diff --git a/kstars/ekos/align/align.ui b/kstars/ekos/align/align.ui index a43e12c64..841bb728e 100644 --- a/kstars/ekos/align/align.ui +++ b/kstars/ekos/align/align.ui @@ -1,1865 +1,1865 @@ Align 0 0 873 570 3 3 3 3 3 0 3 Solver Control Qt::AlignLeading|Qt::AlignLeft|Qt::AlignVCenter 3 3 3 3 3 true Capture && Solve true true Load a FITS image and solve. Slew mount to image central coordinates. Load && Slew... false Stop Select which action to perform after the captured image is solved Select what action to take once a solution is found. Solver Action 3 3 3 3 3 Synchronize the telescope to the solution coordinates S&ync true gotoModeButtonGroup Synchronize the telescope to the solution coordinates and then slew to the target coordinates S&lew to Target gotoModeButtonGroup Just solve &Nothing gotoModeButtonGroup Telescope Coordinates Accuracy threshold in arcseconds between solution and target coordinates. Plate solver shall be repeatedly executed until the solution coordinates are below the accuracy threshold 1 1200 10 30 DE: true After telescope completes slewing, wait until it settles for this many milliseconds before capturing the next image. Settle true After telescope completes slewing, wait until it settles for this many milliseconds before capturing the next image. 15000 100 RA: Accuracy threshold in arcseconds between solution and target coordinates. Plate solver shall be repeatedly executed until the solution coordinates are below the accuracy threshold Accuracy Solution Coordinates 3 3 3 3 3 Image scale in arcsecs/pixel true Image scale in arcsecs/pixel Pix: Effective field of view size in arcminutes. false Image rotation angle, East of North true true RA: Difference between telescope coordinates and solution coordinates in Declination dDE Difference between telescope coordinates and solution coordinates in Right Ascension dRA: true Effective field of view size in arcminutes. FOV: Image rotation angle, East of North Rot: Difference between telescope coordinates and solution coordinates in Declination font-weight: bold; true DE: Difference between telescope coordinates and solution coordinates in Right Ascension font-weight: bold; true Select which telescope to use when performing Field of View calculations. Primary Scope Guide Scope Solver Options 3 3 3 3 3 1 1 CCD: 22 22 22 22 Toggle full screen Exposure duration in seconds 0.100000000000000 60.000000000000000 0.500000000000000 3.000000000000000 Exp: Subtract dark frame. If no suitable dark frame is available, a dark frame shall be captured. Dark Camera binning Bin: 22 22 22 22 Show in FITS Viewer FW: Filter: 3 Options: Additional options to be the solver false 22 22 22 22 Edit solver options 3 Solver: Use online astrometry.net solver to solve the image. You must have an Internet connection and a valid API key. Onl&ine true solverTypeGroup Use offline astrometry.net solver. You must install all the necessary index files for your field of view. Offline solverTypeGroup false <p>Use astrometry solver on remote machine running INDI server. You must select <b>Astrometry</b> driver from Auxiliary drivers in your Ekos devices profile for this option to be enabled.</p> Re&mote solverTypeGroup Qt::Horizontal 40 20 Qt::Vertical QSizePolicy::MinimumExpanding 20 1 0 0 Qt::Vertical 0 0 320 240 0 Solution Results 5 0 0 0 0 0 0 The results from Astrometric Solutions from the Capture and Solve Tool, the Load and Slew Tool, and the Mount Model Tool will be displayed below. true 0 0 Qt::Horizontal 0 0 6 75 RA AlignCenter DEC AlignCenter Obj Name AlignCenter ~~ AlignCenter dRA AlignCenter dDE AlignCenter 0 32 32 32 32 Clear all of the solutions from the solutions table. Be careful because you cannot get them back. 32 32 32 33 Remove the selected row from the solutions table. This can be useful for getting rid of results that did not actually solve from the table and/or results that you do not need any more. It can clean up clutter on both the graph and table. 