turn pick-up loop but found the signals were too weak. This was probably because of the very low impedance of the single turn, its physical length only being about 16 feet. I ended up using a three turn pick-up loop and found this gave much better performance. The pick-up loop is fed with RG-58U and connects to the receiver in use. The loop itself is connected to a small plastic box that contains the varactor diode board, connectors and a switch that selects the tuning range. The loop is tuned by varying the bias voltage (0 to +9vdc) on the varactor diodes. The frequency range is from approximately 195kc up to 440kc in two tuning ranges. This loop antenna is very directional and strong stations that are perpendicular to the antenna axis can almost be nulled out. Since this loop is relatively small, I have it indoors in the same room as the receivers. This location has eliminated the wind damage issue. Rotation is manual and since the upstairs floor is wood, I can set the antenna on the floor with no noticeable losses. In operation, signals received on this indoor 6' loop with a three turn pick-up are just about as strong as the outdoor 10' loop was and since it is directional it has the added advantage of increased signal strength when pointed towards the signal source.
Loop Details: The spacing of the loop wires is not especially critical. About
.25" seems to work fine. If the wires seem to get tangled, again, this doesn't
really seem to affect antenna performance much. The combs that keep the wires
separate are made of .25" thick oak and have sawn notches for the wire mounting.
The combs are held in place at the arm's end with glue and screws. To achieve two tuning ranges,
I use switched parallel varactor diode sets. The capacitance for a single
set is about 30pf to 300pf and a parallel set is about 60pf to about 500pf. The
switch is located at the antenna box which would be inconvenient if the antenna
wasn't indoors. I use a 9vdc transistor battery as the bias voltage source and a
ten turn, 10K pot with some limiting resistors to control the bias voltage to
the varactor diode junctions.
|Schematic for Loop Remote Tuning - Shown
to the right is a schematic for a very simple way to remotely tune a
loop antenna by using varactor diodes. As described in the section
above, this circuit can be built into a weather-proof plastic box that
can be mounted at the loop. RG-58U coax cable can be used to connect the
box to the remote tuning box that will be mounted beside the receiver. A
standard project box can be used for the remote tuning box.
Battery voltage is provided with a nine-volt transistor battery and
tuning is accomplished with a ten-turn potentiometer. The remote tuner
is also mounted inside a box for ease of operation. An "ON-OFF" switch
is provided to isolate the battery when the loop is not being used. The coax can be any
reasonable length. The longest I've used is around 50 feet with no
problems. You can use PL-259 connectors on the coax and SO-239 box
connectors on the remote tuning box and the loop box. The resistors and
the capacitor are not critical and only provide a filter for the bias
supply to the varactor diodes. I used three turns on the pick-up loop as
I found two turns didn't provide strong enough signals. Best results
will depend on the antenna input Z of your receiver.
To increase the lower end of the tuning range it is possible to switch in a fixed 500pf silver mica capacitor in parallel with the loop terminals. This will reduce the overall tuning spread but will lower the frequency bottom end by about 40kc or so. As shown, the loop tunes 240kc up to 440kc. With a parallel cap switched in, the low frequency is 195kc. If the parallel cap is added a double switching arrangement can be used for better isolation. A higher value cap can be installed to lower the bottom end frequency more if desired but the variable tuning range will decrease as the frequency is decreased. A three position switch (with an off position, too) could be installed to allow a selection of 500pf, 1000pf and 1500pf fixed value capacitors to allow loop tuning to go down to about 150kc or so.
|Additional Loop Antenna Information as of Jan. 29, 2009:
I'm very pleased with the performance of the six-foot loop. I really think its
performance is at least equal to the ten foot loop that was mounted outside and,
many times, I think it's actually better. During the past two months (12/08 and
1/09) I have
logged over 100 new NDBs using the 6' loop. That's not total NDBs heard - it's just new NDBs I hadn't heard before. Best DX was YY 340kc in Mont Joli, Quebec at around 2500
miles. Also, in the other direction, LLD 353kc at Lanai City, Hawaii - also around
2500 miles. Greatest DX wasn't a new NDB for me - it was DDP 391kc in San Juan, Puerto
Rico at around 3500 miles - but DDP is a transatlantic beacon running 2KW - it's
not hard to receive. I think the main advantage of the six-foot loop is the
ability to point it in the direction of the stations and exclude other stations
that are perpendicular to the antenna axis. LLD is a good example since Reno's
NO is very strong and transmitting on 351kc and LLD is on 353kc. LLD is a
transpacific beacon running 1-2KW and would be an easy copy if NO was not a
local NDB. Fortunately, those two NDB
signal paths are physically about 90 degrees apart at my location so I can somewhat null NO and copy LLD by
pointing the loop SW. Signal levels on the six-foot loop are about the same as
the ten-foot loop was. The receiving limitations are primarily the atmospheric noise and
relative conditions, then local noise and finally the receiver's ability to
pull signals out of the noise. The RAZ-1 is very good at weak signal
UPDATE - 2015: I've used this loop antenna with many different LW receivers and it seems to work quite well with just about any receiver. When I acquired the Hammarlund SP-600VLF receiver I found that the loop acted differently with respect to the apparent Q of the loop with tuning seemingly so "broad" that it was difficult to find a "peak." I ended up removing one turn on the pick-up loop and with two turns, the loop "peak" could be tuned although it was still somewhat broad. The recommendation is that depending on your receiver input Z you may have to work with the length of the pick-up loop (number of turns) to determine optimum tuning response.
