81 lines
		
	
	
		
			4.1 KiB
		
	
	
	
		
			Plaintext
		
	
	
	
	
	
		
		
			
		
	
	
			81 lines
		
	
	
		
			4.1 KiB
		
	
	
	
		
			Plaintext
		
	
	
	
	
	
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								 __       __   ______      _____  ________      __    __ 
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								|  \  _  |  \ /      \    |     \|        \    |  \  |  \
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								| $$ / \ | $$|  $$$$$$\    \$$$$$ \$$$$$$$$    | $$  | $$
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								| $$/  $\| $$| $$___\$$      | $$   | $$ ______ \$$\/  $$
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								| $$  $$$\ $$ \$$    \  __   | $$   | $$|      \ >$$  $$ 
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								| $$ $$\$$\$$ _\$$$$$$\|  \  | $$   | $$ \$$$$$$/  $$$$\ 
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								| $$$$  \$$$$|  \__| $$| $$__| $$   | $$       |  $$ \$$\
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								| $$$    \$$$ \$$    $$ \$$    $$   | $$       | $$  | $$
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								 \$$      \$$  \$$$$$$   \$$$$$$     \$$        \$$   \$$
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								Copyright (C) 2001 - 2016 by Joe Taylor, K1JT.
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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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								the program name stand for  “Weak Signal communication by K1JT,” while
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								the  suffix “-X”  indicates that  WSJT-X started  as an  extended (and
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								experimental) branch of the program WSJT.
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								WSJT-X Version  1.6 offers five  protocols or “modes”: JT4,  JT9, JT65
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								WSPR, and Echo.  The first three are designed for making reliable QSOs
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								under  extreme  weak-signal  conditions.  They  use  nearly  identical
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								message  structure and  source encoding.   JT65 was  designed for  EME
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								(“moonbounce”) on the VHF/UHF bands and has also proven very effective
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								for worldwide QRP communication on the HF bands.  JT9 is optimized for
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								the LF, MF, and  lower HF bands.  It is 2 dB  more sensitive than JT65
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								while using less than 10% of the bandwidth.  JT4 offers a wide variety
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								of tone  spacings and has proved  very effective for EME  on microwave
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								bands up  to 24 GHz.   All three of  these modes use  one-minute timed
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								sequences of alternating transmission and  reception, so a minimal QSO
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								takes  four to  six  minutes  — two  or  three  transmissions by  each
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								station, one sending in odd UTC minutes  and the other even. On the HF
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								bands, world-wide QSOs are possible using  power levels of a few watts
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								and compromise antennas.   On VHF bands and higher,  QSOs are possible
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								(by EME  and other  propagation types)  at signal levels  10 to  15 dB
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								below those required for CW.
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								WSPR  (pronounced  “whisper”)  stands   for  Weak  Signal  Propagation
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								Reporter.   The  WSPR  protocol  was designed  for  probing  potential
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								propagation  paths   using  low-power  transmissions.   WSPR  messages
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								normally carry the transmitting  station’s callsign, grid locator, and
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								transmitter power in  dBm, and they can be  decoded at signal-to-noise
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								ratios as  low as  -28 dB  in a  2500 Hz  bandwidth.  WSPR  users with
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								internet access can automatically upload  their reception reports to a
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								central database  called {wsprnet}  that provides a  mapping facility,
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								archival storage, and many other features.
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								Echo mode allows you to detect and measure your own lunar echoes, even
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								if they are far below the audible threshold.
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								WSJT-X provides spectral displays for  passbands up to 5 kHz, flexible
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								rig control for nearly all modern  radios used by amateurs, and a wide
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								variety of  special aids  such as automatic  Doppler tracking  for EME
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								QSOs  and Echo  testing.  The  program runs  equally well  on Windows,
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								Macintosh, and Linux systems,  and installation packages are available
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								for all three platforms.
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								WSJT-X is an  open-source project released under the  GPL license (See
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								COPYING). If  you have  programming or  documentation skills  or would
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								like to  contribute to  the project  in other  ways, please  make your
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								interests known  to the  development team.  The  project’s source-code
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								repository can be  found at https://sourceforge.net/projects/wsjt, and
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								most  communication among  the  developers takes  place  on the  email
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								reflector      https://sourceforge.net/p/wsjt/mailman.      User-level
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								questions and answers, and general  communication among users is found
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								on   the    https://groups.yahoo.com/neo/groups/wsjtgroup/info   email
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								reflector.
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								Project web site:
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								http://www.physics.princeton.edu/pulsar/K1JT/wsjtx.html
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								Project mailing  list (shared  with other  applications from  the same
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								team):
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								https://groups.yahoo.com/neo/groups/wsjtgroup
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