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User Guide edits from Dave, KC3GPM.
This commit is contained in:
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@ -1,7 +1,7 @@
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// Status=review
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// Status=edited
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Source code for _WSJT-X_ is available from a public repository at
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{devrepo}. To compile the program you will need to install at least the
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{devrepo}. To compile the program, at a minimum you must install the
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following packages:
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- Git
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@ -19,7 +19,7 @@ cd wsjtx
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git checkout wsjtx-{VERSION}
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=====
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and for the current development branch,
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and for the current development branch:
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=====
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git clone git://git.code.sf.net/p/wsjt/wsjtx
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@ -1,16 +1,14 @@
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// Status=review
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// Status=edited
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Debian, Ubuntu, and other Debian-based systems including Raspbian:
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NOTE: The project team release binary installer packages for Linux
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when a new _WSJT-X_ release is announced. These are built to
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target one contemporary version of a Linux distribution. Although
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these may work on newer Linux versions or even different
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distributions, it is unlikely that they will work on older
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versions. Check the notes provided with the release for details of the
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targeted Linux distributions and versions. If the binary package is
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not compatible with your Linux distribution or version you must build
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the application from sources.
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NOTE: The project team release binary installer packages targeted for
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one contemporary version of a Linux distribution. Although these may
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work on newer Linux versions or even different distributions, it is
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unlikely that they work on older versions. Check the notes provided
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with the release for details of the targeted Linux distributions and
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versions. If the binary package is not compatible with your Linux
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distribution or version, you must build the application from sources.
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* 32-bit: {debian32}
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- To install:
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@ -1,12 +1,12 @@
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// These instructions are up-to-date for WSJT-X v2.2
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*OS X 10.12* and later: Download the file {osx} to your desktop,
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double-click on it and consult its `ReadMe` file for important
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*macOS10.13* and later: Download the file {osx} to your desktop,
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double-click it and consult its `ReadMe` file for important
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installation notes.
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If you have already installed a previous version, you can retain it by
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changing its name in the *Applications* folder (say, from _WSJT-X_ to
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_WSJT-X_2.1_). You can then proceed to the installation phase.
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changing its name in the *Applications* folder (such as from _WSJT-X_ to
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_WSJT-X_2.2_). You can then proceed to the installation phase.
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Take note also of the following:
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@ -4,7 +4,7 @@ _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 "`**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 e**Xt**ended and e**X**perimental branch of the program _WSJT_,
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an extended and experimental branch of the program _WSJT_,
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first released in 2001. Bill Somerville, G4WJS, and Steve Franke,
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K9AN, have been major contributors to program development since 2013
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and 2015, respectively.
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@ -16,7 +16,7 @@ making reliable QSOs under 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 some advantages over JT65, including better performance
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QRA64 has some advantages over JT65, including better performance
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for EME on the higher microwave bands. JT9 was originally designed
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for the LF, MF, and lower HF bands. Its submode JT9A is 2 dB more
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sensitive than JT65 while using less than 10% of the bandwidth. JT4
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@ -27,7 +27,7 @@ reception, 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. FT4 is
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faster still (7.5 s T/R sequences) and especially well suited for
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faster still (7.5 s T/R sequences) and especially well-suited for
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radio contesting. On the HF bands, world-wide QSOs are possible with
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any of these modes 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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@ -45,7 +45,7 @@ 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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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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@ -80,4 +80,4 @@ be beta releases leading up to the final release of v2.1.0.
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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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the air after a full release with the same number is made.
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@ -1,7 +1,9 @@
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//status: edited
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A basic logging facility in _WSJT-X_ saves QSO information to files
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named `wsjtx.log` (in comma-separated text format) and `wsjtx_log.adi`
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(in standard ADIF format). These files can be imported directly into
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other programs, for example spreadsheets and popular logging programs.
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other programs (such as spreadsheets and popular logging programs).
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As described in the <<INSTALL,Installation>> and <<PLATFORM,Platform
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Dependencies>> sections, different operating systems may place your
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local log files in different locations. You can always navigate to
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@ -12,30 +14,32 @@ applications like {jtalert}, which can log QSOs automatically to other
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applications including {hrd}, {dxlsuite}, and {log4om}.