UPDATE - 2018: I've been having trouble with the loop working well with two receivers. The SP-600VLF seemed to make the loop very broad tuning with difficulty finding a "peak." I removed one turn on the loop which helped a little. Then with the R-389, I didn't seem to have enough signal strength from the loop. To try to "fix" the two problems, I've removed the pick-up loop and have now increased the number of turns to four to increase gain. In order to increase selectivity, I've reduced coupling by reducing the size of the pick-up loop. It had been spaced about 1.5" inside the primary loop. I've doubled the distance so now the pick-up loop is 3" inside the primary loop. I'm hoping that the four turns results in strong signals and the greater distance will make the loop "tune" sharper. In a quick test I tuned the R-389 to the nearby DGPS 314kc node as a test signal during mid-day. The loop peak tuning showed 25db on the carrier level meter. As a reference, the 135'x100' "T" outdoor wire antenna showed 40db. The tuning Q didn't change too much but with the R-389 the peak is easy to find. Further testing will reveal if this change benefits DX reception for both the R-389 and the SP-600VLF.
Adding the HP 461A Broadband Amplifier to the
Several years ago, N7ID loaned me a Hewlett-Packard 461A Broadband Amplifier to use with the RAK-7 receiver I was then using for longwave. I installed the 461A between a wire antenna and the receiver. All I got was a tremendous increase in noise and not much, if any, signal gain. I returned the 461A and didn't think about that type of amp again. A few years later I had tried a homebrew solid-state amplifier on my six foot remotely tuned loop but its performance was terrible. It seemed to have so much gain that I'd tune in the AM BC band stations along with various NDBs. Recently, I began thinking about the HP 461A again. When I had used it before, it was an untuned input coming from a random length wire antenna. If I installed the 461A with the loop's pick-up loop as the input that would add the tuned frequency input ability of the main loop along with the pick-up loop's selectivity. This would tend to reduce the amount of noise while enhancing a specific tuned frequency. The output of the 461A would be connected to the antenna input of the receiver.
HP-461A Specs - These small solid state amplifiers had a built in power supply and had selectable fixed gains of either 20db or 40db. Input and Output impedance is 50Z ohms. Frequency bandwidth is 1Khz up to 150Mhz. The input voltage limit is 2vdc and 1vac.
Performance - For the first test I used the Collins R-389 and a 160' End-Fed Wire. This is about as noisy of an antenna that can be found. With the 461A connected between the EFW and the receiver all that seemed to be increased was noise. Signals that were audible disappeared into the noise with 20db of amplification. Next, I substituted the loop antenna and tuned in the DGPS node on 314kc. It was pretty strong with no amplification and very strong with 20db but with 40db of amplification the input overloaded the receiver and the signal seemed to disappear. Returning to 20db and then the 314kc node was again present. At 2230 hours I tuned in NDB MOG 402kc. I showed about 20db on the carrier level meter (a strong signal) without the 461A on. With 20db of amplification, as one would expect, the meter read 40db. But, if 40db of amplification was selected, then the signal disappeared because the input was so strong that it "blocked" the receiver front end.
Now, that was the 461A performance receiving fairly strong signals. What about really weak signals? Here's where receiving conditions really matter. It's a fine line between the loop + amp responding mainly to noise or responding to a weak signal that is just above the noise. Several times, I would tune in a signal that could be heard without the 461A connected but when the 461A was added, even with just 20db selected, the weak signal would just disappear although the noise had a major increase. Since all DX LW signals are weak and basically just slightly above the noise, it seems like the 461A usefulness will be nil. >>>
Headphones versus Loudspeaker
|The final necessity for successful reception of weak LW
signals is using the
proper audio output reproducer. If you use a loudspeaker you can
just about eliminate 70% of the NBDs that you would probably hear if you used
headphones. Nearly all of the DX NDB signals are weak in signal
strength. Most signals are in the noise. Much of the time you are trying
to copy the weakest NDB that's on the same frequency as a couple of strong NDBs. Listening
with a set of 'phones enhances your
perception when copying weak signals that are buried in QRM and QRN.
Most vintage military LW radio receivers provide a 600Z ohm audio output. Finding a set of 600Z ohm 'phones is pretty easy. If you are looking at the WWII military headsets that provide a short cable with a small phone plug that then plugs into a six-foot extension cable, then you look at the color of the small phone plug shell. If it's red then it's Low-Z or 600Z ohms, if the shell is black then the 'phones are Hi-Z or around 10K Z ohms. This color code only applies to WWII 'phones. Later, in the 1950s, 600Z 'phones were considered Hi-Z, so these types should be measured to verify actual impedance.
Most early vintage LW receivers have high impedance outputs that might have the 'phones connected directly between B+ and the audio output tube plate. You must use Hi-Z 'phones for this type of receiver. Generally the older style 'phones work fine, especially those from the 1920s that were designed for direct B+ to plate connection. >>>
>>> If the headset is not marked then measure the DCR at the connecting plug or the phone tips to determine the probable impedance. Hi-Z phones will measure above 1K ohms DCR while 600Z ohm phones will measure around 100 ohms DCR. If you measure a very low DCR (< 5 ohms) then the impedance is 4 or 8 ohms. This test is an approximation to estimate probable impedance. Remember, 'phone impedance is "nominal impedance" and dependent on what frequency is used in the calculation. Generally, nominal impedance meant that the specified Z was the lowest Z that the would be encountered when the 'phones were used in a standard configuration listening to average signals at average levels. Pretty vague,...so don't take the specified Z as something that is ultra-critical,...close is okay.
