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Radio
Boulevard Shipboard Radio
Receiving Equipment 1. Navy Department - Bureau of Steam
Engineering - SE-143 - National Electrical Supply
Co. (NESCO) Histories, Circuit Designs,
Operation and Performance Testing by: Henry Rogers - Radio Boulevard-Western Historic Radio Museum |
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According to RCA, the 1918 SE-143 was the first radio receiver available that performed adequately and was able to receive all types of signals whether they were from Spark Transmitters, Arc Transmitters, Alexanderson Alternators or from Vacuum Tube CW Oscillators. Surprisingly, RCA supplied manuals for the SE-143 as late as 1936. But, how could a WWI RF Tuner be in use onboard ships years after it should have been obsolete? UPGRADES! The SE-1387 and the impressive SE-1834 were especially designed, in 1922, to be used with the SE-143 (and similar Receivers) to upgrade this WWI RF Tuner into a seven-tube TRF receiver with three broadband RF amplifiers, a detector, a tunable heterodyne oscillator for CW and two stages of audio amplification. All accomplished externally with no modifications necessary other than wire-connecting these two devices to the already existing SE-143 terminals. After WWI ended, the radio receiver designs only got better with the SE-1420 Receiver that was introduced in 1919. The SE-1420 was so popular that it continued to be built as late as 1927. The SE-1420 paved the way for the incredible IP-501-A receiver that was used onboard ships and at coastal stations into the late-thirties with manuals available from RCA as late as 1938. The following examples of WWI and 1920s electro-technology illustrate how incredibly fast radio circuit designs and vacuum tube evolution were improving the communications equipment being built for commercial and military use. |
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U.S. Navy - Bureau of Steam Engineering S.E.143 - Short Wave Receiver - SN:848N - NESCO - 1918 Contract
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To allow the SE-143 to tune to VLF a Secondary Loading Coil, a Primary Loading Coil and a Tickler Loading Coil could be connected using the front panel terminals so marked. The SE-143 didn't have an onboard detector or an onboard audio amplifier,...it was an RF tuner only. The VT detector was originally provided by the Audion Control Box that was designated as the SE-1071. It provided just one tube that operated as a regenerative detector for the SE-143. There was a two-stage audio amplifier available, the SE-1000 that could also be added. If the SE-143 was operated with an external regenerative detector tube, the SE-143 internally provided the "Tickler" coil (an untuned, adjustable rotational-position coil located inside the Secondary coil) connection since the regeneration function had to provide an in-phase EM field in close proximity to the secondary coil for sufficient feedback. The crystal detector function was mainly provided for emergency situations and its inclusion into the design was a stipulation of Navy regulations. Ambiguous Tuning Range Specs Explained - The SE-143 tuning range is typically shown as 250M to 6400M (1200kc down to 47kc.) The Secondary Condenser tuning dial agrees with the 250M to 6400M range. However, the actual data plate on SN:848N indicates a tuning range of 250M to 3000M (1200kc down to 100kc.) Interestingly, the 1936 RCA SE-143 manual indicates 300M to 3200M tuning coverage (1000kc down to 95kc.) These ambiguous tuning range specifications might have been the result of the difficulty involved with adjusting the SE-143 to easily and reliably tune its full range due to the seemly insufficient Primary LC tuning range. But, with an experienced radio operator setting up the receiver, the lower end of the Primary LC tuning range can easily extend to 6400M. Usually, if the stock Primary LC versus antenna hook-up is used, the longest wavelengths can't be tuned to resonance or "peak" response using the Primary LC tuning. George Sterling's "The Radio Manual" indicates the 250M to 6400M tuning range and continues on (in the Loading Coils section) to explain how to easily change the Primary Condenser connection from the standard series LC to a parallel LC connection. The series LC presents a very low Z at resonance while the parallel LC would present a very high Z at resonance. Depending on the antenna used and the wavelength received, the parallel connection can be an advantage at lower frequencies. Although Sterling's Radio Manual information is for extending the longer wavelength end of the tuning range to function with LF loading coils, the parallel connection of the Primary LC could also benefit the tuning of longer wavelengths between 3000M and 6400M. The procedure for parallel connecting the Primary LC is simple. Just leave the PRI LOAD strap in place and connect the antenna lead wire to the left terminal of the PRI LOAD. Then jumper the ANT to GR terminals with the GR terminal remaining grounded. Now the Primary LC is parallel tuned and should respond better at longer wavelengths. |
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| Series versus Parallel Tuning for
the Primary LC
- Tuning the Secondary LC to 6400M is easily accomplished but not with
the stock connections to the Primary LC. In fact, it might be impossible
if series tuning is used on the Primary LC. I've tested the standard series LC and the
parallel LC for a comparison when using a 250' wire antenna with the
secondary LC tuned to WWVB on 5000M (60kc.) The difference is significant.
Since the Primary LC can actually be "tuned" in parallel the increase in signal
level is tremendous, at least when tuning WWVB (which is a strong
signal anyway.) When tuning to longer wavelengths starting at about
3000M or 100kc, the inability of the Primary LC to tune the antenna will
begin to be noticed and you won't be able to find a "peak" response. If
that's the case, the change the antenna hook-up so that the Primary LC
is parallel tuned. Now, finding resonance or "peak" response should be
easy.
I've found that with careful set up, using the SE-143 with the SE-1387 (Heterodyne Oscillator) and the SE-1834 (RF amp, detector, AF amp,) I can easily and consistently receive WWVB on 5000M or 60kc (over the air) using a 250' end-fed wire antenna. It's a very strong signal if the Primary LC is parallel tuned. Using an HP3312A signal generator set to 47kc with the output connected to a 50' wire laying on the floor and the SE-143 setup using the outdoor 250' wire antenna, I can actually receive that type of signal on the SE-143 set to 6400M or 47kc with the SE-1387 providing the heterodyne for easy detection (47kc is the absolute lowest tunable frequency possible since it's at the maximum C-setting on the Secondary Condenser dial when on Position 6, the maximum secondary L,...to tune lower in frequency requires Loading Coils.) At the other end of the range, 300M or 1000kc is easily tuned and, with careful set up on Position 1 and a series Primary LC connection, I was able to easily receive KNNR, a Reno AM-BC station on 1400kc or 215M. The confirmed actual full tuning range of SE-143 SN:848N is 47kc up to 1400kc or 6400M to 215M,...BUT, that tuning range is only possible IF the user is willing to switch the Primary LC from series to parallel as needed. Sterling's Radio Manual shows a DPDT switch arrangement to accomplish the series-parallel change but just moving the wires is pretty easy to do. What the Specific Controls Do - The Primary Condenser dial has a 180º scale for half of the dial and linear scales for notations on the other half. The Secondary Condenser is calibrated in wavelength and also has the "letter designations" that were used during WWI and somewhat after as specifying important wavelengths (or frequencies.) Wavelength scaling is the figure shown times 100. A logging scale is also included in the other half of the dial. The inductance switches have letter designations on the Primary LC and numbers on the Secondary LC. The scales for the TICKLER COUPLER and the INDUCTIVE COUPLER are 0 to 180 with a MIN and MAX indication at each end. The scales imply the degrees of rotation for the specific coil. The BUZZER was used as a "potent" signal generator to be used when trying to find a sensitive spot on a crystal detector. The typical battery voltage for the BUZZER is no more than 2vdc if the buzzer is in good condition and adjusted correctly. There's spark gap between the ANT and GND terminals to provide a method to dissipate static charges on the antenna (common problem at sea or in windy areas.) Two sets of terminals are for LW loading coils that, when connected, allow the SE-143 to tune lower than it's 6400 meters (47kc) lower tuning limit. Additionally, a Tickler Loading Coil could be added in series with the internal Tickler Coil by using the front panel TICKLER terminals. Various types of loading coils could be used (see vintage shipboard photo further down showing a DeForest Duo-lateral LW coil apparatus being used for VLF frequencies.) The DETECTOR terminals were provided for connecting the Crystal Detector. The eight vertically aligned terminals allow mating the SE-143 to the SE-1071 Audion Control Box. However, it's not specifically necessary to use the SE-1071. The terminals provide connections to the TICKLER COIL, AUD TEL, TELEPHONES (for Crystal Detector) and the receiver secondary LC outputs RA (grid-audion) and RE (filament-return.) The SECONDARY SWITCH allows selecting TUNED or UNTUNED with the latter routing the SECONDARY LC to an untuned coil that's closely coupled to the secondary inductance for a broad frequency response for easier tuning when using a Crystal Detector (it can also be used with an Audion detector when searching for unknown stations.) The actual "tuning" is performed using the PRIMARY CONDENSER since the secondary is "untuned." This allows the user to tune the antenna-primary circuit to allow a stronger response for the crystal detector. Then switching to "TUNED" switches out the untuned coil and allows using the SECONDARY CONDENSER to further "peak" the signal response. As mentioned, this process can also be used with an Audion detector when searching for weak or unknown stations. The DETECTOR SWITCH routes the secondary LC as necessary for either CRYSTAL or for AUDION. It's possible to use the CRYSTAL position of the DETECTOR switch to connect to an alternate type of detector rather than a crystal detector. By using terminal TEL (#75) to access the RA terminal and DET (#81) terminal to access the RE terminal when the DETECTOR switch is placed in CRYSTAL, now the Secondary LC can be connected into an alternate type of VT detector. This use of the CRYSTAL position was used later (in the early-1920s) when external RF amplifiers, heterodyne oscillators operating with non-regenerative detectors and audio amplifier stages became available. With this ability to have two selectable types of signal processing available using different types of VT detector circuits, the radio operator could, depending on receiving conditions, select a regenerative detector utilizing the TICKLER coil in the circuit, or he could select a circuit that provided RF amplifiers, non-regenerative detector, a heterodyne oscillator (for CW reception) and audio amplifiers. The radio operator would still have a crystal detector somewhere in the radio room and be able to connect it to the SE-143 if there was an emergency since this was part of Navy and Maritime regulations. |
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Cabinet Work - The SE-143 cabinet is made out of walnut stained a dark reddish-brown color. The interior has no metal shielding installed. The right side front of the cabinet has two broken pieces of wood that are the full length of the height of the side piece. I had to remove the two latch-bails to be able to glue these pieces back correctly. The bottom front section is split and broken requiring gluing and clamping. I use Franklin's Genuine Hide Glue for this type of repair. This Hide Glue is not the old type (rendered from horse hoofs and hides) that needed to be a hot smelly liquid that was quickly painted on and set-up as soon as it cooled. Franklin's is synthetic hide glue with all of the good properties and minus the disadvantages. This glue is amber colored and transparent so it looks old if it happens to show in the joint. It does take a fairly long time to set-up but the glued joint has to be clamped and let set for about an hour. For full strength the glue joint must dry overnight. Unfortunately, with these types of breaks, I have to use a combination of hand clamps and pipe clamps because of the distance between the glue joint and the back of the cabinet and because of the angle of the breaks. The need for pipe clamps is common with most cabinet repairs involving glued joints. The complete gluing took about a day to accomplish and used three pipe clamps and about half a dozen hand clamps. I do have the rare front cover for this SE-143. It has had some crude repairs done to it. The cover piece of wood was replaced with 1/2" plywood, apparently many years ago. It's stained to a color that's sort of close and has a vintage-look to it. Also, one of the side pieces was replaced and the dove-tail joints not reproduced. Instead, the "dove-tails" were cut off and the wood nailed in place. It's pretty crude. Overall, the condition is probably a little worse than average BUT, at least, I do have the top cover, which is rare to find with an SE-143 receiver. The back of the cabinet ended up missing sometime in the past. Someone cut some 1/4" birch plywood, glued two pieces in a sandwich to create a 1/2" thick, stepped-type of back that fits okay. It wasn't stained and finished however, just left bare wood. Luckily, it's mounted with only four screws, so it can be easily removed for rework and staining. I have lots of red mahogany stain but I think I'll have to mix some golden oak in to get the correct color. I'll also work on getting a better fit, touching up the edges so they don't look like plywood and then stain to match. For the time period and that fact that most of the SE-143 receivers were expected to be "at sea" I'd expect varnish was the original finish used. However, after 100 years, there's not too much original finish left now. NOTE: Close examination of the SE-143 cabinet with this make-shift cover removed seems to indicate that perhaps there never was a rear cover. I can't find any residue of glue, there are no nail or screw holes. I can't imagine that there wasn't a back to the cabinet,...I just can't find any evidence that shows how one would have been installed. However, since this make-shift cover fits and after staining it matches fairly well, I'm going to install it. If I find out later that SE-143 cabinets didn't have back covers, it can easily be removed, though a side-benefit of this back cover is that it significantly strengthens the cabinet joints.
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VT detector and
Regeneration Test - The SE-143 was normally used as an RF
Tuner ahead of a Vacuum Tube detector. Using a Crystal Detector was
generally only for emergencies where no power was available to operate
the tube or tubes. The SE-1071 was the Audion Control Box and it
interconnected with the eight vertically aligned terminals on the right
side of the receiver.
