Small Station EME at 10 and 24 GHz:GPS Locking, Doppler Correction, and JT4
Rex Moncur, VK7MO, and Joe Taylor, K1JT

Abstract
GPS frequency locking and automatic Doppler correction, together with a recently improved
JT4 decoder make it possible for small portable stations (40 W and 80 cm dishes) to work
the larger (3 meter dish) home stations on 10 GHz EME, even with libration spreading inexcess of 100 Hz. While 24 GHz JT4F EME signals from a home station (100 W, 2.4 m dish)have been received and decoded using a 47 cm dish, a two way QSO is still a challenge.

1. BackgroundThe digital mode JT65C has been widely used for EME on the lower microwave bands, but
not at 10 or 24 GHz. Doppler shifts on these bands can be as large as 50 kHz and can change
by more than 200 Hz in a minute. Such frequency excursions are well beyond the capabilityof the AFC system currently programmed in WSJT; moreover, at 10 and 24 GHz librationinduced Doppler spreading can be as large as several hundred Hz, much more than the 10.8
Hz tone spacing of JT65C.
WSJT provides a mode called JT4 that offers a range of tone spacings up to 315 Hz. The
submodes with wider spacings are especially appropriate for EME on the higher microwave
bands. JT4 spreads its energy evenly over 4 tones, and does not have an easily identified
synchronizing tone like the one in JT65C. As a consequence, very weak JT4 signals can be
hard to find by tuning across the band. For these and other reasons, making EME contacts isgreatly facilitated by accurate frequency control and automatic real-time Doppler
correction.
Several years ago VK7MO experimented with JT65C on 1296 and 2301 MHz using GPS
locking [1] and Doppler correction controlled by software written by Glen English, VK1XX[2]. The VK1XX program obtains Doppler information from a file written by WSJT andapplies corrections automatically to the IC910-H transceiver at VK7MO. After many hours of
testing with other GPS-locked stations, it has been found that EME signals reliably staylocked to within a few Hz.
In 2010 Charlie Suckling, G3WDG [3], drew attention to the existence of predictable times ofminimum libration on a specified EME path and how to calculate the libration spreading on
own echoes and between stations. The necessary calculations were soon incorporated into
WSJT and also Moonsked, a program by David Anderson, GM4JJJ and EME Planner and
LibCalc by Doug McArthur, VK3UM. Using Moonsked VK7MO was able to find predicted1

times of libration spreading as small as a few Hz at 10 GHz, suitable for use with JT65C [4].
Tests were arranged with Alan Devlin, VK3XPD (75 W, 3 m dish) and after a few attempts a
JT65C EME QSO was completed using the VK7MO portable 10 GHz station — a 64 cm offset
dish and 7 watts at the feed [5]. The deep libration minima last only a few minutes, and it
was surprising at first to discover that VK7MO could copy VK3XPD’s 75 watt transmissions
even when spreading was as large as 150 Hz, well beyond the 10.8 tone spacing of JT65C.
The explanation is contained in a paper by K1JT, presented at the 2010 International EME
Conference [6] (see especially Figures 6 and 7 of that paper, and associated text). While thelimb-to-limb spreading may be over 150 Hz, much of the received energy falls within aquasi-specular peak reflected from the central part of the moon, with much lower
spreading. An example of this effect is shown in Figure 1, the spectrum of a 10 GHz EME
signal received at a time when limb-to-limb libration spread was around 90 Hz, as indicatedby the horizontal bar. The half-power width of the spectrum is only 19 Hz, and nearly half ofthe power falls within ± 5 Hz. JT65C can decode such a signal by taking advantage of thenarrow central peak.