32 32 32 33 Export all of the solutions in the Solution Results table to CSV file of your choosing for further analysis in a spreadsheet. 32 32 32 33 Auto scale and center the Solution Results graph. Qt::Horizontal 40 20 Launch the mount model tool. This tool enables you to create pre-programmed list of points to go to and solve. It can aid in building a pointing model for better accuracy. Mount Model 0 0 100 100 190 190 Polar Alignment 0 0 0 0 true 0 150 Polar Alignment Assistant 3 3 3 3 3 true <p>Polar Alignment Helper tool requires the following:</p><p>1. German Equatorial Mount</p><p>2. Wide FOV &gt; 1 degrees</p><p>For small FOVs, use the Legacy Polar Alignment Tool.</p> QFrame::NoFrame 0 true 3 3 3 3 3 true - <html><head/><body><p>This tool provides a simple method to polar align a German equatorial mount. <span style=" font-weight:600;">Park</span> your mount to home position where it <span style=" font-weight:600;">points</span> toward the celestial pole. Select mount direction and speed and then click <span style=" font-weight:600;">Start</span> to begin the process.</p></body></html> + <html><head/><body><p>This tool provides a simple method to polar align a German equatorial mount. <span style=" font-weight:600;">Park</span> your mount to home position where it <span style=" font-weight:600;">points</span> toward the celestial pole with the counter weight down. Select mount direction and speed and then click <span style=" font-weight:600;">Start</span> to begin the process.</p></body></html> true <html><head/><body><p><span style=" font-weight:600; color:#ff5500;">Disabled: FOV must be 10 arcmins or wider. 60+ arcminutes is recommended.</span></p></body></html> Qt::RichText 3 false Direction: false Mount direction West East false Rotation magnitude in degrees 15 60 15 30 Speed: false Toggle for manual slewing with non-GOTO mounts Manual slew Qt::Horizontal 40 20 3 3 3 3 3 <p>The assistant requires three images to find a solution. Ekos is now capturing the first image...</p> true 3 3 3 3 3 <p>Executing the <span style=" font-style:italic;">first</span> mount rotation...</p> true Qt::Horizontal 40 20 Done 3 3 3 3 3 <p>Capturing the second image...</p> true <p>Executing the <i>second </i>mount rotation...</p> true Qt::Horizontal 40 20 Done <p>Capturing the <i>third</i> and final image...</p> true 3 3 3 3 3 Error Occurred true 3 Angle between expected perfectly aligned mount center and the actual center Polar Error: 0 Qt::Horizontal 40 20 3 0 0 <p>Correction vector is plotted above. <b>Select</b> a bright star to reposition the correction vector. Proceed next when done.</p> true Next 3 3 3 3 3 <p>Adjust mount's Altitude and Azimuth knobs until the selected star is centered within the crosshair. Click <b>Refresh</b> to begin continuous capture. You are <b>Done</b> when star is centered.</p> true 3 Refresh Exposure duration in seconds during refresh phase 4 0.000100000000000 30.000000000000000 1.000000000000000 Qt::Horizontal 40 20 Done 3 Qt::Horizontal 40 20 false Start Start false Stop Stop Legacy Polar Alignment Tool Qt::AlignLeading|Qt::AlignLeft|Qt::AlignTop 3 3 3 3 3 3 Az Error: true true Measure Az Error false Correct Az Error Qt::Vertical 3 Alt Error: true true Measure Alt Error false Correct Alt Error QCustomPlot QWidget
auxiliary/qcustomplot.h
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solveB loadSlewB stopB syncR slewR nothingR ScopeRAOut ScopeDecOut accuracySpin delaySpin SolverRAOut SolverDecOut dRAOut dDEOut pixScaleOut RotOut FOVOut FOVScopeCombo tabWidget CCDCaptureCombo showFITSViewerB exposureIN alignDarkFrameCheck toggleFullScreenB binningCombo FilterDevicesCombo FilterPosCombo solverOptions editOptionsB onlineSolverR offlineSolverR remoteSolverR solutionTable clearAllSolutionsB removeSolutionB exportSolutionsCSV autoScaleGraphB mountModelB correctAltB altError azError correctAzB measureAzB measureAltB PAHCorrectionsNextB PAHRefreshB PAHExposure PAHDoneB PAHManual toggled(bool) PAHfirstDone setEnabled(bool) 699 392 388 316 PAHManual toggled(bool) PAHsecondDone setEnabled(bool) 699 392 385 316