The Hook-up - To operate the SE-143 with a VT requires a vintage triode tube and tube socket, an adjustable filament voltage source and another adjustable voltage source to provide plate voltage. A couple of things to observe are RE is connected directly to F- and B- is connected to F+. The 'phones are connected to the AUD TEL terminals. The plate voltage B+ is also connected the lower AUD TEL terminals that has one lead of the 'phones. The top AUD TEL terminal has the other lead of the 'phones but also has a jumper to connect the upper AUD TEL terminal to the lower TICKLER terminal (the use of the AUD TEL terminals was later found to be unnecessary.) Then the upper TICKLER terminal is connected to the Plate terminal on the tube socket. The jumper has to be externally installed because this connection was actually made inside the SE-1071. Additionally, the connections to 'phones, Tickler Coil and VT plate were all internal to the SE-1071 and controlled by a switch that selected OSCILLATOR (Regen going through the Tickler coil) or DETECTOR (Tickler coil shorted for a non-regenerative detector.) The Ship's Generator as a B+ Source - Interestingly, the SE-1071 could provide B+ plate voltage either from storage batteries or it could be provided by the ship's +125vdc generator. There was an adjustable potentiometer to adjust the plate voltage but the +125vdc ship's generator only has a couple of filter chokes inline inside the SE-1071, so one has to wonder exactly what the plate voltage was and what the value of the variable resistance was (neither are indicated anywhere on the SE-1071 schematic. Sterling's Radio Manual indicates the resistance was 30,000 ohms. Plate voltage could be adjusted between +60vdc and +90vdc if the ship's generator was used.) There's a switch and terminals provided for selecting either storage batteries or the ship's generator as a B+ voltage source. If the SE-1000 Audio Amplifier was also to be used, then the ship's generator couldn't be used and only storage (or dry) plate batteries could be used. When using B batteries, the adjustable plate voltage function is disconnected. Vacuum Tubes Available in 1918 - Another consideration is the actual type of vacuum tube used in the SE-1071. In 1918, a Moorhead "ER" Electron Relay tube might have been used or perhaps a Western Electric VT-1. Other tubes specified in Sterling's Radio Manual are the Western Electric W-933 or the General Electric CG-890. Both of these tubes have 1 amp filament requirements indicating a pure tungsten filament and a plate voltage specified from +20 up to +60vdc. The specs of those two types of VTs are similar to the UV-200 or UV-201 but those tubes weren't introduced until around mid-1921, along with most of the other consumer-broadcast radio vacuum tubes (although the UV-200 or UV-201 tubes weren't available in 1918, they can, of course, be used today.) The WE-215A tube might have been available in 1919, but the special socket required for that tube seems to eliminate it for use in the SE-1071. The most likely VT used in 1918 would have been the WE VT-1 or the Electron Relay (there were several manufacturers for the ER type of VT during WWI) or those specified in Sterling's Radio Manual. For initial testing of VT detector and regeneration, I'm going to use the UV-200. What Doesn't Work - My first attempt with the UV-200 had clip-leads improvised with very long lead connections and didn't follow what the SE-1071 schematic indicated. As expected, while this lash-up worked fine as a non-regenerative Detector, I couldn't get the Detector to break into oscillation. I tried using a UX-201A and a Type-30 with the same results. I tried plate voltages from a low +15vdc up to +70vdc and could never get any of the Detector tubes to oscillate. What Does Work - Finally, I decided to follow the SE-1071 schematic and hook-up closely, in fact, almost exactly. I used wire connections that were as short and direct as possible. I connected one lead of the 'phones to the lower TICKLER terminal and the other 'phones lead to +45vdc. The upper TICKLER terminal was connected to the detector tube plate. Connecting to the AUD TEL terminals isn't necessary. I think the non-oscillating problem was that, initially I had connected the RE terminal to F+/B- but, the SE-1071 schematic shows RE connected directly to F- battery terminal. I made the change so that the F- connection agreed with the SE-1071 schematic. I replaced the 250pf grid blocking cap with a 500pf. The grid blocking cap is a switch-selected value in the SE-1071 and 500pf is in the middle of the range of capacitors. I changed the grid-leak resistor from 1.2meg ohm to 680K (600K on the SE-1071 schematic.) I connected the grid-leak to B- as indicated on the SE-1071 schematic rather than in parallel with the grid blocking cap. I installed a 0.004uf capacitor from the junction of the 'phones and the Tickler coil as indicated on the SE-1071 schematic. It's a switch-selected value but the capacitor values aren't shown on the SE-1071 schematic. The capacitor shunts any RF on the 'phones to B-. Following the SE-1071 schematic and the hook-up exactly as shown resulted in tremendous regeneration capabilities with being able to easily adjust the TICKLER COUPLER for detector oscillations. In actually operating the SE-143 and testing various wavelengths of reception, I've discovered that it helps to have the filament voltage adjustable. The B+ can be a fixed value. I use +45vdc on the detector plate. I found best improvement was when I eliminated the clip-leads and installed wires that were soldered to lugs that were then installed to the tube socket terminals. Where the wire went through the hole in the SE-143 terminals I tinned wire end to make as good of a joint as can be expected from thumb-nut terminals. Also, making sure that the RE terminal connected directly to F- and that the filament adjustment pot was connected from F- on one end and to F- at the tube socket on the other end. With careful wire connections that followed the SE-1071 schematic, I was able to tune down to 5000M (60kc) and could easily maintain an oscillating condition for the regeneration. |
| Long Wavelength Loading Coils - Necessary below 50kc - If it was necessary to receive stations transmitting on wavelengths longer than 6000M (50kc) and the SE-143 was the only receiver available, then additional inductance in the Primary, Secondary and Tickler coils had to be connected to the appropriate front panel terminals. With the additional inductance, the Primary tuning can become ineffective at longer and longer wavelengths (although the antenna used is a very important factor at these lower frequencies.) Both vintage photos (below) of SE-143 stations show that LF Loading coils were in place. The NAA Station used massive inductances with tapped switches. The USN Shipboard station used a DeForest Duo-lateral Tuner with LF plug-in coils. Sterling's Radio Manual gives the number of turns for the specific plug-in honeycomb coils used in the DeForest Duo-lateral Tuner (and the plug-in DeForest-type coils usually have a label on the inside indicating the number of turns in the coil.) On average, 750 to 1000 turn coils can be used for the Primary and Secondary Inductances and a 600 to 750 turn coil used for the Tickler. When setting up for using Loading Coils, Position 6 should allow the SE-143 to tune slightly below 50kc (approximately 47kc) without the Loading Coils connected. I believe that if LW loading coils were used, the operator would place the Secondary Inductance switch to position 6 and then connect the LW coils. The LW coil setup should have a method to "short" each of the coils to remove them from the circuit (like the shorting straps do for the Primary and Secondary L and, since the Long Wavelength Tickler coil is connected in series, shorting it is also proper to remove it from the circuit.) When the LW coils are placed into the circuit, that would then allow tuning to wavelengths longer than 6000M (50kc) with the Secondary Inductance in position 6. Of course, adding the LW Loading Coils will affect the total inductance and thus all tuning ranges would be effected. However, with LW Loading coils installed, the receiver's standard Primary and Secondary total L is very low when compared to the large inductance of the loading coils, so the action of changing the L switches on the SE-143 doesn't have too much of an effect on tuning (the tuning is all in the variable condensers.) With a setup for LW coverage at wavelengths longer than 6000M, then the selection of position 6 allows the user to add markers (pencil notations) to the Secondary Condenser tuning dial in the blank area just above the position 6 scale These pencil notations could be used to set the Secondary Condenser dial for the desired wavelength. Sterling's Radio Manual also shows a method to connect the Primary Condenser in parallel to the Primary Inductance for better LW tuning (it depends on the antenna used. It's easily accomplished by just using the PRI LOAD COIL terminal for the antenna input and shorting the ANT to GND terminals) Sterling also indicates that the TICKLER coil might have to be reverse-connected when using LW Loading Coils and operating on long wavelengths although he's not specific if the reversal is for the Tickler Loading Coil connections or for the SE-143 Tickler terminals (experimentation would be required.) From examining vintage photos it seems obvious that LW Loading Coils were common in the typical SE-143 installations and there certainly were a lot of stations operating in the part of the spectrum during the post-WWI time period. All USN Alexanderson Alternator Transmitters were operating below 50kc. Many other VLF stations were used for "Navy Radio Central" type communications to various fleets. Time signals, some navigation uses, etc., were also found in the VLF (the frequencies below 30kc) part of the spectrum. Loading Coils were definitely going to be necessary if the SE-143 was the only receiver available in the ship's radio room. |
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Adding a Single Stage of Audio Amplification - I have a Pilot Radio Redi-Blox Single Stage Audio Amplifier from about 1930 that I use with the SE-1420 receiver to boost the output of the detector tube for that receiver. It provides enough audio level to actually hear very weak signals, like NDBs, using headphones. I've also used this audio amplifier with the Spherical Audion Receiver with good results. To hook-up the single-stage AF amp, the primary winding of the input transformer is connected to the two points where the headphones were connected,...to the lower TICKLER terminal directly with one end of the primary and the other TICKLER terminal connecting to the detector plate. The other transformer primary terminal is connected to detector B+ with the voltage being +45vdc for a UX-201A tube. For the Audio Amplifier tube I use a UX-201A tube and use +90vdc on the plate and that is routed through the 'phones before going directly to the amp's plate terminal. The F+ and the B- are connected to the B- terminal of the A-B power supply (B- is connected to F+.) Audio Output can be controlled by the tube filament voltage. A 1920s Horn Speaker could be used on just about any of the AM-BC stations. Hearing NDBs (the few left, anyway) will require 'phones and listening during LW Season (between the Autumnal Equinox and the Vernal Equinox - definitely not in mid-July.) The NDBs are MCW signals but having the detector oscillating will make finding the NDB's carrier easy. Just tune for zero-beat and the MCW tone will be easy to copy. The photo to the right shows the SE-143 after cleaning and installation into the repaired cabinet. The white and black leads near the Buzzer are the Antenna and Ground connections. The antenna is one half of a Collinear Array or about 250 feet of wire that's end-fed and the ground is a combination of the house ground and a large counterpoise. The power supply is a homebrew, active regulated type with full switched metering. I designed and built this A-B-C eliminator in the late-1970s. Filament supplies are +1.5vdc, +4.5vdc and +6vdc. B supplies +22.5vdc, +45vdc, +67.5vdc and +90vdc. The C bias supply is -4.5vdc. Since the A supplies aren't adjustable, I've connected an external filament rheostat (0 to 10 ohms adjustable.) I've eliminated as many of the clip-leads as possible. Most wires are soldered to lugs that are then installed to the terminals. This careful setup has resulted in a greatly improved performance. Of course, the Audio Amplifier helps, too. |
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| Over-the-Air Reception Testing
- As can be seen in the photo above-right, I have the SE-143 tuned to
5000M or 60kc and I'm receiving WWVB quite well. The detector is oscillating so
sensitivity is excellent. The strongest signals in LF around here are
the Loran-E Master Station "M" located in Fallon, Nevada running 400KW on 100kc, then
there's an unknown MSK station (possibly USN) around 75kc that's pretty strong and then WWVB
on 60kc. Going lower in frequency, that would be lower than 50kc, would
require a LW Loading Coil setup (I'm working on constructing one
using a DeForest Duo-Lateral Tuner and plug-in LW coils.) The next strong stations are the Navy Sub-Comm
MSK VLF stations transmitting around 24kc. There are five large USN VLF
Stations that transmit at incredible power levels to immense antenna
arrays so their signals are formidable and easily received. Also, JJY is
Japan's LF Time station on 40kc. JJY isn't a terribly powerful signal
here near the West Coast of the USA but just before sunrise it's easy
to receive (JJY 40kc runs 10KW.) On 12kc, 14kc and 15.6kc, the Russian RSDN-20 Alpha Nav
transmitters operate. These are also easy to receive since they run
500KW to large array antenna systems. There are three major Russian
Alpha transmitting sites and three other support sites. All are in
central Russia. The 12kc RSDN-20 signal is the lowest frequency
identifiable signal that's fairly easy to receive. Since the SE-143 has absolutely no shielding, when the regenerative detector is oscillating there is some "hand-capacitance effect" on the TICKLER COUPLER control, on the SECONDARY INDUCTANCE SWITCH and to a lesser extent on the SECONDARY CONDENSER and the INDUCTANCE COUPLER controls. Since these components are part of the oscillating detector there's an associated EM field around the components and when the hand is on the control knob there will be a slight de-tuning because the hand adds "capacitance to ground." This is a common effect with unshielded regenerative receivers. The SE-1420 solved this problem by entirely shielding the front panel and the cabinet along with a divider shield between the Antenna Tuner and the Secondary LC. Summer conditions are terrible for MW and LF reception,...but I thought I'd try to at least receive the NBD MOG 405kc located in Montegue, California. It's the closest NDB to Dayton Valley, Nevada that's still in operation with a distance of about 150 miles. I pre-tuned the SE-143 using a signal generator for the marker signal. With a slight amount of "peaking" I was able to hear MOG very well. Time of reception was 2135hrs PDT on Jul 14, 2026. I tuned around by didn't hear any other NDBs (and that's not particularly surprising for mid-July listening.) |
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| During testing the SE-143 with the single-stage audio amplifier, I ran a test on the SE-143's full tuning capabilities. I was very surprised to tune in KNNR-Reno on 1400kc. That's 215 meters, a somewhat shorter wavelength than the 250 meter spec (or 1200kc.) I also was at the other end of the tuning range and was able to go to 6400 meters or 47kc. This LF testing was done mainly using a signal generator loosely-coupled to the antenna so I could hear any transmitting signals and could also zero-beat to confirm frequencies. I was mainly testing to try to figure-out what the "letter" designations on the Secondary Condenser indicated. The results of that test follow,... |
| Letter Assignments for Wavelengths
as Shown on SE-143 and SE-1420 Secondary Condenser Dials - WWI to 1921 I've searched and searched the Internet (and AI) and I've never found anything on these "letter to wavelength" assignments although they were obviously in use during and after WWI by the U.S. Navy and probably the U.S. Army Signal Corps and the U.S. Coast Guard. I've always been curious why the letters were present on these dials. They must have been to ease the tuning difficulties when trying to set up the receiver to specific wavelengths (all those numbers that required multiplying by 100 for the actual wavelength must have been confusing to neophyte radio operators.) The combination of a specific letter plus (maybe) the numerical indication on the 0-180 scale would have been an accurate "set up" method that probably referenced some sort of chart that gave all of the proper control settings for the receiver to operate correctly on a desired wavelength using a specified antenna. I've never seen a copy of this type of chart, or even heard of one,...a "letter wavelength reference chart" isn't mentioned in any of the wireless books that I've seen. Nothing is mentioned in Sterling's Radio Manual. Another hint at their use is that the letters are on the Secondary Condenser Tuning dials of the SE-143 and SE-1420 BUT the letters aren't on the Secondary Condenser tuning dial of the IP-501-A, a commercial receiver. That would seem to date the use of the letters from WWI to maybe a short while after that, about 1920 or so. By 1922, the letters weren't needed and weren't included on the Secondary Condenser tuning dials. I decided to do a test to find out what wavelengths the letters indicated. I don't think any definite answers will be forthcoming but it would be interesting to see what wavelengths were involved.
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| Renewed Usability for the SE-143 for
the 1920s
- The SE-143 "aged" quickly and, by 1920, other more advanced designs
were being developed and introduced into the Navy. Possibly, the need
for specific types of detector tubes became a problem as vacuum tubes
evolved (although Sterling's Radio Manual gives the specs for using
UX-201A tubes implying the continued use of the SE-1071 into the 1920s.)
