Category Archives: WM

“SOME” DIGITAL MODES USED IN HAM RADIO (and signal ID guide, Thanks hfradio!)

Digital modes are becoming more and more popular on the amateur bands. This is mainly due to the following reason: Affordable home PC’s with built in soundcards. This has brought forth a multitude of decoding software, some free, others not. There are new modes being invented all the time and keeping track of these is turning into a full time job! One of the main problems encountered by the newcomer to digital modes (or digimodes as they are known) is how to identify what they are seeing/hearing. Most of the decoding software uses a visual ‘waterfall’ display to facilitate easy tuning.

With that in mind I went on the bands and captured images of the most common digital modes in use at the moment. Below you will see images of each mode together with some brief notes on the mode. The images show the most common variant(s) of the mode, although some have many different ‘flavours’! I will add to this list as and when I hear/identify a new mode that is being used on a regular basis (last popular ‘new’ one is Olivia which wasn’t around when I did this page on my original site)

Click on the name of the mode (where the name is underlined) to hear an mp3 of how the mode sounds on air (these are to give you an idea of how that mode sounds, not for analysis purposes) I have included some sound files of mode variants – more to come as I find them).


PSK, or Phase Shift Keying has become the most popular of the newer digital modes. There is a wealth of information on the web regarding BPSK (Binary PSK) and QPSK (Quadrature PSK)

Because PSK31 has a bandwidth of only 31Hz, many signals can fit into the same bandwidth that would be occupied by an SSB signal (2.4kHz approx.). It is quite common to see 15 or more signals on a 2.5kHz waterfall display.

A ‘clean’ BPSK31 signal. This is how your signal should look!

Here are a couple  of  BPSK31 signals that are badly distorted. This is probably due to overdriving. Reducing the input to the soundcard or reducing the output level would improve the quality of this signal. Note that although some way from the adjacent signal on the left, the distorted signal is sufficiently wide to cause interference to the other signal.

Here we see a station that has an unstable signal and is drifting badly. A stable and ‘clean’ transmitter is vital when using narrow modes such as PSK31 and it’s variants so as not to cause QRM to nearby stations


PSK63 is gaining popularity, with many programs now supporting this mode. The pro’s for this mode are the fact that data is sent and received at twice the rate of normal PSK31, so is great for chatting and contest exchanges. The con’s to this mode are the increased bandwidth required over PSK31, the increase in power required to maintain the same level of copy as PSK31 and that not all software decoders support PSK63.  PSK63 can be identified quite easily as it looks like a ’fat’ psk31 signal!

Other variations of PSK31 are PSK16 (half bandwidth/speed of PSK31); PSK125 (4 times bandwidth/speed) and other experimental variations such as PSK10 (to be found in MultiPSK) and even PSK250. The other  common variant of BPSK31 is QPSK31,  (the ‘Q’ stands for ‘Quadrature’, rather than the usual B which is ‘Binary’ Phase Shift Keying), which is sideband dependent (i.e. both transmitter and receiver must be using the same sideband) but is not in common use despite it’s superior decoding ability during poor conditions.

Here is an waterfall shot of QPSK63 (the wider of the signals. If you compare it to the BPSK63 signal above, and also on the left of the picture  you can see there appears to be more information contained within the same signal, this is the easy way to tell QPSK from BPSK.

This picture shows the bandwidth difference between PSK31 and PSK63, PSK63 being the wider signal.

Here we can see the difference between a PSK31 signal and a PSK125 signal. The PSK125, although much faster, takes 4 times the bandwidth and requires 4 times the power for the same s/n ratio as PSK31. It is a great mode when conditions are good and signals are strong, especially on the higher bands where there is more space.


SSTV (Slow Scan TV)

Slow Scan TV has been popular for many years, although the vast majority these days is computer generated. The most common modes are Martin and Scottie. Robot still has a following. Most SSTV programs handle these modes and others too. The received pictures are built up line by line over the course of nearly a minute so you need to be patient! Quality can be very good, even over long distance paths. Here are two pictures received by me — the topmost one is from Hawaii (KH6AT) and the bottom one is from Sweden (SM7UZB).



RTTY (Radio Teletype)

The ‘original’ data mode. RTTY (pronounced ‘Ritty’) has been around for many, many years and is still just as popular. Years ago the only way to get on RTTY was to use a mechanical terminal unit such as the Creed 7 series, which were big, noisy and messy. These days, virtually all RTTY is done by the computer/soundcard combination. Amateurs (hams) use 45 baud (the speed) with 170Hz shift (between mark and space). Commercial stations use 50 or 100 baud with shifts of 425 or even 850Hz. Most software caters for differing speeds and shifts. Unlike most digital modes, RTTY is transmitted on LSB.




MFSK is similar to the commercial Piccolo system. MFSK is very good under poor propagation conditions. The usual variant of MFSK is MFSK 16, but other types such as MFSK 8 are in development, along with other similar modes to MFSK (such as Domino). MFSK is sideband dependant, so you must have your receiver set to the correct sideband in order to decode it properly. Also tuning is quite critical, although AFC helps somewhat. The top image is of an MFSK16 signal and the lower image is of an MFSK32 signal (which as you can see is nearly 500Hz wide, twice as wide as an MFSK16 signal).




MT63 is very robust and offers 100% copy when other modes fail. The tradeoffs however are bandwidth and speed. MT63 is quite slow and occupies anything from 500Hz to a full 2kHz (which is still less than a single voice channel). Because of the wide bandwidth, MT63 is usually confined to 14MHz and above, where there is sufficient space to accommodate it.

mt63 long2_308x85



Hellschreiber (or Hell as it is commonly known) is a bit different from most other data modes. When receiving a Hell signal, your eyes do the filtering! The decoded text is displayed on a ‘ticker tape’ display (as shown in the picture). Hell has a very distinctive ‘grating’ sound and is a narrow band mode. The Hell signal is on the left of the picture (with the green flag above it), with an MFSK signal on the right—note the bandwidth required for the MFSK signal compared to the Hell signal. Even weak signals can be decoded as your eye/brain combination can ‘fill in the blanks’ where the signal fades.

Here is a waterfall of a Hell signal, together with a decode (showing how it appears on screen)

feld hell 2feld hell



HF mailboxes etc. use packet to forward messages to users. The usual data rate on HF is 300 baud, with 1200 and 9600 baud being common place at VHF and UHF. The picture shows a mailbox/BBS in Turkey negotiating with a BBS in the UK. The short burst at the bottom of the picture is header and callsign information whereas the longer burst is the actual data. Several of these packet BBS/mailboxes can be heard chirping around 14.1MHz.




HF mailboxes etc. also use PACTOR  to forward messages to users. PACTOR has had a lot of bad press recently, mainly due to the actions of a few inconsiderate operators who are apparently causing interference deliberately to existing users of the digital sub bands. I cannot comment on this as I have not experienced it personally. The picture shows the PACTOR signal trying to establish contact. Once established the transmission of data can begin. Because PACTOR uses error correction, it can take quite a time to send a message particularly over a less than perfect path—but the transmitting station will keep trying until the message is received perfectly. The picture is of a PACTOR 1 signal, however there are PACTOR 2 and 3 variants, but these require hardware encoders/decoders.




Throb is one of the newer digital modes and although it can be heard, it is nowhere near as popular as other modes such as PSK31 or RTTY. As with the other modes, there are various variations of Throb, 1 throb/second; 2 throbs/second and 4 throbs/second. 1 throb is the slowest and 4 is the quickest. Throb is actually quite a slow mode and is therefore probably quite resilient to the effects of fading etc. although is does take quite a time to complete a contact!

throb1-1_76x111throb2 - 16_78x108throb4_99x102

Left to Right: Throb 1; Throb 2; Throb 4 (click each type to hear the different sounds).



Olivia is a fairly new digital mode and it seems to be extremely resistant to fading and QRM. I can get full copy on stations that are barely audible (even ones that fade down to almost zero seem to still print well). As with other modes, Olivia has different variants each having a different bandwidth (from 500Hz to 2kHz) and different number of tones. Olivia can be very slow (in the order of 2-3 characters per second) but a slow contact is better than none at all! In the below pictures, the 8/250 indicates 8 tones over a 250Hz bandwidth and 32/1000 is 32 tones over a 1kHz bandwidth. To avoid interference to other stations is it usual to start an Olivia transmission on a full kHz (i.e. 14.108.0 rather than 14.108.3 for instance).


Here are some waterfall shots of some other Olivia modes:

olivia 8-250olivia 32-1000



Contestia is another very new mode to be found on the ham bands. It is not, as yet, very popular and so far I have heard only one station transmitting this mode. Again I have included a sound file and a waterfall capture so that you may see what it looks and sounds like. This image is of a Contestia 4-250 signal from RW3AS on 20m.




JT6M is a specialised mode found in the WSJT software suite  (from Professor Joe Taylor, K1JT) designed for weak signal working (such as EME—Moonbounce and Meteor Scatter). JT6M is the favoured mode for MS and Sporadic E and can be heard on 6m around 50230.  I have done some monitoring recently using JT6M and have seen full decodes from stations that were not audible to me by ear, which I think is quite impressive!



Similar in principle to the broadcast DRM signals heard on the SW broadcast bands. DRM is a very experimental mode at the moment, with the main exponents being found on 80m around 3733kHz. I have not had much success with this mode as yet, despite having good signal levels. The signals need to be very clean and strong in order to decode. Pictures can be sent using DRM, but time will tell as to how/if this mode grows in popularity. Below is a waterfall ident from DD9ZO, sadly this station was not strong enough to decode. This mode does not seem to have taken off in the way that others have, mainly I think due to the fact that it requires a very strong and noise/fade free signal in order to decode. This is much like broadcast DRM. Unfortunately, the disadvantage with this mode and most other digital modes is that the signal is either fully readable or not copiable at all. With analogue signals (and some digital modes) you can usually fill in the blanks when you get fading or noise on the signal, also they are copiable when they are barely audible. Some newer modes do work very well at signal levels that are at or below the threshold of human hearing (WSPR for instance, which is mode that has only been around for a few months but unfortunately it is a one way mode, that is it is a beacon mode rather than a ‘conversation’ mode).




If you tune on 14.233 you may well hear a strange signal that sounds very similar to the HAM DRM signals mentioned above. This will be one of the new Digital SSTV modes. Like all DRM modes, Digital SSTV produces excellent, noise/distortion free pictures which can be in high definition. However for this to occur, the received signal needs to be very strong and relatively free from noise etc. If the program loses any part of the signal, due to a noise spike or a brief fade, the whole picture is lost. This is the big disadvantage with this mode on HF, it really is all or nothing. The software I am using to decode this mode is called  ‘EASYPAL’ and is available from . If you don’t want to transmit a picture, you can send short text messages in the ‘waterfall’. I haven’t used this program much so don’t know all the ins and outs but it’s good to be able to decode this new mode. Below is a waterfall grab of a digital SSTV signal (as seen in the MixW waterfall)

hd sstv-4

Example of waterfall text received in EasyPal

hd sstv-5

Digital / HD SSTV picture received on 14.233MHz in August 2010


Here are some more pictures captured using EasyPal, on both 20m and 80m. I am finding that there is more activity now than when I originally wrote this piece. The pictures are of stunning quality and, as they are digital, there are no traces of noise, QSB or any of the other problems that affect analogue SSTV pictures. The downside is that with these you either get the entire picture, or nothing at all – plus the transmission time seems rather lengthy. You do need a strong/clean signal in order to use digital SSTV, but it is well worth it. There are some received pictures I cannot show on this site as they are rather ‘risqué’ and show women in various states of undress – pleasing to the male eye, perhaps, but not really suitable for ham radio.

These were received on 80m (again, note the quality of the decode, even on the noisy 80m band at night:



And here are some from 20m:




Here is another of the new modes which can be decoded by many different software packages. Domino is another mode that uses MFSK (Multi-Frequency Shift Keying). MFSK sends data using many different tones, sent one at a time. As with ‘normal MFSK, it has excellent performance but was developed specifically to cope with the noisy conditions of the lower HF bands. For more information and technical details, visit:

As with the other MFSK modes (such as MSFK16, Throb, Olivia etc.) Domino is used with different parameters, the best mode variant to use is dependent on band conditions.

domino1 - 8_109x121domino1 - 16_169x106domino2 - 8_111x102domino2 - 16_175x108domino3_169x95DominoEx

Above Left to right are:

DominoF 1-8; 1-16; 2-8; 2-16, Domino 3 and lastly DominoEX. However DominoEX (click to hear sound file) has superceded DominoF. Like DominoF, DominoEX has a multitude of variants to suit various bands/conditions..


Thor is a new mode and is very closely related to DominoEx. It is an extremely robust mode and is well suited to HF weak signal conditions. A single carrier of constant amplitude is stepped between 18 tone frequencies in a constant phase manner. This means that no unwanted sidebands are produced, and it does not require the same kind of linearity requirements as some modes (PSK in particular). The tones change according to an offset algorithm which ensures that no sequential tones are the same or adjacent in frequency, considerably enhancing the inter-symbol interference resistance to multi-path and Doppler effects. Thor, like other similar modes has a variety of speeds and tones to choose from, dependent on band conditions and signal levels. The modes are Thor 4, 5, 8, 11, 16 and 22. Speeds vary from the equivalent of 14wpm right up to 78wpm for Thor 22. and bandwidths vary from 173Hz up to 524Hz.


THOR 16 better 2

This is a waterfall grab of a Thor 16 signal.


JT65 was developed originally as part of the WSJT weak signal modes software package by Joe K1JT. JT65 can also be decoded by other packages, such as MultiPSK. The screen grab below is taken from MultiPSK. JT65 has found a use on HF and can be found around 14.076MHz and 21.076MHz amongst others. Signals that are virtually inaudible can give perfect copy so its  performance is excellent on the noisy HF bands. The transfer rate is slow, as are most modes that excel in low signal decoding. I am now monitoring JT65 most days and am amazed how well signals come through, day after day!

jt65a in multipsk 2jt65 2jt65 1


This is a screenshot of another JT65 program. This is JT65-HF by W4CQZ, a free decoder that is specially written for those of us that like to play around with JT65 on the HF bands. I have been using this for quite a time now, and I am very impressed by it. I like the interface, it is easy to use and easy to set up. It will decode multiple signals at the same time and stores the results in a CSV (comma separated values text) file for later analysis. Another useful feature is that, like DM780, it sends spots to the PSK Reporter website and they are displayed on a map. You can interrogate the system to display all spots seen by any particular callsign etc.  As you can see from the above screenshot JT65 works very well on HF and I have heard signals from all over the world from stations using fairly simple equipment and low power. Also the program reports to the RB (reverse beacon) network, which is found at: . The above screenshot shows stations in Brazil, UK, Netherlands and Asiatic Russia, all on a very quiet 10m band.


JT65 grab

This screenshot shows the spots my receiving station has sent to the PSK reporter network over a 24 hr period, using JT65a. As you can see, all four corners of the world have been heard! There are some stations active from Africa, mainly in South Africa (ZS) and it is not uncommon to hear them – however none were active then this screenshot was taken.

