diff --git a/doc/CMakeLists.txt b/doc/CMakeLists.txt index 48922b208..88aaec6fd 100644 --- a/doc/CMakeLists.txt +++ b/doc/CMakeLists.txt @@ -113,6 +113,7 @@ set (UG_IMGS images/tools-menu.png images/traditional-msg-box.png images/tx-macros.png + images/VHF_controls.png images/view-menu.png images/wide-graph-controls.png diff --git a/doc/common/links.adoc b/doc/common/links.adoc index d10d7870d..22a674273 100644 --- a/doc/common/links.adoc +++ b/doc/common/links.adoc @@ -109,6 +109,7 @@ d). Edit lines as needed. Keeping them in alphabetic order help see dupes. :QRA64_EME: http://physics.princeton.edu/pulsar/K1JT/QRA64_EME.pdf[QRA64 for microwave EME] :svn: http://subversion.apache.org/packages.html#windows[Subversion] :win32: http://physics.princeton.edu/pulsar/K1JT/wsjtx-{VERSION}-win32.exe[wsjtx-{VERSION}-win32.exe] +:wsjt-devel: https://lists.sourceforge.net/lists/listinfo/wsjt-devel[here] :wsjt_svn: http://sourceforge.net/p/wsjt/wsjt/HEAD/tree/[WSJT Source Repository] :wspr_code: http://physics.princeton.edu/pulsar/K1JT/WSPRcode.exe[WSPRcode.exe] :wspr_svn: http://sourceforge.net/p/wsjt/wsjt/HEAD/tree/branches/wspr/[WSPR Source Repository] diff --git a/doc/user_guide/en/images/Astronomical_data.png b/doc/user_guide/en/images/Astronomical_data.png index caf4bb1ba..b6f35b548 100644 Binary files a/doc/user_guide/en/images/Astronomical_data.png and b/doc/user_guide/en/images/Astronomical_data.png differ diff --git a/doc/user_guide/en/images/FreqCal_Results.png b/doc/user_guide/en/images/FreqCal_Results.png index d1e93f5c8..cce1a686e 100644 Binary files a/doc/user_guide/en/images/FreqCal_Results.png and b/doc/user_guide/en/images/FreqCal_Results.png differ diff --git a/doc/user_guide/en/images/JT65B.png b/doc/user_guide/en/images/JT65B.png index 6eaa61c1c..31307a373 100644 Binary files a/doc/user_guide/en/images/JT65B.png and b/doc/user_guide/en/images/JT65B.png differ diff --git a/doc/user_guide/en/images/QRA64.png b/doc/user_guide/en/images/QRA64.png index 8e31f57b2..929f5c9fc 100644 Binary files a/doc/user_guide/en/images/QRA64.png and b/doc/user_guide/en/images/QRA64.png differ diff --git a/doc/user_guide/en/images/VHF_controls.png b/doc/user_guide/en/images/VHF_controls.png index 27452c36b..1f0888844 100644 Binary files a/doc/user_guide/en/images/VHF_controls.png and b/doc/user_guide/en/images/VHF_controls.png differ diff --git a/doc/user_guide/en/images/auto-seq.png b/doc/user_guide/en/images/auto-seq.png index 0f464cd23..0b155310a 100644 Binary files a/doc/user_guide/en/images/auto-seq.png and b/doc/user_guide/en/images/auto-seq.png differ diff --git a/doc/user_guide/en/images/main-ui.png b/doc/user_guide/en/images/main-ui.png index cf58498d2..8268af411 100644 Binary files a/doc/user_guide/en/images/main-ui.png and b/doc/user_guide/en/images/main-ui.png differ diff --git a/doc/user_guide/en/images/misc-controls-center.png b/doc/user_guide/en/images/misc-controls-center.png index d8db86dc9..773501a19 100644 Binary files a/doc/user_guide/en/images/misc-controls-center.png and b/doc/user_guide/en/images/misc-controls-center.png differ diff --git a/doc/user_guide/en/images/settings-general.png b/doc/user_guide/en/images/settings-general.png index 6caa98836..1cd2a8dff 100644 Binary files a/doc/user_guide/en/images/settings-general.png and b/doc/user_guide/en/images/settings-general.png differ diff --git a/doc/user_guide/en/images/special-mouse-commands.png b/doc/user_guide/en/images/special-mouse-commands.png index 9b8868cb3..92fa6760e 100644 Binary files a/doc/user_guide/en/images/special-mouse-commands.png and b/doc/user_guide/en/images/special-mouse-commands.png differ diff --git a/doc/user_guide/en/measurement_tools.adoc b/doc/user_guide/en/measurement_tools.adoc index d7718aa46..07bb3113e 100644 --- a/doc/user_guide/en/measurement_tools.adoc +++ b/doc/user_guide/en/measurement_tools.adoc @@ -70,13 +70,15 @@ Measuring Tests. image::FreqCal_Graph.png[align="left",alt="FreqCal_Graph"] After running *Execute frequency calibration cycle* at least once with -good results, the line-fitting procedure can be carried out -automatically by clicking *Solve for calibration parameters* on the -*Tools* menu. The results will be displayed as in the following -screen shot. Estimated uncertainties are included for slope and -intercept; `N` is the number of averaged frequency measurements included -in the fit, and `StdDev` is the root mean square deviation of -averaged measurements from the fitted straight line. +good results, check and edit the file `fmt.all` in the log directory +and delete any spurious or outlier measurements. The line-fitting +procedure can then be carried out automatically by clicking *Solve for +calibration parameters* on the *Tools* menu. The results will be +displayed as in the following screen shot. Estimated uncertainties +are included for slope and intercept; `N` is the number of averaged +frequency measurements included in the fit, and `StdDev` is the root +mean square deviation of averaged measurements from the fitted +straight line. image::FreqCal_Results.png[align="center",alt="FreqCal_Results"] diff --git a/doc/user_guide/en/support.adoc b/doc/user_guide/en/support.adoc index 055d79286..0a7e74b09 100644 --- a/doc/user_guide/en/support.adoc +++ b/doc/user_guide/en/support.adoc @@ -14,8 +14,10 @@ volunteer programmers to make the program better. Bugs may be reported to {wsjt_yahoo_group} (email address wsjtgroup@yahoogroups.com) or the WSJT Developers list (wsjt-devel@lists.sourceforge.net). Again, you will need to join the -group or subscribe to the list. To be useful, bug reports should -include at least the following information: +group or subscribe to the list. You can register for the list {wsjt-devel}. + +To be useful, bug reports should include at least the following +information: - Program version - Operating system diff --git a/mouse_commands.txt b/mouse_commands.txt index 18be98c15..d159ff5e1 100644 --- a/mouse_commands.txt +++ b/mouse_commands.txt @@ -13,8 +13,8 @@ Decoded text: - Double-click to copy second callsign to Dx Call
- and locator to Dx Grid, change Rx and Tx frequency to
+ Double-click to copy second callsign to Dx Call,
+ locator to Dx Grid, change Rx and Tx frequency to
decoded signal's frequency, and generate standard
messages.
If Hold Tx Freq is checked or first callsign in message