Fig. 1 — Measured spectrum of the VK7MO EME signal at 10 GHz as received by G3WDG.
The width of the central peak is much less than the total limb-to-limb libration spreading,
about 90 Hz at this time.
2

Given this success in using JT65C with wide spreading (albeit one way with higher power)
VK7MO improved his portable station to a 77 cm prime focus dish and a 45 watt DB6NT
power amplifier (Figure 2). After this upgrade it was no longer necessary to wait for the few
minutes of low libration that occur only two or three days a month; it became possible tocomplete QSOs with VK3XPD on about half of all days, at times when the libration spreading
was less than 150 Hz.

Fig. 2 — The VK7MO portable setup for 10 GHz EME.

VK7MO then examined Moonsked predictions to find times of low libration spreading
between Australia and either Europe or North America. On such paths, times of extremely
low spreading were not found; nevertheless, there are many opportunities with spreading
well below 100 Hz. Tests were arranged with Vlada Masek, OK1DAK and Tonda Jelinek,
OK1DAI at the OK1KIR club station, and with Al Ward, W5LUA. EME QSOs at 10 GHz werecompleted easily with these stations from the small VK7MO portable station, using JT65C.
In November 2012 VK7MO set off on a grid square tour across Australia, working from 25
different locators. Many contacts were made with OK1KIR, W5LUA, VK3XPD, and VK3NX [7].
3On returning home VK7MO set his mind to what could be done on 24 GHz with his verysmall portable station (4 W, 47 cm offset dish). Initial 24 GHz tests with W5LUA (100 W, 2.4
m dish) showed clear evidence of his single tone signals (see Section 4 below). After
improving the feed illumination it was occasionally possible to gain synchronization, anecessary prerequisite to successful JT65 decoding. However, no decodes were achieved
despite signal levels and total limb-to-limb spreading at a level that would have decoded on
10 GHz. A likely cause for decoding failure was evident in the appearance of single-tonetransmissions on the waterfall display. The signal was much more evenly distributed overthe full range of Doppler spread, with little evidence of the narrow central peak seen at
10 GHz (cf. Figure 1).
Having pushed JT65C to its limit, VK7MO made some tests with W5LUA using the JT4E mode
(78.75 Hz tone spacing). Sync was achieved on nearly all transmissions, but again there
were no decodes. Some of the test files were sent to K1JT, to see what he could do withthem. Within a few days the files were decoded — we had confirmed that it’s possible tocopy W5LUA’s EME signal on 24 GHz using a 47 cm offset dish.

2. Development and Description of JT4 modes
K1JT has viewed design of the various WSJT protocols and their decoders as a learn-as-yougo process. Some features have been tried and abandoned, while others have beenretained and built upon. JT65 uses a low-rate (high redundancy) code, with 63 six-bit
symbols transmitted to convey just 72 bits of information, and it devotes half of thetransmitted energy to a synchronizing tone. This approach helps the mode to perform wellunder conditions of QSB and intermittent QRM or QRN, and the sync tone provides a handy
visible marker on a waterfall spectral display. A well-designed JT65 decoder often succeeds
even on a signal with deep fades or dropouts, or when two or more signals overlap in both
frequency and time. But JT65’s ratio of occupied bandwidth to information rate is rather
large, and arguably devoting half the transmitted energy to the synchronization is overkill.
For amateur radio use, another downside is that the soft-decision Reed Solomon decoder
uses a patented algorithm [8] and its source code is not “open”. The soft-decision KoetterVardy decoder distributed in executable form with WSJT, MAP65, JT65-HF, and several
other programs yields a 2 dB advantage over hard-decision decoding for steady signals, andeven more under conditions of Rayleigh fading. For long-term viability of the JT65 mode, it’sa pity that the source code is not openly available. The patent expires in 2020.
JT4 was created in 2007 to facilitate experiments with a structured, time-sequenced digitalmode offering more bandwidth flexibility than JT65. For educational reasons, JT4 was built
to use a non-patented, soft-decision sequential decoding algorithm by Fano [9], with opensource code and a very different synchronizing scheme. JT4 and JT65 both use efficient
source-encoding of basic QSO information (callsigns, grid locators, signal reports, and4