I have decided that in 2011 I will be devoting a fair amount of time to JT65a (each year I choose a particular mode or band that takes preference – in the past I have done CW, 160m, PSK31, WSPR, 6m and now is the turn of JT65). There has been a marked increase in JT65a activity on the HF bands, mostly due to the efforts of Joe and his excellent JT65-HF software. I am intending to promote activity on this weak signal mode wherever possible. When using this mode, it is advisable to keep the transmitter power to 50w or less or no more than half the rated output of your transceiver. Most of the time 20-30w is more than adequate and quite often contacts over amazing distances can be achieved using just a couple of watts. It is interesting to note that even when a band appears to be closed, the chances are that there may well be a JT65 path open. If you have restricted antennas, power or both, this could be the mode for you. Signals that are 24dB below the noise level can be decoded with relative ease.

Joe is constantly developing the software and releases new versions regularly. Each release sees a further improvement in functionality, but without sacrificing ease of use.

To download the latest version of the software (v1.093), click HERE.


This introduction is taken from Joe Taylor (K1JT)’s WSPR 2.0 online user guide. WSPR (pronounced “whisper”) stands for “Weak Signal Propagation Reporter.” The WSPR software is designed for probing potential radio propagation paths using low-power beacon-like transmissions. WSPR signals convey a callsign, Maidenhead grid locator, and power level using a compressed data format with strong forward error correction and narrow-band 4-FSK modulation. The protocol is effective at signal-to-noise ratios as low as –28 dB in a 2500 Hz bandwidth. Receiving stations with internet access may automatically upload reception reports to a central database.

For more detailed information on WSPR and to download the programs, see the WSPR website or the WSPRnet website where the database etc. are hosted.

wspr waterfallwspr screen grab3


Here are the USB dial frequencies for WSPR:

Band Frequency (MHz)
LF 0.502.4
160m 1.836.6
80m 3.592.6
60m 5.287.2
40m 7.038.6
30m 10.138.7
20m 14.095.6
17m 18.104.6
15m 21.094.6
12m 24.924.6
10m 28.214.6
6m 50.293.0
2m 144.488.0


Below is a summary of stations heard on WSPR over course of a month (27 November to 27 December 09).

30m has been the band I have spent most time monitoring as can be seen by the fact I have decoded over 270 stations on that  band alone. What I have found strange is the lack of African stations – not a single one has been decoded to date. I guess it hasn’t caught on over there yet. Hopefully as the mode develops and interest increases some stations will take it up as it would be interesting to see how the propagation paths to Africa open and close during the course of a day or month. Asia is quite sparse too here. I know there are stations on from Japan etc. but I am not hearing them here very often. Same with Australia. No path to VK for me yet. It is nice to see some North American’s on 80m, proving that there has been a path most nights and it should be workable with modest powers and antennas. If I can hear a 1 watt American station on 80m WSPR at a reasonable level,  then I should be able to hear ones running 100w of CW/SSB or 30w of PSK with little problem.

By Continent
17m 8 1 7 0 0
20m 28 17 11 0 0
30m 273 223 48 1 1
40m 30 29 0 1 0
80m 177 169 8 0 0
160m 63 62 0 0 1

Over the past few weeks I have been transmitting on WSPR (and a few other modes) with 5 watts or so into my inverted Vee and have been very impressed with the results. I still feel that I would be better with proper dipoles for each of the main bands I am interested in and I will hopefully work on that during the summer.


I have now been using the OCF dipole/Windom arrangement for a few weeks on various bands/modes and can report that it works well although it does not have quite the same impact on 30 and 40m as the G5RV. The reason is because tthe OCF is designed for use on 20m and above so operation below 14MHz is a compromise. That said, it still radiates a fairly good signal on 30m as borne out by the WSPR reports I have collected.

So far this year I have been heard in 56 entities, which are:

Prefix Country/Entity
4X Israel
9A Bosnia
9H Malta
CT Portugal
CX Uruguay
DL Germany
EA Spain
EA6 Ballearic Isl
EA8 Canary Isl
EI Eire
ES Estonia
EX Kyrgyzstan
F France
FR Reunion Isl
G England
GI Northern Ireland
GM Scotland
GW Wales
HB9 Switzerland
I Italy
JA Japan
KH2 Guam
KL7 Alaska
KP4 Puerto Rico
LA Norway
LU Argentina
OE Austria
OH Finland
OK Czech Republic
ON Belgium
OX Greenland
OY Faroe Islands
OZ Denmark
PA Netherlands
PY Brazil
S5 Slovenia
SM Sweden
SP Poland
SV Greece
T6 Afghanistan
TF Iceland
TK Corsica
UA0 Asiatic Russia
UA3 European Russia
UN Kazakhstan
UR Ukraine
VE Canada
VK Australia
VU India
YO Romania
YU Serbia/Montenegro
YV Venezuela
Z2 Zimbabwe
ZL New Zealand
ZS South Africa

As you can a see there are a spread of countries from all continents, which is gratifying as it means that I am at least radiating some sort of signal in every direction.

Here is a summary, by band, of where my WSPR signals have been heard (The term ‘ODX’ refers to ‘longest distance’, so in this table ODX means the furthest that I my signals have been heard):


Band ALL 10m 17m 20m 30m 40m
Hrd by number of stations 630 46 26 366 336 49
ODX (km) 18934 2078 12028 18934 18934 14549
Avg Distance (km) 2534 793 3057 2420 2538 1188
Hrd in DXCC 52 11 15 46 40 15
Lowest SNR reported -33dB
Highest SNR reported +11dB
WW QRA locator Squares: 264

So from this I can see that on 10m there have only been reports from single hop sporadic E openings and the average distance on that band is quite short at just under 800km. This short distance is due to the MUF being high and the skip distance decreasing as a result of the higher angle reflections. I have not spent much time on 10m because the high MUF sent me packing up to 6m where the band would usually be open. There have been multi-hop Es on 10m, but I have been on 6m when these have been about! On the 20 and 30m bands there is not much to choose between them and the average distance is about that of a single F-layer hop. The 40m average is about half the distance so my antenna must have quite a high angle of take off to reflect at this short distance. Experiments like this are interesting in assessing antenna effectiveness. I can see that even though my antenna is 3/4 of a wavelength above ground, it is physically short (a quarter wave in length, but the feed arrangement does not make it an efficient DX antenna on this band). However it does seem to be suited to local/semi local (i.e. within the UK and Europe) working – with the odd longer distance QSO possible when conditions are favourable. Looking at the signal to noise ratios (SNR) there is a huge difference between the strongest and weakest (44dB – that means that the best SNR is over 20,000 times stronger than the worst SNR!). -33dB is extremely weak and must be right at the very limit of the decoding capability of the software. To quantify this and put it into figures that are more easily understood, say I was running 1 watt output and my signal was received with an SNR of -33dB, in order for me to improve that report by 10dB, I would, in theory,  need to increase my output by 10 times (which is 10dB), therefore I would need to run 10w. To increase my received SNR by a further 10dB another 10 times power increase is needed – taking my output power to 100w (10x10w). A further 10dB increase (giving a 30dB overall increase) would take the power output to 1kW (1000w) or a 1000 times our starting power. Reversing the situation, let’s see how that kind of change would affect the s-meter of a receiver. S-meters are not usually that accurate and calibration can be all over the place. there is a standard though and that is 6dB per s-point, so if we say the worst SNR gave a reading of s1, the best SNR would indicate just over s7. If we were talking about pure signal strength this would be the case, but with Signal to Noise ratios this would not be true as we are talking about dB above the noise level and dB below the noise level. The human ear can decode CW signals down to about -15dB or possibly -18dB SNR but certainly not much, if at all, lower than that (and believe me, that is a weak signal and takes all your concentration to hear it!). That is still a good 15-18dB above the weakest SNR that WSPR has decoded my signals at!


ROS is a fairly new mode that is in it’s first year or two of use. ROS uses multiple tones over a 2kHz or 500Hz bandwidth, (the frequencies for each mode/bandwidth are hard coded in the software which is causing some annoyance amongst some users. ROS has three main speeds, 16 baud, 8 baud and 4 baud. There are some special modes, such as 7bd/100Hz for 136 and 502kHz (and 80m for some reason), plus an ‘EME’ mode for use on 2m and some other bands, for weak signal work as it has, in theory at least, the capability to decode signals that have a Signal to Noise Ratio (SNR) of -35dB, which is even lower than  WSPR. There are, however, questions as to the legality of using the mode on HF in North America, as spread spectrum is not allowed below 222MHz and the authorities are still undecided if ROS is SS or not.

This will all be hammered out as the mode grows. It will either become widely used or, as is sometimes the case, just disappear through lack of interest. Only time will tell on that. One thing that has come to light is that ROS has just been accepted into the ADIF standard (Amateur Data Interchange Format), which is the common ‘language’ that is used for exporting and importing log data. Also (the electronic QSL exchange centre) has updated it’s system to accept ROS QSO’s.


Click on pic below to hear the sound of 16 tone, 500Hz ROS

ROS 500Hz-4ROS 16

The above pics are taken from the ROS program, which uses a monochrome waterfall. As most software uses a color waterfall, I have included a screenshot of a ROS signal (in this case the same as above, 16 tones / 2000Hz) as viewed on the HRD waterfall.

ROS 16-2

To download the software and users guide: – it is worth checking there at least weekly as new versions are being released frequently in response to users requests for features etc. (the latest version is v 7.0.8). Here are the latest frequencies, as of May 2012. Note: these are considerably different to the previous version that appeared on this page.

136 kHz 2190m
500 kHz 600m
1840 kHz 160m
3583 kHz 80m
3585 kHz 80m
3587 kHz 80m
3589 kHz 80m
5367 kHz 60m
7040 kHz 40m
7044 kHz 40m
7046 kHz 40m
7048 kHz 40m
10132 kHz 30m
10134 kHz 30m
14101 kHz 20m
14103 kHz 20m
14116 kHz 20m
14118 kHz 20m
18107 kHz 17m
18111 kHz 17m
21110 kHz 15m
21115 kHz 15m
24916 kHz 12m
24926 kHz 12m
28185 kHz 10m
28295 kHz 10m
50245 kHz 6m
144160 kHz 2m
144980 kHz 2m
432097 kHz 70cm

There is a buzz of excitement as Joe Taylor, K1JT, has now released the first version of WSJT 9 – which can be downloaded from: There are some new modes in this version although I have not had time to investigate them as work is very busy at the moment and will be for another few weeks. There was a brief beta test version of WSJT, version 8, that investigated a host of new modes and this research and it’s findings have gone into producing the public release of version 9. I will provide more information on these modes as it becomes available (screenshots and mp3’s etc). It’s a busy time in digimodes, there always seems to be a new mode or refinement of an existing mode being released. ROS is still finding it’s feet and is under constant development – it still has its critics, but that is true of most modes but it does seem to be getting quite popular, although I doubt if it will ever be as widely used as, say, PSK31.


RSID is a method of identifying certain digimode signals. RSID stands for “Reed Soloman IDentifier”. The way it works is that the station who is transmitting can, in certain software, enable RSID. When enabled, RSID sends out a numeric code in the form of an MFSK signal which is identified by the receiving software (if it is capable of RSID) and sends alerts to the user and advises of the mode used. This is particularly useful with the lesser used/recognised modes, however it can be rather tedious to have an alert every time someone starts transmitting in, say PSK31 or RTTY as these are extremely common modes and you can find yourself inundated with alerts. In some software RSID can be configured to be active for certain modes only. In DM780, a box appears on the desktop alerting the user to a transmission and gives the frequency and mode (such as Olivia 23/1000 on 1500Hz) and you can tune to that transmission by clicking on the alert box which will change the mode and frequency of your radio (providing you have computer/software control set up).


Video ID is different to RSID in that it can be seen by anyone using software with a waterfall display. Again, video ID is enabled in the transmitting software and it is not supported by every software. If you are watching a waterfall trace, you may, at the end of the transmission, see some text or even a crude picture in the actual waterfall – this is video ID and confuses many people who have not seen it before.


waterfall pic sstv 2
psk125 with 73 pic


Below are some less common modes, together with sound files. This list is certainly not exhaustive (not by a long, long way!) but it might just give you an idea of what that strange noise was that you heard when tuning around on SW. New data modes are emerging all the time and it is difficult to keep up with them. I usually follow the development of new modes that I think might interest me – some of these modes become popular, some much less so.

Unfortunately I do not have waterfall traces for these signals yet, but I will endeavor to track some of these signals down and capture them (that’s why they call it ‘hunting’ 🙂

For technical details of the modes below, and others, visit: (where some of the following information has been verified/sourced.)

SITOR: SITOR  is a commercial teletype mode it means SImplex Teletype Over Radio) used for sending text messages between stations, SITOR may be run in interactive (ARQ – Automatic  Repeat reQuest) mode, which is known as SITOR-A (also called AMTOR). When SITOR is run in broadcast (FEC – Forward Error Correction) mode, it is known as SITOR-B (or NAVTEX). The mode uses special error correction techniques. There are many ARQ and TOR modes to be found on the HF bands, SWEDISH ARQ, G-TOR and CLOVER are just some. If you start investigating, you will be surprised by just how many commercial digital modes are in use.

CHIP: This mode was created by IZ8BLY back in 2005. Chip is a PSK mode which uses “Spread Spectrum” modulation and comes in 2 variants, Chip64 and Chip128. Chip has a bandwidth of almost 600Hz, but is an extremely robust mode and has a good throughput speed.

ALE: (Automatic Link Establishment), is now finding more use in amateur circles, thanks to the efforts of the writers of some of the multimode decoders, such as MultiPSK. ALE, when running correctly, can initiate and establish connections between two stations without human intervention (hence the ‘Automatic’ part.)

PAX, PAX2: PAX is another MFSK mode which is derived from Olivia. PAX2 is the same as PAX but runs at a higher baud rate (62.5bd for PAX and 125bd for PAX2), therefore PAX2 is twice as fast as PAX but requires a better signal to noise ratio. The following frequencies are used for PAX/2: 3.590, 7.042, 10.148 and  14.075MHz .

STANAG: Used by the military, comes in many different variations. Pretty much all Stanag traffic is encrypted. STANAG 4285 is the NATO standard for HF communication. It consists of several sub modes (75-2400 bps) and two different interleaving options (short and long). The receiver should be in USB mode and provide flat frequency response from 600 Hz to 3000 Hz. Another Stanag mode is 5066, which includes mode identification in it’s data and can therefore be detected correctly by multimode auto detectors that are built into some software.

HFDL: HFDL stands for High-Frequency Data Link. It is used on the HF bands and is a comprehensive, global, air-ground, communications system. (It also uses VHF and satellite). ACARS (Aircraft Communications Addressing and Reporting System) is part of  this system and with the appropriate software, aircraft routes and progress can be seen on a pc screen. HFDL is a single-tone, phase-shift keyed, text-based, error-checking mode, with a base band audio carrier frequency of 1440 Hz. It is tuned in USB, and the 1440 Hz center is critical for decoding. (Thanks to Monitoring Times blog for the info on this)

NAVTEX: NAVTEX is a world-wide system which transmits navigational and meteorological warnings, and urgent information through coastal stations. Transmissions are on 490kHz (National NAVTEX, broadcasts in local languages) or 518kHz (International NAVTEX, in English), in FEC/SITOR-B mode with special coding. The receiver should be in USB on 489 or 517kHz. Transmissions are at fixed times, the schedules for which can be found on the internet ( is one source).

navtex 517-2

NAVTEX transmission received on 518kHz on 9th October 09, the text shows the co-ordinates of two special buoys.

