Many more updates to WSJT-X v1.7 User Guide.
git-svn-id: svn+ssh://svn.code.sf.net/p/wsjt/wsjt/branches/wsjtx@7184 ab8295b8-cf94-4d9e-aec4-7959e3be5d79
@ -12,6 +12,7 @@ set (UG_SRCS
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docinfo.html
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docinfo.xml
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acknowledgements.adoc
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astro_data.adoc
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compiling.adoc
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config-details.adoc
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controls-functions-center.adoc
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@ -58,8 +59,11 @@ set (UG_SRCS
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set (UG_IMGS
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images/130610_2343-wav-80.png
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images/AstroData_2.png
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images/Astronomical_data.png
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images/band-settings.png
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images/colors.png
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images/config-menu.png
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images/decode-menu.png
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images/decodes.png
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images/file-menu.png
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@ -69,7 +73,7 @@ set (UG_IMGS
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images/keyboard-shortcuts.png
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images/log-qso.png
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images/MacAppMenu.png
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images/main-ui-1.5.png
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images/main-ui.png
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images/main-ui-controls.png
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images/misc-controls-center.png
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images/misc-main-ui.png
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44
doc/user_guide/en/astro_data.adoc
Normal file
@ -0,0 +1,44 @@
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A text box entitled Astronomical Data provides information needed for
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tracking the sun or moon, moon, compensating for EME Doppler shift,
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and estimating EME Doppler spread and path degradation. Toggle the
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*Astronomical data* on the *View* menu to display or remove this window.
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image::AstroData_2.png[align="center",alt="Astronomical Data"]
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Available information includes the current *Date* and *UTC* time; *Az*
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and *El*, azimuth and elevation of the moon at your own location, in
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degrees; *SelfDop*, *Width*, and *Delay*, the Doppler shift, full
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limb-to-limb Doppler spread, and delay of your own EME echoes; and
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*DxAz* and *DxEl*, *DxDop*, and *DxWid*, corresponding parameters for
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a station located at the DX Grid entered on the main window. These
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numbers are followed by *Dec*, the declination of the moon; *SunAz*
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and *SunEl*, the azimuth and elevation of the Sun; *Freq*, your stated
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operating frequency in MHz; *Tsky*, the estimated sky background
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temperature in the direction of the moon, scaled to the operating
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frequency; *Dpol*, the spatial polarization offset in degrees; *MNR*,
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the maximum non-reciprocity of the EME path in dB, owing to spatial
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polarization; and finally *Dgrd*, an estimate of the signal
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degradation in dB, relative to the best possible time with the moon
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at perigee in a cold part of the sky.
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The state of the art for establishing three-dimensional locations of
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the sun, moon, and planets at a specified time is embodied in a
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numerical model of the solar system maintained at the Jet Propulsion
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Laboratory. The model has been numerically integrated to produce
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tabular data that can be interpolated with very high accuracy. For
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example, the celestial coordinates of the moon or a planet can be
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determined at a specified time to within about 0.0000003 degrees. The
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JPL ephemeris tables and interpolation routines have been incorporated
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into _WSJT-X_. Further details on accuracy, especially concerning
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calculated EME Doppler shifts, are described in
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The sky background temperatures reported by _WSJT-X_ are derived from
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the all-sky 408 MHz map of Haslam et al. (Astronomy and Astrophysics
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Supplement Series, 47, 1, 1982), scaled by frequency to the (-2.6)
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power. This map has angular resolution of about 1 degree, and of
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course most amateur EME antennas have much broader beamwidths than
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this. Your antenna will therefore smooth out the hot spots
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considerably, and the observed extremes of sky temperature will be
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less. Unless you understand your sidelobes and ground reflections
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extremely well, it is unlikely that more accurate sky temperatures
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would be of much practical use.
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@ -1,22 +1,24 @@
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// Status=review
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At the center of the main window are a number of controls used when
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making QSOs:
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making QSOs. Controls not relevant to a particular mode or submode
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may be "grayed out" (diabled) or removed from the display.