acknowledgments) in a fixed-length 72-bit message. Both modes include strong forms oferror-control coding (ECC) — a Reed Solomon (63, 12) code for JT65, and a long-constraint
convolutional code (constraint length K=32, rate r=1/2) for JT4. In both cases the ECC isstrong enough that decoders nearly always produce exactly the message that wastransmitted, or otherwise a flag indicating that decoding has failed. The modulation forboth modes is continuous-phase frequency-shift keying: JT65 uses 65 tones, JT4 uses 4.
With just 4 tones, JT4 can use tone spacings up to 315 Hz to cope with wide libration
spreading and still fit within a standard SSB passband. In both JT65 and JT4 the transmitted
signal has a constant envelope, so full “key down” power is present at all times during atransmission. A detailed description of the JT65 protocol was published in QEX in 2005 [10].
Generation of a JT4 signal starts in the same way, by source-encoding the user’s message
into 72 bits. With a “zero tail” of 31 bits (effectively making a continuous code into a fixedlength block code), the rate-1/2 convolutional encoding increases the number of data bits to(72+31) × 2 = 206. These bits are scrambled in order by bit-reversing their indices, and there-ordered bits are merged with those of an equal length pseudo-random synchronizing
vector to form two-bit channel symbols, as follows:
Symbol[i] = 2 × Data[i] + Sync[i]where i is an index running from 1 to 206.

The channel symbols have values 0 to 3. Multiplied by N, a parameter that defines the tone
separation for each JT4 submode, the symbols control the transmitted audio frequency foreach tone interval, using the equation
Frequency[i] = 118 × 11025/1024 + (Symbol[i] – 1.5) × 4.375 × N.
Values of expansion factor N, the tone separation, and total occupied bandwidth for the JT4
submodes are summarized in Table 1. For comparison, we note that JT65C has tone
spacing 10.8 Hz and total bandwidth 711 Hz.
Table 1. — Expansion factors N, tone spacings, and total bandwidths of the JT4 modes.

Mode

Expansion
Factor N

Tone Spacing(Hz)*

Bandwidth
(Hz)

JT4A
JT4B
JT4C
JT4D
JT4E
JT4F
JT4G

1
2
4
9
18
36
72

4.375
8.75
17.5
39.375
78.75
157.5
315.0

17.5
35
70
158
315
630
1260

* The four tones are spaced around a centre frequency of 1270 Hz

5

The EME experiments at 10 and 24 GHz described in this paper motivated several
improvements to the implementation of JT4 in WSJT. Capability for message averaging has
been added, providing opportunities for decoding a signal 1 to 3 dB below the threshold fora single transmission. A correlation-type decoder has also been added, similar to the one in
JT65. The correlation algorithm can help to determine which message (from a list ofplausible or likely messages) has been received, even when the signal is several dB too weak
to be decoded by the fully general convolutional algorithm. Of course, this approach works
only if the received message is one of those in the list; but there's no reason why a decoder
must be equally sensitive to all possible received messages.
Inverted sync vectors (0 replaced by 1, and vice-versa) are now used for messages that
include two callsigns and a signal report. As with JT65, the decoder now marks mostsynchronized messages with “*”, but those including reports with “#”. As described in
section 4, this scheme helps the receiving operator to decode messages for which averaging
is required.
Regrettably, the prospect for further coding and modulation improvements useful for
microwave EME is not very bright. Phase-coherent techniques are out of the question; therough lunar surface ensures that EME signals on these bands will always have arbitrary,
rapidly varying phases. One could use GPS-based timing and calculated EME delays to doaway with the need for signal energy devoted to synchronization. Such an approach could
gain another 2 dB, approximately [11]. If receiver bandwidths as large as 10 to 20 kHz wereavailable — perhaps by using special equipment similar to that used for MAP65 — a widespaced JT65-like mode with 65 tones (perhaps called JT65G ?) could be used, yielding maybe
another 2 dB from the more efficient modulation [11]. These approaches would require
special hardware, as well as a number of software changes.

