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LTVT scripts
Scripts allow you to automate LTVT operations. They can be run using the Run script... dialog in the Files menu in the upper right of the main screen.
- Note: This menu item is available only in LTVT_v0_21_5x and beyond
New in LTVT_v0_21_5, this menu item produces a window in which scripts can be entered and run.
- Script commands are entered in the upper memo box, one command per line.
- For details of the permissible command syntax see:
- LTVT_Script_Syntax.txt (7 KB; rev. 8 November 2010)
- Note: to view this text file with the intended word-wrap, it may be necessary to download it to disk and then open the saved copy, turning word-wrap on in the View options.
- For details of the permissible command syntax see:
- Clicking Run starts execution with the first command.
- Clicking Pause halts execution after completion of the currently-executing command.
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Here is an animation produced with the following script which asks LTVT to generate the "Texture 1" image for each day from November 1 to November 27, 2010, and save them to disk as "1.bmp", "2.bmp", .. "27.bmp":
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The Main Screen controls were set with Time at 00:00 UT, the Location = Geocentric and the Texture 1 file used was the LOLA grayscale DEM with a red dot placed at the Moon's mean center (0ºE/0ºN), and the "Mark center" option was selected.
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The images were then loaded into ImageJ with the "File...Import...Image sequence..." command, which resulted in the following animation:
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It shows the Moon's nominal center point (the red dot) revolving around the sub-observer point. Unfortunately when saved as a GIF animation Image J did not preserve the original red color for the dot in all frames.
- Here is another example: an animation of sunrise over Plato produced by incrementing the sub-solar longitude in steps of 0.5°
- Earth-based view (click to see full size, also available in an overhead view):
- This is the script used to produce the two animations:
- After adjusting the display and simulation parameters as desired, the script redraws the simulation with each specified sub-solar longitude and saves the sequentially numbered results to disk. The sub-solar latitude and the geometry of the Earth-based view were set to match those at the time of the famous observation of a "hooked" shadow on the floor of Plato, as seen by Wilkins and Moore using the great Paris Meudon refractor, assuming it was made 1952 Apr 3 at 19:30 UT.
This page has been edited 6 times. The last modification was made by - JimMosher on Dec 15, 2010 12:44 pm