Once you have your 600Z ohm 'phones, check the schematic on your particular LW receiver to see how the audio output is designed. Most military LW receivers were designed for "headphones only" use and the 600Z ohm audio output is at the phone jack on the front panel (usually.) Later LW receivers might have the phone jack connect to the 1st AF stage or the second detector (on a superhet) and it might be that the phone jack might have circuitry added to assure that the headset is not "over-driven." Best results will be obtained by connecting the 600Z ohm 'phones to the "actual" 600Z ohm audio output stage. This may or may not be "at the phone jack" so check your receiver's schematic and connect your 'phones to the "actual 600Z ohm audio output." You'll have to be careful and only use enough gain to hear the average noise level in the receiver output. Even then, sometimes "pops" and "clicks" can get thru the Noise Limiter and "over-drive" your ear drums. Keep the 'phone cups just slightly in front of your ears to avoid problems.
Using a good set of headphones will enhance your listening and your DX NDB log.
US Coast Guard - Loran C Master Station 'M'
NOTE: As of February 8, 2010 the Loran-C system will begin its permanent shut down
On February 8, 2010, I tuned in Loran-C Master Station 'M' at 8:30AM PST and it was operating as usual. Tuning in later in the afternoon, at 5:15PM PST, Master Station 'M' had ceased operating. In August 2010, it was noted that Station 'G,' the last remaining West Coast Loran signal, was not transmitting.
Consider all Loran-C operations "OFF THE AIR"
Fortunately, we toured Master
Station "M" in July, 2007 and were able to take several photos of the
station including the Megapulse Transmitter and the Control Room -
photos and description below...
photo right: Loran C Station Fallon "Master of the Pacific Since 1977" Arm Patch
Above: The Loran C antenna from main gate. The mast is 625 feet tall with each side measuring about six feet across. The capacity hat is about 900 feet diameter and is formed by the 24 top cables drooping down to large isolators. The size of the installation can be compared to the street lamps near the base of the antenna and just visible is the roof of the station house.
Just outside of Fallon, Nevada is the U.S. Coast Guard Loran-C Station which provides a navigation utility for the Pacific Ocean and the West Coast. Loran-C is part of a world-wide system of navigation mostly used for sea going craft. The Fallon station is designated 'M' since it is the Master Control station for the other three West Coast stations designated 'Y' in Searchlight, Nevada, 'X' in Middletown, California and 'G' in George, Washington. These three stations along with the master station in Fallon allow navigators to determine their position by use of a special Loran C receiver that accurately measures the pulse characteristics of the received signal to determine station ID and then accurately measures the time delay of the precisely timed signal (based on a Cesium atomic clock standard) to determine the receiver's distance from the transmitter. By using the master station signal and at least one slave station signal, the receiver position is determined by timing the two wave fronts to determine their intersection point in reference to the receiver's location. If another slave station can be received then the calculation of intersection point becomes more accurate and likewise the receiver's position. Various corrections are incorporated into the computations to allow for skywave propagation (if any,) terrain (over land or over water) and other minute interferences. Three HP Cesium atomic clocks keep the accuracy of the system constant since correct timing to the nanosecond is essential for determining true position. The best accuracy of Loran C is about 50 to 150 feet.
The transmitter is running 400KW at 100 kHz. The antenna mast is 625 feet tall and 24 top conductors drooping down to large isolators form the enormous capacity hat for the system. The signal consists of a rapid, continuous "tick-tick tick..." centered at 100 kHz. The signal is actually a pulse train made up of eight pulses from each Loran C station. The Master 'M' station has an extra pulse in the train for identification as a "master." Timing is critical as every Loran C station is on 100 kHz and each station has to send its pulses at a precise time for the system to maintain accuracy.
The Fallon Loran C is easy to receive anywhere in the west. It is particularly strong in Virginia City as we have "line of sight" to the Loran-C antenna, even though it is nearly 60 miles away. This is because VC is on the east slope of Mt. Davidson at 6200 feet elevation and looking 60 miles east is Fallon at 3980 feet elevation. You can see Mt. Davidson from the Fallon Loran-C Station. The USGC station and antenna are located West of Fallon at the end of Soda Lake Rd. with a right turn onto Loran Rd. to the site.
Below are some photos taken at the station in July 2007.
Above: The Control Room with Signal Generators, three Cesium atomic clocks, signal and transmitter monitoring, alarms, communications with slave Loran stations. Everything has a duplicate for redundancy.
|Above Left: The 625' Antenna base stands on five ceramic
insulators. The entire weight of the tower and guy system is supported by
these 5" diameter insulators. The feed line is an air spaced coaxial feedline
housed in an eight-inch diameter PVC tube that exits from the
transmitter building. The box at the
end of the feedline is the lightning arrestor. The output of the
feedline connects to the tower base with 2" diameter copper pipe. The
device to the left of the tower is a coupling transformer for the tower
lights - it allows isolation from the AC line if the tower is struck by
lightning. The ground connection can be seen at the base of the
insulators - four copper sheets 2 ft. wide and .125" thick are buried
and also connect to the radial system that is about 900 feet
diameter. For a scale to the size of this installation, the sides of the
tower are 6 feet across. The circular pads at the top of the triangular
section are for fitting spacers to hydraulically jack the entire tower up for
maintenance to the base mount.