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The program option *Show DXCC entity and worked before status*
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(selectable on the *Settings | General* tab) is intended mostly for
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(selectable on the *File | Settings | General* tab) is intended mostly for
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use on non-Windows platforms, where {jtalert} is not available. When
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this option is checked _WSJT-X_ appends some additional information to
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this option is checked, _WSJT-X_ appends some additional information to
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all CQ messages displayed in the _Band Activity_ window. The name of
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the DXCC entity is shown, abbreviated if necessary. Your "`worked
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before`" status for this callsign (according to log file
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`wsjtx_log.adi`) is indicated by highlighting colors, if that option
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has been selected.
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is selected.
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_WSJT-X_ includes a built-in `cty.dat` file containing DXCC prefix
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information. Updated files can be downloaded from the {cty_dat} web
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site when required. If an updated `cty.dat` is present in the logs
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folder and readable, it will be used in preference to the built-in
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one.
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site when required. If an updated and readable `cty.dat` file is
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present in the logs folder, it is used in preference to the
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built-in file.
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The log file `wsjtx_log.adi` is updated whenever you log a QSO from
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_WSJT-X_. (Keep in mind that if you erase this file you will lose all
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_WSJT-X_. (Keep in mind that if you erase this file, you lose all
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"`worked before`" information.) You can append or overwrite the
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`wsjtx_log.adi` file by exporting your QSO history as an ADIF file
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from another logging program. Turning *Show DXCC entity and worked
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before status* off and then on again will cause _WSJT-X_ to re-read
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before status* off and then on again causes _WSJT-X_ to re-read
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the log file. Very large log files may cause _WSJT-X_ to slow down
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when searching for calls. If the ADIF log file has been changed
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when searching for calls. If the ADIF log file has been changed
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outside of _WSJT-X_ you can force _WSJT-X_ to reload the file from the
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*Settings | Colors* tab using the *Rescan ADIF Log* button, see
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<<COLORS,Decode Highlighting>>.
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Additional features are provided for *Contest* and *Fox* logging.
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(more to come, here ...)
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@ -37,7 +37,7 @@ assigns more reliable numbers to relatively strong signals.
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NOTE: Signals become visible on the waterfall around S/N = –26 dB and
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audible (to someone with very good hearing) around –15 dB. Thresholds
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for decodability are around -20 dB for FT8, -23 dB for JT4, –25 dB for
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JT65, –27 dB for JT9.
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JT65, and –27 dB for JT9.
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NOTE: Several options are available for circumstances where fast QSOs
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are desirable. Double-click the *Tx1* control under _Now_ or _Next_
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@ -75,7 +75,7 @@ When calling CQ you may also choose to check the box *Call 1st*.
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_WSJT-X_ will then respond automatically to the first decoded
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responder to your CQ.
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NOTE: When *Auto-Seq* is enabled the program de-activates *Enable Tx*
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NOTE: When *Auto-Seq* is enabled, the program de-activates *Enable Tx*
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at the end of each QSO. It is not intended that _WSJT-X_ should make
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fully automated QSOs.
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@ -259,7 +259,7 @@ that a second callsign is never permissible in these messages.
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NOTE: During a transmission your outgoing message is displayed in the
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first label on the *Status Bar* and shown exactly as another station
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will receive it. You can check to see that you are actually
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receives it. You can check to see that you are actually
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transmitting the message you wish to send.
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QSOs involving *Type 2* compound callsigns might look like either
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@ -287,7 +287,7 @@ standard structured messages without callsign prefix or suffix.
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TIP: If you are using a compound callsign, you may want to
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experiment with the option *Message generation for type 2 compound
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callsign holders* on the *Settings | General* tab, so that messages
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callsign holders* on the *File | Settings | General* tab, so that messages
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will be generated that best suit your needs.
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=== Pre-QSO Checklist
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@ -1,6 +1,8 @@
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//Status: edited
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=== Frequency Calibration
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Many _WSJT-X_ capabilities depend on signal-detection bandwidths no
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Many _WSJT-X_ capabilities depend on signal-detection bandwidths of no
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more than a few Hz. Frequency accuracy and stability are therefore
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unusually important. We provide tools to enable accurate frequency
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calibration of your radio, as well as precise frequency measurement of
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@ -11,11 +13,11 @@ measuring the error in dial frequency for each signal.
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You will probably find it convenient to define and use a special
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<<CONFIG-MENU,Configuration>> dedicated to frequency calibration.
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Then complete the following steps, as appropriate for your system.
