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Last modified: Sat Sep 20 18:17:31 2025.

# Directory Listing of Routines

# general/missions/rbsp/efw/examples

- B1_STATUS_CRIB
- MINI_GEM_CRIB
- RBSP_BOOM_DIRECTIONS_CRIB
- RBSP_EFW_BURST_FA_ROTATE_CRIB
- RBSP_EFW_CONVECTION_EFIELD_CRIB
- RBSP_EFW_DCFIELD_REMOVAL_CRIB
- RBSP_EFW_EDOTB_TO_ZERO_CRIB
- RBSP_EFW_POSITION_VELOCITY_CRIB
- RBSP_EFW_POYNTING_FLUX_BURST_CRIB
- RBSP_EFW_POYNTING_FLUX_CRIB_SCOTT
- RBSP_EFW_POYNTING_FLUX_SURVEY_CRIB
- RBSP_EFW_SPEC_CRIB
- RBSP_EFW_SPINFIT_CRIB
- RBSP_EFW_SPINFIT_VXB_SUBTRACT_CRIB
- RBSP_EFW_SUMMARY_CRIB
- RBSP_EFW_VXB_SUBTRACT_CRIB
  Creates vxB subtracted tplot variables for the 32 S/s EFW efield data
- RBSP_EFW_WAVEFORM_CRIB
- RBSP_EFW_XSPEC_CRIB
- RBSP_LOAD_COLLECTION
- RBSP_LOAD_CONTACT
- RBSP_MAGEIS_EXAMPLE_CRIB_OLD
- TWAVPOL_MODIFIED

# Routine Descriptions

## B1_STATUS_CRIB

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     NAME: b1_status_crib.pro
     SYNTAX:
     PURPOSE: Create tplot variables pertaining to EFW burst existence
     INPUT:
     OUTPUT:
     KEYWORDS:
    	PROCEDURE: .run b1_status_crib
     HISTORY: Created by Kris Kersten, kris.kersten@gmail.com
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/b1_status_crib.pro $

(See general/missions/rbsp/efw/examples/b1_status_crib.pro)

## MINI_GEM_CRIB

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     NAME: mini_gem_crib.pro
     SYNTAX:
     PURPOSE: EFW crib sheet for the mini-GEM meeting at Fall AGU 2012.
    					 Loads a bunch of useful data products
     KEYWORDS:
     HISTORY: Aaron Breneman, UMN, Dec 2012 (awbrenem@gmail.com)

(See general/missions/rbsp/efw/examples/mini_gem_crib.pro)

## RBSP_BOOM_DIRECTIONS_CRIB

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     NAME: rbsp_boom_directions_crib
     SYNTAX:
     PURPOSE: find the pointing direction of the EFW booms in GSE coord
     INPUT: times -> array of times to find boom directions for
    		 probe -> 'a' or 'b'
     OUTPUT: tplot variables of each antenna direction in GSE ['vecu_gse','vecv_gse','vecw_gse']
     KEYWORDS:
     HISTORY: Written by Aaron W Breneman 05/12/2014
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_boom_directions_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_boom_directions_crib.pro)

## RBSP_EFW_BURST_FA_ROTATE_CRIB

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     NAME: rbsp_efw_burst_fa_rotate_crib
     SYNTAX:
     PURPOSE: Rotate RBSP EFW burst data to field-aligned coordinates
     INPUT:
     OUTPUT:
     KEYWORDS:
     HISTORY: Created by Aaron W Breneman, Univ. Minnesota  4/10/2014
     VERSION:
       $LastChangedBy: aaronbreneman $
       $LastChangedDate: 2020-09-11 13:35:30 -0700 (Fri, 11 Sep 2020) $
       $LastChangedRevision: 29139 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_burst_fa_rotate_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_burst_fa_rotate_crib.pro)

## RBSP_EFW_CONVECTION_EFIELD_CRIB

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     NAME: rbsp_efw_convection_efield_crib
     SYNTAX:
     PURPOSE: Calculate RBSP convection electric field and velocity
     INPUT:
     OUTPUT:
     KEYWORDS:
     HISTORY: Written by Aaron W Breneman, July 2016. Based on Scott Thaller's crib
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_convection_efield_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_convection_efield_crib.pro)

## RBSP_EFW_DCFIELD_REMOVAL_CRIB

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    *****************************************************************************************