Left: The Loran C 400 KW transmitter built by Megapulse. Most of the transmitter consists of sixteen drivers (eight panels on each side) that shape the final output signal. The station can operate with up to two drivers not working. Past the drivers is the output stage followed by the output coupler. The output coupler attaches to the feedline via two large cables (this 8" PVC feedline exits the transmitter building wall and goes directly to the antenna.) The incredibly large switching load on the transmitter power supplies results in a very loud audible representation of the transmitted signal.
Right: Looking into the rear of the transmitter bay. The red tags remind the technicians that 30,000 volts is present when the transmitter is operating. Also note the yellow sign regarding the noise present around the transmitter.
The output coupler stage of the transmitter. One
inductor is hand tuned for a "rough" setting while the final tune is
accomplished remotely with the motor driven inductor. Below the
inductors is the solid state output magnacoupler. Large capacitance can
be used with solid state transmitters resulting in smaller inductors.
These inductors are about 10" diameter. The coils are wound with a cloth covered multiconductor cable.
Note the output cable routed thru the fiberglass wall. This is then
routed up to the antenna to feedline coupler that can be seen in the
Right: The output tank
stage which is adjacent to the output coupler. The tuning inductance is
adjusted with a special tool that fits onto the eccentric knob on the
shaft. This allows adjustment with the panel installed and the
transmitter operational. Below are the massive capacitors that allow the use of smaller
inductors. For size reference, the inductor is about 10 inches diameter.
NOTE: These photos were taken of the standby units. The access
doors to the operational units cannot be removed while the transmitter
is running without causing a system shutdown. Even removing these
standby unit access doors would have triggered an alarm had it not been
bypassed in the Control Room prior to opening.
Thanks to USCG ET1 Chris Shanks for the tour of the facility.
Non-Directional Beacon Stations
NDBs in Nevada
Ah,...the good old days, when there were loads of NBDs everywhere,...even in Nevada. Today (2014,) there are no active NDBs in the state. Here's information and some photos of the last two NDBs in operation in Nevada. Both have gone "off the air" in the past few years - AEC 209kc (OTA 2009) and NO 351kc (OTA 2013.) Additionally, I've added information on some of the older NDBs that were operating here in Nevada in the past.
"NO" - 351 Khz - Reno, Nevada - NDB for Reno-Tahoe International Airport
Located on 351 KC is the NDB for Reno-Tahoe International Airport. "NO" runs 25 watts and is a marker beacon physically located at the north end of the airport, in an empty lot, across the street (Mill Street) from the beginning of runway 16R. The antenna is only about 15 feet of vertical radiator with a capacity hat that is about 15 feet off the ground and about 150 feet long. The capacity hat is strung between two "not very tall" telephone poles. The transmitter and climate control equipment are located in and around a small building below the center of the capacity hat. The feed actually enters on the west side of the building through an underground conduit. Coverage is quite good considering the low power of the transmitter and the small antenna. Since "NO" is a marker beacon, it usually isn't listed on any of the NAV-AID sites - but it is operating 24 hrs a day, on 351 KC. About once a year, "NO" is "off the air" for a period of 2-3 weeks. Whether this is due to failures or scheduled maintenance is not known - the signal always seems to return after a few weeks.
"OFF THE AIR"
NO has been off the air for over three months now. This is the longest shutdown yet. Hopefully, NO will return to the air pretty soon. When in Reno last (end of Oct.2013) I drove over to Mill St. to look at the NO site. Everything is still there, the shack, the antenna. Everything appears normal but as of November 7, 2013, NO is still OTA.
No change as of July 1, 2014. Consider NO "Off The Air." See updated photo lower right.
NOTE: As far as I can tell, "NO" was the last operational NBD in Nevada.
photo above: I took this shot of the NO site on September 21, 2015. As can be seen, nothing is left of the NO radio shack, transmitting equipment, antenna or associated structures. The property has been totally cleared. Compare this shot to the shot directly above and it can be seen that the NO shack was located just about center of the view and slightly to the right of the Nugget Towers. I took this shot from the same location behind the auto-repair dealership on Mill St. This pretty much concludes that NO 351kc will not be returning to the air.
"AEC" - 209 kHz - NDB for Base Camp, Nevada
AEC is on 209 kc and can be received here day or night, indicating that the transmitter might be running power higher than the 25 watts normal for NDBs. AEC is located near Warm Springs, Nevada on Hwy 6 about 60 miles east of Tonopah, Nevada. The site is called Base Camp. The antenna is an "inverted L" configuration with the shack located at one end near the pole support. From aerial photos it appears that there are a number of ground radials running out from a central location between the two poles. At one time AEC transmitted voice weather along with the MCW ID, however nowadays just the CW ID is transmitted. Base Camp is a US government controlled, fenced air field with a maintained runway and some minor support buildings. Though the runway was recently repaved, there are large "X"s painted at each end of the runway to indicate "as viewed from the air" that it is closed and not in use. Apparently no hangers are at the site. What the exact use of Base Camp is remains unknown, although once it was part of the Tonopah Test Range. Though some speculate it now has some connection with Groom Lake/Area 51, this is highly unlikely. AEC is not listed on any of the NAV-AID sites yet it is in operation 24 hours a day, everyday. It is listed on LF websites that show logs of received stations.