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Then complete the following steps, as appropriate, for your system.
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- Switch to FreqCal mode
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- In the _Working Frequencies_ box on the *Settings -> Frequencies*
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- In the _Working Frequencies_ box on the *File | Settings | Frequencies*
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tab, delete any default frequencies for *FreqCal* mode that are not
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relevant for your location. You may want to replace some of them with
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reliably known frequencies receivable at your location.
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@ -29,14 +31,14 @@ of WWV at 2.500, 5.000, 10.000, 15.000, and 20.000 MHz, and CHU at
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3.330, 7.850, and 14.670 MHz. Similar shortwave signals are available
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in other parts of the world.
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- In most cases you will want to start by deleting any existing file
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`fmt.all` in the directory where your log files are kept.
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- In most cases, start by deleting any existing file `fmt.all` in the
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directory where your log files are kept.
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- To cycle automatically through your chosen list of calibration
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frequencies, check *Execute frequency calibration cycle* on the
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*Tools* menu. _WSJT-X_ will spend 30 seconds at each
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frequency. Initially no measurement data is saved to the `fmt.all`
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file although it is displayed on screen, this allows you to check your
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file although it is displayed on screen; this allows you to check your
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current calibration parameters.
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- During the calibration procedure, the radio's USB dial frequency is
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@ -61,7 +63,7 @@ the nominal frequency itself (in MHz). For example, the 20 MHz
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measurement for WWV shown above produced a measured tone offset of
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24.6 Hz, displayed in the _WSJT-X_ decoded text window. The resulting
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calibration constant is 24.6/20=1.23 parts per million. This number
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may be entered as *Slope* on the *settings -> Frequencies* tab.
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may be entered as *Slope* on the *File | Settings | Frequencies* tab.
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A more precise calibration can be effected by fitting the intercept
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and slope of a straight line to the whole sequence of calibration
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@ -81,19 +83,19 @@ After running *Execute frequency calibration cycle* at least once with
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good results, check and edit the file `fmt.all` in the log directory
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and delete any spurious or outlier measurements. The line-fitting
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procedure can then be carried out automatically by clicking *Solve for
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calibration parameters* on the *Tools* menu. The results will be
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calibration parameters* on the *Tools* menu. The results are
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displayed as in the following screen shot. Estimated uncertainties
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are included for slope and intercept; `N` is the number of averaged
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frequency measurements included in the fit, and `StdDev` is the root
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mean square deviation of averaged measurements from the fitted
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straight line. If the solution seems valid you will be offered an
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*Apply* button to push that will automatically set the calibration
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parameters in *Settings -> Frequencies -> Frequency Calibration*.
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straight line. If the solution seems valid, you are offered an
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*Apply* button to push that automatically sets the calibration
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parameters in *File | Settings | Frequencies | Frequency Calibration*.
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image::FreqCal_Results.png[align="center",alt="FreqCal_Results"]
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For a quick visual check of the resulting calibration, stay in
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*FreqCal* mode with the *Measure* option cleared. _WSJT-X_ will show
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*FreqCal* mode with the *Measure* option cleared. _WSJT-X_ shows
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the adjusted results directly on the waterfall and the displayed
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records.
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@ -103,8 +105,8 @@ _WSJT-X_ provides a tool that can be used to determine the detailed
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shape of your receiver's passband. Disconnect your antenna or tune to
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a quiet frequency with no signals. With _WSJT-X_ running in one of
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the slow modes, select *Measure reference spectrum* from the *Tools*
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menu. Wait for about a minute and then hit the *Stop* button. A file
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named `refspec.dat` will appear in your log directory. When you check
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menu. Wait for about a minute and then click *Stop*. A file
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named `refspec.dat` appears in your log directory. When you check
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*Ref Spec* on the *Wide Graph*, the recorded reference spectrum will
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then be used to flatten your overall effective passband.
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@ -122,39 +124,39 @@ response* generates an undistorted audio waveform equal to the one
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generated by the transmitting station. Its Fourier transform is then
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used as a frequency-dependent phase reference to compare with the
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phase of the received frame's Fourier coefficients. Phase differences
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between the reference spectrum and received spectrum will include
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between the reference spectrum and received spectrum include
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contributions from the originating station's transmit filter, the
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propagation channel, and filters in the receiver. If the received
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frame originates from a station known to transmit signals having
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little phase distortion (say, a station known to use a properly
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adjusted software-defined-transceiver) and if the received signal is
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little phase distortion (such as a station known to use a properly
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adjusted software-defined transceiver), and if the received signal is
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relatively free from multipath distortion so that the channel phase is
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close to linear, the measured phase differences will be representative
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of the local receiver's phase response.