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//.Misc Controls Center
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image::misc-controls-center.png[align="center",alt="Misc Controls Center"]
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* Check *Tx even* to transmit in even-numbered UTC minutes. Uncheck
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this box to transmit in the odd minutes. This selection is made
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automatically when you double-click on a decoded text line, as
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described in the <<TUTORIAL,Basic Operating Tutorial>>.
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* Check *Tx even* to transmit in even-numbered UTC minutes or
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sequences, starting at 0. Uncheck this box to transmit in the odd
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sequences. The correct selection is made automatically when you
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double-click on a decoded text line, as described in the
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<<TUTORIAL,Basic Operating Tutorial>>.
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* The Tx and Rx audio frequencies are usually set automatically by
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* The Tx and Rx audio frequencies can be set automatically by
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double-clicking on decoded text or a signal in the waterfall. They
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can also be adjusted with spinner controls.
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can also be adjusted using the spinner controls.
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* You can force Tx frequency to the current Rx frequency by clicking
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the *Tx<Rx* button, and vice-versa for *Rx<Tx*. Check the box *Lock
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the *Tx<-Rx* button, and vice-versa for *Rx<-Tx*. Check the box *Lock
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Tx=Rx* to make the frequencies always track one another. The
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on-the-air frequency of your lowest JT9 or JT65 tone is the sum of
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dial frequency and audio Tx frequency.
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|
@ -29,6 +29,10 @@ return to the original frequency.
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* *Erase* clears the right-hand decoded text window.
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Double-clicking *Erase* clears both text windows.
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* *Clear Avg* is present only in modes that support message averaging.
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It provides a way to erase all previous decode information, thus
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preparing to start a new average.
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* *Decode* tells the program to repeat the decoding procedure at the
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Rx frequency (green marker on waterfall scale), using the most recently
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completed sequence of received data.
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@ -36,8 +40,8 @@ completed sequence of received data.
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* *Enable Tx* toggles the program into automatic T/R sequencing mode
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and highlights the button in red. A transmission will start at
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the beginning of the selected (odd or even) sequence, or immediately
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if appropriate. A transmission will not be started any later than 24
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s into a UTC minute.
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if appropriate. Toggling the button a second time will remove the
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highlighted background color and
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* *Halt Tx* terminates a transmission in progress and disables
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automatic T/R sequencing.
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@ -47,5 +51,6 @@ unmodulated carrier at the specified Tx frequency (red marker on
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waterfall scale). This process may be useful for adjusting an antenna
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tuner. The button is highlighted in red while *Tune* is active.
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Toggle the button a second time or click *Halt Tx* to terminate the
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*Tune* process.
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*Tune* process. Note that activating *Tune* interrupts a receive
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sequence and will prevent decoding during that sequence.
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@ -16,6 +16,10 @@ WSJT-X* appears here rather than on the *Help* menu.
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==== File menu
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image::file-menu.png[align="left",alt="File Menu"]
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[[CONFIG_MENU]]
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==== Configuration Menu
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image::config-menu.png[align="left",alt="File Menu"]
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[[VIEW_MENU]]
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==== View Menu
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image::view-menu.png[align="left",alt="View Menu"]
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@ -12,6 +12,11 @@ recent transmitted message, and whether *Double-click on call sets Tx
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enable* has been selected on the *Settings | General* tab. The first
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label (operating state) can be Receiving, Tx (for Transmitting), Tune,
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or the name of file opened from the *File* menu; this label is
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highlighted in green for Receiving, yellow for Tx, and red for Tune.
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When transmitting, the Tx message is displayed exactly as it will be
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decoded by receiving stations.
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highlighted in green for Receiving, yellow for Tx, red for Tune, and
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light blue for a file name. When transmitting, the Tx message is
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displayed exactly as it will be decoded by receiving stations. A
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progress bar shows the elapsed fraction of a Tx or Rx sequence.
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Finally, if the Watchdog timer was enabled on the *settings | General*
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tab, a label in the lower right-hand corner diaplays the number of
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minutes remaining before timout.