AEC 209kc has been Off the Air since Sept.2009
Consider AEC "OFF THE AIR"
photo left: AEC at Base Camp, NV - this great photo is by Steve McGreevy N6NKS, from www.auroralchorus.com
Other Nevada NDBs (Inactive)
EMC - 375kc - Winnemucca, NV - Off the air since
NDB Station Log 2006 to 2017
From Virginia City, Nevada - 2006 to 2012 - A large percentage of the following NDB stations are ones that I copied from Virginia City, Nevada using only vintage, tube-type receivers. I used several different types of vintage LW receivers. Many NDBs were heard using the 1941 RAZ-1 receiver, but I have also copied quite a few with the 1945 RAK-7 and 1944 RBL-5 receivers. I also logged some "newly heard" NDBs during experiments when testing the 1920 SE-1420, the 1922 RMCA IP-501A and the 1940 Hammarlund SP-200-LX receivers. For the 2009-2010 season, I added the 1945 RBA-6 receiver. My first dedicated LW antenna was a 10' diameter remotely tuned loop but that was destroyed by wind. Now, the main LW antenna is a 6' remotely tuned loop located indoors (as of Nov'08.) I also found some new NDBs using various wire antennas. These NDB stations were received during the 2006 to 2012 seasons. Stations are listed alphabetically along with frequency, location and power of the transmitter, if known. Total was 252 NDBs received from Virginia City 2006 up to 2012.
From Dayton, Nevada, the new QTH beginning in 2012 We are now in Dayton, Nevada (10 miles SE of Va.City.) For a short time (2013-14,) the antenna used was a 300 ft. long end fed wire up about 50 feet. New NBDs for 2012/13 and 2013/14 seasons are shown in Navy Blue. Receiver was the RBA-6. EFW antenna taken down Mar 2014. Six newly heard NDBs were logged with this combination. Total Spring 2014 was 258
2014-2015 Season - Nov. 2014, started using Hammarlund SP-600VLF-31 receiver. New NDBs heard with the SP-600VLF are in Maroon. Changed to 6' Remote-tuned Loop Nov.15, 2014.
2015-2016 Season - Started listening Oct. 2015, Hammarlund SP-600VLF-31 and 6' Remote-tuned Loop. Total newly heard NDBs logged (2015/16) with this combination is 35 - Maroon
2016-2017 Season - Hammarlund SP-600VLF-31 w/ 6' Remotely-tuned Loop - First new NDB this season on Nov.30, 2016 (AN-368kc.) Total new with this combo is 42 - Maroon
2017-2018 Season -
Hammarlund SP-600VLF-31 w/ 6' Remotely-tuned Loop - First new NDB
this season on Oct. 13, 2017 (DUT-283kc.) Total new with this combo is 61
2018-2019 Season - Collins R-389/URR w/ 100' x 135' "T" Wire Antenna or 6' Loop - First new NDB this season on Sept. 24, 2018 (ZZP-248kc) Total new with this combo is 5 - Green
Total NDBs logged as of SEPT 24, 2018 is 330.
AA - 365kc - Fargo, ND - 100W
ADT - 365kc - Atwood, KS
AE - 351kc - Dudle-Albuquerque, NM
AEC - 209kc - Base Camp, NV - OTA
AFK - 347kc - Nebraska City, NE - 25W
AGZ - 392kc - Wagner, SD
AL - 353kc - Trina (Walla Walla,) WA
AM - 251kc - Amarillo, TX - 400W
AN - 368kc - San Antonio, TX
ANR - 245kc - Andrews, TX
AOP - 290kc -Rock Springs, WY - 100W
AP - 260kc - Denver, CO - 100W
AP - 378kc - Active Pass, BC, CAN
ATS - 414kc - Artesia, NM - 25W
AVQ - 245kc - Tucson, AZ
AZC - 403kc - Colorado City, AZ
BAJ - 392kc - Sterling, CO
BBD - 380kc - Brady, TX - 25W
BI - 230kc - Jadan-Bismarck, ND
BKU - 344kc - Baker, MT - 80W
BO - 359kc - Boise, ID - 400W - OTA
BR - 233kc - Brandon, MB, CAN
BWR - 412kc - Alpine, TX - 25W
CBC - 415kc - Cayman Brac, Cayman Islands
CC - 335kc - Buchanan AF, CA - 25W
CEP- 278kc - Ruidoso, NM - 25W
CG - 227kc - Castlegar, BC, CAN
CH - 329kc - Ashly-Charleston, SC - 400W
CHD - 407kc - Chandler, AZ
CII - 269kc - Choteau, MT - 50W
CIN - 397kc - Carroll, IA - 25W
CKP - 423kc - Cherokee, IA - 25W
CL - 515kc - Port Angeles, WA
