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PROCEDURE: mag_mola_orbit PURPOSE: Plots a set of [longitude,latitude] positions over a MAG-MOLA map. USAGE: mag_mola_orbit, lon, lat INPUTS: lon: East longitude (0 to 360 degrees). lat: Latitude (-90 to 90 degrees). Note: lon and lat must have the same number of elements. KEYWORDS: PSYM: Symbol type (same as for plot). LSTYLE: Line style (same as for plot). COLOR: Line/symbol color (same as for plot). RESET: Read in the MAG-MOLA image and calculate the plot size and position. NOERASE: Do not refresh the plot for each [lon, lat] point. BIG: Use a 1000x500 MAG-MOLA image. TERMINATOR: Overlay the terminator at the time specified by this keyword. SHADOW: If TERMINATOR is set, specifies which "terminator" to plot. 0 : Optical shadow boundary at surface. 1 : Optical shadow boundary at s/c altitude. 2 : EUV shadow boundary at s/c altitude. $LastChangedBy: dmitchell $ $LastChangedDate: 2017-01-09 16:53:18 -0800 (Mon, 09 Jan 2017) $ $LastChangedRevision: 22552 $ $URL: file:///disks/socware/thmsvn/repos/spdsoft/trunk/projects/maven/maven_orbit_tplot/mag_mola_orbit.pro $ CREATED BY: David L. Mitchell 04-02-03
(See projects/maven/models/sep_elec/mag_mola_orbit2.pro)
PROCEDURE: maven_orbit_snap PURPOSE: After running maven_orbit_tplot, this routine plots the orbit as viewed along each of the MSO axes. Optionally, the orbit can be superimposed on models of the solar wind interaction with Mars. Also optionally, the position of the spacecraft can be plotted (in GEO coordinates) on a map of Mars' topography and magnetic field based on MGS MOLA and MAG data. All plots are generated at times selected with the cursor on the TPLOT window. Hold down the left mouse button and drag for a movie effect. USAGE: maven_orbit_snap INPUTS: KEYWORDS: PREC: Plot the position of the spacecraft at the selected time, superimposed on the orbit. Otherwise, the periapsis location for each orbit is plotted. For time ranges less than one day, the default is PREC = 1. Otherwise the default is 0. MHD: Plot the orbit superimposed on an image of an MHD simulation of the solar wind interaction with Mars (from Ma). 1 : Plot the XY projection 2 : Plot the XZ projection HYBRID: Plot the orbit superimposed on an image of a hybrid simulation of the solar wind interaction with Mars (from Brecht). 1 : Plot the XZ projection 2 : Invert Z in the model, then plot the XZ projection LATLON: Plot MSO longitudes and latitudes of periapsis (PREC=0) or the spacecraft (PREC=1) in a separate window. CYL: Plot MSO cylindrical projection (x vs. sqrt(y^2 + z^2)). XZ: Plot only the XZ projection. MARS: Plot the position of the spacecraft (PREC=1) or periapsis (PREC=0) on an image of Mars topography and magnetic field based on MGS data (from Connerney). 1 : Use a small image 2 : Use a large image NPOLE: Plot the position of the spacecraft (PREC=1) or periapsios (PREC=0) on a north polar projection (lat > 55 deg). The background image is the north polar magnetic anomalies observed at 180-km altitude by MGS (from Acuna). ALT: If set and keywords MARS and/or NPOLE are set, then indicate the spacecraft altitude next its symbol. TERMINATOR: Overplot the terminator and sub-solar point onto the Mars topography plots (see MARS and NPOLE above). SPICE must be installed and initialized (e.g., mvn_swe_spice_init) before using this keyword. The following values are recognized: 0 : Do not plot any shadow boundary. (default) 1 : Plot optical shadow boundary at surface. 2 : Plot optical shadow boundary at s/c altitude. 3 : Plot EUV shadow boundary at s/c altitude. NOERASE: Don't erase previously plotted positions. Can be used to build up a visual representation of sampling. NODOT: Do not plot a filled circle at periapsis or spacecraft location. RESET: Initialize all plots. COLOR: Symbol color index. KEEP: Do not kill the plot windows on exit. TIMES: An array of times for snapshots. Snapshots are overlain onto a single version of the plot. For evenly spaced times, this produces a "spirograph" effect. This overrides the interactive entry of times with the cursor. Sets KEEP, NOERASE, and RESET. BDIR: Set keyword to show magnetic field direction in three planes, In each plane, the same two components of B in MSO coordinates are shown, i.e. in XY plane, plotting Bx-By. The color shows if the third component (would be Bz in XY plane) is positive (red) or negative (blue). BCLIP: Maximum amplitude for plotting B whisker. SCALE: To change the scale/length of field lines, the default value is set to 0.05 THICK: Line thickness. MAGNIFY: Change size of plot windows. PSNAME: Name of a postscript plot. Works only for orbit plots. $LastChangedBy: dmitchell $ $LastChangedDate: 2017-10-02 17:58:29 -0700 (Mon, 02 Oct 2017) $ $LastChangedRevision: 24100 $ $URL: file:///disks/socware/thmsvn/repos/spdsoft/trunk/projects/maven/maven_orbit_tplot/maven_orbit_snap.pro $ CREATED BY: David L. Mitchell 10-28-11
(See projects/maven/models/sep_elec/maven_orbit_snap2.pro)