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	Documentation updates
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								README
									
									
									
									
									
								
							| @ -11,11 +11,11 @@ | |||||||
|                                                           |                                                           | ||||||
|                                                           |                                                           | ||||||
|                                                           |                                                           | ||||||
| Copyright (C) 2001 - 2019 by Joe Taylor, K1JT. | Copyright (C) 2001 - 2021 by Joe Taylor, K1JT. | ||||||
| 
 | 
 | ||||||
| WSJT-X Version 2.1 offers ten different protocols or modes: FT4, FT8, | WSJT-X Version 2.3 offers ten different protocols or modes: FT4, FT8, | ||||||
| JT4, JT9, JT65, QRA64, ISCAT, MSK144, WSPR, and Echo. The first six | JT4, JT9, JT65, QRA64, FST4, ISCAT, MSK144, WSPR, FST4W, and Echo. The | ||||||
| are designed for making reliable QSOs under weak-signal | first seven are designed for making reliable QSOs under weak-signal | ||||||
| conditions. They use nearly identical message structure and source | conditions. They use nearly identical message structure and source | ||||||
| encoding. JT65 and QRA64 were designed for EME (“moonbounce”) on the | encoding. JT65 and QRA64 were designed for EME (“moonbounce”) on the | ||||||
| VHF/UHF bands and have also proven very effective for worldwide QRP | VHF/UHF bands and have also proven very effective for worldwide QRP | ||||||
| @ -35,7 +35,12 @@ dB. FT4 is faster still (7.5 s T/R sequences) and especially well | |||||||
| suited for radio contesting. On the HF bands, world-wide QSOs are | suited for radio contesting. On the HF bands, world-wide QSOs are | ||||||
| possible with any of these modes using power levels of a few watts (or | possible with any of these modes using power levels of a few watts (or | ||||||
| even milliwatts) and compromise antennas. QSOs are possible at signal | even milliwatts) and compromise antennas. QSOs are possible at signal | ||||||
| levels 10 to 15 dB below those required for CW. | levels 10 to 15 dB below those required for CW. FST4 has similarities | ||||||
|  | in use to JT9 but offers more flexibility as it offers different | ||||||
|  | period lengths allowing QSO completion time to be traded off against | ||||||
|  | sensitivity. In its base form of FST4-60A it has better sensitivity | ||||||
|  | than JT9A and should be considered as an upgrade where JT9 has been | ||||||
|  | the preferred slow QSO mode. | ||||||
| 
 | 
 | ||||||
| Note that even though their T/R sequences are short, FT4 and FT8 are | Note that even though their T/R sequences are short, FT4 and FT8 are | ||||||
| classified as slow modes because their message frames are sent only | classified as slow modes because their message frames are sent only | ||||||
| @ -64,6 +69,11 @@ internet access can automatically upload reception reports to a | |||||||
| central database called WSPRnet that provides a mapping facility, | central database called WSPRnet that provides a mapping facility, | ||||||
| archival storage, and many other features. | archival storage, and many other features. | ||||||
| 
 | 
 | ||||||
|  | FST4W, like WSPR, is a quasi-beacon mode, it targets LF and MF bands | ||||||
|  | and offers a number of T/R periods form 2 minutes up to 30 minutes for | ||||||
|  | the most challenging weak signal paths. Similarly to WSPR reception | ||||||
|  | reports can be automatically uploaded to the WSPRnet.org web service. | ||||||
|  | 
 | ||||||
| Echo mode allows you to detect and measure your own station’s echoes | 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. | from the moon, even if they are far below the audible threshold. | ||||||
| 
 | 
 | ||||||
| @ -78,11 +88,12 @@ WSJT-X is an open-source project released under the GPLv3 license (See | |||||||
| COPYING). If you have programming or documentation skills or would | COPYING). If you have programming or documentation skills or would | ||||||
| like to contribute to the project in other ways, please make your | like to contribute to the project in other ways, please make your | ||||||
| interests known to the development team.  The project’s source-code | interests known to the development team.  The project’s source-code | ||||||
| repository can be found at https://sourceforge.net/projects/wsjt, and | repositories can be found at | ||||||
|  | https://sourceforge.net/p/wsjt/wsjtx/ci/master/tree/, and | ||||||
| communication among the developers takes place on the email reflector | communication among the developers takes place on the email reflector | ||||||
| https://sourceforge.net/p/wsjt/mailman.  User-level questions and | https://sourceforge.net/p/wsjt/mailman.  User-level questions and | ||||||
| answers, and general communication among users is found on the | answers, and general communication among users is found on the | ||||||
| https://groups.yahoo.com/neo/groups/wsjtgroup/info email reflector. | https://wsjtx.groups.io/g/main email reflector. | ||||||
| 
 | 
 | ||||||
| 
 | 
 | ||||||
| Project web site: | Project web site: | ||||||
| @ -92,4 +103,4 @@ https://www.physics.princeton.edu/pulsar/K1JT/wsjtx.html | |||||||
| Project mailing list (shared with other applications from the same | Project mailing list (shared with other applications from the same | ||||||
| team): | team): | ||||||
| 
 | 
 | ||||||
| https://groups.yahoo.com/neo/groups/wsjtgroup | https://sourceforge.net/projects/wsjt/lists/wsjt-devel | ||||||
|  | |||||||
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