3. Results achieved with JT4, and Comparisons with JT65
WSJT and JT4 have now been thoroughly tested with EME signals on both 10 and 24 GHz.
Among highlights of these tests are the following:

VK3XPD (12 W, 3 m dish) worked W5LUA (100 W, 2.4 m dish) for a 24 GHz World
record distance for any mode, 14496 km.



VK3XPD (6 W, due to longer waveguide run when working to his Moonset, 3 m dish)worked OK1KIR (21 W, 4.5 m dish) to extend the 24 GHz World record to 15874 km.



VK7MO (45 W, 0.77 m dish) worked G3WDG (15 W, 3 m dish) for a 10 GHz VK
distance record of 17410 km. G3WDG was copied when using as little as 8 watts.

6

VK7MO (0.47 m dish) copied W5LUA (100 W, 2.4 m dish) under good conditions on 24
GHz. Usually this required averaging of several transmissions. (W5LUA did not detect
the 4-watt signal of VK7MO.)



Subsequently VK7MO upgraded his 24 GHz portable station to a 77 cm dish and 10watt DB6NT PA. With this arrangement VK7MO could decode W5LUA reliably on 24
GHz, mostly without need for averaging. Averaging was still required whenabsorption was high due to cloud cover or elevations less than 10 degrees. (W5LUA
still did not detect the 10 watt signal of VK7MO.)



OK1KIR (4.5 metre dish and 21 watts) was copied on 24 GHz by VK7MO (77 cm dishand 10 watts). OK1KIR was able to detect single tones from VK7MO but not decodesignals.

Revisions 3021 and higher of WSJT include a facility to add noise to a recorded signal so you
can determine the amount of S/N you have “in reserve”. This feature is activated byentering (for example) $-3 in the Tx6 message box, where the -3 indicates a 3 dB
degradation in S/N. Using this facility, VK7MO established that there was a 5 to 6 dBreserve on W5LUA’s signal under good conditions. W5LUA has 10 dB more power than the
VK7MO portable setup and receives additional moon noise on his bigger dish; the differencein system performance is around 12 dB. So even with 6 dB in reserve, another 6 dB is
required to achieve a QSO with a small dish and 10 watts.
Four days of 24 GHz tests between VK7MO and W5LUA showed that the median frequency
error after Doppler correction was less than 20 Hz. On a few occasions the W5LUA antennadrifted off moon centre toward the limb, and the signal shifted in frequency by around 100
Hz. The total limb-to-limb spreading at the time was 200 Hz, so it’s clear that this shift wascaused by the differing Doppler shifts at the centre of the moon and the limb. When
tracking was accurate, apparent frequency variations were always less than 40 Hz at 24 GHz— a clear demonstration of the value of GPS locking and automated Doppler correction.
Atmospheric absorption by water vapour can add several dB of attenuation at 24 GHz,
especially when the moon elevation is low and the atmospheric path longer. The
atmosphere holds much less water vapour in winter, so winter conditions are generally best.
Of course, for trans-equatorial paths it cannot be winter at both ends, and for Australia to
Europe or North America elevations will always be rather low. Atmospheric absorption willthen be more of an issue.
On-the-air tests with the latest versions of WSJT show that for narrow signals the sensitivityof JT4 is only 1 to 2 dB worse than JT65C. As Doppler spreading increases beyond 10 Hz thewide-spaced JT4 submodes lose around 1 dB of sensitivity for each doubling of spreading,while JT65C loses more like 3 dB — the exact amount depending on shape of the Dopplerspread profile. Thus, as spreading increases JT4 becomes the preferred mode. In practice7