The SE-143 was
still an excellent RF Tuner that could still provide very selective
tuning so newly designed "add-on" units were introduced
around 1922. These add-ons enhanced the performance capabilities of the
SE-143 allowing the Navy to continue using it, in combination with some
of the external devices, to modernize the performance and that allowed
the SE-143 to continue on as a shipboard tuner-receiver for several more
years. Two of these types of "add-ons" are profiled in the following
section. NOTE 1: Where did this SE-143 come from? I received a 'phone call from Ethan, the owner of Ham & Hi-Fi in Sparks, Nevada, saying "I have something here that's right up your alley!" He was right, of course. I had to think about it for a couple of weeks due to the condition problems. Ethan had texted me a few photos of the receiver that showed some of the issues (that looked worse than they actually were.) When I decided to go ahead with the purchase, then Ethan was out of town for about three weeks. Finally, after our mutual delays, I was able to purchase the SE-143 on June 30, 2026. Ethan told me that the SE-143 had been stored in Santa Rosa, California. NOTE 2: The U.S. Navy created the Bureau of Steam Engineering in the 1860s as a technical engineering department, initially to help with the transition from sailing ships to steam powered ships. Later, new technologies like electrical and wireless engineering were added. In 1920, the name was changed to Bureau of Engineering and, in 1940, it was renamed Bureau of Ships. NOTE 3: Although I've seen some written references to an "A" version of the SE-143 (supposedly the NESCO builds,) I really haven't found any early (contemporary to the SE-143 production and use) that specified an "A" version. Sometimes information that's derived from Procurement Books will have ordering numbers that are specific to what and where items were purchased from. This type of ordering information isn't always on data plates or referenced in operating manuals. NOTE 4: The "Short Wave" designation is relative to the time period and to the typical frequencies that the Navy used during WWI. A more modern designation would be that the SE-143 is an LF/MW RF Tuner-Receiver (Low Frequency or LF is from 30kc to 300kc and Medium Wave or MW is from 300kc to 3000kc.) |
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SE-1387 - R.F. Driver
(Tuned Heterodyne Oscillator) Navy Department -
Bureau of Engineering
- National Electrical
Supply Company (NESCO) - 1922 Contract Post-WWI Radio Improvements - As radio evolved post-WWI, the need for new radio equipment was offset by the reduced post-war Navy budget that limited extravagant purchases to a certain extent. This resulted in the newest and largest Navy ships being prioritized for the newest equipment while an older or smaller ship would have to utilize older, maybe even WWI-era, radio gear. Improvements were much easier to fit into the budget and, as radio evolved, these external circuit additions allowed older radio equipment to be updated to provide usable service. Most peripheral equipment came in the form of RF amplifiers to be used ahead of a regenerative detector provided stronger signals and antenna isolation. Audio amplifiers to provide stronger post-detection signals to drive multiple outputs. Devices for interfacing specialized antennas such as loop antennas for direction finding. By 1922, there were several types of "add-on" devices available to improve the performance and usability of older receivers. This SE-1387/SE-1834 combination (shown to the right) was specifically for the SE-143, IP-500, SE-1220 or other similar RF Tuners. Although the SE-1387/SE-1834 combination appears to be a receiver, it's far from being a "complete" receiver. The SE-1387 is actually a "tuned" Heterodyne Oscillator and the SE-1834 is almost a complete receiver but it's minus any selective RF tuning capability. Both units have to be used with RF Tuner sets like the SE-143. Unlike the earlier shipboard radio equipment that were housed in wooden cases, perhaps lined with metal shielding, the SE-1387/SE-1834 combo was built with an aluminum front panels and housed in an aluminum case. Both units are installed into individually shielded compartments to prevent any stray coupling between the units. The size of the metal cabinet matches the height of the SE-1420 so it's somewhat smaller than the enormous cabinet of the SE-143. Most Navy installations would place the "add-on" units on top of the SE-143 and wires interconnecting the units were routed around the panels to access the needed terminals. Although this particular example has the SE-1387 and the SE-1834 housed into a single cabinet, most vintage photographs show individual "add-on" units were single-function devices that were housed in their own individual cabinets (see the vintage photos further below.) |
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The SE-1387 Details - This device was called an R.F. Driver, though nowadays that's an unfamiliar term that doesn't describe the circuit's true function. During the WWI era, Wireless Specialty Apparatus Company produced a device called an "Eaton Oscillator" that when connected to a tunable LC would provide a constant oscillation for detecting undamped waves (a Continuous Wave signal.) By adding a few parts, the Eaton Oscillator became the "Eaton Circuit Driver" that performed as an Eaton Oscillator but also could produce an output from a damped wave via a buzzer that could "drive" a wavemeter for calibration. At the time the SE-1387 was designed, the "RF Driver" term was probably used because, while it didn't directly use the secondary LC, it was used to "modulate" a continuous wave signal to produce an audible heterodyne, something like the Eaton Circuit Driver but acting as a much more versatile "heterodyne oscillator." The SE-1387 tunes from 125M up to 30,000M (2400kc down to 10kc.) It uses a single WECO 215A tube that's designed to function as a tunable RF oscillator and, when connected in series with the SE-143's RE connection to the VT detector, it provided an electro-statically and variably-coupled RF oscillator that when tuned to the RF Tuner's operating frequency would provide heterodyne action (a beat note) for CW reception from Arc transmitters, Alexanderson Alternators and Vacuum Tube transmitters. This type of on-frequency heterodyne action allowed reception of the CW mode without requiring a self-oscillating detector (a regenerative Autodyne detector.) The advantage of using the SE-1387 was it's consistent ability to provide a heterodyne tone regardless of the received frequency. Using a regenerative detector set up for self-oscillation works quite well but its adjustment needs are constant and in some cases, due to antenna loading or plate and filament voltages used, a regenerative detector won't oscillate. With the heterodyne oscillator, a beat note could be set-up at any frequency the receiver was tuned to. These types of heterodyne oscillators had to be tuned to the received frequency since there was no down-conversion of the tuned frequency as would be found in later superheterodyne receivers where the BFO operated at the Intermediate Frequency of the receiver and was capacitively-coupled into the detector stage. Later, this RF on-frequency heterodyne reception method, when mechanically coupled to the receiver's main tuning function, was referred to as a "Tracking BFO" and it was employed in many types of shipboard VLF, LF and MW TRF CW receivers up through WWII. |
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| The RECEIVER terminals route the SE-143 RF Tuner output
(RA)
directly to the GRID INPUT of the SE-1834's RF amplifiers. The SE-1387 (oscillator)
output is from the variable coupling coil inside the unit that is
connected in series between the SE-143's RE terminal and the lower
AMPLIFIER terminal that connects through an adjustable wire-wound
resistance to the B- connections within SE-1834, the STABILIZER control
(this is an "implied" connection based on the terminal layout.) The Coupling Coil adjustment should be placed so that the
letters on the COUPLING control nomenclature matches the letter of the
tuning range selected. From that setting of the COUPLING, the output can
be adjusted by slightly varying the Coupling Coil position to provide
sufficient heterodyning to the SE-1834 but to not overwhelm a weak CW signal. In simple terms, the tuned LC from the SE-143
is connected directly to the SE-1834's WE 215-A RF Amplifiers and the RF
Driver provides a heterodyne at the received frequency for CW reception
from VT, Arc or Alternator transmitters.
For Spark or Radiophone reception the SE-1387 could be turned off (turn
the INCREASE pot fully CCW - like turning off the BFO.) Shown in the photo to the right is the "Eaton Circuit Driver" built by Wireless Specialty Apparatus Company. The Eaton Circuit Driver was an Eaton Oscillator to which was added a tube socket, an amp meter, a buzzer and a filament adjustment pot. Like the standard Eaton Oscillator, the Eaton Circuit Driver was connected into the secondary LC of a tuner to provide a constant oscillation that didn't depend on the tuned frequency. The "Undamped" selection would have this device perform as the normal Eaton Oscillator. The "Damped" selection added the buzzer to the circuit, apparently "driven" from the received signal to produce a buzzer-modulated signal for wavemeter calibration purposes. The vacuum tube pictured is probably an Atlantic-Pacific ER or a Moorhead ER. This photo is from "Design Data for Receivers and Transmitters" by Milton B. Sleeper, 1922. |
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The SE-1834 Details - This is essentially a complete receiver minus any selective RF tuning. It uses six WECO 215-A tubes. The three stage RF amplifier uses three broadly-tuned RF transformers with their fixed-frequency ranges selected by the four position front panel switch (WAVELENGTH.) Each RF coil assembly has four RF transformers (primary and secondary windings) that are actually "iron core" transformers. The range of operation is 125M to 30,000M (or 2400kc down to 10kc in four ranges.) The amplified RF output is routed to a grid-leak detector tube that uses a glass grid resistance cartridge. At the time, in 1922, it was common for only the grid capacitor to be used and a grid leak resistor wasn't used. If that's the design in the SE-1834, then all four of the glass plug-in cartridges would have been small value capacitors. If the SE-1387 RF Driver/Heterodyne Osc. is used, then the SE-143's Tickler coil doesn't need to be utilized and the strap between the two "TICKLER" terminals is installed. If just the SE-1834 is used, then the TICKLER strap is removed and two wires are installed to connect the SE-143 TICKLER terminals to the SE-1834 TICKLER terminals. The connection allows the SE-1834 Plate voltage to be routed through the 1st AF transformer primary to one of the TICKLER terminals, then to one of the SE-143 TICKLER terminals, through the SE-143 Tickler coil, back to the second SE-143 TICKLER terminal and back to the second SE-1834 TICKLER terminal to the Detector plate. There was a glass tubular small value capacitor installed in clips that connected the interstage transformer side of the TICKLER terminals with the other clip connected to A+/B- to shunt RF off of the interstage transformer primary. |
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| The complete setup
using the SE-1387/SE-1834 Combo
would have SE-143 RF Tuner operating with three
stages of broadly-tuned RF Amplification, a
grid-leak detector with the SE-1387 providing a CW heterodyne oscillator (manually
tuned on-frequency heterodyne oscillator) and
then two stages of transformer-coupled Audio Amplification. By turning
off the SE-1387, the SE-143 operates as a standard TRF receiver and can
demodulate signals from spark transmitters or Radiophone signals. Fellow LW enthusiast, Dave Samson, gave me this SE-1387/SE-1834 Combo about six years ago, in August 2020. Dave shipped it from his QTH in Western New York out to Nevada along with a FTC/Mackay RC-123. When I inspected the unit, the first thing I noticed was that it used WE 215-A tubes and all seven tubes were gone. I didn't have any WE 215-A tubes left. I had sold most of my collector tubes,...to a tube collector,...and the WE215-A tubes were part of the sale. I did a visual inspection through the two top lids but never took the two units out of the cabinet. That resulted in an assumption that the SE-1387 and SE-1834 were some type of RF amplifier. Not quite six years went by and I then acquired the SE-143 receiver. In some way, I knew that the SE-1387 and SE-1834 required an RF Tuner like the SE-143. That piqued my interest enough to disassemble the unit and see exactly what it was supposed to do. The Interconnection and Operation - The SE-143 RF Tuner was directly connected to the SE-1834's three stage, RF transformer-coupled RF amplifier by connecting the SE-143 RA and RE terminals to the RECEIVER terminals on the SE-1387. It was mentioned in the SE-143 manual that since the RA wire is a "grid connection" it had to be isolated, as much as possible, from other wires ("not bunched with the other wires" was the terminology used.) However, note that the SE-1387 terminals does provide a grounded SHIELD terminal implying that the RA/RE SE-143 connection should use a shielded cable. Internally, the RECEIVER terminals connect directly to the AMPLIFIER-GRID terminals and are "strapped" to the GRID INPUT of the SE-1834. This allowed the SE-143 a direct connection via its RA terminal to the first RF amplifier grid. The SE-143 Secondary LC ground-return is routed through the pick-up coil in the SE-1387 to allow the heterodyne oscillator to modulate the incoming signal to the SE-1834 RF amplifier grid (if the SE-1387 is powered-up.) Since the heterodyne is modulating the ground-return, there is a wire-wound resistance that's adjustable to "stabilize" the actual heterodyne versus signal ratio. The actual practicality of this connection relies on the oscillator coupling coil having a low enough impedance and that the oscillator has enough pk-pk voltage output to overcome the losses of this type of hook-up. As mentioned, this hook-up is implied by the location of the terminals and, without any documentation, an actual functioning interconnection has to be determined by experimentation using operational equipment. Testing has shown that this hook-up works quite well. The RF amplifiers were broadly tuned via three RF transformers that provided four broadly-tuned ranges. This is essentially also where the incoming tuned radio signal was heterodyned with the SE-1387's variable-coupled oscillator output to allow detecting CW signals from VT, Arc or Alternator transmitters. The output of the 3rd RF amplifier stage was then routed to the detector stage. The output of the detector was routed to a two-stage, transformer-coupled audio amplifier. The audio output was routed to the TEL. terminals. Total gain was controlled by the filament voltage control and by the STABILIZER control. The purpose of the switch RADIO-AUDIO/AUDIO is to allow all filaments to operate in the RADIO/AUDIO position and turns off the filaments to the Detector tube and the two AF amplifier tubes in the AUDIO position allowing just the three RF amplifier tubes to operate (although this seems opposite of the expected function, measuring the continuity confirmed that the detector and audio tube filaments are turned off in the AUDIO position. However, the nomenclature might imply using only the SE-1837 RF amplifiers ahead of the receiver's regenerative detector and audio stages.) The STABILIZER control is a wire wound resistance of the SE-143 RE connection terminal (secondary tuned LC ground return) to the B- line. The FILAMEOSTAT adjusts the filament voltage on the WECO 215-A tubes (set to 1vdc fil voltage.) For use of the SE-1387/SE1834 combo, the TICKLER terminals have the strap installed and the AMPLIFIER-GRID INPUT straps are also installed. If just the SE-1834 was used with an SE-143 RF Tuner, it would be possible to remove the TICKLER strap and use the TICKLER connections on the receiver for a regenerative detector. The RA-RE connections on the SE-143 would then be connected to the SE-1834 GRID INPUT directly. Again, these are implied connections. An actual functioning hook-up has to be determined by experimenting with operational equipment. There was an SE-1834A version that eliminated the filament voltage meter (shown in two of the vintage B&W photos further below.) The Western Electric Co. 215-A tube
- WECO 215-A tubes, also known as VT-5 or D-80039, are very similar
internally to the WD-11 tube. However it's quite probable that the internal design of the later WD-11
that was used in Westinghouse-RCA battery operated Broadcast consumer radios from
1922 up to 1925 was actually based on the 215-A since Westinghouse and
AT&T (Western Electric) were cross-licensed in the GE-RCA "Radio
Group." The
215-A tube envelope and base are significantly smaller than the WD-11.