CLB - 216kc - Wilmington, NC - 1KW
CN - 235kc - Cochrane, ON, CAN 100W
CNP - 383kc - Chappell, NE - 25W
COR - 205kc - Corcoran, CA - 25W
CRK - 389kc - Spokane, WA
CRR - 245kc - Circle, MT - 100W
CRZ - 278kc - Corning, IA - 25W
CSB - 389kc - Cambridge, NE - 25W
CUH - 242kc - Cushing, OK - 25W
CVP - 335kc - Helena, MT - 150W
CY - 353kc - Cheyenne, WY
CYW - 362kc - Clay Center, KS - 25W
CZX - 332kc - Crosbyton, TX
DAO - 410kc - Ft. Huachuca, AZ
DB - 341kc - Burwash Landing,YK,CAN
DC - 326kc - Princeton, BC, CAN
DDP - 391kc - San Juan, PR - 2KW
DIW - 198kc - Dixon, NC - 2KW
DN - 225kc - Dauphin, MB, CAN
DPG - 284kc - Dugway Prov Gnds, UT
DPY - 365kc - Deer Park, WA - 25W
DQ - 394kc - Dawson Creek, BC, CAN
DUT - 283kc - Dutch Harbor, Amakrak Is., AK
DWL - 353kc - Gothenburg, NE - 25W
EC - 217kc - Cedar City, UT - 25W
EHA - 377kc - Elkhart, KS - 25W
EKS - 286kc - Ennis, MT - 25W
EL - 242kc - El Paso, TX - 400W
ELF - 341kc - Cold Bay, AK - 1KW
ENS - 400kc - Ensenada, Mexico
ENZ - 394kc - Nogales, AZ - 100W
ESY - 338kc - West Yellowstone, MT - 100W
EUR - 392kc - Eureka, MT - 100W
EX - 374kc - Kelowna, BC, CAN
FCH - 344kc - Fresno, CA - 400W - OTA
FIS - 332kc - Key West, FL
FMZ - 392kc - Fairmont, NE - 25W
FN - 400kc - Ft. Collins, CO
FO - 250kc - Flin Flon, MB, CAN
FOR - 236kc - Forsyth, MT - 25W
FQ - 420kc - Fremont, MN - 25W
FS - 245kc - Sioux Falls, SD - 100W
FS - 375kc - Ft. Simpson, NWT, CAN
GB - 253kc - 'Garno' - Marshall, MN
GC - 380kc - Gillette, WY
GDV - 410kc - Glendive, MT - 100W
GEY - 275kc - Greybull, WY
GGF - 359kc - Grant, NE
GLS - 206kc - Galveston,TX-2KW - OTA
GLY - 388kc - Golden Valley-Clinton, MO
GNC - 344kc - Seminole, TX - 25W
GRN - 382kc - Guerrero Negro, Mexico
GRN - 414kc - Gordon, NE
GUY - 275kc - Guymon, OK - 25W
GW - 371kc - Kuujjuarapik, QC, CAN
GYZ - 280kc - Guernsey, WY - 50W
HAU - 386kc - Helena, MT
HBT - 390kc - Sand Point, AK
HCY - 257kc - Cowley, WY
HDG - 211kc - Gooding, ID - 50W
HE - 245kc - Hope, BC, CAN
HF - 241kc - Hearst, ON, CAN 100W
HIN - 275kc - Chadron, NE - 25W
HJH - 323kc - Hebron, NE - 25W
HLE - 220kc - Hailey, ID - 50W
HQG - 365kc - Hugoton, KS - 25W
HRU - 407kc - Herington, KS - 25W
HRX - 341kc - Hereford, TX
IB - 209kc - Atikokan, ON, CAN
ICL - 353kc - Clarinda, IA - 25W
ID - 324kc - Idaho Falls, ID
IKY - 429kc - Springfield, KY - 25W
ILT - 247kc - Albuquerque,NM - 400W
IN - 353kc - International Falls, MN
INE - 521kc - Missoula, MT - 400W
IOM - 363kc - McCall, ID - 25W
IP - 201kc - Mobile, AZ
ITU - 371kc - Great Falls, MT - 100W
IY - 417kc - Charles City, IA - 25W
JDM - 408kc - Colby, KS - 25W
JHN - 341kc - Johnson, KS
JM - 396kc - Jamestown, ND
JW - 388kc - Pigeon Lake, AB, CAN
K2 - 376kc - Olds-Didsbury, AB, CAN
LAC - 328kc - Ft. Lewis, WA - 25W
LBH - 332kc - Portland, OR - 150W
LD - 272kc - Lubbock, TX
LF - 336 - LaSalle, MB, CAN 50W
LFA - 347kc - Klamath Falls, OR
LGD - 296kc - LaGrande, OR - 25W
LLD - 353kc - Lanai City, HI - 2KW
LLN - 266kc - Levelland, TX
LU - 213kc - Abbotsford, BC, CAN
LV - 374kc - Livermore,CA - 25W
LW - 257kc - Kelowna, BC, CAN
LWG - 225kc - Corvallis, OR
LWT - 353kc - Lewiston, MT - 400W
LYI - 414kc - Libby, MT - 25W
LYQ - 529kc - Manchester, TN
L7 - 395kc - Estevan, SK, CAN
MA - 326kc - Midland,TX - 400W
MA - 365kc - Mayo, YK, CAN
MDS - 400kc - Madison, IA - 25W
MEF - 356kc - Medford, OR
MF - 373kc - Rogue Valley, OR
MKR - 339kc - Glascow, MT - 50W
ML - 392kc - Charlevoix, QC, CAN
MLK - 272kc - Malta, MT - 25W
MM - 388kc - Fort McMurray,AB,CAN
MNC - 348kc - Shelton, WA
MNZ - 251kc - Hamilton, TX - 25W
MO - 367kc - Modesto, CA
MOG - 404kc - Montegue, CA - 100W
MR - 385kc - Monterey, CA
MW - 408kc - Moses Lake, WA
NA - 337kc - Orange County AP, CA
NM - 278kc - Matagami, QC, CAN
NO - 351kc - Reno, NV - 25W - OTA