at 10 GHz, where the spreading has a significant central peak, the crossover point is around
50 – 80 Hz. At 24 GHz, where the spreading is more evenly distributed, the crossover ismore like 20 – 40 Hz and there would rarely be any advantage in using JT65c. For very small
10 GHz stations working a station at the same longitude it is sometimes possible to choose atime when the spreading is low enough (say, < 40 Hz on 10 GHz) to give the advantage to
JT65C; but most of the time JT4 is preferred. In general we recommend using submodeJT4F: its 157.5 Hz tone spacing is usually enough, and its total bandwidth of 630 Hz is smallenough to fit comfortably within a SSB receiver’s passband, with some reserve toaccommodate possible frequency-control issues. Finally, we note that another advantage of
JT4 over JT65C is that its wider tone spacing allows nearly smooth Doppler corrections onradios such as the FT-817 with 10 Hz incremental tuning steps. For JT65C, it’s importantthat Doppler corrections be done with 1 Hz tuning steps.

4. Procedures for Microwave Doppler Corrected EME
The latest version of the WSJT software can be downloaded from a link posted at
http://physics.princeton.edu/pulsar/K1JT/wsjt.html
In JT4 mode the program works similarly to JT65, but there are some significant differences.
Single Tones: JT65 offers two-tone shorthand messages for the common EME information
RO, RRR and 73. With GPS locking and automatic Doppler correction we can use frequency
offset of a single tone to convey such simple information. A single tone is easier to see on
the waterfall, since the full Tx energy is focused in one place. JT4 has therefore adopted
the following meanings for single-tone messages:@1500 Hz = RRR@1700 Hz = 73
Single tones are sent by using the @ symbol followed by a number representing frequencyof the tone. As described below, single-tone messages for RRR and 73 usually appear in Tx
message boxes 4 and 5. For a station that is not fully GPS locked (for example, the IF radio is
free-running) it is important to establish the centre frequency as a reference against which
to measure other tones such as RRR and 73. For this purpose a 1270 Hz tone may betransmitted at the start of a QSO. If a station appears slightly off frequency you can click on
the waterfall to centre the green tick on the received 1270 Hz tone; the two red ticks to theright then respectively represent RRR and 73. The @1270 tone can be manually added inplace of the CQ message in Tx6. It is also possible to replace the CQ message with @1270 in
the Tx6 message template, on the Setup screen.
@1000 Hz: Often when working portable it is impossible to align on the moon visually due
to cloud. As moon noise is too weak on a small dish the best way of alignment is to peak on
8