The tube socket is
unique and only fits the 215-A. Filament specs are 1.0vdc at .25A (WD-11
is 1.1vdc at .25A.) If the filament structure is like the
WD-11/WD-12, then the 215-A uses an iridium-platinum ribbon that's
oxide-coated. The 215-A behaves like a WD-11 in that filament emission
takes place at a very low temperature and low current level (much
lower than the .25A spec.) Most of the time, the 215-A filament isn't
really incandescent at all but the emission is at specifications. In a
day when a typical UV-201 tube required 5vdc at 1amp and the pure tungsten
filament incandesced like a 5 watt lamp, the 215-A and the WD-11 behaved
quite differently with many users unnecessarily increasing the filament
current up to the point of filament incandescent visibility with disastrous results. Plate voltage maximum is +100vdc though usually
the tubes are operated at +40vdc to +60vdc. The amplification factor is
typically about 5 but could go up to 7 or 8 at higher plate voltages
and if the tube has good emission. The 215-A tube was only used for a
short time and was commonly found in the Western Electric Broadcast
Monitoring Superheterodyne Receivers, like the 3-series and 4-series,
also other WE BC monitors and apparently in a hearing testing device. Its common use was in the
period of 1921 up to about 1928 although there are some indications that
the Signal Corps had some use for VT-5/215-A tubes as late as the
early-1940s. Although the WD-11, WD-12, WE239A and, the more
modern replacement, the RCA 864 all have almost identical specs as far
as the tube elements and function, the physical structure of these
electrically-similar tubes is completely different. For initial testing,
since I sold my collector tubes years ago that had included five good
215-A tubes, I'm going to have to buy seven of them,...ouch! The WE215-A
is relatively inexpensive but the
WE239-A is astronomically priced (WE tube dealers,...and for an anemic
triode with an amplification factor of 5???) WD-11/WD-12 tubes
seem to be somewhat fragile because most of the ones I've found had open
filaments. I'm going to use the 864 tube for initial testing. It's a
little more stoutly built and seems to function okay as a substitute.
It's a moderately priced tube but I have several of them that didn't get
included in the collector tube sale. I only used the 864
until I actually had a WE 215-A tube to use.
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Photos of Typical Vintage SE-143 Setups with Various "add-ons" Vintage photographs of radio stations are always interesting but they are even more interesting if the equipment in the photo can be identified. I've provided as much information as I can as far as recognizable equipment, the frequencies being used and the various "hook-ups" being used. These three photographs are just about the best at showing a lot of 1918 to 1925 equipment that is in an actual working environment and with the radio operator present. The first photo is an "at work" shot that shows the radio operator doing his job. It's a real impromptu photo that is slightly over-exposed and the operator moved his head during the exposure (but he didn't move his writing hand,...hmmm.) The second photo is a "posed" photo that has a lot of equipment shown but it looks like the operator is not actually "working the equipment." However, this photo was taken with an excellent camera lens, it's superbly focused and, when the original is enlarged, the year on the calendar on the wall can be read. The third photo is a "posed" photo that was probably intended to show the type of equipment being used at NAA at the time of the photo. It's a lot of nicely focused gear and when the original is enlarged the data plates on the equipment can be read. |
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U.S. Navy Station NAA - Ft. Myer-Arlington, Virginia The photo to the left shows a standard SE-143 set up with the SE-1071 Audion Control Box and the SE-1000 Two-Stage Audio Amplifier. These two accessories were the most commonly used accessories for the SE-143, especially towards the end of WWI and immediately after. On the right side of the table is another SE-1000 and SE-1071. The LW Loading Coils are quite large in this setup. These coils appear to be "single layer" wound coils rather than "bank wound" or "honeycomb" coils which would be noticeably smaller in size. These LW Loading Coils have a set of tap switches in front of the coil to allow selecting various taps on both the primary and secondary. It's difficult to tell if the coupling can be changed but the reduced size of the upper coil seems to imply that it can slide into the lower coil and therefore increase the coupling. The coil assembly mounted to the wall is probably an antenna coupler. The lower area under the desk riser appears to have what looks like individual variable condensers but it's unknown exactly what their function would have been. Note that the SE-143 is tuned to a rather high frequency. It looks like about 400kc. This is a "non-posed" photo since the radio op moved his head during the exposure. Note the over-exposed ceiling lamp. Even though the lighting and focus are not very good, this is an incredibly valuable historical document showing how radio equipment was set-up post-WWI. Photo date is probably about 1920. This photo is all over the Internet but I got it from navy-radio.com NOTE: Navy Radio Station NAA was built in 1912. The station house is still used today by the Navy for administration work. The incredible 600 ft tower that was flanked by two 425 ft towers (called The Three Sisters) were razed in 1941 due to their proximity to the Washington D.C. airport. All radio equipment and communications were moved to USN Station NSS at Annapolis, Maryland |
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U.S. Navy Shipboard Radio Room - 1920s The photo to the right shows part of a Navy shipboard installation (note the open porthole to the upper left of the photo.) This installation is using the SE-143 and on the top left of the receiver is the SE-1387 RF Driver (or a similar type like the SE-1372,) then a duo-lateral LF loading coil assembly (looks like a Remler Type 400) and an SE-1834A (no filament meter so it's the "A" version) on the far right. Note that the SE-143 is set to "CRYSTAL" on the Detector Switch. It's possible to setup the SE-143 to connect to two different signal processing circuits selected by either CRYSTAL or AUDION using the front panel switch on the SE-143. The setup could use AUDION to route the Secondary LC from RA and RE terminals to the Heterodyne Oscillator and through its terminals to the SE-1834A RF amp, Detector and AF amplifier. A second setup could be selected with CRYSTAL with the connections to TEL 75 and DET 81 terminals to access the Secondary LC and then route these wires to the SE-1834A as a RF, Regenerative Detector and AF amplifier (and not using the Heterodyne Oscillator.) The external switches would connect or disconnect the TICKLER terminals on the SE-1834A as needed. In essence, using the CRYSTAL and the AUDION switch allows the SE-143 to work with two different setups, e.g., regenerative detector in one position and non-regenerative detector with heterodyne oscillator in the other position (of course, with this type of setup, Maritime regulations would require that a Crystal Detector be available somewhere in the Radio Room.) The tuned frequency appears to be fairly high as indicated by the where the Inductance switches are placed. A close look at the SE-143 and it appears that both dial pointers are missing. If the op has the LW coils in the circuit, the placement of the Inductance switches won't have very much of an effect on the tuning since the LW coils have much more inductance than the SE-143 inductors. Since the LW Loading coil set includes a Tickler coil, one can assume that the SE-1834A is operated as a regenerative detector when operating below 50kc. Note that the SE-1834A has the TICKLER strap pointing up indicating that it's operating as a regenerative detector. That assumption then implies that the Heterodyne Oscillator might be a version that doesn't operate below 50kc (the SE-1387 will operate down to 10kc.) Incidentally, the transmitter is a Quenched-Gap Spark Transmitter, probably one of the 2KW Navy Standard types. Several companies built these for the Navy, like Wireless Specialty Apparatus Co., Kilbourne-Clark Mfg., RCA, Federal Telegraph Co. and others. The full-size version of this U.S. Navy photo is the "header photo" at the beginning of this write-up. That photo actually shows another USN Officer standing behind the radioman. On the wall behind that Officer is a calendar. This photo is exceptionally well-focused with an excellent camera lens and, although partially obscured by the Officer, the year on the calendar can be read and is "192-" with the last digit not visible. A believable date for this photo would be around 1925. |
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(R to L) SE-1420 Receiver, SE-1372 LF RF Driver (?), SE-1597 Loop Antenna Amplifier, SE-1834A RF amplifier, detector, AF amplifier and a Receiving Antenna Coupler (being held by RMC Gilmour) NOTE: As can seen in the photo, none of these devices are interconnected implying that the equipment was probably arranged for the photograph and not necessarily that all of the equipment was "used" together. |
U.S. Navy Station NAA - Ft. Myer-Arlington, Virginia Another setup is shown to the left, from USN station NAA. The receiver on the right side of the photo is the famous SE-1420, a single-tube regenerative detector receiver. Next is the SE-1372, a three band, possibly a specialized version of the SE-1387 with less heterodyne frequency coverage. The next unit is a Loop Antenna Tuner, the SE-1597. The left most unit is the SE-1834A with the "A" being the version without the filament voltage meter. That's quite a Loose Coupler that RMC (Radioman Chief Petty Officer) Gilmour is holding though it's probably an antenna coupler of some sort,...note the similarity to the coupler in the older NAA photo above. A believable date for this photo would be around 1925. photo from navy-radio.com. IF these accessory devices were to be used with the SE-1420 then some circuit changes would be necessary since the SE-1420 already has a detector. It would be possible to use the SE-1387 (or the SE-1372) by itself as a Heterodyne BFO ahead of the SE-1420 detector by connecting the SE-1387 output to the SE-1420 Antenna terminal (just wrapping the output wire from the SE-1387 around the Antenna lead wire should provide sufficient coupling or connecting to SEC COND and XTAL terminals can access the secondary LC directly.) Then the SE-1420's TICKLER/regeneration can be adjusted to the point just before the detector oscillates. The only thing accomplished would be to eliminate the oscillating detector and replace it with a heterodyne oscillator. Actually getting sufficient regeneration for oscillation is highly dependent on the frequency tuned, the detector plate and filament voltages and the antenna used. The lower frequencies are particularly difficult to actually get the detector tube to oscillate. It's impossible to get the detector tube to oscillate at VLF unless loading coils are installed and the SE-1420 doesn't provide terminals for installing LF Loading Coils, so about 40kc is the lower frequency limit. A Heterodyne Oscillator would tend to make CW reception easier for a wider frequency tuning range. The left-most unit is an SE-1834A and it might be possible to switch the SE-1420 control to CRYSTAL-RF AMPL to access the SE-1420's RF tuner section only by using the SEC COND, XTAL and TELEPHONES terminals and run the SE-1387 (as described in the preceding paragraphs) with the SE-1834A. No battery voltages would be required for the SE-1420 since only the Primary and Secondary LC tuners would be used. A lot of experimenting was certainly necessary when using these "add-on" pieces of equipment to achieve an actual functioning "upgraded" receiver. |
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SE-1420, IP-501 and IP-501-A Receivers
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The Navy preferred the silicon detector because of its ease of
operation and it reliable nature (what could go wrong with it? It was a
rock!) Hazeltine was a vacuum tube expert, he had invented the term
"mutual conductance" and thoroughly understood how vacuum tubes
operated. He designed the SE-1420 to use a regenerative VT detector and
to have the ability to greatly reduce interfering signals. Hazeltine first utilized a three-circuit tuner, that is, adjustable tuning of the antenna circuit, variable coupling to the tuned detector grid circuit and the detector plate circuit, to provide excellent sensitivity. He then used a completely shielded cabinet and isolated the Antenna Tuner circuit from the Secondary Tuner circuit with another shielded panel. This complete shielding would eliminate any stray pick up, hand-capacity effects or any coupling between the two circuits. Using a sharply tuned Antenna Tuner helped to improve selectivity and reduce adjacent frequency interference. By using a small Coupling Coil mounted inside the Antenna Coil and only allowing the energy from the Coupling Coil into the Secondary Tuner, further reduction of unwanted signals was realized. The two main inductors used bank-wound Litzendraht wire coils to reduce capacitive losses. "Dead turns" on all switched inductances were grounded by the action of the switches to further reduce losses. All of these efforts increased the selective nature of the SE-1420's tuning ahead of the detector input. The regeneration, called "TICKLER," was provided by a variometer that was built into the secondary inductor form. One stator coil of the variometer was connected to the secondary coil while the other stator coil was connected through the rotor to the plate circuit. The wiring connections provide for the proper phase reversal for coupling between the plate and grid circuits to occur. The adjustment of the rotor position within the variometer allowed resonating the L of the plate to the grid circuit for detector inter-electrode capacitance feedback and also simultaneously increasing the EM coupling by way of the EM field intensity of the variometer and its relationship to the grid tickler stator coil allowing positive detector feedback and oscillation at the proper physical adjustment of the variometer rotor. |
| The TICKLER adjustment controlled the sensitivity and
somewhat the selectivity of the receiver. The TICKLER also would
allow the detector to be operated as an Autodyne or oscillating
regenerative detector. Since the detector was oscillating at the
tuned frequency this provided a heterodyne action with the
incoming signal that the allowed demodulation of an arc
transmitter's continuous wave (CW) signal. When operated as an autodyne, the receiver
requires complete shielding to eliminate hand-capacity effects and stout
construction for stability. The detailed design effort was necessary because all Navy (and most other maritime vessels) used either spark or arc transmitters which usually produced very broad spectrum signals. Early receivers were so insensitive and tuning so crude that the broad transmitted signal was usually an advantage at attracting attention. The inability to have simultaneous operation of nearby stations led to sharing "airtime" - a gentleman's agreement that allowed most wireless operators to co-exist. Wartime was a different situation however and better, more powerful transmitters required better, more selective receivers. As the spark gap transmitter was improved by employing an oscillation transformer that narrowed the bandwidth, the receivers became more sensitive but not necessarily more selective. They still responded to the fairly broad spectrum signals that prevailed. At the time the SE-1420 made its appearance, its ability to function in the presence of nearby spark and arc transmitters made it an instant necessity for all sea going vessels. The photo to the right is from Milton B. Sleeper's 1922 booklet "How to Make Commercial Type Radio Apparatus." |
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| Several contracts were issued for SE-1420 receivers in late 1919. The initial contracts were for 400 receivers from AMRAD (American Radio & Research Corporation,) 400 receivers from Wireless Specialty Apparatus Company and 300 receivers from Sperry Gyroscope Company. These contacts were renewed and extended into 1920. Westinghouse designed their version of the SE-1420 receiver late in 1920, probably for use by the International Radio Telegraph Co., one of their subsidiaries. In 1921, Westinghouse submitted this version to the Navy for assessment but they were not offered a contract. Westinghouse designated their version as the Type RB Medium Wave Receiver and then offered it to the commercial user market but there was little interest and very few RB receivers were built. The various SE-1420 receivers will have some differences depending on the contractor and the time period of manufacture. AMRAD versions did not use a Telephone Condenser switch and mounted an ID tag on the front panel where the TC switch is on the WSA version. Also, AMRAD binding posts use hex nuts rather than knurled thumb nuts. "National Electrical Supply Company," a supplier of electrical and automotive parts located in Washington D.C., was added to the contractors rather early in the SE-1420 build history. "National Electrical Supply Company" is sometimes confused with Reginald Fessenden's company, "National Electrical Signaling Company" since both are usually referred to by the acronym, "NESCO." (Fessenden's NESCO was reformed into International Signaling Company in 1917 and then, after WWI, was purchased by Westinghouse to form their International Radio Telegraph Co.) Most National Electrical Supply Co. (NESCO) versions are very similar to the earlier AMRAD versions. Since AMRAD was bankrupt by 1924, later similar appearing versions are usually NESCO builds. |
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Later Signal Corps versions are sometimes designated as BC-131
receiver. The later versions of the SE-1420 and IP-501 receivers will
have less elaborate tube sockets that utilize a standoff mounted bakelite platform to mount a conventional bayonet-twist type
tube socket. The filament ammeter on the early SE-1420 is a "live zero"
meter with a .5-0-1.5A scale. The meter is generally marked as "CAY
260." Later SE-1420 receivers will have a DC Voltmeter rather than
the CAY-260 current meter. The Westinghouse Type RB did away with the meter
entirely. Tube types used in the SE-1420 depended on the time period and the end user. In early receivers, generally, if the Navy used the SE-1420, a Moorhead Electron Relay (ER) was used as a detector, while the Signal Corps preferred the Western Electric VT-1. There were many variations of the Moorhead ER tubes with different manufacturers building them from 1919 up to the early twenties. Both the VT-1 and the ER tubes specify filament current rather than voltage (.5A@ ~3vdc for the VT-1 and .4A@~4vdc for the ER.) There were other tubes also available, like the military triodes that had the internal structure mounted so that when the tube was operated in the horizontal position (as in the SE-1420) the actual tube structure is in the vertical position. This prevented filament sagging that could happen with standard tubes operated in the horizontal position. Later SE-1420 receivers used the 201A and these tubes specify filament voltage (5vdc@.25A) The panel meters were changed from ammeters to dc volt meters as tube use evolved. Apparently, many early SE-1420 receivers were rebuilt by the military as the receiver aged. This included upgrading the receiver to the SE-1420C or BC-131 configuration. This upgrading included adding a grid-leak resistor and capacitor assembly, usually mounted on the Secondary Inductor mount near the Tickler coil. Early versions of the SE-1420 relied on self-biasing of the detector tube and, although this does work, it requires fine adjustments of the filament and plate voltages for best results since there isn't a fixed negative bias source in the SE-1420. As vacuum tubes improved, the grid-leak arrangement worked better since it allowed for rectification (detection) and would "leak" off the excessive negative charges quickly though a high-value resistor. |
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variations are seen of the replacement tube socket. The original socket
is overly complex (77 parts are required to construct just the tube
socket assembly) and was probably a constant source of problems. The
simpler replacements are seen on rebuilt SE-1420 receivers and usually
are utilizing the original stand-offs and lugs but have additional
stand-offs to support a bakelite or fiberboard platform that has the tube
socket integral with the platform. Some of the platforms seen are round,
others are triangular. More than likely it depends on when the rebuild
was performed, with the triangular platform being the latest version.