      FUNCTION :   rbsp_efw_DCfield_removal_crib
      PURPOSE  :   Subtract off DC magnetic field from Bw values. Saves as new tplot files

      REQUIRES:   Need: SSL THEMIS software and IDL Geopack DLM both found at
    			   http://themis.ssl.berkeley.edu/software.shtml

      INPUT:
    		probe   -> 'a' or 'b'
    		model   -> Any of the Tsyganenko models or 'igrf'. Defaults to 't96'
    		ql -> set to load quicklook EMFISIS data
                   cadence -> cadence of EMFISIS data. 'hires', '4sec', '1sec'
                   nodelete -> don't delete various tplot
                   variables upon exit
      _extra --> useful keywords are:
             no_spice_load
             no_rbsp_efw_init

      EXAMPLES:

    				Produces the following variables (ex for magname = 'rbspa_mag_gsm', model='t96')
    					rbspa_mag_gsm_t96
    					rbspa_mag_gsm_t96_dif

    					If the model is not t89 then produces:
    					rbspa_mag_gsm_t96_wind
    					rbspa_mag_gsm_t96_wind_dif
    					rbspa_mag_gsm_t96_ace
    					rbspa_mag_gsm_t96_ace_dif
    					rbspa_mag_gsm_t96_omni
    					rbspa_mag_gsm_t96_omni_dif

       NOTES:    ruthlessly pilfered from THEMIS crib sheets
                 Subtracts off Tsyganenko values using input from ACE, Wind and OMNI, as
    			  well as user defined input.

       CREATED:  2012/12/12
       CREATED BY:  Aaron W. Breneman
        LAST MODIFIED:  08/26/2012   v1.0.0 - major update. Much simplified
        MODIFIED BY: AWB

    *****************************************************************************************

(See general/missions/rbsp/efw/examples/rbsp_efw_dcfield_removal_crib.pro)

## RBSP_EFW_EDOTB_TO_ZERO_CRIB

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    NAME: rbsp_efw_edotb_to_zero_crib.pro
    PURPOSE: Crib sheet to calculate the RBSP spin-axis Efield (short boom) under the
     assumption that E*B=0.
    CALLING SEQUENCE:
     rbsp_efw_edotb_to_zero_crib,'2014-01-01','a'
    INPUT:
     date: e.g. '2014-01-01'
     probe: 'a' or 'b'
    KEYWORDS:
     noremove - Don't remove ExMGSE (spinaxis) values when By/Bx>3.732 or Bz/Bx>3.732
     anglemin --> Min allowable angle b/t spinplane and Bo. Defaults to 15 deg
                Smaller angles will lead to less removed data, but can result
                in larger errors due to division by small numbers

    OUTPUT: tplot variables of the spinfit, MGSE electric field with xMGSE
     calculated assuming E*B=0
    NOTES: Bad E*B=0 data are removed
     Spin axis values calculated from E*B=0 as
     Ex = -1*(EyBy + EzBz)/Bx

     The ratios By/Bx and Bz/Bx can fluctuate wildly when Bx gets too small. Therefore we
     require that these ratios are less than a certain size (i.e. sufficiently big Bx).
     The standard (from Cluster) is to assume that the angle between any of the spinplane directions
     (MGSE y and z in this case) and Bo is greater than 15 degrees.
     	delta = angle(Bz, Bo) > 15
     	epsilon = angle(By, Bo) > 15
     	gamma = angle(Bx, Bo) < 75

     Writing out the dot products we get:
     	cos(delta) = Bz/Bo
     	cos(epsilon) = By/Bo
     	cos(gamma) = Bx/Bo

     We can rearrange these as:
     	By/Bx = cos(epsilon)/cos(gamma)
     	Bz/Bx = cos(delta)/cos(gamma)

     To find the max value of these ratios let epsilon = 15 deg, delta = 15, gamma = 75 deg.
     	By/Bx = 3.732
     	Bz/Bx = 3.732
    HISTORY: Written by Aaron W Breneman (UMN) - 2013-06-19
    $LastChangedBy: aaronbreneman $
    $LastChangedDate: 2020-09-11 13:33:33 -0700 (Fri, 11 Sep 2020) $
    $LastChangedRevision: 29137 $
    $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_edotb_to_zero_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_edotb_to_zero_crib.pro)