NY - 350kc - Enderby, BC, CAN
ODX - 355kc - Ord, NE - 25W
OEG - 413kc - Yuma Prov. Gnds., AZ
OEL - 381kc - Oakley, KS - 25W
OIN - 341kc - Oberlin, KS - 25W
OJ - 239kc - High Level, AB, CAN
OKS - 233kc - Oshkosh, NE - 25W
OLF - 404kc - Wolf Point. MT - 100W
ON - 350kc - Newport, OR
ON - 356kc - Penticton, BC, CAN
ONO - 305kc - Ontario, OR
ORC - 521kc - Orange City, IA - 25W
OT - 378kc - Bend, OR
OUN - 260kc - Norman, OK - 25W
OWU - 329kc - Woodward, OK
PA - 347kc - Prince Albert, SK, CAN
PBT - 338kc - Red Bluff, CA -400W OTA
PBY - 259kc - Kayenta, AZ
PD - 230kc - Pendelton, OR - 400W
PDG - 327kc - Watsonville, CA - 25W
PG - 353kc - Portage, MB, CAN
PI - 383kc - Tyhee, ID
PN - 360kc - Port Menier, QC, CAN
PNA - 392kc - Pinedale, WY - 25W
POA - 332kc - Pohoa-Hilo, HI
POH - 428kc - Pocahontas, IA - 25W
POY - 344kc - Powell, WY
PPA - 450kc-Puerto Plata, Dominican Republic
PRZ - 407kc - Portales, NM - 25W
PTT - 356kc - Pratt, KS - 25W
PYX - 266kc - Perryton, TX - 25W
QD - 284kc - The Pas, MB, CAN
QL - 248kc - Lethbridge, AB, CAN
QN - 233kc - Nakina, ON, CAN
QQ - 400kc - Comox, Van.Is., BC
QR - 290kc - Rigina Int'l, SK, CAN
QT - 332kc - Thunder Bay, ON, CAN
QU - 221kc - Grand Prairie, AB, CAN
QV - 385kc - Yorkton, SK, CAN
QW - 302kc - North Battleford, SK, CAN
RA - 254kc - Rapid City, SD - 100W
RD - 367kc - Redding Muni, CA - 25W
RD - 411kc - Redmond, OR - 400W
RG - 350kc-Will Rogers World AP, OKC,OK
RL - 218kc - Red Lake, ON, CAN
RMD - 204kc - McDermitt, OR - 25W
RNT - 353kc - Renton, WA - 25W
RPB - 414kc - Belleville, KS
RPX - 362kc - Roundup, MT - 25W
RWE - 528kc - Camp Roberts, CA
RWO - 394kc - Kodiak, AK - Voice WX
RYN - 338kc - Tuscon, AZ - 400W
SA - 356kc - Sacramento,CA
SAA - 266kc - Saratoga, WY - 25W
SAK - 515kc - Kalispell, MT - 25W
SB - 397kc - San Bernadino,CA
SB - 362kc - Sudbury, ON, CAN
SBX - 347kc - Shelby, MT - 25W
SC - 271kc - Stockton,CA
SCO - 283kc - Scobey, MT
SDA - 411kc - Shenandoah, IA - 25W
SDY - 359kc - Sidney, MT - 25W
SF - 379kc-San Francisco Intn'l AP, CA
SG - 341kc - Santa Fe, NM
SIR - 368kc - Sinclair, WY
SKX - 414kc - Taos, NM - 25W
SL - 266kc - Salem, OR - OTA (now SLE)
SLB - 434kc - Storm Lake, IA - 25W
SLE - 266kc - McDerrmit AP, Salem, OR
SM - 230kc - Metre/Sacramento, CA
SM - 254kc - Fort Smith, NWT, CAN
SOW - 206kc - Show Low, AZ - 25W
SRL - 270kc - Santa Rosalia, MEX
STI - 333kc - Mt. Home, ID
SWT - 269kc - Seward, NE - 25W
SWU - 350kc - Idaho Falls, ID
SX - 367kc - Cranbrook, BC, CAN
SYF - 386kc - St. Francis, KS - 25W
SYW - 428kc - Greenville, TX - 25W
SZT - 264kc - Sandpoint, ID
TAD - 329kc - Trinidad, CO
TCY - 203kc - Tracy, CA
TF - 373kc - Pueblo, CO
TH - 244kc - Thompson, AB, CAN
TOR - 293kc - Torrington, WY
TQK - 256kc - Scott City, KS - 25W
TV - 299kc - Turner Valley, AB,CAN
TVY - 371kc - Tooele, UT - 25W
TW - 389kc - Twin Falls, ID
U6 - 360kc - Creston, BC, CAN
UAB - 200kc - Anahim Lake, BC,CAN
UK - 371kc - Kearn, CA
ULS - 395kc - Ulysses, KS - 25W
UNT - 312kc - Penticton, BC, CAN
UVA - 281kc - Uvalde, TX - 25W
VC - 317kc - LaRonge, SK, CAN
VG - 230kc - Vermillion, MB, CAN
VQ - 400kc - Alamosa, CO
VT - 332kc - Buffalo Narrows, SK, CAN
WG - 248kc - Winnepeg, MA,CAN
WL - 385kc - Williams Lake, BC, CAN
XC - 242kc - Cranbrook, BC , CAN
XD - 266kc - Edmonton, AB, CAN
XE - 257kc - Saskatoon, SK, CAN
XH - 332kc - Medicine Hat, AB, CAN
XJ - 326kc - Fort Saint John, BC, CAN
XS - 272kc - Prince George, BC, CAN
XT - 332kc - Terrace, BC, CAN
XX - 344kc - Abbotsford, BC, CAN
YAG - 376kc - Fort Frances, ON, CAN
YAT - 260kc - Attawapiskat, ON, CAN
YAZ - 359kc - Tofino,Van.Is., BC, CAN
YBE - 379kc - Uranium City, SK, CAN
YBL - 203kc - Campbell River, BC, CAN
YBV - 370kc - Berens River AP, MB, CAN
YC - 244kc - Cranbrook, BC, CAN