Rebuilt receivers will usually have a newer ID tag mounted in place of
the original tag or sometimes just an additional tag with the rebuild
information. The cabinets were sometimes painted olive-drab when the Signal
Corps converted the receiver to the BC-131 configuration.
New SE-1420 receivers were built through most of the 1920s by several different contractors over the years. Shown in the photos to the right is the CGR-5A, made for the Coast Guard on a contract from June 1927. This version doesn't have the buzzer or the circuit selector switch and is housed in a metal cabinet. Also, the dial is calibrated in frequency rather than meters. The contractor on this particular CGR-5A was NESCO. This version also references itself to the SE-1420C as indicated on the CGR-5A data plate, "similar to Navy Type S.E. 1420-C/Army Type BC-131." The receiver shown belongs to Chris Dockery, who has also provided the photos. |
1927 - CGR-5A built by National Electrical Supply Company for the U.S. Coast Guard |
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History - IP-501 & Wireless Specialty Apparatus Company - In 1907, Wireless Specialty Apparatus Company (WSA) was formed by Greenleaf Pickard (who had cataloged over 1500 minerals and combinations that worked as detectors in 1903 - Pickard didn't discover the crystal detector, Karl Ferdinand Braun of Germany had invented the point-contact diode in the 1890s.) Additional WSA associates were Col. John Firth and his patent attorney, P. Farnsworth. John Firth also worked with Reginald Fessenden's NESCO at the same time and, probably because of this association, all WSA model numbers have the "IP" prefix which meant "Interference Preventer" - a Fessenden term for "selective tuning." United Fruit Company was an early user of WSA gear on their ships and in their shore stations. United Fruit Company had been somewhat in the radio business since 1903 and, in 1911, they bought WSA. Later, in 1913, United Fruit formed another radio company, Tropical Radio Telegraph Company, mainly for setting up and operating communications around their extensive property holdings in Central and South America. United Fruit was aware that their purchase of WSA gave them all rights to all Crystal Detector patents that WSA had through Greenleaf Pickard's association. The crystal detector dominated wireless receiver operation, especially through WWI. Right after WWI, the crystal detector patents were still of major importance and because of this patent, United Fruit Company was invited into the new cross-licensing agreement that was headed by General Electric and included Radio Corporation of America (GE's creation in 1919) along with AT&T (vacuum tube patents) and Westinghouse (Regenerative Detector and Superheterodyne patents and International Radio Telegraph Co.) With the cross-licensing agreement, these companies shared patents and products toward their advantage and tried to exclude most other companies and their competition by threats of lawsuits. The cross-licensing also allowed UF/WSA to now produce the SE-1420 for commercial users and have them sold by RCA (RCA hadn't created a division specifically to handle all maritime equipment and operate coastal communications stations - yet.). For the new commercial market, the designation of the receiver was changed to IP-501. A matching two-stage audio amplifier was now available, the Triode Type-B Amplifier (an updated civilian version of the SE-1000.) A Long Wave Adaptor was also available for operation at VLF frequencies. To accommodate the Long Wave Adaptor, hook-up terminals were added along the top of the panel to align with the LW Adaptor's terminals. Though early versions may have used ERs or VT-1s, after about 1923, the IP-501 receivers used UV or UX-201-A tubes. |
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History - IP-501-A & Radiomarine Corporation of America
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>>> RCA handled the sales of IP-501 receivers and
accessories from around 1921 until sometime in 1923. By 1924, Wireless Specialty Apparatus disappeared from
the scene, apparently purchased or absorbed by RCA. It's likely that
RCA
also acquired the WSA manufacturing plant in the deal since all later
IP-501s and IP-501-As were built still using WSA parts. From 1924 up to
sometime in 1927, RCA apparently carried on building receiver using WSA
components and selling those marine receivers. In 1927, RCA acquired
Independent Wireless Company and it was combined with Wireless Specialty
Apparatus to form Radiomarine Corporation of America. Independent
Wireless' Chas. Pennill became Radiomarine's Vice-President and J.P.
Duffy came from RCA to act as Superintendent of Production. With the
formation of RMCA, all marine operations and
sales were then transferred to Radiomarine Corporation of America as a
division of RCA. RCA had been operating many of the coastal wireless
stations and providing "Radiogram" communications and those
responsibilities were passed on to Radiomarine. By the late twenties, the IP-501 family of receivers were beginning to show their age.
The later versions eliminated some of the unnecessary or expensive
circuits and parts but the basic style was still easy to recognize. Many receivers were still in use well into the
late thirties. Their operation was easy, they were
reliable and their excellent performance in the hands of experienced
radio ops had resulted in the receiver becoming the "standard" shipboard
receiver for at least a decade and a half. Advertising for RMCA was
still using photographs of shipboard installations showing the IP-501-A
as late as the post-WWII time period. The selling price of the IP-501-A
was $550 in 1922 (listed in "Radio Enters the Home," a catalog of
products available through RCA though built by WSA at this time.) By 1930, RCA had acquired most of the patents and power
that had formerly been shared by the GE-Westinghouse-AT&T Group as part
of a settlement of an Anti-trust suit brought by the government. That
resulted in the consolidation of RCA into the omnipotent corporation
that controlled everything in radio in the thirties and forties. By the
thirties, RMCA was running many of the coastal marine stations that
provided Radiogram service to ships at sea. RMCA built marine radio gear
that was installed on commercial ships. During WWII, RMCA supplied the
Liberty ships with radio gear. Around the
mid-1960s, RMCA was eliminated as a division and RCA handled all of the
maritime business directly - at least, what was left of it. United Fruit Company went on to political involvement in some Central and South American countries in an effort to protect and/or enhance their extensive banana and pineapple properties. Eventually, United Fruit Company merged to become United Brands (in 1970) and then was reorganized in 1984 as Chiquita Brands International. |
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The photo left is a close up of the ID tag of an IP-501-A showing Radiomarine Corporation of America as the builder of the receiver. This
tag is from the receiver shown in the photo right - a beautiful later version
of the IP-501-A. This receiver is probably from the 1927 to 1930 time
period. Note that the telephone condenser switch was eliminated and bakelite
capped binding posts are used on these later receivers.
both of these great photos are from: Grant Kornberg - "TechnoGallerie" |
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Receiver Circuit and Construction Details |
| One look into the SE-1420, the IP-501 or the IP-501-A reveals an
approach to construction where reliability was a major consideration,
along with superior performance and ease of operation. The receiver uses
a three-circuit tuner with regenerative/autodyne detector. The IP-501-A
includes a built-in two-stage audio amplifier. The Antenna Tuner and
Secondary Tuner circuits and the Detector circuits are similar in all
receivers. The Antenna Tuner is labeled "ANTENNA INDUCTANCE" and
"ANTENNA CONDENSER." The condenser is gear driven and the dial is
calibrated 0-180º on its graduated scale. The Inductance taps are
switched, "dead turns" are shorted to ground and an articulated pointer
shows which band or scale is used. The Antenna Condenser dial has no
nomenclature other than the 0-180º scale and ample room was provided on
the upper non-scaled area for the operator to write in any markings he
needed. The "COUPLING" control rotates a small coil located at one end
of the Antenna Coil. The wires from the Coupling Coil are placed next to
the front panel shield and then routed through a small opening at the
base of the vertical shield that divides the cabinet into two shielded
compartments. Only the energy within the variable Coupling Coil is
transferred to the Secondary Tuner circuit. The shielding provides
complete isolation and eliminates stray
pick-up or any hand-capacity effects when operated as an autodyne
detector. What comes down the antenna and is tuned in the Antenna Tuner
circuit is then variably coupled into the Secondary Tuner circuit. This
provided the excellent selectivity necessary for operation of the
receiver in the presence of nearby spark and arc transmitters. The Secondary Tuner circuit is labeled "SECONDARY CONDENSER" and "SECONDARY INDUCTANCE" - this is the main station selector tuning. The Secondary Inductance control selects the tuning range via the tapped inductance, "dead turns" are shorted to ground and the Secondary Condenser tunes the receiver frequency within that range. An articulated pointer shows which tuning range has been selected. On the IP-501 and IP-501-A, the Secondary Condenser dial is scaled in both Degrees and Meters with the various bands covering 300 meters up to 7500 meters, or approximately 1000kc down to 40kc and the condenser is gear driven, (most receivers will tune 1200kc down to 37kc.)
The detector is a regenerative type using a variometer and tickler built onto the secondary coil form. Variometer controlled regeneration relies on detector tube inter-electrode capacitance and the EM field coupling of the variometer rotor position relationship to the tickler coil (which is one of the stator coils inside the variometer.) For reception of damped wave spark transmitters using rotary gaps the "TICKLER" is adjusted to a setting just before the oscillation point. If an arc transmitter was to be received then the "TICKLER" can be set into oscillation to allow a heterodyne action (autodyne detector) to hear the arc signal since it is continuous wave or CW. For the reception of a voice transmission via AM, the "TICKLER" would be set to just before oscillation occurs. The greatest sensitivity and selectivity occurs just at either side of the oscillation point in a regenerative detector and that is usually where the operator would adjust his "TICKLER." Since the load on the "TICKLER" (plate variometer) is fairly constant (because of the Antenna Tuning) there is very little change in where the "TICKLER" is set until the receiver is operated below 100kc. Since the regeneration is tuned, lower frequency reception requires a little more total variometer inductance so the "TICKLER" control will have to be increased (higher on the scale) as frequencies below 100kc are tuned. The "TICKLER" tunes total inductance in 90º of rotation (sign changes happen in quadrants) but, depending on the receiver, all "TICKLER" action is usually centered around 45º and increases to 90º as the lowest frequencies are tuned. The push button switch labeled "OSCL'N TEST" is for testing if the detector is actually oscillating or not. If the button is pushed, it shorts the TICKLER coil and, if the detector was oscillating, a "click" will be heard in the earphones. If no click is heard that indicates the detector is not oscillating and the "TICKLER" control needs to be adjusted. Detector tube is normally a UV/UX-201-A. |
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The audio amplifier circuit used in the IP-501-A is a standard two-stage type using interstage transformer coupling. The
AF interstage transformers are typical RCA units and probably were products of that company. The
ratio is around 3.5:1. Tubes normally used were UV/UX 201-A. There are ni-chrome windings on the bakelite wire
carrier of the tube socket assembly. These provide about 1ohm resistance
in the filament line to each tube as filament protection in case one of
the tubes was removed with the A+ on. C bias voltage is used on both
AF amplifier grids. The AF amplifier plates are usually run at 90vdc B+ and
the C bias is usually -4.5vdc. The Detector plate is run at 45vdc B+.
Filament control telephone jacks are used for output and the three
provided allow for Detector only, Det.+1AF or Det.+2AF operation.