the single tone being sent from the other station. In order that the other station knows thatyou have completed alignment and are ready to receive messages, the recommended
procedure is to start with a 1270 Hz tone for both frequency and pointing alignment; when
you are ready to receive messages you send a 1000 Hz tone. The change can be done in the
middle of a transmission: indeed, it proves to be more positive if the other station sees sucha frequency discontinuity within a single transmission.
@2000 Hz: The 2000 Hz single tone is used to represent QRT so that a portable station canlet people know that they are closing.
Yellow Graph to help identify weak single tones: The Setup menu includes a new option“Plot average JT4 spectrum”. If this is ticked, a yellow curve will be displayed in thegraphical section of the main window. This can be used to identify the frequency of single
tones too weak to show up on the waterfall. Moving the mouse cursor vertically along theline of the yellow peak will activate a highlighted yellow box showing the frequency
difference from the nominal 1270 Hz. Thus if you see a highlighted DF of 230 Hz thisidentifies an RRR tone and 430 Hz identifies a 73 tone. A starting @1270 Hz tone will show
up close to DF=0. If the starting @1270 is slightly off you will need to do some mentalarithmetic to check the RRR and 73 tones. But if the tones are sufficiently strong to see on
the waterfall and the green tick is on @1270 then the correction is automatically done andyou just read below the red markers.
Signal Reports: We recommend using numerical signal reports for microwave digital EME.
Among other obvious advantages, such reports ensure that you exchange some unknown
information as well as identifying the callsigns of both stations, thereby complying with theoriginal 1957 Tilton VHF definition of a minimal QSO [12]. Message generation is madeeasier by setting message templates on the Setup/Options screen, as follows:
Tx 1: %T %M %G
Tx 2: %T %M %R
Tx 3: %T %M R%R
Tx 4: @1500 (RRR)
Tx 5: @1700 (73)
Tx 6: @1270 (START)
If you double-right-click on the other station’s callsign in the decoded text window, WSJT
will automatically generate messages with the correct report. If you achieve a decode only
after averaging, estimate a dB value, insert it manually into the Rpt box, and click Gen Msgs.
It’s probably best to insert a report the first time you get a good signal in the average (goodDT and DF) and then click Gen Msgs so you’re ready to send a report as soon as you get an9average decode. Once having started to send a report you should stick to it, since the otherstation may need to use averaging and that requires a constant message.
Message Averaging: Averaging has always been a feature of JT65, but in our tests it rarely
came into play even at 10 GHz. We have found that at 24 GHz averaging is the norm. In
part this is because our signals have been weaker, but the diffuse 24 GHz reflections also
give a more consistent signal level. When averaging is likely to be important you should
clear the average as soon as the other station starts sending messages. The first message
sent by both stations will include callsigns and grid locators. This message is accompanied
by a “*” sync indicator. Once one station copies the other they move to Tx2 and themessage will change to a “#” sync. As soon as you see the “#” sync, click on Clr Avg to starta new average and press the Decode button again. The use of averaging requires you to pay
attention to the values of DT and DF, rejecting inconsistent transmissions with the Exclude
button. Effective use of averaging requires some practice, but it can help you to pick up thatlast 1 or 2 dB.
Sync Setting: The default setting of WSJT’s Sync control is 1, which may help to limit the
number of false decodes. In practice on 10 and 24 GHz there are few birdies to trigger false
decodes, and our operational experience is that it‘s best to set Sync to 0, so as to see andevaluate the weakest signals.
MinW control: The JT4 decoder starts by assuming minimum frequency spreads
comparable with the setting of the MinW control, using the same labels A–G as those for
the JT4 submodes, see Table 1. If decoding fails, it proceeds to the next higher width. By
this means the decoder optimises the bin-width to match the spreading of the signal. To
speed up the decoding process and avoid the picking up false syncs at lower widths,
experience suggests it is best to set the starting width just one or two steps below thepredicted spreading. For example, if the predicted limb-to-limb spreading is 200 Hz you
might set MinW at the "E" level, representing a bin-width of 78.25 Hz. The final column in aline of decoded text will contain a letter representing the bin-width actually used.
Freeze and Tolerance: When you have identified your QSO partner’s signal, limit thefrequency range over which decoding is attempted by using the Freeze and Tol (tolerance)
controls. We find that Tol = 50 is generally sufficient for Doppler corrected signals, evenwith spreading in excess of 200 Hz. Freeze can be set at the time you see the initial @1270
Hz tone, and reset if you should see DF drifting, for signals that are otherwise correct — forexample, they decode or have DT consistent with previous transmissions.

5. Prospects for a 24 GHz Portable Station
We have shown that it’s possible for a 24 GHz portable station with a 47 cm dish to copy agood home station such as W5LUA (100 W TWT, 2.4 m dish). However nothing has been
10

copied from the portable station even when running 10 watts to a larger 77 cm dish. As
discussed in Section 3 it seems that at least another 6 dB will be required to complete a QSO
with a small portable station, and then only under good conditions.
In Section 2 we argued that the prospects for improving system performance with bettercoding and modulation are limited. Making up 6 dB by increasing antenna size would
require a dish of 1.6 metres, which is a practical upper limit for convenient portable
operation. Another option is to increase power. High power TWTs run at around 12000
volts; the necessary HV supplies are heavy and susceptible to breakdowns with humidity inopen air. They are hardly good candidates for portable operation. Some amateurs, forexample JA8CMY [13], are home brewing up to 38 watt solid state amplifiers based 8
TGA4915 modules giving almost 6 dB over the 10 watt DB6NT amplifier used to date.
Alternatively 21 watts solid state has been achieved by OK1KIR with a pair of DB6NT PAs. It
seems that a viable portable operation able to cope with more-than-minimum atmosphericand libration losses will require improvements in both dish size and power — perhaps anincrease in dish size to around 1.6 m and a home-built 30 watt PA. It will be a challenge.