SYNOP: Synop is used by ships, and shore based weather stations to report prevailing conditions and forecasts. It is RTTY that has specially coded messages which allow the display of ships and weather buoys/stations and shows weather forecasts and conditions, when used in conjunction with the appropriate software. There is a SYNOP station on 10.101MHz in Germany, it runs at 50baud, with 425Hz shift and is reversed/inverted (when received on USB).

COQUELET: Screenshots and audio are being prepared. This mode is not used a great deal on HF but can sometimes be heard on 18.181MHz where there is an Algerian station (possibly a diplomatic service) that uses Coquelet and broadcasts some non encrypted text in French.


coqulet 8 on 18181-3


coqulet 8 on 18181-4


Using DM780 (part of the excellent and free Ham Radio Deluxe radio control, logbook and decoder package, by Simon Brown HB9DRV) and PSK Reporter (By Phil Gladstone) I am able to set my radio up on any one of the designated PSK31 frequencies and let it monitor for as long as I wish. Each time a callsign is decoded, it is logged, along with its WWlocator. These locators are shown on the PSK reporter page as pins in a scalable map (the map can be displayed as a map, a satellite image or a hybrid of both). Occasionally a callsign is recorded that is not correct (might be a fragmented call or a call that has been corrupted due to noise or QRM). These are surprisingly rare considering the amount of traffic that the program decodes and shows just how good the programming is. It is fascinating to see the map at the end of a monitoring session, and seeing what the chosen band has had to offer that day. I have been doing this for some months now and am noticing interesting propagation trends that tie in with established theory. Below are some screenshots from the DM780 program taken at various times and dates that  illustrate the diversity of stations on the air. Some callsigns appear most days, others of course are only heard once.

Click on each map for a bigger and more detailed picture, then use your browser ‘back’ button to return here.


L-R:  PSK31 stns on 20m (23 Aug 09); PSK31 stns on 20m (25 Sep 09); DXCC count on 20m PSK31 (2 weeks monitoring)

4_192x1125_194x1186 oct 09 20m_341x129

USA on 20m PSK31 (25 Sep 09); DXCC count on 20m PSK31 (1 month monitoring); Screenshot of 20m taken on 6 Oct 2009 showing stations heard on all 6 continents (for ‘All Continents’ awards, Antarctica is not counted) on 20m PSK31. Although I have shown stations from all continents, they were not the first heard from the particular continent. I have chosen the stations listed below because they have the shortest time frame from first to last.

Elapsed time between hearing the first continent and the last was a mere 53 minutes! just think how quick it could have been done if I was using good antennas!

Continent Time Callsign
Africa 1620 EA8CCA
Europe 1624 IW5BAX
Asia 1631 RU9SL
N.America 1637 W5NA
Oceania 1639 YB4IR
S.America 1713 PT7DX


It is not unusual for me to hear over 90 countries on PSK31 during the course of a week (last week was 96 for instance), certainly that has been the case over the spring/summer, with 50-60 countries per day being about average. – and that is at the sunspot MINIMA! I would think that in a few years time I should be hearing over 100 countries in a week without a problem. Bearing in mind I am using a very low antenna, it just goes to show that even when you think the bands are quiet and there is no propagation – most of the time you would be wrong! 20m has been open from early morning to late night, and probably 24 hours but I have not monitored in the small hours of the early morning – yet!


Below are some shots taken from the ‘Spectrum Laboratory’ program (freeware). Each shot covers about 1 hour of elapsed time and shows the amount of activity on the given sub band during that time. Click on each thumbnail for a full size image, together with explanatory text.




**If you have problems playing back the MP3 files  please read this, it might help:-  I found that Windows media player would not play one of my mp3’s but Quicktime would. Having done some research I see it is a common problem with WMP.  Use the free Apple Quicktime player or similar – also consider installing a codec pack (again many can be downloaded and installed for free) such as the AC3 codec pack and that will (or should allow you to play any, or most,  mp3’s you come across as well as other formats)**

To read a more updated info you can visit the Source of this article here :

OLD-SCHOOL stuff: “How to Become a Wireless Operator (1916)”

This eight-part series gives directions for constructing a tuned spark transmitter plus a crystal receiver. This article doesn’t mention anything about licencing, apparently under the assumption that the transmitter’s range was limited enough not to require it. One feature omitted from this review, which likely would have come in handy, was some sort of setup to disconnect the outside aerial during lighning storms.

Popular Science Monthly, September, 1916, pages 449-452:

How  to  Become  a  Wireless  Operator

I.–Why  Wireless  is  Interesting

By  T.  M.  Lewis
NOBODY knows just how many amateur wireless operators and experimenters there are in the United States; the total number has been estimated as somewhere between twenty thousand and fifty thousand. Nearly ten thousand licenses for amateur stations have been issued by the Department of Commerce. Each one of these licenses is for an amateur station which contains both a transmitter and a receiver. No license is required for stations equipped for receiving only, and it is believed that there are many more of these than of the sending stations.
Why have so many American boys and young men taken up this subject? What is there about it that interests them, and induces them to spend their time and money in buying, building and using wireless instruments? The answer to these questions is simply that wireless or radio telegraphy represents one of the latest developments of electrical science, and that it offers both amusement and profit to whoever cares to work upon its problems.
Whether you wish merely to make a pastime of wireless experimenting or desire to study radio telegraphy with the intention of making some part of it your profession, you will find time spent on it well worth your efforts. In the first instance you will be able to receive messages through the ether from stations many miles away, getting press reports of important news items, and the results of races and ball games and so forth, before they are published in local papers. In the second case, you will be able to train yourself as a radio operator or installation engineer, or possibly you will make new inventions or discoveries of commercial value. Either way you will constantly be learning more and more about electricity and its applications, as well as getting a better knowledge of many important physical principles which may be used in almost any kind of work.
In addition to all this, there lies before you the fascination of sitting at your receiving instruments and listening to wireless messages from stations located all about you. Soon after you begin it is possible to hear from distances of several hundred miles, and after you have gained a thorough knowledge of your instruments and their possibilities it becomes feasible to listen to the tremendously powerful transmitters even so far away as Germany and the Hawaiian Islands.

Elementary  Principles

This article is the first of a series which will describe a number of really practical and useful instruments for use in radio telegraphy, both for sending and for receiving. The ways to make and use these various pieces of apparatus will be discussed in detail, but it is not proposed to go into the theory of wireless telegraphy at all. By going to your library you will be able to find books and periodicals which describe the principles of ether-waves and their uses in wireless; some of the books you will wish to buy and have in your own workshop for ready reference. Among the most interesting and valuable of these are the following, which are named in the approximate order of their complexity:
“The Elementary Principles of Wireless Telegraphy,” by R. D. Bangay.
“Experimental Wireless Stations,” by P. E. Edelman.
“Wireless Telegraphy,” by A. B. Rolfe-Martin.
“Textbook on Wireless Telegraphy,” by Rupert Stanley.
“Wireless Telegraphy,” by W. H. Marchant.
“Elementary Manual of Radio Telegraphy,” by J. A. Fleming.
“A Handbook of Wireless Telegraphy,” by J. Erskine-Murray.
“Wireless Telegraphy,” by J. Zenneck, translated by A. E. Seelig.
The above list should be useful as a guide in hunting for technical information about radio telegraphy. There are many other books on the subject, a large number of which are excellent. Those named, however, include one or more of each type from the most elementary to the most advanced.

A  Simple  Transmitter
Fig. 1
In beginning experiments on wireless telegraphy it is best to take up first the least complicated arrangements, which are suitable for very short distances, and then to work along gradually from these to the more important instruments. This first article, therefore, will describe the use of a complete wireless set which is capable of demonstrating the principles involved. By its use you should be able to send messages a distance of a few hundred feet, from one part of the house to another; by using long aerial or antenna wires, upward of a quarter of a mile may be covered.
The sending station involves nothing more than a simple buzzer, a telegraph key, a tuning coil and a few cells of dry battery. These are to be connected together as shown in Fig. 1; a good kind of wire to use is No. 18 annunciator, since this has a strong waxed double cotton covering which is easily removed. The buzzer can best be purchased from any electrical supply store for about forty cents; the key may be bought, or simply improvised by cutting and bending some thin strips of brass as shown in Fig. 2; the dry cells will cost from twenty to thirty cents each.
The tuning coil may easily be built by winding about fifty turns of annunciator wire on a cardboard tube approximately three inches in diameter. The ends may be fastened and at the same time made available for convenient connection by attaching them to binding posts let into the tube at the top and bottom. There is no need of building this tuning coil of any specific size. The diameter may be anything from two to four inches, and the number of turns from thirty to seventy. It is only necessary that two identical coils be built, one for the sender of Fig. 1, and the other for the receiver of Fig. 4. Fig. 2
In setting up the sender it will be found that one end of the tuning coil must be attached to the contact post of the buzzer, which is marked 3 in Fig. 1; this can be done by removing the cover of the buzzer and wrapping a bare copper wire firmly about the post. Care must be used to prevent the contact wire from touching the metal base, however, or the operation of the buzzer will be stopped. Binding post 2 is to be connected with “earth” as indicated at E in the diagram. The earth connection is easily made by running a wire to a water pipe or steam radiator and wrapping the bare end tightly about a scraped or plated portion of the pipe. The upper end of the tuning coil is to be led to the aerial or antenna wire, at A. This antenna may be of any convenient size, but the larger it is the farther you will be able to signal. For transmitting from room to room within the house, it will be sufficient to string some twenty feet of wire around the picture moulding near the ceiling.
If you have set up the apparatus properly the buzzer will hum strongly as long as you hold down the sending key and thus close the battery circuit. By pressing the key for short and long intervals you can produce short and long buzzes which correspond to dots and dashes in the Morse telegraph code; in this way messages can be spelled out letter by letter.

A  Microphone  Receiver

For the receiving station you will need to make another ground connection by fastening a wire to the steam or water pipes, and then the next thing is to build a second antenna or aerial wire system exactly like that at the sender. The second tuning coil, an old dry cell (preferably one which has become very weak), a telephone receiver and the microphone detector are to be connected together as shown in Fig. 4. Any telephone receiver will do; you can buy a 70-ohm watchcase instrument from an electrical store for about 75 cents, but if you intend to continue with wireless experimenting it will pay you to invest several dollars in a pair of telephones of high sensitiveness. These will not only make it possible to receive messages from longer distances, but because of the headband with which they are fitted you will be relieved of the nuisance of holding the receiver to your ear and will have both hands free for manipulation of your apparatus. Fig. 3
The microphone detector is to be made as shown in Fig. 3, which indicates how two large double binding posts are to be mounted upon a hard rubber or wooden base. Two sharp sewing needles are inserted into the upper holes of the binding posts, and between their points is lightly supported a short length of graphite from a soft pencil. The piece of graphite should be about one-half inch long, and should have its ends partially hollowed out so that it will hang easily upon the needle points. It is not to be damped firmly, but allowed to rest so loosely that it may be revolved freely and even slid a very short distance back and forth. Fig. 4

Operation  of  the  Apparatus

After you have set up both stations according to the diagrams, have someone work the transmitter key, making regular test signals such as “V” or “D”, and go to the receiver. Listen carefully to the telephone receiver, and move the graphite piece of the microphone around slightly. You will notice that you can hear every touch; when the microphone is adjusted to its most sensitive condition there will be a continuous slight hiss in the telephone receiver, and even the slightest taps on the table or instrument base will be dearly heard. When the apparatus is adjusted in this way you should hear the buzzes of the transmitter reproduced in your telephone, and so should be able to copy the signals sent out from the transmitting station.
If you have any difficulty in getting good results, try again with the receiver nearer to the sending station. When you have once transmitted good signals, move the stations farther apart. Remember that it is necessary to have good ground connections, that the two tuning coils must be exactly alike, and that the sending and receiving antennas must be identical. If you are able to erect fairly large aerials for the two stations, such as, for instance, sixty foot lengths of wire supported by trees or poles, you should be able to transmit signals a distance of five hundred or a thousand feet; with larger aerials even greater distances can be covered. Begin in a small way, however, and make your progress a step at a time.
If you are near a commercial or Naval wireless station you will be able to receive signals from it by using the apparatus of Fig. 4; better arrangements which will operate over longer distances will be explained in later articles, however. The microphonic detector of Fig. 3 is quite useful when connected to a commercial wireless tuner, and knowing how easily it may be built from material commonly at hand may be of value even to the commercial wireless operator, in times of emergency.
You will find it important to become a good telegraph operator if you propose to continue wireless experimenting. There are a number of pamphlets and books published which explain methods of learning the Morse code; Chapter IV of “The Book of Wireless,” by A. Frederick Collins, gives a good method to follow. Cards showing the International Morse Code in full may be obtained from the Radio Inspectors’ offices at Boston, New York, Baltimore, Savannah, New Orleans, San Francisco, Cleveland and Chicago. It is only by constant practice that you can become proficient.

October, 1916, pages 627-629:

II.–Construction  of  a  One-Mile  Wireless  Transmitter
IN  AN article published last month, directions were given for putting together a little buzzer wireless telegraph set which would operate over a distance of a few hundred feet or even more. This small outfit was sufficient to demonstrate such of the principles of wireless telegraphy as should be known by every student and to send messages from one house to another nearby. The receiver was sensitive enough to pick up messages from commercial stations for some distance around, provided that a fairly long antenna wire was connected to it and properly tuned.
The amateur who has built and tested the buzzer set will want next to own and operate an outfit with which he can signal over greater distances. It is the purpose of this article to describe the construction of a wireless telegraph sender which can be made cheaply and easily, and which will give good strong signals at a suitable receiving station located as much as a mile or more away. The apparatus for the receiver will be taken up in later articles; the experimenter may well spend the intervening time in building his sender.