Insertion of the 'phone plug into one of the jacks will determine
which tube filaments are lighted. A panel meter shows the applied
filament voltage which is adjusted with the control "INCREASE." On
SE-1420 receivers, the panel meter measures current drawn by the
detector filament. It was changed to a voltmeter early in the IP-501
production. The early versions of the SE-1420 are wired with the input
ground "floating" and tied to the shield and B- through a fixed
capacitor. This was changed in later versions to have the shielding
connected directly to the input ground and then the B- connected to the
shield through a fixed capacitor. The "TELEPHONE CONDENSER" switch allows selecting various values of input capacitors to the RF pi-filter that is connected between the output of the TICKLER variometer and the audio output line. The RF pi-filter also uses a series iron core choke and a fixed output capacitor. The selectable input capacitors allow varying the audio response, specifically rolling off the high frequency audio. This is particularly effective for relief from static and other atmospheric noise. This function is only on the WSA versions of the SE-1420. It is also on the early versions of the IP-501 and IP501-A. The Telephone Condenser (TC) switch was never used in the AMRAD SE-1420 and was eliminated from the later versions of the WSA receivers. The TC switch was really not a necessity. It was probably installed on the WSA receivers for shipboard operation where static and antenna noise can hamper reception. RCA/RMCA eventually eliminated the TC switch, probably because of expense, potential problems and the fact that an optimum fixed-value capacitor resulted in effective static relief along with increased reliability by eliminating the switch. |
| The SE-1420, IP-501 and the IP-501-A all provide operations with
crystal detectors utilizing the low-capacitance lever switch labeled "CRYSTAL OR R.F.AMPL" - "SEND" - "TUBE" ("AUDION" on SE-1420 sets.) Usually the standard
crystal detector used was the "Three Detector Stand" that WSA offered.
Typical shipboard operation had to provide for the possibility that all
of the vacuum tubes, those in the set and the spares, could be destroyed
during wartime with a possible torpedo hit. There was also the
possibility that given enough time and bad luck all tubes and spares
might just fail while still at sea. Or, maybe the batteries might need
charging or replacement and there were no spares. In other words, many
different things could affect whether or not the vacuum tubes could be
used. The crystal detector was the back-up and it always would work. For
many years, USN regulations and Maritime regulations required that all
ships must have some type of emergency radio receiver that could
function without power, a crystal set, in other words. Even in WWII, all
Maritime Radio Consoles contained a Crystal Detector receiver of some sort for
emergency communications (well,...reception.) The "BUZZER" provides a "signal generator" of sorts. When looking for a sensitive spot on the crystal detector, it would help if a really loud signal was present. Pressing the buzzer button will actuate a small mechanical buzzer that arcs and creates tremendous wideband RF. This is coupled into the antenna circuit with a brass sleeve capacitor on the wiring to the Antenna Inductance switch on SE-1420 sets and by a wire coil wrapped around the same wiring in the later receivers. The buzzer battery is usually a 1.5vdc dry cell battery. It's not critical, but 2vdc was considered the maximum for the buzzer. DO NOT PRESS the buzzer button (with Buzzer battery connected) while in the vacuum tube mode of operation - if you do and you're using 'phones in the AF2 jack, the resulting "signal" will be so intense that you probably won't be able to hear anything for a few minutes afterward (yes, I did it.) The Buzzer circuit was only for finding a sensitive spot on a crystal detector. Additionally, a Long Wave Adaptor was sometimes used if operation below 40kc was needed. This unit sat on top of the receiver and its connections match the binding posts located at the top of the panel on the IP-501 and the IP-501-A (the Long Wave Adaptor units were not used with the SE-1420.) The Long Wave Adaptor had series inductors inside that when connected allowed the receiver to tune down into the VLF part of the spectrum. |
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The oak box that the receiver is mounted in is entirely lined with copper sheeting to act as the shielding. Complete contact is assured by way of the metal screw mounts that contact the receiver's panel shielding. Early receiver boxes sometimes had a front cover that was held on with bale clamps. The ID tag is located on the side of the box and these are almost always missing. This was probably due to the "military surplus" regulations of the time that required all mil-tags to be removed before sale. Something about if the tag wasn't there then the unit wasn't stolen. This regulation may have also applied to commercial surplus. Weight of the box with all of the copper inside is substantial and the entire receiver is quite heavy for a battery operated receiver - about 40lbs for an IP-501-A. The box for the SE-1420 is similar in construction but the shielding is not painted and is left bare copper. The finish on the SE-1420 box is somewhat dark, usually about the color of "iced tea." The later IP-501 and IP-501-A receiver boxes are finished in golden oak. Most BC-131 boxes are olive-drab paint. The front panels are .312" thick and is made of "Hard Rubber" sometimes called "Condensite" or "Bakelite-Delecto." This material is not brittle like bakelite or formica. The manuals say that the panel can be wiped with oil to protect it. Probably, with all of the salt-air present onboard a ship at sea, wiping oil on the entire panel, dials, knobs and cabinet would have gone a long way to protect the receiver's overall finish. All screw and nut connections in the receiver are tightened and then soldered. This method is also used on the mechanical assembly. Soldering is easily accomplished since all of the hardware is nickel plated brass. This securing of all joints with solder was necessary because of the constant vibration of the ship while at sea in addition to adding protection from salt-air corrosion problems. The solder joint itself is not particularly strong and can easily be disassembled, however, much like modern "loc-tite," it was meant to keep the screws and nuts secure after tightening. |
| Chronology of SE-1420, IP-501 and IP-501-A
Development and Production 1918 - Initial design of the
SE-1420 by Louis Hazeltine |
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Restoration and Operating the SE-1420, IP-501 and IP-501-A Receivers |
| Restoration shouldn't be desired or even considered if
your receiver is complete and original. However, this is by far the
minority of surviving SE-1420, IP-501 or IP-501-A receivers. Most of
these great receivers were destroyed in the past 80+ years by scrap
dealers, by the scrap drives of WWII,
by parts dealers, by surplus dealers selling to "hamsters" and just by years of
abuse, poor
storage and neglect. This section is for the restorer that wants to have
his incomplete receiver as accurately restored as possible and to have it
operational and functioning correctly. Most SE-1420, IP-501 and IP-501-A receivers that are found today are far from complete. It isn't unusual to find the receiver missing all of its buss wiring or missing major components and almost always some of the minor parts will be gone. I one time found the Antenna Tuning Condenser of an IP-501 that had been "sawn" out of the front panel - not dismounted from the panel - just sawn out, panel and all. Such destruction was common. Anything is possible to find since these receivers were considered surplus unusable junk in the forties and fifties. How likely your receiver is able to be completely restored depends on your interest, your abilities at replicating parts and how much of the receiver you have to start with. Generally, the major parts necessary for
considering a complete and
functional restoration of the receiver are: |
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SE-1420, IP-501 and IP-501-A - Schematics and Documentation Documentation is very important when restoring the SE-1420, IP-501 and IP-501-A receivers. To say that they were poorly documented would be an understatement. None of the schematics available are complete. Most will provide a general idea of how things are connected but details are certainly lacking. The various schematics are shown in several books, e.g., Elmer Bucher's book on Wireless Equipment or early editions of George Sterling's "The Radio Manual" or others, but all are incomplete schematics that are only provided as general information. The IP-501 schematic shown to the right is about as good as they get. Not a lot of details but it is basically complete and does show the connections to the complicated "Circuit Selector" switch. However, mistakes are common, e.g., the "Grounding Condenser" is not a variable, it is a fixed condenser. This schematic is good for the IP-501 produced around 1922. Earlier SE-1420 is similar but without the Long Wave Adaptor terminals. The later IP-501-A is a very different receiver but still a lot of this schematic is applicable. What one has to do is use good photos of the interior of original receivers combined with the information provided in the better schematics to ascertain what is correct for your particular receiver. This is assuming that your receiver needs to be restored and is missing some of the original buss wiring or original components. Be aware that the buss wiring techniques and routings changed over the production period, so early receivers look very different inside from the later versions of the same model. Interior photos are the most helpful to determine what is correct. Since the advent of eBay, which has now had many auctions/sales of SE-1420 and IP-501-A receivers, photographic documentation of these models has become excellent. However, it's up to the interested restorer to go in and "save" these photographs because eBay doesn't keep them very long. Operator's manuals are around. Some are available on the Internet and some basic operating instructions are included in various books. Sterling's "The Radio Manual" - First and Second Editions have instructions for both the SE-1420 and the IP-501, along with the Long Wave Adaptor. However, these instructions are brief so they contain very few details. No details are provided about typical antennas for these receivers (although the 200' end-fed wire seems to be what is often specified.) The RCA and RMCA manuals are by far the best and most accurate. |
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Useful Hints for Restoring the SE-1420, IP-501 and IP-501-A Receivers Synchronizing the Tickler Variometer - The variometer has to increase total inductance with the proper sign (+ or - are used to indicate the increase or decrease of total inductance as the rotor turns inside the stator coils) as the pointer is advanced up the TICKLER scale. This results in the receiver requiring higher TICKLER settings as the wavelength is increased (lower frequency.) The correct wiring is the detector plate is connected to one coil of the variometer stator as the input. The grid circuit is wired to the other stator coil to provide the feedback path. The variometer rotor output (rotor-front) goes to the Circuit Selector Switch, RF pi-filter and on to the audio output and detector B+. To check that the variometer is synchronized, place the TICKLER pointer straight up on the scale. Look at the variometer rotor just visible on the shortwave side of the Secondary Inductor and you should be able to see the wire splice joint that connects the two rotor inductors together. If you don't see the splice joint then the rotor is 180º out. Remove the TICKLER knob and pointer, then rotate the variometer rotor so that the splice joint side is visible, then re-install the knob and pointer with the pointer straight up on the scale (or nearly straight up.) Check the flexible connections on the variometer rotor to make sure they aren't coiled too tight at each extreme of TICKLER adjustment.
NOTE 1: Although you do get a change of
total inductance through each 90º of rotation with a variometer,
the two 90º quadrants in 180º of rotation are of opposite sign + or - (there is
a mutual inductance change also.) When the variometer is operated in the opposite
two 90º quadrants, the
receiver will not regenerate on lower frequencies or will oscillate
uncontrollably due to improper phase relationships to the grid coils. With the proper variometer synchronizing the receiver's
oscillation is controllable on all tuning ranges. Dismounting the Primary and Secondary Condensers - The condensers are mounted using 10-32 screws and nuts with stand-offs between the condenser mounting plate and the back of the panel. The nuts are secured by soldering after assembly. To remove either condenser first remove the associated fine adjustment knob and the dial by removing the large knob and collar, then remove the dial. The dial is only held in place with two locating pins and should easily come off. You will now see that the flange that the dial mounted to will just barely fit though the hole in the panel shield. You have to be careful not to bend the shielding too much when removing the condenser otherwise you will end up shorting the condenser to the shield when reinstalling the unit. Unsolder the buss wire connections to the condenser. Then remove the screws and nuts. The soldered nuts will come off easily. Solder is not particularly strong and usually with a open-end wrench on the nut and a large screw driver on the screw head, the solder joint comes loose with minimum effort. You can also heat the joint up with a larger soldering gun or iron and then break the joint loose. Heated solder is even weaker and the screws will loosen with almost no effort. After the screws and nuts are off, carefully rotate the condenser assembly while lifting it off of the panel. You will find some interference between the panel shield and the dial flange but by rotating the assembly, the flange will clear the shield hole. Be sure to check the shield hole for bends - it should be straight and even with the back of the panel. Be sure to keep track of the four stand-offs. Remount in the reverse order. Dismounting the Primary and Secondary Inductor Assemblies - Fortunately, the inductor assemblies are held to the panel with 10-32 flat-head screws that are not soldered. They screw directly into threaded stand-offs that are mounted to the assemblies. Remove the associated knobs and pointers. Disconnect the buss wires going to the inductor assembly. Remove the four 2-56 screws that hold the dial pointer cover-guide to the panel. The pointer has a .125" diameter pin that is a push-fit into the lifter mechanism behind the panel. Remove the dial pointer. The pointer should be slightly twisted while pulling it away from the panel. The pin fits into a bakelite holder, so it should come off with very little effort. Remove the four 10-32 flat-head panel screws and lift the inductor assembly from the panel. Remount in the reverse order.Dial Pointers - These are rather complex assemblies for the simple job they do. The "lifter" mechanism is located on the associated inductance assembly. The lifter is gear driven by the inductance switch and the lifter itself is attached to a rack gear. Two guides keep the rack's alignment. The lifter has a "L" shaped bakelite piece that the pointer pin is inserted into. The pointer itself is mounted to the front panel by a two-piece cover-guide that is nickel-plated. The cover-guide is mounted to the front panel with four 2-56 round-head machine screws. To remove the pointer just take out the four guide screws, remove the cover-guide pieces and remove the pointer from the lifter by pulling it away from the panel. If you need to work on the lifter mechanism itself, you will have to remove the associated inductance assembly. Buss Wire Details - Buss wiring changed as production methods evolved. The early SE-1420 receivers use a reddish-brown varnished tubing (spaghetti) for insulation. The wiring style for these receivers is very square and the buss wires actually run much longer than necessary. This was for appearance and was typical of the style of wiring at the time. When the IP-501 and IP-501-A were being produced by RMCA, the varnished tubing was changed to black. The style of wiring also changed in that the runs are much shorter and though still somewhat square looking, there are some angles and bends that are for better durability or performance rather than appearance. The late IP-501-A receivers still use black varnished tubing but more and more the square-look is giving way to more direct connections. Finally, in the 1927 CGR-5A (SE-1420C) the spaghetti is entirely eliminated and enameled buss wire used. When replacing missing buss wire, try to find an interior photo of a comparable receiver for reference. Buss wire was usually 13 gauge tinned-copper, which is impossible to find. I have used 14 gauge and 12 gauge, both work fine, although the 12 gauge is more difficult to work. Before using either size, the wire should be "drawn" - that is stretched by anchoring one end and then pulling the other - hard. This straightens the wire and slightly reduces it's diameter. It will make the buss wiring look very straight and professional. |