## RBSP_EFW_POSITION_VELOCITY_CRIB

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    NAME: rbsp_efw_position_velocity_crib.pro
    PURPOSE: Loads and plots RBSP (Van Allen probes) position and velocity related data
    CALLING SEQUENCE:
     timespan,'2014-01-01'
     rbsp_efw_position_velocity_crib
    INPUT:
    KEYWORDS:
     probe = set to specify to load only "a" or "b" other than both.
     no_spice_load -> set if you've already loaded the spice kernels
    	noplot -> set to avoid tplotting
    	notrace -> skip the ttrace2equator call. This takes a lot of computational time
     nospinaxis_calcs -> skip the part that loads the spinaxis pointing direction.
       This can be problematic on certain dates. Only set if you don't need the
       spinaxis direction or the sc velocity in mGSE coord
     _extra --> possible useful extra keywords include:
           no_spice_load
           no_rbsp_efw_init
    OUTPUT: various tplot variables
    HISTORY:
     Written by Aaron Breneman, UMN, Dec 2012
    	email: awbrenem@gmail.com
    REQUIRED: Need to have the SPICE ICY software package installed

    $LastChangedBy: aaronbreneman $
    $LastChangedDate: 2020-09-11 13:32:39 -0700 (Fri, 11 Sep 2020) $
    $LastChangedRevision: 29136 $
    $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_position_velocity_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_position_velocity_crib.pro)

## RBSP_EFW_POYNTING_FLUX_BURST_CRIB

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     NAME: rbsp_efw_poynting_flux_crib.pro
     SYNTAX:
     PURPOSE: Crib sheet for calling rbsp_poynting_flux.pro, which creates
    					 Poynting flux tplot variables (including spectra) from EFW
    					 and EMFISIS data in various coord systems. Plots results
     INPUT:
     OUTPUT:
     KEYWORDS:
    	PROCEDURE: load EMFISIS data in GSE.
    			Transform EMFISIS GSE -> MGSE
    			Load EFW despun waveform data in MGSE
    			Call Poynting flux program
     HISTORY: Created by Aaron W Breneman, UMN awbrenem@gmail.com
     VERSION:
       $LastChangedBy: aaronbreneman $
       $LastChangedDate: 2020-09-11 13:39:04 -0700 (Fri, 11 Sep 2020) $
       $LastChangedRevision: 29141 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_burst_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_burst_crib.pro)

## RBSP_EFW_POYNTING_FLUX_CRIB_SCOTT

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     NAME: rbsp_efw_poynting_flux_survey_crib.pro
     SYNTAX:
     PURPOSE: Crib sheet for creating Poynting flux tplot variables from EFW and
              EMFISIS survey data.
              This is called by the program rbsp_efw_make_pflux.pro, but can
              be used independently.
     INPUT:  smoothing -> period (sec) to smooth over
             detrending -> period (sec) to detrend over
             cadence_mag -> '1sec','4sec','hires'
             spinfit -> spinfit the Efield data? Otherwise uses the 32 S/s MGSE data
     OUTPUT: tplot variables of Poynting flux in various coord systems
     KEYWORDS:
     NOTES:  The burst and tt0 and tt1 keywords were added (by Aaron) to test the
             results of this crib sheet with rbsp_poynting_flux.pro. They compare
             almost identically for a test chorus event. (see aaron_scott_pflux_comparison.pro)

     HISTORY: Adapted from Scott Thaller's Poynting flux crib by Aaron Breneman

     VERSION:
       $LastChangedBy: aaronbreneman $
       $LastChangedDate: 2020-09-11 13:39:41 -0700 (Fri, 11 Sep 2020) $
       $LastChangedRevision: 29143 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_crib_scott.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_crib_scott.pro)

## RBSP_EFW_POYNTING_FLUX_SURVEY_CRIB

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     NAME: rbsp_efw_poynting_flux_survey_crib.pro
     SYNTAX:
     PURPOSE: Crib sheet for creating Poynting flux tplot variables from EFW and
              EMFISIS data.
              This is called by the program rbsp_efw_make_pflux.pro, but can
              be used independently.
     INPUT:  smoothing -> period (sec) to smooth over
             detrending -> period (sec) to detrend over
             cadence_mag -> '1sec','4sec','hires'
             spinfit -> spinfit the Efield data? Otherwise uses the 32 S/s MGSE data
     OUTPUT: tplot variables of Poynting flux in various coord systems
     KEYWORDS:
     NOTES:  The burst and tt0 and tt1 keywords were added (by Aaron) to test the
             results of this crib sheet with rbsp_poynting_flux.pro. They compare
             almost identically for a test chorus event. (see aaron_scott_pflux_comparison.pro)