Transmitting  Coil

One of the first requisites in increasing the distance over which messages can be sent is to increase the effective power of the sender. The buzzer run from a couple of dry cells is not strong enough to make waves which will carry very far, so it becomes necessary to get an instrument which will do better. Such an apparatus is the ordinary induction or spark-coil. The amateur may build his own spark-coil by following the descriptions which are given in a great many books on experimental electricity, but in the long run he will find it cheaper and more satisfactory to buy one. An automobile jump-spark coil is about as good a small induction coil as can be obtained. Often it is possible to get one at a nominal price from a garage or an electrician in the neighborhood. Even if purchased new from an electrical supply house, a good coil capable of giving a 1-in. spark between needle points in air will not cost more than three or four dollars. Fig. 1
There is also needed a Morse key, for sending the dots and dashes which make up the signal letters. This may be an ordinary telegraph key, which costs about seventy-five cents, or even a “strap” or signal key of the kind that sells for only twenty-five or thirty cents. If he desires, the experimenter may build his own key as shown in last month’s article. For the heavier currents used in the spark-coil (as compared to the buzzer) it is a good plan to use larger key-contacts than those illustrated. They may be made by soldering copper washers on each of the contact screws.
To furnish power for the coil, the best thing is a 6 or 8-volt storage-battery. This is quite expensive, however, and also requires occasional recharging. Satisfactory results may be secured by using 12 dry cells connected as shown in Fig. 1. With the battery arranged in this way the voltage is no greater than can be had from 6 cells, but the load is distributed between two sets of cells working side by side in parallel. As a result, the battery will last much longer than if only 6 cells were used. The vibrator on the spark-coil should be adjusted so that it buzzes freely, with a high-pitched sound, whenever the sending key is pressed. A spark-gap connected across the secondary winding will break down whenever the vibrator is started buzzing, and a singing, clear spark will jump across as long as the key is held down. Fig. 2

The  Spark-Gap

A good spark-gap for the wireless sender can be made as shown in Fig. 2. Two battery zincs, Z, Z1, which can be bought from any electrician, are cut off to about 3 in. in length, leaving the connection screws at the head of each. Holes to fit these a trifle loosely are bored through two stubby brass standards or pillars, P, P1. A smaller hole is bored lengthwise through each pillar and tapped to take a 10-24 machine screw, such as S and S1, to clamp the zinc electrodes in any position desired. Similar screws, S2 and S3, pass upward through counter-bored holes in a hard rubber base, B, and serve to fasten the pillars in place. Hardwood boiled in paraffin may be used for the base, but rubber is better because it is a better insulator. The ends of the zinc rods, where they come close together, should be filed perfectly smooth and parallel. Fig. 3 & 4

The  Loading  Coil

It is essential to use a “loading coil” with this outfit in order to get the best results, and to make the transmitter meet the requirements of the Federal laws governing the operation of wireless telegraph senders. This coil can easily be made by following the suggestions given in Figs. 3 and 4. Two square boards, about 12 by 12 in. with rounded corners, are first cut out of hardwood about 1 in. thick. A hole ¼ in. in diameter is drilled at the center of each, and counter-bored to about 1 in. in diameter in the bottom of the baseboard at C. Four ½-in. holes are then bored in each, at points a little less than 2 in. from the corners, along diagonals as shown in Fig. 4. Twelve porcelain insulators of the sort shown in Fig. 5 are slipped over each of four ½-in. hardwood dowels, whose ends pass through the ½-in. holes just referred to and are cut off flush with the upper and lower surfaces of the top and base. A long ¼-in. brass bolt is passed upward through the central holes, so that its head drops into the counter-bored space in the base and its threads project a short distance above the top. A washer and nut put on the upper end will then hold the entire framework together.
Some No. 10 bare copper wire, or some stranded bronze tiller-rope or aerial wire, is to be wound spirally on the insulators. Referring to Fig. 3, the end is first wrapped around the upper front right-hand insulator A and spliced on itself. The wire is then led straight back to the top insulator of the back right upright, then across to the top back left insulator, as shown by the dotted line, then forward to the top front left insulator, and then to the next lower front right porcelain. The winding is continued as shown until the last insulator, B, is reached; there the wire is made fast by splicing, as before.
Two connected clips must be made or purchased. The spring testing clips sold by electrical supply houses are admirable for this, though anything of the sort will do. Flexible wires are soldered to each of them, so that connection to any part of the bare wire-spiral may be made merely by clipping on the desired point. Fig. 5 & 6
The laws permit amateur wireless stations to use any wavelength up to 200 meters, provided that the wave sent out is sharp and pure. This means that the aerial wire system to be used with the sending apparatus described must not be more than 75 ft. long, measured along the conductor from its top to the ground connection. It is a good plan to use two wires about 50 ft. long running side by side to the top of a tree or chimney or specially built pole, keeping the wires about five feet apart by fastening them at each end to a light wooden spreader. The top, and in fact the whole aerial, must be thoroughly insulated, if good results are to be secured. An excellent plan for preventing electrical leakage is to connect in series, with loops or rope, five or six porcelain insulators of the kind used in building the loading coil (Fig. 6). These are inserted between the spreader which carries the antenna wires and the rope halyard which is used to haul up the aerial. Similar strings of insulators must be used to guy out the bottom of the aerial. Where the lead-wire enters the house and connects to the instruments it should pass through a thick porcelain tube, as shown in Fig. 7. Fig. 7
The ground connection may be made by wrapping several turns of bare copper wire tightly around a scraped water or steam-pipe. The connection should be made at a point near to the sending instruments.
If no water pipes are available, a large copper or iron plate may be buried deeply in moist earth. As a rule, though, such earth connections are not as satisfactory as a pipe forming part of the town water system.

Connecting  the  Set

The several instruments making up the complete sending set must be connected up as shown in Fig. 7. The spark-gap should be adjusted with its electrodes quite close together–never more than 1/8 in. apart and at least half of the loading coil is to be put in series with the antenna. Unless a large part of this coil is used the transmitter will not radiate pure, sharp waves, and its use will violate the law and make its operator liable to prosecution by the government. If the spark-gap is kept short and a considerable portion of the loading coil used, there will be nothing to fear so long as neither of the aerial wires is over 75 ft. in length.
Whenever the key is pressed, if the set is properly connected and adjusted, a bright, snappy, singing spark will jump across the gap. Each spark starts a train of high frequency currents oscillating back and forth in the aerial wires, and a train of electromagnetic waves is radiated into space. A suitable wireless receiver located where a portion of these radiated waves will reach it, will pick up some of their energy and produce from it a sound which indicates the dot-and-dash buzzes of a Morse signal.

November, 1916, pages 789-792:

III.–The  Construction  of  a  One-Mile  Receiver
IT  IS most important for a student of wireless telegraphy to learn all about the operation of the various forms of receiving apparatus. The best way to become familiar with the instruments is to build and operate them. The simple buzzer-sender and microphone receiver which were described in the first article of this series served to illustrate the principles which are followed in all wireless apparatus, but were of such small signaling range that they could not demonstrate fully the details of modern instruments. The one-mile transmitter shown last month, however, when used in connection with the receiver now to be explained, is of sufficient size to approach the conditions of operation existing in commercial radio stations. By studying its action carefully the experimenter can learn much which will be of inestimable value to him in his later practice of wireless telegraph operation.
The student should remember that the use of a transmitter as powerful as that described in the second article, even though it is a very small one when compared to some of the great commercial plants, may cause interference at nearby receiving stations. He should therefore be very careful to observe all of the regulations and courtesies as to transmitting, and should send only when he actually has a message which he wishes delivered to his communicating station. One of the first habits which a successful wireless operator should cultivate is to refrain from sending except when it is absolutely necessary. Testing of the spark-gap should be done with the aerial disconnected, and code practice should be carried on with buzzers. There is never any objection to the amateur who sends actual messages with a wavelength of less than 200 meters (the range assigned to amateur stations by the Government) but the man who keeps tapping his key and sending out interfering waves which hold up legitimate messages soon becomes extremely unpopular with both the serious amateurs and the professional operators. Fig. 1

The  Detector

Probably the most important element of any receiving outfit is the detector, which is an instrument for converting the received high-frequency current into pulsations which operate the telephones. The microphone which was described in the first article is a wave-detector of a very easily constructed type, and is always worth remembering for use in an emergency. It is very delicate, but is not so reliable nor so sensitive as the crystal detector which is illustrated in Fig. 1. A well made crystal detector is about the best instrument for all around use that can be had. Apparatus of this type is installed at by far the greatest number of commercial radio stations, and every operator should be familiar with its adjustment and use.
A side view of a detector-stand, which has been found very satisfactory in practical work, is shown in Fig. 1. The construction should be clear from the drawings, and a brief description. Dimensions are not given, since it is usually most convenient to modify them slightly to suit whatever material may be on hand. The base 1 may be made of hard rubber, fiber or hardwood, and should be about 4¼ in. by 2 in. by ½ in. thick. Four holes to take 8-32 machine screws are drilled in the positions shown in Figs. 1 and 2 and directly beneath the parts and are counterbored from the bottom to about ¼-in. depth to take the nuts and washers. A disk 2, of copper or brass about 1/16 in. thick and 1¼ in. in diameter, is soldered to the head of a machine screw 3 and forms a sort of table on which the crystal-cup may slide. The screw 3 is fastened in place by a washer and nut, as indicated, and is connected to binding post 14 through the channel shown in dash lines in Fig. 2. Fig. 2
A flat brass cup as at 4, Fig. 1, 5/8 in. in diameter and ¼ in. deep, may be made by cleaning out thoroughly the cap of a shotgun shell. In this is secured a piece of fused silicon, galena, or other sensitive crystal 6 (which may be purchased from almost any wireless supply house) by melting and pouring in solder around it. The heat of molten solder will partially destroy the sensitiveness of some crystals, so it is better to use Woods’ metal or a mercury amalgam if it can be obtained; solder will generally do for silicon, however. A hard rubber or fiber ring 5, about 1/8 in. thick, should be forced on over the outside of the completed cup, so that the crystal may be moved around without making contact between the metal cup and the operator’s fingers.
A needle point 13 is to be supported directly above the crystal, and this may best be done by the pillar arrangement shown. A long machine screw 7 is passed down through two bushings 9 and 8, and is fastened below the base by a nut and washer. Between 8 and 9 is clamped a tapered strip of spring-brass 10, to one end of which is soldered a binding-post from the zinc terminal of an old dry cell. The shape of this strip may be seen in Fig. 2, where the upper part of the detector is omitted.
At the top of the pillar is fastened the adjustment arm 11, which should be made of brass about 1/8 in. thick cut as shown in Fig. 3. The left hole is threaded to take the pressure-adjusting screw 12, Fig. 1, and is slit as indicated at 15, Fig. 3. Thus the screw 12, Fig. 1, may be held snugly by the screw-threads. A hard rubber or fiber hand-wheel should be affixed to the top of 12 by a washer and nut, as in Fig. 1. Connection is made from the screw 7 to binding-post 14′ by way of the shorter channel indicated by dash lines in Fig. 2.

The  Telephones

Next to the detector, the most important thing in the receiving station is the telephone. Any ordinary telephone-receiver will give some sort of results, but to get the loudest signals for any particular set of conditions the best telephones should be used. There are on the market a number of head-receivers, designed for wireless telegraph use. These are usually mounted in pairs, one for each ear, on a flexible headband, and are wound for resistances higher than ordinarily used in wire telephony. Reasonably good results can be secured from two ordinary 75-ohm watchcase receivers, if they are connected in series and mounted upon an improvised headband. Thus, there is no need for any one to be discouraged by the high price of the most expensive types. It is good policy, however, for the student to invest as much as he can spare in good telephones, even if a saving must be effected by cutting down the size of the transmitter. Fig. 3 & 4

The  Blocking  Condenser

Another essential part of the receiving apparatus is a blocking condenser, which is used to prevent the tuning coil from short-circuiting the detector or telephones. Such a condenser as shown in Figs. 4, 5, and 6 may easily be made. A “fixed condenser” may be purchased from any wireless supply store, but it is a good plan for the experimenter to make one. By doing so not only is the actual construction of the instrument learned, but the weak points which might cause trouble later are located.
A pattern for the tinfoil sheets is cut as shown in Fig. 4, 2 in. square but each having a lug ¾ in. square at the corner. Thirty of these will be needed for the condenser. It is also necessary to cut out about thirty-five sheets of thin paraffin paper 2½ in. square, as shown by the dash lines in Fig. 4. The condenser is begun by placing a sheet of paraffin paper upon a flat surface, and putting on top of it one tinfoil sheet with the lug at the lower left corner, as shown by Y in Fig. 4. On top of this foil is placed a sheet of paraffin paper, and upon it a second sheet of foil; this time the lug is turned to project at the upper right corner, X (dotted lines) in Fig. 4. Then a sheet of paper is added, and upon it a third piece of foil with its lug in the Y (lower left) position. Another sheet of paper is put in place, and then a fourth piece of foil with its lug in the X position. Thus paper and foil are alternately added, and the position of the lug changed each time. The result is a pile of thirty sheets of tinfoil separated by thin paraffin paper, fifteen lugs projecting to the left and the fifteen alternate lugs projecting to the right. Care must be taken that none of the alternating sheets of foil touch each other, since this would short-circuit the condenser. Fig. 5
A holder for the paper-and-foil condenser is made by cutting out two pieces of 1/8 in. or 3/16 in. hard rubber or fiber or hardwood about 2¾ in. by 4 in., and drilling four holes in each as shown in Fig. 5. An 8-32 machine screw is passed through each of these holes, washers being placed between the clamping pieces in such number that the condenser is firmly gripped. The upper right and lower left screws X’ and Y’ clamp the groups of tinfoil lugs X and Y, as shown in Fig. 6, and the binding posts X” and Y” mounted upon their upper ends serve to make electrical connection. The other screws 16 and 16 are merely for mechanical strength.
When the condenser is finished, paraffin may be melted and poured in to fill the entire space between the two clamping plates. If the construction has been careful and if the condenser is in good condition, when a dry cell and telephone are connected in series with the binding posts X” and Y” only a very faint click will be heard as the circuit is made and broken. If the condenser is short-circuited (and therefore useless until repaired) the telephone will click as loudly with it in series as when connected directly across the dry cell. Fig. 6

Additional  Apparatus

In the next article there will be described the buzzer-testing arrangement which is used to adjust the crystal-detector to its sensitive receiving condition, and a complete wiring diagram for the entire transmitting and receiving station will be given. The manipulation of the apparatus, the methods of calling and answering and of sending messages, as well as the construction and use of the antenna change-over and the detector-protecting switches will be discussed. The remaining instruments needed for the receiver are even easier to construct than the detector and condenser outlined here. It would be a good plan for the experimenter to complete his transmitter (as described last month) now and the apparatus shown in this article, so that he will be all ready to put his station into complete operation soon after the appearance of the next article. It should be remembered that for exchange of messages between two stations it will be necessary to build two of each of the instruments described, so that each station may be completely equipped and thus prepared both for sending and for receiving.

December, 1916, pages 949-952:

IV.–Simple  Adjustments  and  Connections
IN  THE article published last month there were given descriptions of a crystal-detector and stopping-condenser to be made and used in connection with the transmitting set of the October article, for sending wireless messages over a distance of a mile or thereabout. Both the detector and the condenser are of types which can later be used in receiving stations which will pick up the messages from large commercial or government plants not only nearby, but hundreds of miles away. With the small sender using a spark-coil, however, the range will be limited to a mile or so, unless the aerials at both stations are large.

The  Test-Buzzer

In using a crystal-detector it is necessary to be able to find out instantly whether or not the adjustment is sensitive. When the needle-point bears lightly upon some parts of the crystal, the receiver is sensitive and able to translate messages coming from a distance; with the contact at other points, however, the instruments seem absolutely dead.
Obviously, to be certain that messages can be received effectively, one must be sure that his detector is properly adjusted. The best way to do this, and the way which is used by the professional operators in most large stations, is to take advantage of the feeble signal-waves induced by a buzzer. By setting up a small sending-outfit, such as described in the September issue of the POPULAR SCIENCE MONTHLY in the first article of this series, the sensitiveness of the detector may be tested by listening in the receiving telephones and at the same time pressing the testing-key. Fig. 1
Figure 1 shows how to wire up the buzzer, strap-key and dry cell described in the first article. The only difference from the little sender used to signal from one room to another is that the vibrator-contact post of the buzzer is connected to a miniature aerial wire only a foot or two long, instead of to a genuine, full-sized antenna. The miniature aerial is run along the table about 2 or 3 in. from one of the wires leading to the detector, as indicated in the illustration, Fig. 2.

