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Last modified: Tue Apr 3 11:50:06 2018.

Directory Listing of Routines

Routine Descriptions

FLATTEN_SPECTRA

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 PROCEDURE:
         flatten_spectra

 PURPOSE:
         Create quick plots of spectra at a certain time (i.e., energy vs. eflux, PA vs. eflux, etc)
 KEYWORDS:
       [XY]LOG:   [XY] axis in log format
       [XY]RANGE: 2 element vector that sets [XY] axis range
       NOLEGEND:  Disable legend display
       COLORS:    n element vector that sets the colors of the line in order that they are in tplot_vars.options.varnames
                  n is number of tplot variables in tplot_vars.options.varnames
             
       PNG:         save png from the displayed windows (cannot be used with /POSTRSCRIPT keyword)
       POSTRSCRIPT: create postscript files instead of displaying the plot
       PREFIX:      filename prefix
       FILENAME:    custorm filename, including folder. 
                    By default the folder is !mms.local_data_dir and filename includes tplot names and selected time (or center time)      
       
       TIME_IN:     if the keyword is specified the time is determined from the variable, not from the cursor pick.
       TRANGE:      Two-element time range over which data will be averaged. 
       SAMPLES:     Number of nearest samples to time to average. Override trange.      
       WINDOW:      Length in seconds over which data will be averaged. Override trange.
       CENTER_TIME: Flag denoting that time should be midpoint for window instead of beginning.
                    If TRANGE is specify, the the time center point is computed.
       RANGETITLE:  If keyword is set, display range of the averagind time instead of the center time
                    Does not affect deafult name of the png or postscript file 

 EXAMPLE:
     To create line plots of FPI electron energy spectra for all MMS spacecraft:
     
       MMS> mms_load_fpi, datatype='des-moms', trange=['2015-12-15', '2015-12-16'], probes=[1, 2, 3, 4]
       MMS> tplot, 'mms?_des_energyspectr_omni_fast'
       MMS> flatten_spectra, /xlog, /ylog
       
       --> then click the tplot window at the time you want to create the line plots at

 NOTES:
     work in progress; suggestions, comments, complaints, etc: egrimes@igpp.ucla.edu
     
$LastChangedBy: egrimes $
$LastChangedDate: 2018-01-25 09:03:15 -0800 (Thu, 25 Jan 2018) $
$LastChangedRevision: 24588 $
$URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/tags/spedas_3_00/projects/mms/common/util/flatten_spectra.pro $

(See projects/mms/common/util/flatten_spectra.pro)

MMS_DRAW_CIRCLE

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 PROCEDURE:
         mms_draw_circle

 PURPOSE:
         Draws (and fills in) a circle
 
 NOTES:
         Taken from mms_fpi_dist_slice_comparison_crib, 8/26/16
         
 $LastChangedBy: egrimes $
 $LastChangedDate: 2016-08-26 09:12:48 -0700 (Fri, 26 Aug 2016) $
 $LastChangedRevision: 21731 $
 $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/tags/spedas_3_00/projects/mms/common/util/mms_draw_circle.pro $

(See projects/mms/common/util/mms_draw_circle.pro)

MMS_TEAM_KIBANA

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 PROCEDURE:
         mms_team_kibana

 PURPOSE:
         Opens the MMS Kibana page using your web browser; allows you to see which
         data files are available at the SDC, and when they're available
 
 KEYWORDS:
         only one keyword allowed specifying the instrument you're interested in, e.g., 
         /fgm for FGM data, /fpi for FPI data, etc.
         
     
 NOTES:
         The webpage is restricted to MMS team-members only
 
 EXAMPLE:
         to open the Kibana page for FPI CDF files:
         MMS> mms_team_kibana, /fpi
         
         
 $LastChangedBy: egrimes $
 $LastChangedDate: 2018-02-21 09:06:31 -0800 (Wed, 21 Feb 2018) $
 $LastChangedRevision: 24755 $
 $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/tags/spedas_3_00/projects/mms/common/util/mms_team_kibana.pro $

(See projects/mms/common/util/mms_team_kibana.pro)