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Restoration of the IP-501-A Back in 1979, I bought this IP-501-A from a ham friend who had traded a telephone pole for it. The price of $75 took into consideration the substantial amount of work that was going to be required to restore the set. Back then, with no Internet, all parts had to be advertised for in Radio Age magazine with the hope that one of the many collector-readers might have what you needed and would be willing to sell the part. It wasn't unusual for part locating to take a year or more. The IP-501-A was missing almost all of the buss wiring, it had the incorrect AF transformers, the Telephone Switch was gone along with the correct tube socket assembly. Additionally, the set's front panel was in pretty rough condition as were all of the nickel-plated hardware parts. The cabinet was actually in pretty good condition and the parts that remained were also in good condition. My first restoration just got everything cleaned up and looking good but I didn't want the IP-501-A to be just a "shelf queen" so I began to advertise for specific parts I needed to get it operational. That resulted in the second, functional restoration. I used black plastic tubing for the "spaghetti" on the new buss wiring and the interstage transformers were two old Jefferson units. I had to make several parts. I made the tube socket assembly from .25" thick original vintage bakelite. The nickel-plated tube socket shells came from an old TRF battery set. One small knob had to be cast in epoxy resin with black filler so it would come out looking like hard rubber. The metal parts that had to be made were two binding posts and one knob pointer. I got the IP-501-A running and eventually wrote an article on it for Radio Age (April 1984 issue.) Don Patterson (editor for Radio Age) sent me some material on the IP-501-A that included an article written on the IP-501-A receiver back in the 1960s for Popular Electronics. The article had a good photograph of the inside of an original IP-501-A, something I had never seen before. |
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My second restoration had been incorrect in several places and needed to be redone to be an accurate representative of the IP-501-A, both physically and operationally. I started to search for more parts for the new restoration. The easiest to find were the two RCA audio interstage transformers. The new buss wire used was now 12 gauge (I had used 14ga. before) which also was easy to find. The lacquered tubing or "spaghetti" was a reproduction product supplied by one of the few dealers then around and doing business. It looked very close to original. The Condenser Switch and assembly was rebuilt from correct vintage parts and then installed in a painted black, brass metal box I made. All of the hardware on the front panel was removed and then cleaned and re-nickel plated. The tuning dials were listed originally as "German Silver" but that is really just a fancy name for heavy nickel plating that has a small amount of copper in the plating anode. In order to have all of the hardware parts match, since some were new repros, I had to re-nickel plate all of the hardware. That way it all matches and looks the same vintage. Disassembly is difficult because all screw and nut assemblies are soldered. The technique for removal is to use the soldering iron to heat the solder and nut, then while the joint is still hot use a nut driver to remove the nut. While hot, the solder isn't very strong and the nut will back off with very little effort. Clean the screws and nuts before reassembly for better solder flow. This last restoration was done in 1984 and resulted in the IP-501-A looking original and functioning as it should. Or did it? I found that I couldn't get the receiver to oscillate below about 250kc no matter where the TICKLER was set. Reversing the variometer leads got the receiver to oscillate but the wiring layout didn't match photos of original IP-501-A receivers. I finally revised the way I had done the buss wiring which then allowed the variometer stator input to connect to the plate and the front of the variometer rotor to be the output. This got the IP-501-A looking correct inside and working the way it should - able to regenerate down as low as the receiver would tune. |
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Restoration of the SE-1420 I bought this SE-1420 from a fellow in Louisiana who had advertised it in Antique Radio Classified magazine in 1990. He had listed the radio as a "Radiomarine Corp Receiver." I was curious as to what it was so I called and asked him to describe the receiver to me. When I heard "...,two large metal dials, lots of metal binding posts and an oak cabinet...," I was sure it was an IP-501 receiver. The price of $150 plus shipping took into consideration that the receiver was nowhere near complete and had been extensively modified by someone, circa 1940s. The seller described all of the modifications and indicated that no major holes were drilled and the coils and condensers were present. When the SE-1420 arrived I found he had described it very accurately. The most important parts to have present on these types of receivers are all of the coils, condensers, bandswitches, dials and cabinet. Most of the other parts can be found or replicated. It seems to be common to find these types of receivers with most or all of the buss wiring missing. Also, many times they are found with conversions to later vintage tubes. Most of the time this is the work of "hamsters" (radio amateurs who are all too eager to modify vintage equipment into something it was never intended to be.) The SE-1420 family was available surplus in the late thirties and most of the modifications seem to date from that time period. This SE-1420 had all of the essential parts so now I just had to find all of the missing parts. First on the list was a buzzer which was easily found, though it's a Federal T&T type SC BZ-1 (Signal Corps) which is not the original make. I made a replica buzzer switch. Next, I needed a suitable meter. Although a CAY-260 ammeter meter is correct for this vintage SE-1420, I was only able to find a similar vintage Weston DC Voltmeter with 5vdc high-lighted in red. It is not technically correct but probably imparts better information when actually operating the receiver (besides, later SE-1420s had filament voltmeters and probably those receivers updated by the military also had DC voltmeters installed.) Two metal pointers had to be made and two replica knobs cast. The tube access door was missing its knob but a very similar brass type was found at the hardware store, although I had to nickel plate it. A Federal T&T low-capacitance lever switch was found on the Internet (probably after I had owned this receiver for at least 12 years.) Replicating the SE-1420 Tube Socket |
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A template to check size and fit was necessary and was based on the
dimensions of the three mounting holes in the front panel of the
receiver. Also, using proportional measuring, the total height of the
assembly was determined and where each "ring" should be positioned.
Finally, the height of the socket had to also take into account enough
clearance for any type of vacuum tube that might be installed. Typical
SE-1420 tubes were either Moorhead Electron Relays (ER), similar
Atlantic-Pacific types or the Western Electric VT-1. I also wanted to
be sure that I could install a common UX-201A and still be able to close
the tube access door.
I had a local machinist make the standoffs, the shouldered screws and the metal base plate based upon my drawings. I made all of the bakelite pieces and the tube contact pieces. The socket shell and tube pin contacts were from a 1920s battery radio and found in the junk box. Assembly was fitted together to check everything and then, when I was sure of proper fit, the brass screws and nuts were soldered. This duplicated what was normally found in shipboard receivers and was done to prevent assemblies from shaking loose during the constant vibration encountered while at sea. I had to fit brass spacers (like thick washers) inside the springs to keep them centered. From the vintage photos, it appeared that the main support springs had extension spacers. I soldered brass extension spacers to the springs where necessary. The bakelite wire carrier ring has rubber insulated wire connections coming from the tube pin contact strips. These were routed as seen in the vintage photographs. UPDATE 2026: With excellent condition, original SE-1420 receivers showing up on eBay once in a while, I've seen some very good photographs of original spring-suspension tube sockets. My replica is pretty close in appearance and functionality (considering I built it 17 years ago.) Of course, nickel plating the springs and other brass parts should have been done. I should have used non-threaded rods for the spring-suspension assemblies. Original examples have cotton wadding pushed into the springs, probably to reduce microphonics. But, other than those minor points, the 77 piece replica socket looks pretty much like an original. See photo to the right for the assembled tube socket before it was installed into the SE-1420. |
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| Building the Telephone Condenser Switch Unlike the tube socket, I was not able to find a good photo of the Telephone Condenser Switch, that is, until I was given Milton Sleeper's book "How to Make Commercial Radio Apparatus" that shows the Telephone Condenser switch in enough detail to have made an accurate replica. Unfortunately, I was given Sleeper's book in 2026,....or about seventeen years after this SE-1420 restoration. This switch assembly is only in the WSA versions of the SE-1420. Most vintage photos of the receiver interior are of the AMRAD versions (at least they were in 2009.) I decided to make a Telephone Condenser Switch that looked vintage and would appear basically correct, though not a true "replica." First I had to make the switch itself. The spacing of the six positions is not standard - at least by today's standards for 12 positions in 360º rotation, or 30º spacing. The TC switch is about 18º, or 20 positions per 360º rotation. I did a layout having 18º spacing on a bakelite mounting plate and using vintage contact points built up the six-position switch. The front mounting plate acts as a bearing for the 0.5" diameter shaft and also allows the switch assembly to be mounted to the receiver panel utilizing the original mounting holes. The capacitors and choke that are also part of the TC switch assembly are mounted to the rear of the switch plate. The three connections are via rubber insulated wires. Since the capacitors and choke are not 1920s vintage parts (new caps and 1950s choke) a metal cover was fabricated to fit over the switch assembly and terminals were placed on the back of the cover for connection to the receiver's buss wiring. Buss Wiring Technique The original buss wire in the SE-1420 is 13 gauge tinned copper - next to impossible to find. I used 12 gauge bare copper that I had "stretched" by anchoring one end and pulling on the opposite end. This straightens out the wire and also slightly reduces it diameter. I had to make the varnished "spaghetti." I found some vintage fabric tubing but it was bright yellow in color. Using artist's acrylic paint, I mixed up a small quantity of paint that matched the few remaining original sleeved wires. To install the buss wire you first must decide the route your wire is going to take, then measure and cut the buss wire. Next the "spaghetti" tube has to be cut to length and placed over the wire. Then all of the bends are put in place using either your fingers for the longer bends or needle nose pliers for shorter bends. The next step is to paint the wire sleeve the correct color and let it dry. This only takes about 5 minutes, during which time another buss wire can be cut and gotten ready. |
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When the paint
is dry the wire can be installed. In examining photos of original
SE-1420 interiors, the buss wiring bends were not perfectly
square. This work was all done by hand when originally installed, so
some variations are normal and to be expected. I based my wiring appearance on
a vintage photo of a WSA SE-1420 interior. After all of the buss wiring
is
installed,
start applying "amber shellac" to the sleeving with a small brush.
Several coats are necessary for the "spaghetti" to take on the
appearance of old sleeving.
"Patina" is a very important part of replicating old parts. I deliberately left the washing residue on the tube socket and also judiciously added scratches and marring to the TC switch box paint. I used a chemical "patina" to darken solder joints and to darken the brass parts of the tube socket. This imparts the impression that one is looking at original parts, original soldering - a true vintage replication. I did
install one upgrade to the SE-1420 which was a grid-leak RC to improve
performance with 201A tubes. This was a common upgrade done by the
military in the early-twenties as vacuum tube performance evolved and improved. |
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Performance Testing 100 year old Radio Receivers |
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The initial testing of the SE-1420 was pretty exciting. After all,
here was a receiver that I had purchased nearly twenty years before. It
had started out as really nothing more than just the basic necessities for
rebuilding. I'm sure this poor SE-1420 had not been operational since it
was "hamstered" back in the late thirties or early forties and
now here
it was - almost ready to operate once again. I decided to use a UX-201A as
the testing tube and connected up 6vdc for the filament voltage (adjust
to ~5vdc with filament control) and
45vdc for the detector plate voltage. I used the ham station tuned
dipole antenna with the feedline shorted and
ham station ground system.
The initial test was on the AM BC band since signals there are very strong. As soon as the voltage was applied the SE-1420 started to "squeal" through the earphones - a really good sign for regenerative receivers. Backing the TICKLER down brought in the local (Reno) AM BC station on 920kc. A slight tuning of the Antenna Condenser had that station coming in strong in the "Baldie" earphones. I tuned in a few more AM BC stations with very good results, so now it was time to try "NO", the non-directional beacon (on 351kc) at Reno-Tahoe International Airport. Switching to tuning range to "2" and Antenna Tuning to "3", "NO" was found quickly. Since NDBs send MCW signals, the signals are easier to find if the detector is oscillating. In this mode, the Coupling is more critical and most controls interact significantly. Stability is also very difficult to achieve but the SE-1420 seemed to be fairly stable with a UX-201A tube. This isn't the tube type that was normally used with these receivers but this was just a test of operation. The next step was to try the Western Electric VT-1 and then the Moorhead ER, both typical tubes used with the SE-1420 back in 1920 or so. The WE VT-1 works very similar to the 201A tube except the filament voltage is 3.0vdc. The TICKLER settings and the condenser settings are very close to that of the 201A. This indicates that the WE VT-1 has similar inter-electrode capacitance to the 201A tube. Not so for the Moorhead ER. This tube runs about 4.0vdc on it's pure tungsten filament. TICKLER has to be advanced significantly and even though it is sensitive enough, it is difficult to tell when the tube is oscillating. Again, this is an indication of the different inter-electrode capacitance specifications for the Moorhead ER when compared to the 201A. Using a UV-201A tube, I was able to "tune in" 28 NDBs in a 30 minute period that evening. Greatest DX was YZH 343kc, Slave Lake, Alberta, Canada. Pretty good results for a single tube receiver. I next added a Pilot Radio Redi-Blox AF amplifier (ca. 1928) to boost the signal levels a bit. This is a transformer coupled, single stage audio amplifier using a UX-201A tube. With more audio, DDP 391kc in Puerto Rico was received (~3500 miles from here,) also YMW 366kc in Maniwaki, Quebec. Low power 25W marker beacons like SYF 386kc in St. Francis, KS and SBX 347kc in Shelby, Montana were also copied. In all, in two listening sessions, 50 NDBs were received including one newly heard 25W NDB, PA 396kc in Snohomish, Washington. Incredible performance from a 1920 regenerative receiver. NOTE: I performed this SE-1420 testing while living in Virginia City, Nevada in late-February 2009. |
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Operating the IP-501-A
"NDBing"
with the IP-501-A |
As the wavelength
increases, the TICKLER total inductance (physical position) has to be increased (higher on
scale.) Once the TICKLER is set it doesn't have to be adjusted too much
for each particular tuning range.