The  Change-Over  Switch

In order to shift connections from sending to receiving, there must be provided a good-sized double-pole double-throw knife-switch. The lever arms of the switch should be at least six inches long, and the jaws should be mounted upon a slate, marble, or fiber base a corresponding distance apart. If the switch used is too small it will not have enough insulation to prevent the sparks from the secondary of the induction-coil from jumping to ground by way of the receiving contacts.
A second-hand knife-switch of this size and type can be bought for about one dollar or less; if none can be obtained, it is not difficult to improvise from 1/8 by ½-in. strip copper, an instrument which will work perfectly. It is only necessary to observe closely the construction of the big knife-switches of the double-throw type, in some central station, and to imitate them as accurately as possible. A number of brief articles have been published in the technical magazines, giving details of construction and dimensions for such switches. The connections for the changeover switch are shown in Fig. 2.

The  Detector-Protecting  Switch

When the wireless station is completely equipped with detector and spark-coil, it is essential to make some provision which will protect the delicately adjusted crystal from the violent impulses set up by the transmitter. The simplest way to do this is to connect a small single-pole switch (either a knife-switch or a lever-switch of almost any sort will do) directly across the terminals of the detector. In the wiring diagram of the complete station, Fig. 2, the detector-protecting switch is marked S; the wires leading from it to the binding posts of the detector should be kept as short as possible; otherwise they may pick up enough current from the sending-spark to “knock out” or destroy the sensitive adjustment of the crystal-detector. When receiving, the protecting-switch S must be open, so that the detector can operate to rectify the currents produced in it by the incoming waves. When sending, the switch must be closed. In this position the heavy induced currents are shunted past the detector and the adjustment is not disturbed by them.

Connecting  the  Complete  Set

In addition to the parts of the receiving station fully described in last month’s article, the various elements of the transmitter illustrated and discussed in October will be needed for a complete sending and receiving station. In fact, a complete set of parts is necessary for each terminal of the proposed wireless “line.” The following must, therefore, be at each plant:

    1 Antenna and support See September and October articles.
    1 Loading Coil    ”  October article.
    1 Ground Connection    ”  September  “
    1 Change-Over Switch    ”  above.
    Necessary wire for connections.
    1 Set of dry or storage-cells See October article.
    1 Sending Key    ”         ”          “
    1 Induction Coil    ”         ”          “
    1 Spark-Gap    ”         ”          “
    1 Crystal-Detector See above.
    1 Stopping-Condenser    ”      “
    1 Pair of Telephones    ”      “
    1 Test-Buzzer    ”  September article.
    1 Strap-Key    ”          ”            “
    1 Dry Cell    ”          ”            “
    1 Detector-Protecting Switch    ”  above.

The above-named elements of the complete station must be carefully connected together as shown in Fig. 2. It is a good plan to use No. 16 or No. 18 lamp-cord for the wiring of a set such as this. The twisted pair should be separated and smoothed out, and the single conductors used independently.
It is necessary to keep the transmitting apparatus well away from the receiving instruments. The loading coil, for example, should not be nearer than two feet to the detector, telephones and stopping-condenser. As explained in the second article of this series, the lead-wire from the loading coil out to the aerial must be well insulated if good work is to be done. It is very important that the change-over switch be well insulated, also, for three of its contacts are subjected to the full sparking potential of the transmitter (see the diagram of Fig. 2). Fig. 2
The best plan for beginning work is to have the two antennas, one at each station, as nearly alike as possible. If their form and height cannot be made identical, they should at any rate have exactly the same length of circuit. That is to say, there should be the same number of feet measured from the ground connection up through the spark-gap (but not through the loading coil) to the distant insulated end of the antenna, within a few per cent. In this case, i. e., with the lengths practically identical, the loading coils at the two stations can be put entirely in circuit, and the apparatus will be approximately tuned for the interchange of messages.
If one of the aerials is longer than the other, less of the loading coil should be used at that station than at the other. The exact point to clip on to the wire of the loading coil can be determined only by experiment. By trying every turn, it will be found that some one position is best both for sending and receiving messages. The wire in the loading coil has the effect of lengthening the aerial; it is therefore perfectly clear that, since it is desired to have both antenna systems of the same total length, less of the loading coil must be included in circuit with the longer antenna wire. The coiled wire is more effective in increasing the station’s wavelength than the straight wire in the aerial, however; so less of it needs to be added than one would imagine if he merely considered the difference in the lengths of the two aerial wires themselves.

Adjusting  and  Operating

When the apparatus is set up as shown in Fig. 2, the first thing to do is to put the transmitter into operation. Throw the change-over switch to the left-hand or sending side, and set the spark-gap at about 1/16 in. separation. Making dots and dashes with the key, adjust the induction-coil vibrator to the position which gives a clear, sharp spark between the electrodes of the gap. The spark should be white and snappy, and should sing with the tone of the vibrator. If you cannot get this kind of spark, the set is not working properly and you must go over the antenna insulation to be sure that it is good. If the coil gives a good spark without the aerial connected with it, but won’t spark when the antenna and ground are put in the circuit, it is proof that the insulation is not good enough, or that the spark-gap is too wide for the power of the coil. The gap should not be opened more than 1/8 in. at any time. Fig. 3
Having adjusted the transmitter, swing the change-over switch to the right-hand or receiving side. Put on the telephones, see that the detector-protecting switch is open, and hold down the strap-key connected with the test-buzzer. Move the needlepoint of the detector around over the surface of the crystal, with light pressure, until the loudest signals are heard in the telephones. The detector is then adjusted and the receiver is ready for use.
The next step is to arrange a sending schedule with your friend who operates the other station. At some fixed time, say four o’clock, let him close his detector-protecting switch, throw his change-over switch to the sending side, and send some predetermined test signal such as “B” in Morse, over and over again, for five minutes. During these same five minutes have your telephones on, your detector-protecting switch open, your detector adjusted to its best sensitiveness, and your change-over switch in the receiving position. If you have built your apparatus correctly and have set it up in accordance with the instructions of these articles, you should have no difficulty in recognizing the “dash-dot-dot-dot” signals being sent from the other station. Promptly at 4:05 your correspondent should stop sending, throw his change-over switch to the receiving side, open his detector-protecting switch, put on his telephones and adjust his detector. At the same time you should go through the opposite change-over, and begin to send him test signals for five minutes. If all is well he will “pick them up” at once, and when you stop at 4:10 he will be ready to reply to you by wireless that he has heard you; you can then give him the corresponding information and proceed to exchange messages.
You must always bear in mind, however, that whatever your station or his sends out will be heard by other stations which happen to be within range and tuned to the same wavelength. Your signals may even cause interference, and prevent the other stations from reading important messages addressed to them. For these reasons, only such transmitting as is necessary should be attempted; and the Government regulations as to the use of a pure wave shorter than 200 meters should be strictly observed. As pointed out in the October article, if over half the loading coil is used at each station and if neither antenna is more than 75 ft. in length, the federal requirements will, as a rule, be met.

Station  for  Receiving  Only

If it is desired to transmit messages in only one direction, the change-over and detector-protecting switches may be omitted at the receiver. A loading-coil will be necessary, but since it is to be used for receiving only it may be made as described in the September article instead of highly insulated in accordance with the October description. The transmitter should be connected as shown in October, and the receiver should be wired as in Fig. 3. The comments in this article as to the adjustment will still apply, except that the two switches need not be considered.
The receiving apparatus described here will work one mile easily, and is capable of hearing signals much farther away. In the next article an adjustable receiving set will be discussed, by the use of which signals may be heard from stations located hundreds of miles away.

January, 1917, pages 153-156:

V.–Increasing  the  Range  of  the  Receiver  by  Tuning
THE December article of this series gave directions for completing and operating the receiver which was designed for working over distances of about one mile. The apparatus was intended for use with the small transmitter which was described in the October number of the POPULAR SCIENCE MONTHLY; when a larger transmitter is used, the possible working range is, naturally enough, considerably greater. It is necessary for each receiver to be adapted for the wireless waves sent out by the transmitter to which it is listening, however, if the best results are to be secured.

Production  of  High-Frequency  Oscillations

Every transmitter for wireless telegraphy which is permitted to operate under the present radio laws must send out what is called a pure and sharp wave. That is to say, the sending apparatus must be so adjusted that its radiation has a single and definite wavelength or frequency. The main purpose of the regulations insisting upon this condition of sharpness and purity of wave is to enable a receiving station to “tune-in” a sending station without interference. Senders which emit waves neither sharp nor pure are the cause of interference, and sometimes prevent all other stations in their neighborhood from working effectively.
To understand this matter of tuning, one must realize first of all that the currents in a wireless telegraph antenna are of the high-frequency alternating sort, which change in direction very rapidly. In a simple transmitter, with the spark-gap directly in series between the antenna and the ground, as described in the October and December articles, the effect of the induction-coil is to charge the aerial by storing in it a quantity of electricity just before each spark takes place. The induction-coil secondary tries to charge the antenna up to its maximum pressure, or to drive into it all the electricity possible. Before this top-point is reached, however, the spark-gap breaks down and the charge of electricity rushes across it to the ground. Because of the electrical property of the aerial wire (and of the coils in series with it) called inductance, the charge overshoots itself somewhat, and the antenna is left charged in the opposite direction for an instant. Therefore, in the natural attempt to restore equilibrium or electrical balance, the charge rushes back out of the ground into the aerial; this time it overshoots also, but not by so much. The electrical energy thus oscillates back and forth, like a swing left to itself, until it is all used up in radiation, or in losses in and near the circuits.

Period  and  Frequency

A certain amount of time is required for the electrical charge to travel from the top of the antenna to the ground and back again, just as a certain time is required for a pendulum to swing from one end of its beat to the other and back again. This amount of time, measured in seconds, is called the period of the oscillation. The longer the wire, the longer the time for each trip of the current, and the longer the period. The number of times the electrical charge makes the round trip in one second is called its frequency, and this of course may be calculated by dividing the period, in fractions of one second, into one second. For example, if the period of oscillation of an antenna is one millionth of a second–which merely means that the charge takes that long to travel up and down the antenna once–the frequency is one-millionth second divided into one second, or one million. This is the number of trips the charge will make in one second.


Knowing the frequency of any electrical oscillation or high-frequency alternating current, one can immediately compute the wavelength which it will produce if it flows in a suitable wireless-telegraph antenna. The rule is simply to divide the frequency per second into three hundred million. The answer to this little problem in Arithmetic gives at once the wavelength in meters. For example, taking the frequency of one million per second quoted at the end of the paragraph immediately above, it is found that the corresponding wavelength is three hundred meters. The following table of frequencies and wavelengths will be helpful.

     Period  in
Per  Second    
in  Meters
3  000  000
1  500  000
1  000  000
500  000
300  000
150  000
100  000
50  000
30  000
As the frequency of the sending current varies, the wavelength increases or decreases with it

From an examination of this table it becomes very clear that as the period is increased, the frequency decreases and the wavelength increases. Remembering that the longer the antenna wire, the more time it takes for the charge to pass from the top to the bottom and back again, or the longer the period, it is easy to see that the longer the aerial wire (including the coils connected in series with it), the greater the wavelength will be. As a matter of fact, the fundamental wavelength of a simple aerial, which is its wavelength without any coils in series, is about 4.2 times its actual length measured from ground to top end. To use this rule, both height and wavelength must be measured in the same unit. A table showing the fundamental wavelengths of several heights of plain vertical antenna wires is given in the next column.

Height  (Length)
in  Feet
Fundamental  Wavelength
(in  Feet) (in  Meters)
The fundamental wavelength of a plain vertical antenna increases with its length

The table is strictly applicable only to plain vertical antennas without any loading coils, but it may be used for the approximate fundamental wavelengths of L-shaped antennas if the total length of a single wire is used instead of that of the vertical lead alone. If the antenna is T-shaped, the length from the ground to the center of the flat-top and from there to one end should be used. The two parts of the flat-top should have the same length, as measured from their junction with the vertical lead. Where several wires are used in parallel, whether in a horizontal or vertical antenna, the length is taken as that of one of the wires, and not of the total amount of wire in the aerial system. Neither Table No. II, nor the simple rule must be used when loading coils are connected; for the wire on such coils is much more effective in increasing the apparent length of the antenna than is the straight-away portion.


The bearing of the foregoing discussion upon the adjustment of the receiver’s tuning to get the greatest distance becomes clear on considering that, for this to be obtained, the receiving set must be adjusted “in tune” with the wavelength it is desired to receive. In the simple wireless set described last September, some small degree of tuning was secured by making the antennas and the tuning-coils alike at the sending and receiving station. This receiver, as shown in Fig. 3, has the detector right, in series between the aerial and ground connection. The result of this arrangement as regards tuning is that the high resistance somewhat spoils the sharpness of adjustment. If one makes material changes in the length of the aerial wire, or in the number of turns of coil used, a weakening of signals is noticed. The tuning is neither critical nor “sharp,” however, and even approximate adjustments will give about as good results as exact ones. Fig. 3
When the receiver described in the December article is used, as shown in Fig. 4. the adjustment is much more accurate. Here the detector is removed from the antenna circuit, and the aerial is connected directly to ground through a loading-coil. As a result the effect of the coil is considerably increased. It was pointed out that the coils and antennas at sender and receiver should be made exactly alike, if possible, but that if there should be any difference in the aerials the shorter one should have more turns of coil connected in series with it. This was, of course, to make the effective lengths of the two antennas the same, so that they would be tuned to the same wavelength.

Receiving  Various  Wavelengths

With the senders and receivers limited in their activities to communication between a single pair of stations, it is usually not necessary to provide for variation in the tuned wavelengths of either. That is why the simple arrangement of Fig. 2 in the December article could be used. When it is desired to receive from a large number of outside transmitters, all using different wavelengths, it is necessary to provide apparatus whereby the effective length of the aerial at the receiver may be varied to suit the incoming wavelength. A large number of arrangements may be used for this purpose. Some of them tune the receiver very sharply, or in other words make it respond energetically to a very closely restricted range of wavelengths for each adjustment. Other sets of connections are less critical in adjustment, but easier to handle.
The simplest variable tuning instrument for use at the receiver is the so-called “single-slide tuner.” This is merely an inductance coil with a sliding contact whereby the number of turns in circuit may be varied at will. It may be used in place of the tuning coil shown in Fig. 3, and will allow some latitude of adjustment, though the tuning is very broad and unsatisfactory. A better mode of connection for the single-slide tuner is that of Fig. 4, in which the detector is put in a side or by-pass circuit; this gives sharper tuning and fairly strong signals. Fig. 4
A still better tuning arrangement fuses the “double-slide tuner,” which has two variable contacts. In the catalogs of manufacturers of radio apparatus there are to be found a large number of diagrams showing different ways to connect the double-slide tuner; but the best possible results are to be secured from the arrangement of Fig. 5. One end of the coil is connected to ground and one of the sliders to the antenna. The larger the amount of coil between the grounded end and the first slider, the longer the effective length of the aerial and the greater the wavelength for which it is tuned. The grounded end is also connected to one side of the blocking condenser described in the November article, and the other slider is connected with one terminal of the crystal-detector also illustrated in November. The telephone has one lead connected with ground, and the other joins the open sides of the detector and blocking-condenser. The test-buzzer, which is not shown in Fig. 5, is to be arranged as explained in the December article, so that the crystal-detector can be adjusted to its maximum sensitiveness without waiting for signals from outside stations.