YCD-251kc - Nanaimo, Van. Is, BC, CAN
YD - 230kc - Smithers, BC, CAN
YE - 382kc - Fort Nelson, BC, CAN
YEL - 276kc - Elliot Lake, ON, CAN
YHD - 413kc - Dryden, ON, CAN
YHN - 329kc - Hornepagne, ON, CAN
YIV - 300kc - Island Lake, MB, CAN
YJQ - 325kc - Bella Bella, BC, CAN
YK - 371kc - Yakima, WA
YK - 269kc - Castlegar, BC, CAN
YKA - 223kc - Kamloops, BC, CAN
YKQ - 351kc - Waskaganish, QC, CAN
YL - 395kc - Lynn Lake, MB, CAN
YLB - 272kc - Lac la Biche, AB, CAN
YLD - 335kc - Chapleau, ON, CAN
YLJ - 405kc - Meadow Lake, SK, CAN
YLL - 241kc - Lloydminster, AB, CAN
YMW - 366kc - Maniwaki, QC, CAN
YPH - 396kc - Inukjuak, QC, CAN
YPL - 382kc - Pickle Lake, ON, CAN
YPM - 274kc - Pikangikum, ON, CAN
YPO - 401kc - Peawanuck, ON, CAN
YPW - 382kc - Powell River, BC, CAN
YQ - 305kc - Churchill/Eastern Creek, MB, CAN - 500W
YQA - 272kc - Muskoka, ON, CAN
YQF - 320kc - Red Deer, AB, CAN
YQK - 326kc - Kenora, ON, CAN
YQZ - 359kc - Quesnel, BC,CAN
YSQ - 260kc - Atlin, BC, CAN
YTL - 328kc - Big Trout Lake, ON, CAN
YWB - 389kc - West Bank, BC, CAN
YWP - 355kc - Webequie, ON, CAN
YXL - 346kc - Sioux Lookout, ON, CAN
YXR - 257kc - Earlton, ON, CAN 400W
YY - 340kc - Mont Joli, QC, CAN
YYF - 290kc - Penticton, BC, CAN
YYU - 341kc - Kapuskasing, ON, CAN
YYW - 223kc - Armstrong, ON, CAN
YZA - 236kc - Ashcroft, BC,CAN
YZE - 245kc - Gore Bay, ON, CAN
YZH - 343kc - Slave Lake, AB, CAN
ZEG - 379kc - Edmonton, AB, CAN
ZF - 356kc - Yellowknife, NWT, CAN
ZKI - 203kc - Kitimet, BC, CAN
ZQ - 410kc - Sir Wilfred Laurier CCGS*, BC, CAN
ZP - 368kc - Sandspit, Queen Charlott Is, BC, CAN
ZRG - 414kc - Regina, SK, CAN
ZSJ - 258kc - Sandy Lake, ON, CAN
ZSS - 397kc - Yellowhead-Saskatoon, SK, CAN
ZT - 242kc - Port Hardy, BC, CAN
ZU - 338kc - Whitecourt, BC, CAN
ZVR- 369kc - Vancouver (Sea Is.,) BC, CAN
ZXE - 356kc - Saskatoon, SK, CAN
ZYC - 254kc - Calgary, AB, CAN
ZZD - 308kc - Calmar/Edmonton Int'l AP, AB, CAN
ZZP - 248kc - Sandspit, Queen Charlotte Is, BC, CAN
Z5 - 274kc - Vulcan, AB, CAN
Z7 - 408kc - Claresholm, AB, CAN
3Z - 388kc - Taber, AB, CAN
6T - 362kc - Foremost, AB, CAN
INUU - 395kc - 11/2017 (also in 2016)
EEGU - 378kc - "Key Down" - 11/2017
OTA - Off The Air, Decommissioned
* Canadian Coast Guard Ship - Sea Mobile NDB
** not counted in total received
|Henry Rogers WA7YBS © November 2007, new info added Oct.2008, Nov. 2008, Jan 2009, Nov 2009, updates Sept 2014, updates Jan 2015, update on "NO" 351kc with photo Sept 2015, updates on LW BC, 600M ham, RBA-1 rcvr Oct 2017, info on DGPS, GWEN, FCC Experimental License Grants, Nov 2017, added R-389 info Jan 2018,|
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Website Navigation Index
- WHRM History ~ Nevada Radio History ~ The KOWL XMTR ~ Full Length Articles with Photos -
Nevada Radio History - 1906 to 1930
- Wireless Apparatus, 1920s Radio and Communications Equipment ~ Full Length Articles with Photos -
M.H. Dodd's 1912 Wireless Station
- Vintage Communications & Amateur Radio Equipment ~ Full Length Articles with Photos -
Super-Pro, the R-274 Receiver
- Rebuilding Communications Equipment ~ Full Length Articles with Photos -
Rebuilding the Hammarlund SP-600
Rebuilding the BC-348 Receiver
an Authentic 1937 Ham Station
- WHRM Radio Photo Galleries with Text -
Entertainment Radios from 1922 to 1950
Communications Equipment from 1909 to 1959 - Commercial, Military & Amateur
Vintage Broadcast Equipment, RTTY, Telegraph Keys & Vintage Test Equipment
Western Historic Radio Museum
Vintage Radio Communication Equipment Rebuilding & Restoration Articles,
Vintage Radio History and WHRM Radio Photo Galleries
1909 - 1959
This website created and maintained by: Henry Rogers - Radio Boulevard, Western Historic Radio Museum © 1997/2017