2015-05-27 23:50:08 +00:00
										 
									 
								 
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								// Status=review
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								_WSJT-X_ is a computer program designed to facilitate basic amateur
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								radio communication using very weak signals. The first four letters in
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											2016-10-13 20:28:02 +00:00
										 
									 
								 
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								the program name stand for "`**W**eak **S**ignal communication by
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								K1**JT**,`" while the suffix "`-X`" indicates that _WSJT-X_ started as
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								an extended and experimental branch of the program
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											2016-10-13 20:28:02 +00:00
										 
									 
								 
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								_WSJT_.
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											2015-05-27 23:50:08 +00:00
										 
									 
								 
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											2018-12-07 01:44:19 +00:00
										 
									 
								 
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								_WSJT-X_ Version {VERSION_MAJOR}.{VERSION_MINOR} offers nine different
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								protocols or modes: *FT8*, *JT4*, *JT9*, *JT65*, *QRA64*, *ISCAT*,
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								*MSK144*, *WSPR*, and *Echo*.  The first five are designed for making
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								reliable QSOs under extreme weak-signal conditions. They use nearly
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								identical message structure and source encoding.  JT65 and QRA64 were
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								designed for EME ("`moonbounce`") on the VHF/UHF bands and have also
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								proven very effective for worldwide QRP communication on the HF bands.
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								QRA64 has a number of advantages over JT65, including better
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								performance on the very weakest signals.  We imagine that over time it
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								may replace JT65 for EME use.  JT9 was originally designed for the LF,
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								MF, and lower HF bands.  Its submode JT9A is 2 dB more sensitive than
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								JT65 while using less than 10% of the bandwidth.  JT4 offers a wide
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								variety of tone spacings and has proven highly effective for EME on
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								microwave bands up to 24 GHz.  These four "`slow`" modes use
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								one-minute timed sequences of alternating transmission and reception,
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								so a minimal QSO takes four to six minutes — two or three
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								transmissions by each station, one sending in odd UTC minutes and the
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								other even.  FT8 is operationally similar but four times faster
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								(15-second T/R sequences) and less sensitive by a few dB.  On the HF
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								bands, world-wide QSOs are possible with any of these modes using
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								power levels of a few watts (or even milliwatts) and compromise
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								antennas.  On VHF bands and higher, QSOs are possible (by EME and
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								other propagation types) at signal levels 10 to 15 dB below those
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								required for CW.
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											2016-09-08 17:04:18 +00:00
										 
									 
								 
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											2016-10-17 20:51:16 +00:00
										 
									 
								 
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								*ISCAT*, *MSK144*, and optionally submodes *JT9E-H* are "`fast`"
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								protocols designed to take advantage of brief signal enhancements from
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								ionized meteor trails, aircraft scatter, and other types of scatter
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								propagation. These modes use timed sequences of 5, 10, 15, or 30 s
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								duration.  User messages are transmitted repeatedly at high rate (up
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								to 250 characters per second, for MSK144) to make good use of the
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								shortest meteor-trail reflections or "`pings`".  ISCAT uses free-form
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								messages up to 28 characters long, while MSK144 uses the same
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								structured messages as the slow modes and optionally an abbreviated
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								format with hashed callsigns.  
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								*WSPR* (pronounced "`whisper`") stands for **W**eak **S**ignal
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								**P**ropagation **R**eporter.  The WSPR protocol was designed for probing
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								potential propagation paths using low-power transmissions. WSPR
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								messages normally carry the transmitting station’s callsign, grid
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								locator, and transmitter power in dBm, and they can be decoded at
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											2018-12-04 14:34:08 -05:00
										 
									 
								 
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								signal-to-noise ratios as low as -31 dB in a 2500 Hz bandwidth.  WSPR
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								users with internet access can automatically upload reception
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								reports to a central database called {wsprnet} that provides a mapping
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								facility, archival storage, and many other features.
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								*Echo* mode allows you to detect and measure your own station's echoes
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								from the moon, even if they are far below the audible threshold.
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								_WSJT-X_ provides spectral displays for receiver passbands as wide as
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								5 kHz, flexible rig control for nearly all modern radios used by
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								amateurs, and a wide variety of special aids such as automatic Doppler
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								tracking for EME QSOs and Echo testing.  The program runs equally well
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								on Windows, Macintosh, and Linux systems, and installation packages
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								are available for all three platforms.
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											2018-02-02 19:31:54 +00:00
										 
									 
								 
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								*Version Numbers:* _WSJT-X_ release numbers have major, minor, and
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								patch numbers separated by periods: for example, _WSJT-X_ Version
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											2018-02-08 02:27:24 +00:00
										 
									 
								 
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								1.9.0.  Temporary "`beta`" release candidates are sometimes made in
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								advance of a new general-availability release, in order to obtain user
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											2018-02-07 20:52:01 +00:00
										 
									 
								 
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								feedback.  For example, version 1.9.0-rc1, 1.9.0-rc2, etc., would
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								be beta releases leading up to the final release of v1.9.0.
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								Release candidates should be used _only_ during a short testing
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								period. They carry an implied obligation to provide feedback to the
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								program development group.  Candidate releases should not be used on
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								the air after a full release with the same number has been made.
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