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Complete the following steps to generate a phase equalization curve:
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- Record a number of wav files that contain decodable signals from
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your chosen reference station. Best results will be obtained when the
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- Record a number of `wav` files that contain decodable signals from
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your chosen reference station. Best results are obtained when the
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signal-to-noise ratio of the reference signals is 10 dB or greater.
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- Enter the callsign of the reference station in the DX Call box.
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- Select *Measure phase response* from the *Tools* menu, and open each
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of the wav files in turn. The mode character on decoded text lines
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will change from `&` to `^` while _WSJT-X_ is measuring the phase
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response, and it will change back to `&` after the measurement is
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of the `wav` files in turn. The mode character on decoded text lines
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changes from `&` to `^` while _WSJT-X_ is measuring the phase
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response, and it changes back to `&` after the measurement is
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completed. The program needs to average a number of high-SNR frames to
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accurately estimate the phase, so it may be necessary to process
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several wav files. The measurement can be aborted at any time by
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several `wav` files. The measurement can be aborted at any time by
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selecting *Measure phase response* again to toggle the phase
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measurement off.
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+
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When the measurement is complete _WSJT-X_ will save the measured
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When the measurement is complete, _WSJT-X_ saves the measured
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phase response in the *Log directory*, in a file with suffix
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".pcoeff". The filename will contain the callsign of the reference
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".pcoeff". The filename contains the callsign of the reference
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station and a timestamp, for example `K0TPP_170923_112027.pcoeff`.
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- Select *Equalization tools ...* under the *Tools* menu and click the
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@ -165,23 +167,23 @@ the proposed phase equalization curve. It's a good idea to repeat the
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phase measurement several times, using different wav files for each
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measurement, to ensure that your measurements are repeatable.
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- Once you are satisfied with a fitted curve, push the *Apply* button
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to save the proposed response. The red curve will be replaced with a
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- Once you are satisfied with a fitted curve, click the *Apply* button
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to save the proposed response. The red curve is replaced with a
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light green curve labeled "Current" to indicate that the phase
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equalization curve is now being applied to the received data. Another
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curve labeled "Group Delay" will appear. The "Group Delay" curve shows
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curve labeled "Group Delay" appears. The "Group Delay" curve shows
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the group delay variation across the passband, in ms. Click the
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*Discard Measured* button to remove the captured data from the plot,
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leaving only the applied phase equalization curve and corresponding
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group delay curve.
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- To revert to no phase equalization, push the *Restore Defaults*
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- To revert to no phase equalization, click the *Restore Defaults*
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button followed by the *Apply* button.
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The three numbers printed at the end of each MSK144 decode line can be
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used to assess the improvement provided by equalization. These numbers
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are: `N` = Number of frames averaged, `H` = Number of hard bit errors
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corrected, `E` = Size of MSK eye diagram opening.
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corrected, and `E` = Size of MSK eye diagram opening.
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Here is a decode of K0TPP obtained while *Measure phase response* was measuring
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the phase response:
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@ -196,7 +198,7 @@ scale. Here's how the same decode looks after phase equalization:
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103900 17 6.5 1493 & WA8CLT K0TPP +07 1 0 1.6
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In this case, equalization has increased the eye opening from 1.2 to
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In this case, equalization has increased the eye-opening from 1.2 to
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1.6. Larger positive eye openings are associated with reduced
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likelihood of bit errors and higher likelihood that a frame will be
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successfully decoded. In this case, the larger eye-opening tells us
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@ -206,7 +208,7 @@ equalization curve is going to improve decoding of signals other than
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those from the reference station, K0TPP.