6. Conclusions
We have shown that small-station, portable 10 GHz EME is feasible by taking advantage ofGPS frequency locking, automatic Doppler correction, and recent improvements in the JT4
decoder. Achieving similar capability at 24 GHz is the next challenge, but it will not be easy.
We recommend using digital mode JT4F for amateur EME communication with small
stations at 10 and 24 GHz. It’s worth noting that JT4F, with the improved decoder, should
also work well for rain scatter at 10 GHz.

7. Acknowledgments
The developments and advances reported here owe much to the efforts of the following
stations who provided on-the-air test signals and contributed to discussion of results withina small email group: The OK1KIR club station operated by Vlada Masek, OK1DAK and Tonda
Jelinek, OK1DAI, Al Ward W5LUA, Alan Devlin VK3XPD, Charlie Suckling G3WDG, and Gerald
Williamson, K5GW (who has also developed a separate version of the Doppler correction
program for use with the Flex Radio). Thanks also to Glen English, VK1XX for writing theoriginal Doppler correction program for the IC-910-H, and adding capability for the FT-817.
His program should be useful on most modern ICOM and Yaesu rigs that have CAT control.

References[1] GPS locking: Refer http://www.vk3hz.net/ and scroll down to Rig locking for information
on GPS locking various rigs. GPS locking modules have been developed by VK3HZ and11

VK3XDK available built up for various rigs http://www.vk3hz.net/XRef/XRef_Home.html . At
10 & 24 GHz the DB6NT transverters offer the ability to lock to a 10 MHz GPS reference.
[2] VK1XX software: This is available for download at:www.vk3hz.net/microwave/doppler141.zip[3] “Predicting Libration Fading on the EME Path ”, 14th International EME Conference,
Dallas, August 2010 and DUBUS 3/2010
http://www.vk3um.com/G3WDG_libration%20paper%20revised.pdf[4] Occurrence of low libration spreading, VK7MO:
http://www.vk3hz.net/microwave/Low-Libration-EME.pdf[5] Using JT65C near libration minima VK7MO and VK3XPD:
http://www.vk3hz.net/microwave/10-GHz-EME-QSO-with-64-cm.pdf[6] “Frequency-Dependent Characteristics of the EME Path”, 14th International EME
Conference, Dallas, August 2010;
http://www.physics.princeton.edu/pulsar/K1JT/EME2010_K1JT.pdf.
[7] The VK7MO grid tour:
http://www.vk3hz.net/microwave/10GHz-EME-Grid-Square-Tour.pdf[8] R. Koetter, A. Vardy, “Algebraic Soft-Decision Decoding of Reed-Solomon Codes,” IEEE
Transactions on Information Theory , v49, pp. 2809–2825, 2001.
[9] R. M. Fano, “A Heuristic Discussion of Probabilistic Coding,” IEEE Transactions on
Information Theory, v9, pp. 11–25, 1957.
[10] “The JT65 Communications Protocol”, QEX, September-October 2005;
http://physics.princeton.edu/pulsar/K1JT/JT65.pdf.
[11] J. G. Proakis, Digital Communications, p. 211. McGraw-Hill, New York (1983).
[12] E. P. Tilton, W1HDQ, QST p.56 (March 1957).
[13] 38 watt solid state 24 GHz PA, JA8CMY:
http://millimeterwave.free.fr/PA%2024GHz%20JA8CMY%20TGA4915.htm

12