2015-05-27 19:50:08 -04:00
|
|
|
|
// Status=review
|
|
|
|
|
|
|
|
|
|
_WSJT-X_ is a computer program designed to facilitate basic amateur
|
|
|
|
|
radio communication using very weak signals. The first four letters in
|
2016-10-13 16:28:02 -04:00
|
|
|
|
the program name stand for "`**W**eak **S**ignal communication by
|
|
|
|
|
K1**JT**,`" while the suffix "`-X`" indicates that _WSJT-X_ started as
|
2016-10-17 16:51:16 -04:00
|
|
|
|
an extended and experimental branch of the program
|
2016-10-13 16:28:02 -04:00
|
|
|
|
_WSJT_.
|
2015-05-27 19:50:08 -04:00
|
|
|
|
|
2018-12-06 20:44:19 -05:00
|
|
|
|
_WSJT-X_ Version {VERSION_MAJOR}.{VERSION_MINOR} offers nine different
|
|
|
|
|
protocols or modes: *FT8*, *JT4*, *JT9*, *JT65*, *QRA64*, *ISCAT*,
|
|
|
|
|
*MSK144*, *WSPR*, and *Echo*. The first five are designed for making
|
|
|
|
|
reliable QSOs under extreme weak-signal conditions. They use nearly
|
|
|
|
|
identical message structure and source encoding. JT65 and QRA64 were
|
|
|
|
|
designed for EME ("`moonbounce`") on the VHF/UHF bands and have also
|
|
|
|
|
proven very effective for worldwide QRP communication on the HF bands.
|
|
|
|
|
QRA64 has a number of advantages over JT65, including better
|
|
|
|
|
performance on the very weakest signals. We imagine that over time it
|
|
|
|
|
may replace JT65 for EME use. JT9 was originally designed for the LF,
|
|
|
|
|
MF, and lower HF bands. Its submode JT9A is 2 dB more sensitive than
|
|
|
|
|
JT65 while using less than 10% of the bandwidth. JT4 offers a wide
|
|
|
|
|
variety of tone spacings and has proven highly effective for EME on
|
|
|
|
|
microwave bands up to 24 GHz. These four "`slow`" modes use
|
|
|
|
|
one-minute timed sequences of alternating transmission and reception,
|
|
|
|
|
so a minimal QSO takes four to six minutes — two or three
|
|
|
|
|
transmissions by each station, one sending in odd UTC minutes and the
|
|
|
|
|
other even. FT8 is operationally similar but four times faster
|
|
|
|
|
(15-second T/R sequences) and less sensitive by a few dB. On the HF
|
|
|
|
|
bands, world-wide QSOs are possible with any of these modes using
|
|
|
|
|
power levels of a few watts (or even milliwatts) and compromise
|
|
|
|
|
antennas. On VHF bands and higher, QSOs are possible (by EME and
|
|
|
|
|
other propagation types) at signal levels 10 to 15 dB below those
|
|
|
|
|
required for CW.
|
2016-09-08 13:04:18 -04:00
|
|
|
|
|
2016-10-17 16:51:16 -04:00
|
|
|
|
*ISCAT*, *MSK144*, and optionally submodes *JT9E-H* are "`fast`"
|
2016-09-08 16:30:12 -04:00
|
|
|
|
protocols designed to take advantage of brief signal enhancements from
|
2016-10-17 16:51:16 -04:00
|
|
|
|
ionized meteor trails, aircraft scatter, and other types of scatter
|
|
|
|
|
propagation. These modes use timed sequences of 5, 10, 15, or 30 s
|
|
|
|
|
duration. User messages are transmitted repeatedly at high rate (up
|
|
|
|
|
to 250 characters per second, for MSK144) to make good use of the
|
|
|
|
|
shortest meteor-trail reflections or "`pings`". ISCAT uses free-form
|
|
|
|
|
messages up to 28 characters long, while MSK144 uses the same
|
2016-10-26 13:50:48 -04:00
|
|
|
|
structured messages as the slow modes and optionally an abbreviated
|
2016-10-17 16:51:16 -04:00
|
|
|
|
format with hashed callsigns.
|
2016-09-08 13:04:18 -04:00
|
|
|
|
|
2016-10-17 16:51:16 -04:00
|
|
|
|
*WSPR* (pronounced "`whisper`") stands for **W**eak **S**ignal
|
|
|
|
|
**P**ropagation **R**eporter. The WSPR protocol was designed for probing
|
|
|
|
|
potential propagation paths using low-power transmissions. WSPR
|
|
|
|
|
messages normally carry the transmitting station’s callsign, grid
|
|
|
|
|
locator, and transmitter power in dBm, and they can be decoded at
|
2018-12-04 14:34:08 -05:00
|
|
|
|
signal-to-noise ratios as low as -31 dB in a 2500 Hz bandwidth. WSPR
|
2016-10-26 13:50:48 -04:00
|
|
|
|
users with internet access can automatically upload reception
|
2016-10-17 16:51:16 -04:00
|
|
|
|
reports to a central database called {wsprnet} that provides a mapping
|
|
|
|
|
facility, archival storage, and many other features.
|
2015-05-27 19:50:08 -04:00
|
|
|
|
|
2016-10-17 16:51:16 -04:00
|
|
|
|
*Echo* mode allows you to detect and measure your own station's echoes
|
|
|
|
|
from the moon, even if they are far below the audible threshold.
|
2015-11-15 10:01:57 -05:00
|
|
|
|
|
2016-10-17 16:51:16 -04:00
|
|
|
|
_WSJT-X_ provides spectral displays for receiver passbands as wide as
|
|
|
|
|
5 kHz, flexible rig control for nearly all modern radios used by
|
|
|
|
|
amateurs, and a wide variety of special aids such as automatic Doppler
|
|
|
|
|
tracking for EME QSOs and Echo testing. The program runs equally well
|
|
|
|
|
on Windows, Macintosh, and Linux systems, and installation packages
|
|
|
|
|
are available for all three platforms.
|
2015-05-31 11:29:59 -04:00
|
|
|
|
|
2018-02-02 14:31:54 -05:00
|
|
|
|
*Version Numbers:* _WSJT-X_ release numbers have major, minor, and
|
|
|
|
|
patch numbers separated by periods: for example, _WSJT-X_ Version
|
2018-02-07 21:27:24 -05:00
|
|
|
|
1.9.0. Temporary "`beta`" release candidates are sometimes made in
|
2018-02-02 14:31:54 -05:00
|
|
|
|
advance of a new general-availability release, in order to obtain user
|
2018-02-07 15:52:01 -05:00
|
|
|
|
feedback. For example, version 1.9.0-rc1, 1.9.0-rc2, etc., would
|
|
|
|
|
be beta releases leading up to the final release of v1.9.0.
|
2018-02-02 14:31:54 -05:00
|
|
|
|
Release candidates should be used _only_ during a short testing
|
2018-02-07 15:52:01 -05:00
|
|
|
|
period. They carry an implied obligation to provide feedback to the
|
2018-02-02 14:31:54 -05:00
|
|
|
|
program development group. Candidate releases should not be used on
|
|
|
|
|
the air after a full release with the same number has been made.
|