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More tweaks to user Guide.
git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@7067 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
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@ -112,7 +112,7 @@ d). Edit lines as needed. Keeping them in alphabetic order help see dupes.
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:bill_somerville: mailto:g4wjs -at- c l a s s d e s i g n -dot- com [G4WJS]
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:dev_mail_list: http://sourceforge.net/mailarchive/forum.php?forum_name=wsjt-devel[WSJT Developers Email List]
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:dev_mail_svn: https://sourceforge.net/auth/subscriptions/[WSJT SVN Archives]
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:devmail: mailto:wsjt-devel@lists.sourceforge.net[wsjt-devel]
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:devmail: mailto:wsjt-devel@lists.sourceforge.net[wsjt-devel@lists.sourceforge.net]
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:devmail1: mailto:wsjt-devel@lists.sourceforge.net[Post Message]
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:wsjtgroup_mail: mailto:wsjtgroup@yahoogroups.com[Post Message]
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:greg_beam: mailto:ki7mt@yahoo.com[KI7MT]
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@ -2,9 +2,9 @@
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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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the program name stand for "`Weak Signal communication by K1JT,`"
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while the suffix "`-X`" indicates that _WSJT-X_ started as an extended
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(and originally experimental) branch of the program _WSJT_.
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_WSJT-X_ Version 1.7 offers eight protocols or "`modes`": *JT4*,
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*JT9*, *JT65*, *QRA64*, *WSPR*, *Echo*, *ISCAT*, and *MSK144*. The
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@ -15,29 +15,29 @@ and source encoding. JT65 and QRA64 were designed for EME
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effective for worldwide QRP communication on the HF bands. QRA64 has
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a number of advantages over JT65, including better performance on the
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very weakest signals. We imagine that over time it will replace JT65
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for EME use. JT9 is optimized for the LF, MF, and lower HF bands. It
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is 2 dB more sensitive than JT65 while using less than 10% of the
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bandwidth. JT4 offers a wide variety of tone spacings and has proved
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very effective for EME on microwave bands up to 24 GHz. All of these
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"`slow`" modes use one-minute timed sequences of alternating
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transmission and reception, so a minimal QSO takes four to six minutes
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— two or three transmissions by each station, one sending in odd UTC
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minutes and the other even. On the HF bands, world-wide QSOs are
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possible using power levels of a few watts (or even milliwatts) and
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compromise antennas. On VHF bands and higher, QSOs are possible (by
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EME and other propagation types) at signal levels 10 to 15 dB below
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those required for CW.
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for EME use. JT9 was designed for the LF, MF, and lower HF bands.
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Its submode JT9A is 2 dB more sensitive than JT65 while using less
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than 10% of the bandwidth. JT4 offers a wide variety of tone spacings
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and has proved very effective for EME on microwave bands up to 24 GHz.
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All of these "`slow`" modes use one-minute timed sequences of
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alternating transmission and reception, so a minimal QSO takes four to
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six minutes — two or three transmissions by each station, one sending
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in odd UTC minutes and the other even. On the HF bands, world-wide
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QSOs are possible using power levels of a few watts (or even
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milliwatts) and compromise antennas. On VHF bands and higher, QSOs
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are possible (by EME and other propagation types) at signal levels 10
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to 15 dB below those required for CW.
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*ISCAT*, *MSK144*, and optionally *JT9E-H* are "`fast`" modes designed
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to take advantage of brief signal enhancements from ionized meteor
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trails and other types of scatter propagation. These modes use timed
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sequences of 5, 10, 15, or 30 s duration. User messages are
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transmitted repeatedly at high rate (up to 250 characters per second,
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for MSK144) to make good use of the shortest meteor "`pings`". ISCAT
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uses free-form messages up to 28 characters long, while MSK144 uses
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the same structured messages as the slow modes together with an
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abbreviated format with hashed callsigns for messages sent after
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initial contact has been established.
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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 and other types of scatter propagation. These
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modes use timed sequences of 5, 10, 15, or 30 s duration. User
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messages are transmitted repeatedly at high rate (up to 250 characters
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per second, for MSK144) to make good use of the shortest meteor
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"`pings`". ISCAT uses free-form messages up to 28 characters long,
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while MSK144 uses the same structured messages as the slow modes
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together with an abbreviated format with hashed callsigns for messages
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sent after initial contact has been established between two stations.
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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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