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BIN
doc/user_guide/en/images/AstroData_2.png
Normal file
After Width: | Height: | Size: 9.9 KiB |
BIN
doc/user_guide/en/images/config-menu.png
Normal file
After Width: | Height: | Size: 6.2 KiB |
Before Width: | Height: | Size: 3.4 KiB After Width: | Height: | Size: 2.4 KiB |
Before Width: | Height: | Size: 6.7 KiB After Width: | Height: | Size: 7.2 KiB |
Before Width: | Height: | Size: 4.8 KiB After Width: | Height: | Size: 4.9 KiB |
Before Width: | Height: | Size: 63 KiB After Width: | Height: | Size: 26 KiB |
Before Width: | Height: | Size: 2.2 KiB After Width: | Height: | Size: 2.1 KiB |
Before Width: | Height: | Size: 3.4 KiB After Width: | Height: | Size: 5.4 KiB |
Before Width: | Height: | Size: 6.4 KiB After Width: | Height: | Size: 6.2 KiB |
Before Width: | Height: | Size: 3.4 KiB After Width: | Height: | Size: 2.5 KiB |
Before Width: | Height: | Size: 2.6 KiB After Width: | Height: | Size: 1.5 KiB |
Before Width: | Height: | Size: 53 KiB After Width: | Height: | Size: 17 KiB |
Before Width: | Height: | Size: 4.1 KiB After Width: | Height: | Size: 2.9 KiB |
Before Width: | Height: | Size: 3.6 KiB After Width: | Height: | Size: 3.4 KiB |
Before Width: | Height: | Size: 5.5 KiB After Width: | Height: | Size: 5.4 KiB |
@ -136,6 +136,10 @@ efficiency. On a busy HF band, the conventional 2-kHz-wide JT65
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sub-band is often filled with overlapping signals. Ten times as many
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JT9 signals can fit into the same frequency range, without collisions.
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=== QRA64
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TBD
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=== ISCAT
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ISCAT messages are free-form, up to 28 characters in length.
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@ -176,18 +180,6 @@ symbols in each 24, the user message +@CQ WA9XYZ+ repeats at its own
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natural length, 10 characters. The resulting sequence is extended as
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many times as will fit into a Tx sequence.
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=== JTMSK
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=== MSK144
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The letters MS are often used to abbreviate meteor scatter; the three
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letters MSK mean "Minimum Shift Keying", the modulation scheme used in
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JTMSK. This mode uses the same standard message structure as the slow
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modes JT4, JT9, and JT65. User information is "`source encoded`" to
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72 bits; a 15-bit cyclic redundancy check (CRC) is appended, and a
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convolutional code with constraint length K=13 and rate r=1/2 is then
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applied. This procedure makes for a total of (72+15+12)*2 = 198
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information bits for the encoded message. Three copies of the
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"`Barker-11`" code and three even-parity bits are added for
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synchronization, making a total of 198+33+3 = 234 channel symbols.
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Modulation is carried out using a constant-envelope, continuous-phase
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minimum-shift keying (MSK) waveform, with tone frequencies of 1000
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and 2000 Hz.
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TBD
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@ -21,7 +21,7 @@ The waterfall should look something like this:
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[[X14]]
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image::130610_2343-wav-80.png[align="left",alt="Wide Graph Decode 130610_2343"]
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IMPORTANT: The position pf the blue marker on the waterfall scale is
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The position of the blue marker on the waterfall scale is
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set by the spinner control *JT65 nnnn JT9*, where nnnn is an audio
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frequency in Hz. In *JT9+JT65* mode the program will automatically
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decode JT9 signals only above this frequency. JT65 signals will be
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|
@ -29,18 +29,20 @@ To activate the VHF-and-up features:
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- If you will be doing EME, check the box *Decode at t = 52 s*
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to allow for the EME path delay on received signals
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- If you will use automatic Doppler tracking, check the box *Allow Tx
|
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frequency changes while transmitting*.