Operating  the  Variable  Receiver

In working the apparatus set up as in Fig. 5, the first step is to make sure that the detector is adjusted to a sensitive point and that the connections are all secure and in good condition. Then the slider connected to the detector is set at a position about half-way along the coil, and the antenna slider is moved back and forth slowly along the length of the entire tuner. When the station within range starts to send, his signals will be heard in the telephones; it will be noted that the dots and dashes are loudest with the antenna-slider at some particular setting. Leaving the antenna-slider at this point, the detector-slider is moved back and forth until the position giving the best signals is found. This is the tuned or approximately tuned adjustment of the receiver for the specific wavelength being received.
It often happens with double-slide tuners of this type that there are several positions for both sliders which give good signals for a single wavelength. Therefore it is a good plan to try several settings of the antenna-slider, varying the other contact at the same time; thus one can sometimes find a single pair of settings which give markedly improved signals. This double-setting effect is more noticeable with other connections than that shown in Fig. 5, but with some combinations of antenna and detector it may be found in this arrangement also. The best thing to do is to have a scale, marked in number of turns or in centimeters of coil; fastened close to each slider, and then to make a tabulation of the best settings for each station as it is heard. Such a table makes it possible to leave the apparatus tuned quite close for any desired outside station, and to feel confident that its messages will be received whenever it starts to send. Fig. 5

The  Apparatus

For receiving long distances it is merely necessary to combine the crystal-detector and blocking-condenser, recently described, with a pair of good head-telephones, a fairly long antenna, and a double-slide tuner, in order to receive at night from commercial stations hundreds of miles away. It is wise economy to buy good telephones; for, as a general rule, the more money invested in them (so long as they are purchased from a reliable dealer) the greater will be their effectiveness. For receiving from amateur stations, which are required by law to operate on waves less than 200 meters in length, it is not desirable to have an antenna longer than 100 feet or so, though longer wires may be used if a condenser is connected in series, as will be explained in later articles. To get the best results from the longer wave stations, such as the commercial plants which use 600 meters and the Naval stations on waves of 1000 and 1200 meters, it is best to have antennas about 200 feet long. Using the ordinary crystal-detector, a double-slide tuner, good telephones and a single aerial wire swung between chimneys 750 feet apart and 40 feet above the ground, it is not unusual to receive messages 600 or 800 miles at night during the winter.
The loading-coil described for the one-mile sender, in the October article, may be used in the diagram of Fig. 5, if two clips are utilized. This will not give a very long range of wavelengths, but will do for experiments. For the best receiving, a modification of the double-slide tuner, which is easily made, will be described next month.

February, 1917, pages 309-313:

VI.–Simple  Adjustments  and  Connections
Fig. 1 SKILL in receiving, which includes both the ability to “copy” Morse and Continental signals rapidly and accurately, and facility in the adjustment of the receiving instruments, is one of the most important things for a radio-operator to develop. Knowledge of the transmitting apparatus and its manipulation, as well as a clear and firm method of handling the key in sending, is of course essential; but without knowing how to adjust the receiving tuners and detectors so as to get maximum strength signals with the least interference a wireless man soon finds himself in trouble. The only way to gain the needful familiarity is through practice with the apparatus itself; and at the same time the student must realize how and why his instruments work. Unless it is clear to him just what effect will be produced, and why, whenever he makes an adjustment or changes a setting, he will not progress very rapidly.
In the January article of this series it was shown that the detector and stopping condenser previously described could be assembled with either of two types of tuning coil (the “one-slide” and the “two-slide” varieties) so that messages could be received from commercial and naval stations hundreds of miles away. Receiving practice gained through use of receiving apparatus in the ways indicated will form a valuable foundation for further advances in the use of more complicated tuning arrangements, and the experimenter should familiarize himself with the action of the circuits shown in Fig. 3, 4 and 5 of the last article. Fig. 2

Methods  of  Connecting

The method of connection shown in Fig. 5 of the January article is the most effective of all the simple arrangements. It requires a tuning coil with two variable contacts or sliders, in addition to the usual detector, telephones, and stopping-condenser. This same tuner may of course be used for tests of the single-slider “hook-ups,” by using only one of the movable contacts; such trials will demonstrate beyond doubt the fact that, when it is properly adjusted, the two-contact arrangement gives louder signals with greater freedom from interference. Somewhat more skill is required to get the best results from the two-slide than from the one-slide apparatus, but the effort is more than repaid.
Sliding-contact tuning coils for use in any of the circuits described may be purchased from the wireless supply houses, and will give reasonably good results. It is very easy to make such tuners, since all that is required is a coil about 3 in. in diameter and 8 in. in length, wound with insulated wire of about No. 22 gage and fitted with two contacts which slide along rods supported above paths from which the insulation has been scraped. Such instruments have been used in commercial radio-telegraphy, and were very common in the stations of eight or ten years ago. It has been found, however, that the sliding contact upon the coil itself is not particularly desirable, since the slider finally wears through the wire, and there is always difficulty in maintaining good contact. Further the slider usually short circuits several turns at its point of contact, and thus causes mistuning and loss of signal strength. These disadvantages of the sliding contact, taken together with the poor circuit design often employed, have brought the direct-coupled circuit of the sort described into disrepute; there is really little choice between the direct and inductively coupled receivers, however, provided that both are properly built.
By making the loading and transformer coils in separate units, and fitting each with switch contacts instead of sliders, it is entirely practicable to produce a receiving installation which has all the selectivity of the inductively coupled type and still avoid some of its disadvantages. Such coils are described below, and their mode of connection is shown in Fig. 7, which corresponds to Fig. 5 of the December article. Fig. 3

The  Loading  Coil

This instrument is shown in Fig. 1. The basic piece is a paper tube of about 4 in. diameter and 8 in. length. Beginning about 1 in. from one end, No. 20 gage double silk-covered magnet-wire is wound on evenly for about 6 in., which will take 149 turns. A tap must be taken out for each of the first ten turns, and one for each tenth turn thereafter, as shown in Fig. 4. The best plan is to fasten the end of the wire, before beginning winding, through two small holes punched in the paper tube, leaving about 2 in. of wire free for the tap marked “9” in Fig. 4. Then a single turn is wound on, and a small loop twisted in as shown in Fig. 2. This twist and loop stand up from the surface of the coil, and the wire leading to contact “8,” Fig. 4, is later soldered to the loop. The second turn of wire is then wound on the tube, and another twisted loop for the contact “7” is made. Thus a twist is put in for each of the contacts, at the end of each turn, till that marked “0” is reached. Then ten turns are wound without a tap, the twist for “10” being taken out at the 19th turn of the whole coil. Similarly taps for “20”, “30”, etc., are made at each tenth turn thereafter. Fig. 4
The completed coil is to be mounted between two end blocks of wood or hard rubber, A, in Fig. 1. Three small pieces are fastened to the inside faces of each of the end blocks, as shown in dotted lines, to keep the coil from slipping sidewise; and the whole is held together by a piece 1 in. square passing through from end to end in the center of the coil. Screws B, with washers under their heads, pass through holes bored in the end blocks and clamp the tube by threading into the ends of this central stick.
As further shown in Fig. 1, a switch-panel is mounted on top of the end blocks. This should be made of hard rubber or fiber, about ¼ in. thick, though hardwood 3/8 or ½ in. thick will do. It is fastened to the end blocks by means of two wood-screw binding posts D, D1, Fig. 1 and 3, and the screws E, Fig. 3. On it are mounted two rotary switches, one having 10 and the other 15 points, as shown in Fig. 3. Any type of switch-arm will do for these, but the easiest manipulation will be obtained if a center-knob type is used.
The 10-point switch should be marked “Units” and the 15-point “Tens”; the buttons are to be numbered from zero to 9 for the former and from zero to 140 in tens for the latter. The taps from the coil itself are to be connected with these switch-points by means of short soldered leads, as shown in Fig. 4. Great care must be taken to see that no short circuits are made as this wiring is put in place. The central points of the switches, i. e., their arms, have wires leading to the binding posts D, D1. It is best to make the switch buttons marked zero the lowest; then as the switch-arms are turned toward the upper positions, more and more turns of the coil are cut into the circuit between the two binding posts. As is obvious from the diagram, the “tens” switch cuts in ten turns at a time, while the “units” switch gives steps of a single turn. By various combinations of both switches, any number of turns from 1 to 149 can be had. Fig. 5

The  Transformer  Coil

Another coil very much like the first is now to be built. The mechanical features are exactly the same; but only 8 twisted taps are taken out from the 150 turns of No. 20-gage wire. The end of the wire is connected to a binding post F, Fig. 5, and taps at the tenth, thirtieth, fiftieth and each twentieth turn thereafter are led to the corresponding points of two nine-point switches mounted on the panel. These are marked “Coupling” and “Secondary” respectively, and take the places of the 10-point and 15-point switches on the loading coil just described. Their buttons are marked 0, 10, 30, 50, and so on to 150, in steps of 20 turns, and the soldered connections are made as shown in Fig. 5. The binding post F may take the place of one of the screws E in Fig. 3, and the posts G and H are located as D and D1 in Fig. 1.
It is to be noted that in the loading coil the adjustment of inductance may be had in single turn steps by the use of two switches, but that there are only two points of connection. In this last described coil there are three points of connection, two of which are variable in steps of 10 and 20 turns from 0 to 150. Thus the two coils, while superficially alike, may be used for very different purposes.


It is possible to buy lever-switches from the various supply houses, but usually the type with the knob at the outer end of the switch-arm is furnished. This is not nearly so convenient for tuning as the kind with central-knob shown in Fig. 1, 3 and 6, since considerably greater movement of the hand must be made in order to accomplish a given adjustment. Central-knob switches are not difficult to make; a simple and effective design is shown in Fig. 6. The switch-points I may be of any sort whatever; most supply houses will sell these for one or two cents apiece. The switch-arm K is cut out of thin spring-brass, and is formed of two pieces, each having one end punched to fit over the machine-screw O and the other end bent down to make smooth contact with the buttons I. The arms are fastened to the turned hard rubber knob L by means of the brad or escutcheon pin M, and are further clamped by the two nuts N, N1. The central machine-screw O passes through the switch-panel Q within a short sleeve P and through two washers shown but not lettered. Two additional nuts N11 and N111 are clamped on the inside, just enough play being allowed for free turning when the arm K bears upon the contact points. Connection to the arm is made through the spiral R, the free end of which is soldered to the screw O. Soldered connection is made to the switch-points at J. Fig. 6

Setting  Up  the  Receiver

The loading coil and the transformer coil as described above are to be combined with a detector, telephone set and stopping-condenser as shown in Fig. 7. The antenna circuit passes through the loading coil from D to D1 and thence to binding post G of the transformer coil. This leads to the “coupling” switch, and the circuit runs from there through whatever part of the coil is cut in, and out to ground through binding post F. The secondary circuit includes that part of the transformer coil cut in by the “secondary” switch, and runs from binding post H through the detector and stopping-condenser to the ground binding post F. The telephones are connected across the stopping-condenser.
A crystal detector and stopping-condenser suitable for this use were described in the POPULAR SCIENCE MONTHLY for November, 1916, in the third article of this series. The proper sort of telephones to use was also discussed in that article. A test-buzzer arrangement for adjustment of the detector was explained in the December article, and should be combined with the outfit of Fig. 7 in order to make the adjustment easier and more positive.


The circuits of Fig. 7, with the apparatus described, will give excellent results in receiving from the commercial and naval spark stations, if used with an antenna of from 150 to 250 ft. length. For shorter wavelengths than 500 meters the antenna used should be somewhat shorter, and for waves longer than 2500 meters (that on which time signals are sent) it is advantageous to use still longer wires. It is not necessary to erect multiple wire aerials for receiving, nor is great height essential. A 200-ft. single wire, of No. 10 gage copper, or even galvanized iron, swung horizontally between two 50-ft. masts or trees, will prove entirely satisfactory for most purposes. When it is desired to receive the short waves from amateur stations, which are restricted by law to wavelengths under 200 meters, a wire not much over 70 ft. in length should be used. Fig. 7
In attempting to “pick-up” signals with the outfit of Fig. 7, the best plan is to set the “units” switch on 5, the “coupling” switch on about 30, and then to vary simultaneously the “tens” and the “secondary” switches. As the turns on the loading coil are increased in number, those of the secondary should also be increased. When signals are heard, the best point of the secondary is selected, and the loading coil and coupling switches adjusted to give the loudest responses. One must of course be careful that his detector is adjusted properly before starting to tune; for this purpose the test-buzzer is a great time-saver.
It will be noted that more turns of the loading coil and of the secondary are needed for long wavelengths than for short ones, and that when the number of “coupling” turns is reduced, the number of turns in the loading coil must be proportionally increased. This is because the loading coil and the coupling turns in series form a primary circuit, whose effective length must be adjusted for the various wavelengths in the manner described last month. It will also be noted that all stations which have the same wavelength will “come in” best with approximately the same settings, and that the wavelength of any station may be estimated roughly by considering the number of turns in the loading and coupling coils which give the strongest signal from it.
A thing which is very important in the operation of this tuner, however, is not likely to be evident from the first tests made upon it. That is the relation between the sharpness of tuning and the number of turns on the coupling part of the transformer coil. Careful observation will bring out that when the number of turns on the coupling section is reduced, and the loading coil correspondingly increased to the tuning point, better selectivity is obtained. Usually there is a best value of the coupling turns for every station or wavelength, and its use requires the proper corresponding settings of the loading coil and secondary switches. Often when there is interference it is best to use still fewer turns of the coupling section, correspondingly increasing the loading coil, so as to get sharper tuning in spite of a weakened signal. The judicious selection of values for these three coil sections (primary, coupling and secondary), and the proper balancing of signal strength against sharpness of tuning, is one of the items which is most important in commercial radio-telegraphy. Many operators fail to get the most out of their receivers merely because they fail to pick out the best adjustments, or because they do not retune primary or secondary circuits after changing coupling values. Practice with the apparatus of Fig. 7 should make the desirability of correct tuning evident to every experimenter.
In the next article, of this series there will be discussed the secondary variable condenser. When properly used, this instrument is of great value in increasing sharpness of tuning.

March, 1917, pages 475-478:

VII.–The  Variable  Condenser  for  Tuning  the  Secondary
THE direct coupled receiving tuner which was described in detail last month will prove satisfactory for long distance working, up to the limit fixed by the sensitiveness of the detector and telephones used in connection with it. The loudness of signals, if the coils and switches are properly built, should compare very favorably with the best obtainable by using an inductively coupled receiving transformer of equivalent design. To get the strongest signals, in either the direct or the inductively coupled outfit, the operator must determine by trial the best settings of primary and secondary inductance and coupling, as previously pointed out.