     HISTORY: Adapted from Scott Thaller's Poynting flux crib by Aaron Breneman

     VERSION:
       $LastChangedBy: aaronbreneman $
       $LastChangedDate: 2020-09-11 13:39:29 -0700 (Fri, 11 Sep 2020) $
       $LastChangedRevision: 29142 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_survey_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_poynting_flux_survey_crib.pro)

## RBSP_EFW_SPEC_CRIB

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     NAME: rbsp_efw_spec_crib.pro
     SYNTAX:
     PURPOSE: Create tplot variables pertaining to RBSP EFW spectral products
     INPUT:
     OUTPUT:; SPEC returns 7 channels, with nominal data selection:
    		SPEC0: E12AC
    		SPEC1: E56AC
    		SPEC2: SCMpar
    		SPEC3: SCMperp
    		SPEC4: SCMW
    		SPEC5: V1AC
    		SPEC6: V2AC

     KEYWORDS:
     HISTORY: ; Kris Kersten, UMN, June 2012 (kris.kersten@gmail.com)
     					 Modified by Aaron Breneman, UMN, Dec 2012 (awbrenem@gmail.com)

     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_spec_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_spec_crib.pro)

## RBSP_EFW_SPINFIT_CRIB

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     NAME: rbsp_efw_spinfit_crib.pro
     SYNTAX:
     PURPOSE: Crib sheet for crating EFW spinfit electric field in spinning
              spacecraft coord (DSC)
     INPUT:
     OUTPUT:
     KEYWORDS:
     HISTORY: Created by Jianbao Tao, SSL/UCB.
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_spinfit_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_spinfit_crib.pro)

## RBSP_EFW_SPINFIT_VXB_SUBTRACT_CRIB

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    NAME: rbsp_efw_spinfit_vxb_subtract_crib.pro
    PURPOSE: Create the vxb subtracted spinfit data product for EFW
    CALLING SEQUENCE:
     timespan,'2014-01-01'
     rbsp_efw_spinfit_vxb_crib,'a'
    INPUT: probe --> 'a' or 'b'
    KEYWORDS:
     ql -> select to load EMFISIS quicklook data. Defaults to hires L3 data but
    				quicklook data are available sooner.
    	qa -> select to load QA waveform data. Don't want to use this route for normal
    				  data processing.
    	hiresl3 -> loads the EMFISIS high resolution 64 S/s L3 GSE data
     level -> Level of EMFISIS data. Options are:
       'ql', 'l2', 'l3'. Defaults to EMFISIS L3 data
     boom_pair -> select the boom pair for the spinfitting. Any pair is acceptable
     no_reload -> use to not reload any of the base data. Useful if you want to run this
             crib sheet multiple times for different boom pairs.
     _extra --> possible useful keywords include:
             no_spice_load

    OUTPUT: tplot variables of spinfit, vxb subtracted electric field

    NOTES: If doing spinfit on pairs 12, 34, we load the "esvy" waveform. This gives us the Efield array
    (rbsp?_efw_esvy) as [[E12],[E34],[E56]].
    This array is inputted into rbsp_spinfit.pro and the plane_dim is set to 0,1
    depending on which component (E12 or E34) you want to spinfit off of.
    **
    For pairs other than 12, 34, 56, we have to load "vsvy" waveform and construct the components
    manually. The first element of this array (normally E12) will be replaced with the new component.
    For ex, for pair=24, the array (rbsp?_efw_esvy) will be [[E24],[E34],[E56]]. We'll then set plane_dim
    to zero to use this component.