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- If you will use automatic Doppler tracking and your radio accepts
|
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QSY commands while transmitting, check the box *Allow Tx frequency
|
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changes while transmitting*. Transceivers that allow such changes
|
||||
include the IC-735, IC-756 Pro II, IC-910-H, FT-817, FT-847, FT-857,
|
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FT-897, TS-590S, TS-590SG, TS-2000 (with Rev 9 firmware upgrade), Flex
|
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1500 and 5000, HPSDR, Anan-10, Anan-100, and KX3. On the *Radio* tab
|
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select *Split Operation* (use either *Rig* or *Fake It*; you may need
|
||||
to experiment with both options to find one that works best with your
|
||||
radio).
|
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IMPORTANT: Not all transceivers permit computer adjustments of Tx
|
||||
frequency while transmitting. Among those that do are the IC-735,
|
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IC-756 Pro II, IC-910-H, FT-847, TS-2000 (with Rev 9 firmware
|
||||
upgrade), TS-590S, TS-590SG, Flex 1500 and 5000, HPSDR, Anan-10,
|
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Anan-100, and KX3.
|
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|
||||
- On the *Radio* tab select *Split Operation* (use either *Rig* or
|
||||
*Fake It*; you may need to experiment with both options to find one
|
||||
that works best with your radio).
|
||||
- If your radio does not accept commands to change frequency while
|
||||
transmissing, Doppler tracking is accomplished by making a single Tx
|
||||
frequency adjustment before transmitting, using a value computed for
|
||||
the middle of the Tx period.
|
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- The main window reconfigures itself as necessary to include controls
|
||||
supporting features of each mode. For example, in JT4 mode the
|
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@ -83,28 +85,29 @@ will be reset to 12183 Hz _below_ the nominal on-the-moon frequency.
|
||||
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- Select the desired submode, which determines the tone spacing.
|
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Higher spacings are used on the higher microwave bands, to allow for
|
||||
larger Doppler spreads. For example, JT4F is generally used for EME on
|
||||
the 10 GHz band.
|
||||
larger Doppler spreads. For example, submode JT4F is generally used
|
||||
for EME on the 10 GHz band.
|
||||
|
||||
- If using a transverter, set the appropriate offset on the *Settings
|
||||
| Frequencies* tab. Offset is defined as (desired transceiver dial
|
||||
reading) minus (desired on-the-air frequency). For example, when
|
||||
using a 144 MHz radio at 10368 MHz, *Offset (MHz)* = (144 - 10368) =
|
||||
-10224.000. If the band is already in the table, you can edit the
|
||||
offset by double clicking on the offset field itself. Otherwise a new
|
||||
band can be added by right clicking in the table and selecting *Insert*.
|
||||
| Frequencies* tab. Offset is defined as (transceiver dial reading)
|
||||
minus (on-the-air frequency). For example, when using a 144 MHz radio
|
||||
at 10368 MHz, *Offset (MHz)* = (144 - 10368) = -10224.000. If the
|
||||
band is already in the table, you can edit the offset by double
|
||||
clicking on the offset field itself. Otherwise a new band can be
|
||||
added by right clicking in the table and selecting *Insert*.
|
||||
|
||||
image::Add_station_info.png[align="center",alt="Station information"]
|
||||
|
||||
- The JT4 decoder in _WSJT-X_ includes optional facilities for
|
||||
averaging over successive transmissions and also correlation decoding,
|
||||
also known as "`Deep Search`".
|
||||
also known as "`Deep Search`". Either or both of these options may
|
||||
be selected from the *Decode* menu.
|
||||
|
||||
image::decoding_depth.png[align="center",alt="Decoding Depth"]
|
||||
|
||||
- By convention, EME with JT4 can use "`short form`" messages. To
|
||||
activate automatic generation of these messages, check the box labeled
|
||||
*Sh* on the main window.
|
||||
- By convention, EME with JT4 can use "`short form`" messages
|
||||
consisting of a single tone. To activate automatic generation of
|
||||
these messages, check the box labeled *Sh* on the main window.
|
||||
|
||||
IMPORTANT: Thanks to G3WDG, many additional hints for using JT4 and
|
||||
Echo mode on the EME path are available in {jt4eme}.
|
||||
|
@ -198,6 +198,9 @@ include::faq.adoc[]
|
||||
== Protocol Specifications
|
||||
include::protocols.adoc[]
|
||||
|
||||
[[ASTRODATA]]
|
||||
== Astronomical Data
|
||||
include::astro_data.adoc[]
|
||||
|
||||
[[TXRX]]
|
||||
== Implementation Details
|
||||
|