Sharpness  of  Tuning

Although the simple tuners without variable condenser in the secondary will give loud signals, and in fact about as loud as can be obtained by any arrangement of tuning circuits when working with spark stations, the best sharpness of tuning cannot be secured. When two transmitters are heard at about the same intensity and on only slightly different wavelengths, it is difficult to build up the signals of either at will by the mere adjustment of the coupling and primary and secondary inductances, when the circuit without variable condenser is used. For this reason the tuner, whether inductively or conductively coupled, which has the detector directly in series with the blocking condenser (i. e., which has no condenser directly across the secondary terminals for tuning) is called “broad tuned.” However, if a variable condenser is connected as shown in Fig. 1 and 2, the selective powers of the circuit become very much greater and it is called “sharp tuned.”
The details of adjustment which are necessary in order to get the best results from the sharply tuned receiver will be taken up in full next month. The manipulation of this receiver should be second nature to all radio operators, since it is the arrangement of apparatus used by the great commercial companies. In the hands of an unskilled operator better results are sometimes obtained with simpler circuit arrangements; the reason for this is simply that the man does not know how to get the most out of the sharply tuned lay-out. The circuits of Fig. 1 and 2, when correctly adjusted, provide the maximum selectiveness which is to be had in the best commercial receivers in general use. Securing the correct adjustment, once the principles are clearly understood, is merely a matter of practice. It is essential for the student, therefore, to familiarize himself with the actions of such receivers under all conditions likely to be encountered in practice. Fig. 1

The  Variable  Condenser

Since Fig. 1 is exactly the same as Fig. 7 of last month’s article, except for the addition of the variable condenser and a single pole switch for cutting it out of circuit, all of the instruments described in the preceding articles of this series may be tilized. The switch of Fig. 1 is preferably a small single pole, single throw knife-switch, since this type almost invariably gives good contact, though any other form will be satisfactory if kept in good condition. The variable condenser is the important new instrument, and must be of good design if it is to be really useful. The amateur who has sufficient funds at his disposal will do well to buy one of the standard variable condensers now on the market; if he sticks to the ordinary semi-circular rotary type, having a capacity of about .001 microfarad and costing from $5.00 to $25.00, he will be likely to get a good instrument for tuning. The cheapest apparatus, as well as the various freak forms which appear from time to time, are less likely to be satisfactory.
Since good variable condensers are expensive, as compared with the other parts of short-wave receiving apparatus, a simple and yet good design for making them at home will be described. The condenser made in this manner will prove rugged and suitable for continuous operation, will have good insulation between its terminals, and yet will be found easy and comparatively quick to build. Fig. 2

The  Fixed  and  Moving  Plates

The plates of the condenser may be made of almost any conducting material. Aluminum about 1/32 in. in thickness is by far the best, since it is light, soft and easily kept flat. Soft brass or copper will prove suitable though heavy, and even sheet tin can be used if reducing the expense is of the greatest importance. The fixed plates are laid out as shown in Fig. 3. They consist merely of rectangles 2 by 5 in. in size. About 3/8 in. from each corner, on a 45 deg. line a hole is drilled to take the supporting uprights. The relation of the plates to a semi-circle of 2 in. radius, which corresponds to the active surface of the moving plates, is also shown in Fig. 3. The rectangular form of plate is shown for the reason that it is the quickest and easiest to cut out. Obviously, if material is of more importance than time, the corners may be cut off and the outer side of the plate held by a single vertical bolt passing through suitably placed holes at or near the center of the upper edge.
The form of the moving plates is shown in Fig. 4. Essentially, these are portions of circles having a 2-in, radius; they are roughly semi-circular in form, and the exact relation to a half-circle is shown by the dotted lines. A hole to take a 5/32-in. bolt is drilled at the central point where the radii meet, as shown. This design of plate is about the easiest to make of all that have been suggested, and yet is not particularly wasteful of material.
For the tuning condenser, 13 fixed and 12 movable plates may be cut out. The simplest way is to make a full size templet or pattern out of pressboard, and to scratch the outline of each plate on the material by running a needle around the edge of the pattern when held tightly on the surface of the metal sheet. The plates are then trimmed out with sharp shears, clamped together in a vise and filed to exactly the same size and shape. They must be flattened by hammering, preferably between perfectly flat metal surfaces, until no dents or warping can be seen when the plate is held edgewise to the eye.

The  Top  and  Base

Hard rubber or horn fiber, from ¼ to 3/8 in. in thickness is the best material for the top and base. If these cannot be used, hardwood about ½ in. thick will do. In the illustration, Fig. 5, are shown the two pieces that form a 5-in. square, and how they are drilled at each corner, in the center, and at the inner corners of the fixed plates, to take the several bolts. The base must also be drilled and tapped near the center, to take the foot or base bearing of the vertical shaft, to be described later. In Fig. 5 there are shown the outlines of both the fixed and moving plates in their proper relative positions, so that no difficulty should be experienced in laying out the holes once the plates have been finished. Fig. 3, 4, 5

Other  Materials

Practically nothing else is needed except a number of 8-32-hexagon brass nuts (machine screw size No. 8 with 32 threads per inch), a considerable quantity of copper washers or burrs which will slip freely (but not too loosely) over an 8-32-machine screw, six threaded brass rods of 8-32 size and about 5 in. long (the excess is cut off after assembly), a 5 in. by 5/32 in. threaded brass rod with 6 hexagon brass nuts to fit, a number of perfectly flat brass or copper washers of about 5/8 in. outside diameter, which will slip over the 5/32-in. bolt, a little soft brass strip, two small screws and a hand wheel. In Fig. 6 is shown how one of the 8-32 bolts is used to support the top of each corner of the group of fixed plates in proper relation to the top of the condenser itself. As indicated, the completed assembly begins at the top with a hexagon nut and washer, after which comes the 5-in, square top plate. This is clamped in place by means of a second washer and nut, after which come separating washers to space the uppermost fixed plate the proper distance from the lower side of the insulating top, and then that plate itself. After the first plate, enough washers to make a space of ¼ in. are put on the threaded rod, and then the next plate. Thus the thirteen fixed plates are placed on and clamped by the nuts of four of the threaded rods. At the bottom, as shown in Fig. 7, the third nut is screwed upward to hold the plates firmly, and a fourth nut turned on to the point which will hold the lowest fixed plate the correct distance from the upper side of the insulating base. After adding a washer, the base itself is placed on, and then a threaded rubber, wood or fiber foot is screwed on to clamp it all in place. Of course, only the corner posts of the base itself take these feet; the two rods at the inner edges of the fixed plates are fastened by screws and washers on the lower side of the base.
The two corners of the base, shown at the lower part of Fig. 5, where no fixed plates reach, are supported by the fifth and sixth threaded 8-32-rods in the manner shown in Fig. 6 and 7, with the obvious exception that the plates themselves and their separating washers are omitted.

The  Rotary  Part

The moving plates are assembled upon the 5/32-in. threaded rod, clamped by the hexagon nuts and separated by the larger washers, as shown in Fig. 8 and 9. Beginning at the top of Fig. 8, it is seen that the hand-wheel, which may be a knurled disk of ¼-in. hard rubber 2 in. in diameter, is clamped at the top of the 5/32-in. rod or shaft between two washers and nuts. Between the lower nut and washer there is gripped the end of a bent metal indicator-hand which points to a degree scale (a cheap protractor makes a good one) mounted on the upper side of the insulating top. Just below this lower nut is a little brass bushing or tube, forced into the insulating top and having the right inside diameter to act as a bearing for the shaft. Below this come separating washers–one or more–and then two nuts which lock each other and hold the moving plates in place. The uppermost moving or semi-circular plate comes next; immediately below it, and separating it from the next plate, are enough of the larger washers to space the plates just ¼ in. apart.
As shown in Fig. 9, the moving section is built downward, and the lowest plate is clamped in place by two more nuts. The shaft itself continues for about ½ in. farther, and is tapered off to a blunt point so as to reduce friction. Fig. 6, 7, 8, 9

The  Lower  Bearing

In Fig. 9 is also shown how two pieces of 1/16-in. soft brass strip are bent and drilled to form a thrust bearing for the lower end of the shaft. They are secured to the base or lower 5-in. square insulating plate by the two machine screws. Electrical connection is made to the moving plates by soldering a wire to one of these screws, running it out to one of the corner screws which is not associated with the fixed plates, and once more soldering it there. A binding post takes the place of the top nut of Fig. 6 on this outside screw. Similarly, a second binding post substituted for the uppermost nut on one of the screws supporting the fixed plates provides a convenient means of connection with the fixed plates.
For continued service it will not do to depend upon the electrical contact in the bearing of Fig. 9 alone; a small piece of thin spring wire (brass or phosphor bronze) should have one end soldered to the shaft just above the upper plate of the base bearing, its other end being fastened to the bearing itself after one or two spiral turns are made loosely about the shaft. This will prevent any possible trouble from oxidation of the contacts within the condenser. A stop should be provided to keep the plates from turning more than 180 deg. and twisting off the spring wire.

Assembling  and  Adjusting

Manifestly the foregoing descriptions, with reference to Fig. 6, 7, 8 and 9, apply to the completed apparatus. The best way to assemble the instrument is to clamp together the fixed plates on their four rods, independent of either the base or top plates of insulating material. When the conducting plates are all set parallel and with the proper ¼-in. spacing, they are laid aside and the moving plates similarly assembled upon the shaft. The base, hand wheel and top are left apart until the moving plates have been correctly spaced and adjusted. Then the moving plates are slipped interleaf-wise between the fixed plates, and the insulating top put in place. By trial the proper number of washers and the best position of the clamping nuts is determined, and the top is then fastened. Next the base is adjusted to the proper position, and all the fastening nuts tightened. Last of all the hand-wheel and pointer are added, and the scale set to the correct position. It is a good plan to cut a strip of celluloid film to just the width of the space between the insulating top and base, and to bend it around the metal parts so as to exclude dust. When this is to be done, the top and base may be made 5½ in. square to give a little additional edge-space in which the celluloid strip may be fastened by gluing bits of 1/8-in. felt next to it.
The next article of this series will describe fully the use of the variable condenser in the sharp-tuned secondary, as well as methods of adjusting the primary circuit by using the same instrument.

April, 1917, pages 629-633:

VIII.–Tuning  with  the  Variable  Condenser  in  Primary  and  Secondary
LAST month’s article described in detail the construction of a simple variable condenser which could be built at home and which is entirely suitable for use in either the primary or secondary circuit of any normal radio receiving apparatus. It is the purpose of the present article to show how one or more of these variable condensers may be used to the greatest advantage, both for increasing sharpness of tuning (and thereby lessening interference difficulties) and for increasing signal strength. The great advantage which is secured immediately upon the use of a variable condenser is in the flexibility of circuit adjustment which can thus be secured. Practically all the effects of mere tuning to wavelength can be obtained from variable inductances alone, using fixed condensers. However, to change the ratio of inductance to capacity, which is one of the important factors governing sharpness of tuning, it is necessary that both the condensers and the coils be variable; if only one element can be altered, it is not possible to secure any desired ratio at any desired wavelength.
A second advantage gained by using variable condensers is the mechanical simplification of the inductance coils connected with them. Since the condensers are continuously adjustable, and can therefore be set at any desired value of capacity without the limitation of switchpoint steps, it is unnecessary to take out many coil taps in order to get close variation of inductance. Any wavelength can be tuned to with accuracy, with only a few steps or connections on each inductance coil, because the condenser fills in the tuning range. Fig. 1

Advantages  of  the  Sharply  Tuned  Secondary

There has been some dispute as to whether a secondary tuning condenser, connected in the usual way, shown in Fig. 1 and 2, aids in producing a receiver more effective than the simple “broad tuned secondary” circuit. Extended trials have shown beyond a doubt that the sharply tuned circuit of Fig. 1 and 2, when properly adjusted, will give greater selectivity for the same strength signals than the circuit without variable condenser in the secondary. By building the secondaries specially to suit each case, about the same maximum signal strength may be had with both types. With the secondary variable condenser, however, the maximum signals are secured with looser coupling between primary and secondary. As a result, the tuning is sharper and interference is much reduced. The practical actions of such tuners as Fig. 1 and 2 represent should be studied in detail by every operator, and the differences in operation dependent upon closing and opening the condenser “switch” in the secondary circuit should be particularly noted.
The receiver of Fig. 1 is set up by combining the tuning coils described in the February article with the variable condenser of last month. The resulting arrangement is capable of excellent signal intensity and tuning sharpness. Although it is a directly or conductively connected auto-transformer type of receiver, it has variable coupling between primary and secondary, and is therefore not open to much of the criticism applicable to the ordinary “two-slide tuner” combinations. For the same reason it requires more careful handling in order to produce the best results. In operation of the tuners described, in operating any of the tuners described, it must be borne in mind that the instructions of this article apply solely to the proper manipulation of the inductances and condensers. Before beginning to tune, the operator must have made sure that his connections are properly fastened, that his aerial and ground leads are correctly arranged, that the telephones are in good condition and that the detector is adjusted to a sensitive point. The two last-named items are all-important. Each time the receiver is operated they should be tried out by a “test buzzer” equipment such as described in the December, 1916, article of this series. Once these preliminary steps are gone through, the entire attention may be devoted to tuning. Unless you are certain that the rest of the apparatus is in working order, however, much time and effort will be wasted in trying to build up signals by tuning alone. Fig. 2

Tuning  the  Coupled  Receiver

The tuner of Fig. 1 has five tuning adjustments. The positions of switches A, B and C govern the wavelength to which the primary or antenna-to-ground circuit is tuned. The third adjustment (switch C) also determines the coupling between primary and secondary. The fourth switch D, and the secondary variable condenser, fix the wavelength to which the secondary is tuned. The more turns of loading coil included in circuit by the switches A and B, and the more turns of transformer coil cut in by switch C, the greater the tuned wavelength of the primary circuit. Also, the more turns cut in by switch C, the closer the coupling between primary and secondary and, consequently, the broader the tuning of the set. The more turns of the transformer coil cut into the secondary circuit by the switch D, and the greater the active capacity of the secondary variable condenser, the longer the tuned wavelength of the secondary circuit.
Having noted the effects of the various switches and the condenser, as above, and bearing in mind that the object of tuning is to get the primary tuned wavelength and the secondary tuned wavelength to be as nearly as possible equal to the wavelength being received, it is not hard to see how the various elements must be adjusted. There is an additional object, however, which complicates matters a little; that is, the coupling between primary and secondary must be made as loose as possible without sacrificing strength of signals. Since reducing the number of turns cut in by switch C loosens the coupling, it is clear that this switch must be kept as near to zero as possible without weakening the signals too greatly. Fig. 3

First  Operations  in  Tuning

It is almost impossible to adjust the five variables to their best points simultaneously, so the best plan is to eliminate certain of them from the preliminary operations. In beginning to tune in a signal, therefore, open the switch which thus disconnects the secondary condenser. This gives the secondary a broadly tuned character, and makes it much easier to “pick up” a strange, incoming message. Next, cut in nearly all of the secondary inductance by setting switch D to a high value of turns. Since the secondary condenser is cut out, this has the effect of bringing the secondary circuit more nearly in tune with the usual wavelengths than would be the case if fewer turns were used. Third, set the coupling switch at forty or fifty turns (unless the wavelength you expect to receive is very short, when fewer coupling turns will be used) so as to make the coupling quite close and therefore to aid in hearing signals to which the apparatus is not accurately tuned. Fourth, set the single-turn switch B at the middle of its arc, and finally try to pick up your desired signals by moving the ten-turn step primary switch A. As soon as signals are heard, reduce the number of coupling turns by switch C, at the same time compensating for those cut out of the primary circuit by correspondingly increasing the turns of the loading coil. When the best settings of switches A, B and C are found (that is, the points upon which the signals are loudest), close the secondary condenser switch and set the secondary contact D to the button giving the loudest signal. Then adjust the condenser itself until the signals are loudest; and the receiver will be about at its best adjustment.
Further improvement in signal intensity can be secured by readjusting the primary single-turn switch, B, after the secondary is sharply tuned. Sometimes it is best to change the position of the coupling-switch C after the secondary condenser is cut in. All this must be determined by trial for each particular station heard. The important things to remember are, to make the rough primary adjustments first, the secondary adjustments second, the final coupling adjustments third, and to try both the primary single-turn switch B and the secondary condenser last, in order to make further improvement in signal strength or tuning sharpness, every time any other adjustment is changed. Fig. 4