The INDUCTANCE switches select the tuning ranges. You will find that the
Antenna Tuner settings won't necessarily match the Secondary Tuner
settings. They are separate circuits so the Antenna Tuner settings will
vary depending on the antenna and ground system used. The Secondary
Tuner Meter Scale can generally be used for a rough starting point for
tuning around. The dial's Meter Scale accuracy is dependant on several other
factors when the receiver detector is operated as an Autodyne detector. Tuning In NDBs - Setting "Critical Coupling" To receive NDBs, the receiver should be operated as an Autodyne detector. The stations can be roughly located and tuned using the Wavelength Scale on the SECONDARY CONDENSER dial and then using the ANTENNA CONDENSER to tune for maximum signal response. Adjust the TICKLER until you hear the detector go into oscillation. Use just the SECONDARY CONDENSER for station tuning and the ANTENNA CONDENSER to peak the signal. When "peaking" the ANTENNA CONDENSER, as you approach resonance you will hear a couple of loud clicks, a change in received frequency and the detector may stop oscillating. This is a result of too tight of coupling (COUPLING set too high.) Set the COUPLING lower on its scale and again tune through resonance with the ANTENNA CONDENSER. As the ANTENNA CONDENSER is tuned back and forth through resonance, listen to the clicks while reducing COUPLING. At "Critical Coupling" the clicks will stop and the detector will remain in oscillation. Tight coupling will over-drive the detector at resonance, causing the jump in and out of oscillation. The "Critical Coupling" setting is good for a fairly wide tuning range, usually at least 20 to 30kc. The TICKLER setting and the COUPLING setting do interact, so usually just the TICKLER is slightly adjusted when the detector drops out of oscillation. After "Critical Coupling" is set, adjustments to the TICKLER are very slight changes. Most tuning can be done using just the two main tuning controls, SECONDARY CONDENSER for tuning stations and peak with the ANTENNA CONDENSER, along with very slight adjustments of the TICKLER. As the ANTENNA CONDENSER is resonated, you will find that the received frequency changes slightly. This is normal interaction of the autodyne detector. Just slight readjustment of the SECONDARY CONDENSER is necessary for proper tuning. It would be next to impossible to find the weak NDB signals without the receiver set as an autodyne detector. This provides a heterodyne action so the carrier of the MCW NDB signal can be easily heard. Tune to "zero beat" and you hear the MCW signal of the NDB - or maybe two or three NDBs, as there are usually several NDBs assigned to each particular frequency. Tuning for AM BC Operation The same basic set ups are used for receiving AM signals but the detector must be operated as a straight regenerative detector (not oscillating.) The best sensitivity in a regenerative detector occurs just before the oscillation point. COUPLING is not a critical adjustment in this set-up and, though the COUPLING can be set somewhat tighter (higher on the scale) for AM, it's not really necessary. Anywhere from 45 to 100 is good for AM-BC. Set the TICKLER so that you can hear background noise coming in but not so it is oscillating. Tune around and find an AM station. Peak the signal with the ANTENNA CONDENSER and then adjust the TICKLER to just before the detector breaks into oscillation. The receiver is now operating with maximum sensitivity. Operated as a straight regenerative detector (non-oscillating) there is very little interaction between the controls. You have to keep the two main tuning controls in adjustment as you search around for different stations. The TICKLER doesn't need to be adjusted too much unless you find a really weak AM station you want to listen to. Other LW Stations Besides AM BC above 500kc and NDBs below, there are several other interesting signals below 500kc. LW BC stations in Europe and Asia can sometimes be received. Radio Rossii at 279kc on Sakhalin Island is very strong in the West and can be received easily during the winter mornings before 6AM PST. (Russia shut down all LW BC in January 2014.) Also, the are "Lowfers" that operate 1 watt CW transmitters to 50 ft antennas located in the 190kc to 160kc region of the spectrum (hams now have 630M and 2200M bands, CW and data modes only.) Also, WWVB at 60kc, JJY (Japan's equivalent to WWVB) at 40kc and Loran C (Loran E now) stations at 100kc (Loran C shut down in 2010. Replaced with Loran-E in 2024.) Most casual listeners don't receive much of what is on the air below 500kc because they listen for AM/voice signals. Very few AM/voice signals will be encountered below 500kc. Almost everything is data transmissions and is being sent in CW, MCW, Pulse-encoded signals, encrypted very narrow-shift MSK USN signals, etc. Voice is only encountered in LW BC (gone) and very rarely Voice Weather TWEB associated with a few NDBs (usually Alaskan.) To receive most data transmissions you must have the detector oscillating so a heterodyne action allows you to actually hear the signals. Once you listen with the autodyne detector, you'll be surprised just how many signals are below 500kc. Optional Digital Frequency Counter Set-up Since the IP-501-A and the SE-1420 use a regenerative detector with only an Antenna Tuner between the detector and the antenna, it is possible to couple a digital frequency counter to the antenna lead-in and then have an accurate frequency read-out. When the receiver's regenerative detector is oscillating it is partially acting as an oscillator and as a detector (autodyne detector.) The oscillator output couples into the antenna tuner and then into the antenna. Many times the old AM BC radios with regenerative detectors would be adjusted to oscillate for picking up weak stations and would then radiate the oscillating from the antenna. The radiated oscillations were considered interference and would be received by the neighbors over their radio receivers in the form of "bloops" and "whistles" that are mentioned in many old radio magazine articles. The regenerative detector's oscillations can be a fairly high amplitude and will easily drive a modern digital frequency counter. Since the detector is oscillating at the received frequency, the counter's display is the frequency that the receiver is tuned to. A simple three foot long wire connected to the counter's input with the other end of the wire wrapped around the antenna lead will couple enough signal into the counter for a read-out. Don't connect the counter ground to anything. This digital frequency read-out will only work when the receiver is oscillating. If the frequency read-out is erratic try increasing the TICKLER slightly for an accurate reading, then reset TICKLER for maximum sensitivity. Sometimes at the detector oscillation point the counter will respond to the detector frequency, the signal modulation and the received noise causing an erratic display. When you are searching for NDBs, it's a big help to know exactly where you are tuned. DFC for the SE-143 - This method of using a digital frequency counter for a received frequency readout can also be applied to the SE-143 receiver. Since the TICKLER coil is connected to the plate of the detector tube externally on the SE-143, it's easy to wrap about 7 or 8 turns of wire around the TICKLER to detector plate wire as a pick-up. It works a little better if the DFC's ground is connected to A+/B- terminals. Also, as with the SE-1420 and IP-501-A, you have to advance the TICKLER beyond the maximum regeneration/oscillation point or otherwise noise and AM modulation (if present) will cause errors in the readout. Be sure to zero-beat the station's frequency exactly. |
| Kilocycle to Wavelength in
Meters Conversion Chart - The chart to the right is
a very easy way to convert kilocycles to wavelength in meters. ALL of
the receivers covered in this write-up have calibrated Secondary
Condenser dials,...but that calibration is in wavelength. The changeover
to kilocycles from wavelength was ongoing through all of the 1920s and,
by 1930, using wavelength on a tuning dial had all but disappeared. So,
to use the chart, the first column is kilocycles then "three dots" and
then wavelength. For example, if I wanted to tune in the NDB MOG on
405kc, I'd go to 400kc (first column) and see that was equal to
749.6 meters. Tuning the Secondary Condenser dial to 745 meters will
certainly be close enough for finding MOG. This chart was in a 1923
Lefax Radio Handbook so the upper frequency limit is just over 2000kc.
IP-501-A Testing Results IMPORTANT NDB NOTE for 2026: Nowadays this type of NDB reception is impossible with any type of MW receiver, even modern MW receivers. The sheer number of NDBs that have been decommissioned since 2009 is staggering. None of the USA pilots use NDBs for navigation anymore and that's resulted in most airports having decommissioned their NDBs. Regulations don't require airports to provide non-direction beacon transmissions anymore. The few NDBs still in operation are not used for navigation in the USA. The airport is using the NDB as a voluntary radio "airport identification" signal and the transmissions are kept running as an "airport navigation tradition." In addition to NDBs, many of the other traditional aviation navigation signals such as VOLMET (aviation weather reports) are being removed from all parts of the spectrum in the name of "modernization." Airport economics is certainly another factor in the removal of most NDBs, so don't expect these few remaining NDBs to be in operation too much longer,...at least in the USA. Canada is also decommissioning their NDBs at an alarming rate. IP-501-A NDB Log - Jan 21
to Feb 11, 2009 Total as of Feb. 11, '09 is 103. |
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| 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, AB, CAN*
* = Newly NDB heard |
| Operating 100 year old
Radio Receivers in Today's Polluted Electro-Magnetic Environment
- It's not just electro-magnetic-manic-hyperbole when you hear it said that "just about
everything that runs on electricity these days interferes with my radio
reception." Here are a few things to try if all you hear on the
frequencies below 500kc is the roar of
intense static. 1. Check your house - Turn off everything you can in your house and see if the noise goes away. It's amazing, but LED lamps that don't cause any interference above the AM-BC band sometimes cause intense RFI noise below 500kc. Light dimmers are also notorious noise-creators. Wall-wart power supplies, various types of computer accessories, modern modulated furnace blowers, neon pilot lamps,...and just about anything "SMART." If just switching off everything in the house doesn't find the culprit then maybe the noise is external to your house. 2. Other External RFI Sources - External noise can be from any of the devices mentioned above but located in your neighbor's house. Modern real estate trends have houses built with virtually no space between houses making the proximity of RFI-creating devices much closer than they were (are) in older neighborhoods. Solar panel "levelers" and "inverters" can be very potent RFI sources. Reports are that the more modern versions of these devices have eliminated the noise,...maybe. "Grow Lamps" are notorious creators of RFI. Older street lamps using Hg-vapor or Na-vapor lamps can be very intense RFI polluters if the lamp is failing and switching on and off. Most new street light installations are using LED type lamps and they don't seem to create RFI. Some external sources can be "fixed" but most can't. 3. Shielded Magnetic Loop Antennas - If the RFI isn't from your own house then, usually, the listener has to come up with their own solutions to eliminate or, at least, reduce the RFI noise pollution. The most efficient device to use is the Shielded-Magnetic Loop antenna. This type of antenna is very effective at reducing RFI noise. These loops work great on receivers that were built after WWII. The Pixel S-M Loop performs quite well below 500kc and can be used (without too much loss) down to 150kc. Depending on the receiver's front-end design, sometimes S-M Loops won't work very well,...especially with early, 1920s receivers. This mainly due to the Primary LC Tuner's fairly high impedance that was designed for a 200' end-fed wire antenna. The S-M Loop's 75Z input impedance is far too low to work well with early-twenties receivers. It's possible to use an "un-un" balun designed for high-Z end-fed wires and hook-up it up backwards so the loop antenna is fed to the Lo-Z side and the Hi-Z side goes to the receiver. I've successfully used this method with a Rycom LF Receiver that had a 3500 ohm antenna input impedance. Unfortunately, the large wire array antennas that can perform quite well in rural areas can't be used in metro-urban areas. 4. Antennas and
Grounds - In metro-urban areas, with major industry running 24-7 and millions
of potential RFI creators, listening on MW and LW is going to be
impossible. Going mobile to a rural area, operating on batteries and
using some sort of "strung-up" antenna is the usual method for LF and MW
listening for urban dwellers (kind of like a "camp-out.") Suburban areas might have individual RFI
noise polluters that
can destroy any MW or LF listening with their EM RFI noise, but usually
these sources can be dealt with by using a Shielded-Magnetic Loop
operated with an impedance matching "un-un" or other such Lo-Z to Hi-Z
matching device. Shielded-Magnetic Loops DO NOT produce stronger signals
even though they employ a low-noise amplifier as part of their design.
The Shielded-Magnetic Loop provides a better signal-to-noise ratio and
it depends on the receiver having enough gain to take advantage of "not
so strong" signals that are in a much lower noise level. However, with
the 1920s Shipboard receivers, it might be found that the SM Loop signal
just isn't strong enough, even though it's impedance-matched and the
noise level is reduced. A remotely tuned loop is another option. These
are fairly large, maybe up to 10' in diameter, wire loops that are tuned
with varactor diodes. They are easy to build and the pick-up loop (inside
the tuned loop's field) can be designed to impedance-match the Hi-Z
antenna requirements. Due to the high-Q of the remotely-tuned loop, it
tends to work rather well in noisy areas. Remotely-tuned loops generally
produce stronger signals than the S-M Loop and they do have a history of
being used in the 1920s for direction finding applications. Many ground
stations in the 1920s used Beverage Antennas. These were two-wavelength
long antennas that were only about 15 feet off the ground. The Beverage
was directional and did provide moderate gain at a low noise level but it also required
substantial real estate for its installation. One has to remember that
the 1920s shipboard receivers were designed for a 200' end-fed wire
worked against the metal ship's ground that was in a salt-sea
environment (a really good ground that seeming went on forever.) The large antenna, the superb
ground, the excellent location (out at sea away from everything)
and the 1920s low-RFI noise environment is something that can't be
duplicated today. |
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References: 1. Hazeltine, the Professor - by Harold A. Wheeler, SE-1420 origins and history - published in Radio Age, April 1978 2. Radio Manufacturers of the 1920s, Vol 3 - RCA and Wireless Specialty Apparatus history - by Alan Douglas 1991 3. Westinghouse Type RB, photo of Type RB - by Alan Douglas - published in Radio Age, November 1982 4. Tropical Radio and Telegraph Co., United Fruit Co., NESCO, ISC, International Radio Telegraph Co. - Geo. C. Clark "Radioana," Wikipedia and various other online sources 5. "Keeping the Stars and Strips in the Ether" - RCA-Navy relationship, Creation of RCA by General Electric, Purchase of American Marconi by GE - from Radio Broadcast - June,1922 6. "SE-143 Operating Instructions" - RCA manual from Nov 1936 - available online. George Sterling's SE-143 section in "The Radio Manual" First Edition is actually much more detailed in the operation of the SE-143 7. "IP-501-A Manual" - RCA/RMCA from 1938 - available online. This manual has details on setting "Critical Coupling" that greatly improves MW performance. 8. "The Radio Manual" - Descriptions and Operating Instructions for SE-143, IP-501/SE-1420 - by George Sterling, 1st Edition 1928. The 2nd Edition from Sept.1929 has the IP-501/SE-1420 but dropped the SE-143 9. "How to Make Commercial Type Radio Apparatus" by
Milton B. Sleeper - No. 2 in a series of booklets on radio equipment
published in 1922 by The Norman W. Henley Publishing Co., NYC, NY |
NAVY-RADIO.COM - For the most detailed information and lots of photos of Pre-WWII stations, including many photos of SE-143 and SE-1420 installations and other early Navy gear and on all types and all vintages of Navy radio equipment, radio stations, vintage photographs - go to www.navy-radio.com Nick England's incredible Navy-Radio website has the most information available - anywhere! |
| Henry Rogers © Jan 2009 More info added Feb.2009, Apr. 2009, Corrections to RMCA information Dec 2015, more RMCA corrections and minor edits about LW stations June 2018, minor tweaking of RMCA history and production history of IP-501-A - Dec 2020, Added SE-143 RF Tuner, SE-1387 RF Driver, SE-1834 Universal RF-AF Amplifier - Jul 2026, Changed title to "Shipboard Radio Receiver Equipment 1918-1925" - Jul, 2026, |
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