WSJT-X/doc/source/jt65-jt9-differences.adoc
Joe Taylor 784e246557 1. Fix a bug that could cause decoder to hang when presented with
bad data.

2. Fix a bug that could allow a Koetter-Vardy false decode instead of
a valid Berlekamp-Massey decode, sometimes leading to program crash.

3. Many more edits in the User's Guide, *.adoc files.



git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@3664 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
2014-01-27 21:28:54 +00:00

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// Status=review
The JT65 protocol was described in a {jt65protocol} in 2005; details
of the JT9 protocol are presented in the next section of this Guide.
To users already familiar with JT65, the most striking difference
between the two modes is the much smaller occupied bandwidth of JT9:
15.6 Hz, compared with 177.6 Hz for JT65A. Transmissions in the two
modes are essentially the same length, and both modes use exactly 72
bits to carry message information. At the user level the two modes
support nearly identical message structures.
JT65 signal reports are constrained to the range 1 to 30 dB. This
range is more than adequate for EME purposes, but not really enough
for optimum use at HF and below. S/N values displayed by the JT65
decoder are clamped at an upper limit 1 dB. Moreover, the S/N scale
in present JT65 decoders is nonlinear above 10 dB.
By comparison, JT9 allows for signal reports in the range 50 to +49
dB. It manages this by taking over a small portion of ``message
space'' that would otherwise be used for grid locators within 1 degree
of the south pole. The S/N scale of the present JT9 decoder is
reasonably linear (although its not intended to be a precision
measurement tool).
With clean signals and a clean nose background, JT65 achieves nearly
100% decoding down to S/N = 22 dB and about 50% at 24 dB. JT9 is
about 2 dB better, achieving 50% decoding at about 26 dB. Both modes
produce extremely low false-decode rates.
Early experience suggests that under most HF propagation conditions
the two modes have comparable reliability. The tone spacing of JT9 is
about two-thirds that of JT65, so in some disturbed ionospheric
conditions in the higher portion of the HF spectrum, JT65 may do
better.
JT9 is an order of magnitude better in spectral efficiency. On a busy
HF band, we often find the 2-kHz-wide JT65 sub-band filled
wall-to-wall with signals. Ten times as many JT9 signals can fit into
the same frequency range, without overlap.
JT65 signals often decode correctly even when they overlap. Such
behavior is much less likely with JT9 signals, which fill their occupied
bandwisth more densely. JT65 may also be more forgiving of small
frequency drifts.