The  Inductively  Coupled  Receiver

The circuit of Fig. 2 is the usual inductively coupled type used in most receiving sets. It is entirely satisfactory for general receiving, but must be handled carefully in order to give the best results. Its manipulation corresponds very closely with that just set forth in detail for the auto-transformer tuner. The only radical difference is that coupling is changed by moving the primary coil physically with respect to the secondary. As before, the more turns of primary cut in between the single-turn switch B and the ten-turn switch A, the greater the tuned primary wavelength. Similarly, the more turns of secondary coil cut in by switch D, and the greater the active capacity of the variable condenser, the greater the secondary wavelength. Again, the farther apart the primary and secondary coils, the weaker (looser) the coupling between them and, consequently, the sharper the tuning and the less interference difficulties.
The objects of tuning are, as before, to adjust the primary and secondary tuned wavelengths to agree with that being received, while at the same time keeping the coupling as loose as possible without destroying the signals. The plan to follow, therefore, is to open the secondary condenser switch and cut in a large portion of the secondary coil as before. Then close the coupling by sliding the coils well together. Finally, search for the desired signals by making rough adjustments of the primary. When signals are heard, open the coupling by sliding the coils farther apart and at the same time adjust both the primary switches to the point where signals are loudest. Then reduce the number of secondary turns and cut in the secondary condenser, setting these to the points which give best signals. For the last adjustment, open the coupling still further and tune the primary and secondary still more accurately. Always bear in mind that the three groups of settings (primary, coupling and secondary) are physically interlinked and that whenever you change any of them you must try the single-turn primary switch and the secondary condenser in order to find out whether you are hearing the loudest possible signals.
In picking up very weak signals it is sometimes necessary to adjust the large primary and secondary steps together, since in that way the circuits are kept more nearly in tune all the time, and weaker signals can be heard. Under such conditions, it is evident that when few primary turns are in circuit the secondary switch must be near its zero point, and that as the number of primary turns is increased the number of secondary turns must be increased correspondingly. Such detailed handling of the apparatus can only be learned by experience, however, and for cases of this kind these instructions can do little more than suggest a line of action. Fig. 5

Receiving  Long  Waves

For tuning to very long waves it is sometimes necessary to add loading coils to primary and secondary circuits, as shown in Fig. 3. The addition of active turns to the primary of course increases its wavelength range; a similar effect is had in the secondary. The wavelength of the secondary circuit may be increased by enlarging the size of the secondary variable condenser, and when this is done the secondary loading coil is of course unnecessary. Nevertheless, it is a good plan to keep the inductance of the secondary large, and its condenser correspondingly small; the additional loading coil is therefore the preferred method of extending the tuning range to include the very longest waves. When the main transformer is very small and the received waves are exceeding long, it may not be possible to get close enough coupling unless the primary and secondary loading coils are placed near together so that they act as an additional transformer. When this is done, care must be taken that the direction of connection is correct; otherwise the inductive effect between the loading coils may neutralize instead of helping that between the original primary and secondary coils.
Another way of getting long wavelengths with a comparatively small receiving transformer is shown in Fig. 4. Here a second variable condenser is shunted across the primary coil terminals, which has somewhat the effect of increasing the capacity of the antenna. This arrangement has a number of advantages, among which is that by its use the fine tuning of the primary can be accomplished by varying the condenser, and that, as a result, it is unnecessary to build the primary coil with a single-turn switch. Further, and especially when very small receiving antennas are used, signals may be louder with this shunt primary condenser than when the same long wave is received by adding the primary loading coil. In Fig. 4 the secondary loading coil is shown, but, as before, its effect of increasing the tuned wavelength may be obtained by enlarging the secondary condenser. Fig. 6

Tuning  to  Short  Waves

When it is desired to receive wavelengths which are short compared with the fundamental wavelength of the antenna, it is very convenient to insert a variable condenser in series with the aerial connection, as shown in Fig. 5. This has the effect of reducing the size of the receiving antenna, and makes tuning to short waves a very simple matter. As when the primary variable condenser was used in shunt (Fig. 4), small primary inductance steps are not needed, for the sharp tuning may be secured by means of the series condenser. With the arrangement of Fig. 5 it is also possible to tune to wavelengths of the medium range, since the inductance in series may be increased to give the period desired. When used in this way the signals are sometimes weaker than those obtained from the arrangement of Fig. 2, but the tuning is usually sharper, because the ratio of inductance to capacity is increased.
The primary circuit is shown in Fig. 6, which may be arranged with two single-pole double-throw knife switches so as to connect the variable condenser in series or in shunt with the primary, or to cut it out altogether. With both switchblades at the left, in positions W and Y, the condenser is in series, as shown in Fig. 5. When both switchblades are thrown to the right, in positions X and Z, the condenser is in shunt to the primary coil, as in Fig. 4. When the upper switchblade is at the right and the lower at the left, i.e., in positions X and Y, the variable condenser is cut out and the circuits are connected as shown in Fig. 2. This same switching arrangement may also be used with the arrangement of Fig. 1. Practically the same results will be secured, except that the primary turns are changed whenever the switch C (Fig. 1) is moved to vary the coupling.
Experienced radio operators, as well as beginners, will find it worth while to study the principles explained in this article. They are the basis of successful operation of the coupled receiving sets.

(The  end)



Dressler ARA-2000: Active Wideband Receiver Antenna for SDR

Dressler ARA-2000

Software Defined Radio (SDR) has finally reached a much broader mass of people, who wanted to play with RF technology, but didn’t find the time or resources to learn all necessary skills, to build a hardware based radio. Thanks to the work of the GNU-Radio and OsmoCom developer crowd, this barrier is finally gone and everyone can, more or less, directly access, what the antenna receives.

The last Mission-Log about a GNU-Radio based NFM SDR receiver pulled in a lot of people, looking for examples, to better understand GRC and to improve their own SDR projects. The real beauty about it is this: Unlike hardware receivers, which can’t simply be replicated and shared, we only have to come up with good software receivers/transceivers once and then may just share them amongst each other, without any limitation.

However, the antenna itself, is still hardware and will most likely never be replaceable by software. On ##rtlsdr people often ask about antennas, because they are clearly not satisfied (and who could blame them) with the performance of the original L/4 DVB-T stub. Unfortunately, there just is no can-do-it-all-perfectly antenna, even if some despicable corporations try to market their products as such.

Other people often recommend Discone-Antennas for wideband reception, but there also are other, less known alternatives, which still are a very good compromise as a general purpose wideband receiver antenna. Not everyone has the space or possibility to put up a Discone-Antenna, so why not use an antenna, that performs even better than a Discone (at least it did here in direct comparison), is a lot smaller and looks way less “conspicuous”:

One of them was the Dressler ARA-2000, covering 50-2000MHz, designed and built in the 90’s. The company died the usual death by capitalism (bought by another company and then stripped down and moved production to China). Today there are only a few of these left in the wild and are traded for unrealistic prices on $bay. This particular one was used for the Argus-Prototype but sacrificed and disassembled with the hope, that replicating the antenna will be easy, so that this knowledge would get openly reseeded into the wild, instead of being lost in some archives of a dead corporation. It would be great, if the following documentation about the ARA-2000 would inspire more people, to build their own Active Wideband Receiving Antenna (AWRA) and try to improve and evolve the concept even further or come up with completely new ideas.


In order to open the ARA-2000, the black top cap has to be removed first. This can be done with a screwdriver that is pushed under the side of the cover, prying it free. After the cap is removed, the bottom plate needs to come off next. This was a tougher job and required the use of a hot-air gun, to heat up the glue and then carefully applying pressure with a wooden rod through the center of the open tube.

Original Assembly

The following section shows the inner structure of the original ARA-2000 assembly, without the protective white PVC tube. Each image roughly represents a 120° rotation step:

ARA-2000 Assembly View 1

ARA-2000 Assembly View 2

ARA-2000 Assembly View 3

Length 405mm
Diameter 80mm

Antenna Element

The antenna element itself is a simple quadrilateral monopole, in the shape of a wedge, with a narrow start and a wider end. For lack of a common nomenclature and a relatively close optical proximity to a log-per design, this type is going to be ignorantly called log-per-spiral. The monopole is “glued” onto a self-adhesive, semirigid, matte-white material and then rolled to a cylinder with 80mm diameter, thus forming a spiral. Unfortunately, there seems virtually no accessible background data available about the RF properties of this particular antenna design. A NEC simulation would be interesting.

Copper Antenna Element

Antenna Element placed

Original unrolled

The small start of the original copper log-per-spiral begins at a 25mm offset from the bottom part of the white, rolled 80mm cylinder, the wider end extends 75mm over the upper edge. After 55mm from the edge of the white cylinder, the rest of the copper is bent around the outer tube and then covered by the cap. This has probably no effect on RF properties (can someone verify this?) but is probably a way to give the whole structure more mechanical support.


Material Copper
Height 0.2mm


1, 2

Structure Tube

Further analysis and research regarding material and availability lead to the speculative conclusion, that this foil probably is Aslan S22 PVC lamp shade film. The non-adhesive side of the material could be very much described as a satin surface and it’s clearly not paper.

PVC seems like a logical choice for this support structure material. It shouldn’t interfere with the RF properties of the device and can also be used in an outside environment, where it has to withstand a lifetime of exposure to drastic humidity and temperature changes and extremes, without changing its own form or function.

The transparent outer foil with the printed grid pattern (non-adhesive), which is wrapped around the log-per-spiral and PVC foil cylinder assembly, has the same dimensions as the PVC foil (405x405mm). It’s obviously the by-product silicone release liner, that was originally used to protect the adhesive side of the Aslan PVC foil. That approach is actually very neat, since these foils usually end up in the trash and were put to good use here instead.


Material Aslan S22 PVC lamp shade film (high probability)
Length 405mm
Width 405mm
Height 0.3mm

Sources (DE)

1, 2, 3, 4

Judging by the original build quality, it seems that there is some room for tolerances. It should be possible to hack the assembly ghetto-style, out of any rigid PVC foil you can find and just glue the copper log-per-spiral onto it.


The outer cover tube is made of sturdy white PVC, to protect the inner assembly from rain, hail and UV-radiation and is also used to mount the antenna. Even after several years out in the weather, the tube still looks like new. Again, other materials could also be used here, as long as they won’t interfere with RF and can withstand weather and UV-radiation. However, experience has shown, that a more professional looking antenna has a higher chance, that other people like neighbors or landlords won’t raise objections to the installation. Depending on your local circumstances, that is something you should keep in mind.


Material PVC
Length 450mm
Diameter 90mm
Inner 84mm
Color white

Sources (DE)

1, 2, 3,Franz Wolber/ Caps


Typical MSA-1105 configuration

The low-noise amplifier PCB is mounted directly on the bottom plate and consists of 2 cascaded MMIC Amplifiers. Although the types of the MMICs are not 100% known, DD1US speculated that they most likely are Avago (Avantek) MSA-1105 cascadable Silicon Bipolar MMICs. The specification, package type and marking (Top A, bottom H) support this assumption. The typical application circuit in the datasheet also seems to match the actual circuit in a cascaded configuration with etched PCB inductors:

ARA-2000 LNA (assembly view)

ARA-2000 LNA (closeup)

Alternative LNA Proposals

Due to the venerable age of the original LNA, it is very likely, that more recent semiconductors can deliver superior performance compared to the old design. The LNA is going to be replaced by a new LNA based on Infineons BFP420 which is cheap and available and should perform equally or better. The following two schematics show typical LNA configurations for the BFP420, the left one is the most simple approach (to be tested first), the right picture shows a more refined approach, with better base/collector voltage stabilization.

Simple BFP420 LNA

Stabilized BFP420 LNA

Both designs should also be equipped with a 50MHz high-pass filter between the antenna and the LNA input, to increase their large-signal immunity by attenuating lower frequencies, which the rtl-sdr or OsmoSDR can’t handle anyways (everything below 60MHz). Additionally, it would be worth a try to compare the following cases in real-world tests:

  • Antenna element → RTL/Osmo-SDR stick (No LNA).
  • Antenna element → LNA → coax cable → RTL/Osmo-SDR stick (Ext. LNA Power)
  • Antenna element → LNA → coax cable → Bias-T → RTL/Osmo-SDR stick
  • Each setup with and without a high-pass filter after the antenna element

Somebody was also thinking in these directions:


Although it won’t be used anymore, for sake of completeness, here are some images of the original Dressler Bias-Tee, that was used to feed power to the LNA through the coax cable. It was supplied by a 12V power supply. It seems that the voltage feeding the MMIC’s was kept constant and an adjustable attenuator (the blue part) was used to prevent receiver input overloading.

Dressler Bias-Tee Component-Side

Dressler Bias-Tee Solder-Side


Ideally, the log-per-spiral assembly should be simulated with NEC to get a better understanding of the design principle. Afterwards the antenna should be evaluated with a network analyzer, to find out if there is any room for improvement, leading to evolution instead of simple replication. But, as Lord Kelvin already said, a long time ago:

If you can not measure it, you can not improve it.

William Thomson, 1st Baron Kelvin


Since the lab has no vector network analyzer yet (it’s on the Wishlist), there currently is no tool available, to be realistically able to improve the design. Therefore, the antenna element should be replicated according to the original design, because it worked surprisingly well for years. When looking at the production quality of the disassembled antenna, it seems that this design type doesn’t have the usual constraints regarding precision as a resonant design would.

The following assembly guide is a conclusive mini-howto, trying to best guess the original assembly instructions, based on the disassembly and reverse engineering process:

Assembly Instructions:

  1. Cut out the antenna element according to specs above
  2. Solder the small LNA connector to the element
  3. Cut a 405x405mm sheet of Aslan S22 lamp shade film
  4. Place Aslan S22 with satin side down (release liner/adhesive side up)
  5. Remove Aslan S22 release liner (protective foil with the printed red grid)
  6. Place antenna element on self-adhesive side of Aslan S22 according to spec above
  7. Get a cylinder with 80mm diameter and place the right end of the assembly on it
  8. Begin rolling the assembly around the cylinder (clockwise from top view)
  9. Roll the release liner around the assembly and fixate it with tape
  10. Remove the 80mm rolling cylinder from the assembly

As soon as the new LNA prototype is tested and all other relevant parts are delivered, the new prototype is going to be built and a more extensive and practically proved assembly documentation will be released.

This would also be the perfect scope for some SDR-Wideband-Antenna-Building workshops, so if you’re interested in having/building one of these too, please drop a note, so that it can be planned. It should be possible to build this Antenna for less than 50EUR.