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It's a good idea to carry out before and after comparisons using a
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large number of saved wav files with signals from many different
|
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large number of saved `wav` files with signals from many different
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stations, to help decide whether your equalization curve improves
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decoding for most signals. When doing such comparisons, keep in mind
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that equalization may cause _WSJT-X_ to successfully decode a frame
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|
@ -1,3 +1,5 @@
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||||
//status: edited
|
||||
|
||||
[[PROTOCOL_OVERVIEW]]
|
||||
=== Overview
|
||||
|
||||
@ -30,17 +32,17 @@ of 4-digit Maidenhead grid locators on earth is 180×180 = 32,400,
|
||||
which is less than 2^15^ = 32,768; so a grid locator requires 15 bits.
|
||||
|
||||
Some 6 million of the possible 28-bit values are not needed for
|
||||
callsigns. A few of these slots have been assigned to special message
|
||||
callsigns. A few of these slots are assigned to special message
|
||||
components such as `CQ`, `DE`, and `QRZ`. `CQ` may be followed by three
|
||||
digits to indicate a desired callback frequency. (If K1ABC transmits
|
||||
on a standard calling frequency, say 50.280, and sends `CQ 290 K1ABC
|
||||
on a standard calling frequency such as 50.280, and sends `CQ 290 K1ABC
|
||||
FN42`, it means that s/he will listen on 50.290 and respond there to
|
||||
any replies.) A numerical signal report of the form `–nn` or
|
||||
`R–nn` can be sent in place of a grid locator. (As originally
|
||||
defined, numerical signal reports `nn` were required to fall between -01
|
||||
and -30 dB. Program versions 2.3 and later accommodate reports between
|
||||
-50 and +50 dB.) A country prefix or portable suffix may be
|
||||
attached to one of the callsigns. When this feature is used the
|
||||
and -30 dB. Recent program versions 2.3 and later accommodate reports between
|
||||
-50 and +49 dB.) A country prefix or portable suffix may be
|
||||
attached to one of the callsigns. When this feature is used, the
|
||||
additional information is sent in place of the grid locator or by
|
||||
encoding additional information into some of the 6 million available
|
||||
slots mentioned above.
|
||||
@ -147,7 +149,8 @@ following pseudo-random sequence:
|
||||
The synchronizing tone is normally sent in each interval having a
|
||||
"`1`" in the sequence. Modulation is 65-FSK at 11025/4096 = 2.692
|
||||
baud. Frequency spacing between tones is equal to the keying rate for
|
||||
JT65A, and 2 and 4 times larger for JT65B and JT65C. For EME QSOs the
|
||||
JT65A, and 2 and 4 times larger for JT65B and JT65C, respectively.
|
||||
For EME QSOs the
|
||||
signal report OOO is sometimes used instead of numerical signal
|
||||
reports. It is conveyed by reversing sync and data positions in the
|
||||
transmitted sequence. Shorthand messages for RO, RRR, and 73 dispense
|
||||
@ -155,7 +158,7 @@ with the sync vector entirely and use time intervals of 16384/11025 =
|
||||
1.486 s for pairs of alternating tones. The lower frequency is the
|
||||
same as that of the sync tone used in long messages, and the frequency
|
||||
separation is 110250/4096 = 26.92 Hz multiplied by n for JT65A, with n
|
||||
= 2, 3, 4 used to convey the messages RO, RRR, and 73.
|
||||
= 2, 3, 4 used to convey the messages RO, RRR, and 73, respectively.
|
||||
|
||||
[[QRA64_PROTOCOL]]
|
||||
==== QRA64
|
||||
@ -225,7 +228,7 @@ the sync bit.
|
||||
[[SLOW_SUMMARY]]
|
||||
==== Summary
|
||||
|
||||
Table 7 provides a brief summary parameters for the slow modes in
|
||||
Table 7 provides a brief summary of parameters for the slow modes in
|
||||
_WSJT-X_. Parameters K and r specify the constraint length and rate
|
||||
of the convolutional codes; n and k specify the sizes of the
|
||||
(equivalent) block codes; Q is the alphabet size for the
|
||||
@ -305,7 +308,7 @@ available character set is:
|
||||
Transmissions consist of sequences of 24 symbols: a synchronizing
|
||||
pattern of four symbols at tone numbers 0, 1, 3, and 2, followed by
|
||||
two symbols with tone number corresponding to (message length) and
|
||||
(message length + 5), and finally 18 symbols conveying the user's
|
||||
(message length + 5), and, finally, 18 symbols conveying the user's
|
||||
message, sent repeatedly character by character. The message always
|
||||
starts with `@`, the beginning-of-message symbol, which is not
|
||||
displayed to the user. The sync pattern and message-length indicator
|
||||
|
Loading…
Reference in New Issue
Block a user