    HISTORY: Written by Aaron W Breneman
             University of Minnesota
             2013-04-16
    $LastChangedBy: aaronbreneman $
    $LastChangedDate: 2020-10-15 10:55:25 -0700 (Thu, 15 Oct 2020) $
    $LastChangedRevision: 29256 $
    $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_spinfit_vxb_subtract_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_spinfit_vxb_subtract_crib.pro)

## RBSP_EFW_SUMMARY_CRIB

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     NAME: rbsp_efw_summary_crib.pro
     SYNTAX:
     PURPOSE: Create tplot variables pertaining to EFW summary data
    						(waveform, spec, xspec, filterbank)
     INPUT:
     OUTPUT:
     KEYWORDS:
     HISTORY: Kris Kersten, UMN, June 2012 (email: kris.kersten@gmail.com)
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_summary_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_summary_crib.pro)

## RBSP_EFW_VXB_SUBTRACT_CRIB

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    NAME: rbsp_efw_vxb_subtract_crib.pro
    PURPOSE:
     Creates vxB subtracted tplot variables for the 32 S/s EFW efield data
     ****NOTE: IF YOU DON'T NEED THE FULL 32 S/s RESOLUTION THEN CONSIDER USING
     ****rbsp_efw_spinfit_vxb_subtract_crib.pro
     ****THE DATA WILL BE AT SPINPERIOD CADENCE BUT WILL BE CLEANER

     WARNING!!! RESULTS ARE PRELIMINARY. DO NOT PUBLISH OR PRESENT THESE RESULTS
     WITHOUT FIRST CONSULTING THE EFW PI JOHN WYGANT <wygan001@umn.edu>

    CALLING SEQUENCE:
     timespan,'2014-01-01'
     rbsp_efw_vxb_subtract_crib,'a'

    INPUT: 'a' or 'b' for probe
    KEYWORDS:
     ql -> use EMFISIS quicklook UVW data instead of 4sec GSE L3. This will be
           despun and spinfit. This has the advantage of not having to wait for
           the EMFISIS L3 data set to be produced.
           Note: Defaults to 4-sec EMFISIS data in GSE. This is actually superior
           to the hires GSE data b/c it doesn't have spurious data spikes.
           It works about the same as JBT's method of despinning and then
           spinfitting the EMFISIS quicklook UVW data.

     hires -> use EMFISIS hires L3 GSE data instead of 4sec GSE L3.
     qa -> load the QA testing L1 EFW data instead of the usual L1 data
    OUTPUT:
    HISTORY:
     Created by Aaron Breneman, UMN, Dec 2012
    	email: awbrenem@gmail.com
    REQUIRES: THEMIS TDAS software
    			 http://themis.ssl.berkeley.edu/software.shtml
    		   as well as SPICE software

    $LastChangedBy: nikos $
    $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
    $LastChangedRevision: 28720 $
    $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_vxb_subtract_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_vxb_subtract_crib.pro)

## RBSP_EFW_WAVEFORM_CRIB

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     NAME: rbsp_efw_waveform_crib
     SYNTAX:
     PURPOSE: Loads and plots RBSP (Van Allen probes) waveform data
     KEYWORDS:
     HISTORY: Kris Kersten, UMN, June 2012 (kris.kersten@gmail.com)
     	Modified by Aaron Breneman, UMN, Dec 2012 (awbrenem@gmail.com)

     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_waveform_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_waveform_crib.pro)

## RBSP_EFW_XSPEC_CRIB

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     NAME: rbsp_efw_xspec_crib.pro
     SYNTAX:
     PURPOSE: Create tplot variables pertaining to the EFW cross-spectral product
     INPUT:
     OUTPUT:
     KEYWORDS:
    	PROCEDURE: .run b1_status_crib
     HISTORY: Kris Kersten, UMN, June 2012 (kris.kersten@gmail.com)
     				 Modified by Aaron Breneman, UMN, Dec 2012 (awbrenem@gmail.com)
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_efw_xspec_crib.pro $

(See general/missions/rbsp/efw/examples/rbsp_efw_xspec_crib.pro)

## RBSP_LOAD_COLLECTION

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     NAME: rbsp_load_collection
     SYNTAX:
     PURPOSE: Load collection time <remote_dir>/burst_selection/rbspx_b1_rec.dat.
     INPUT:
    	cts, out, dblarr[n,2], req. Collection times in UT second.
       probe, in, 'a' or 'b', opt. Default is 'a'.
     OUTPUT:
     KEYWORDS:
     HISTORY: 2014-04-09, created by Sheng Tian, UMN
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_load_collection.pro $

(See general/missions/rbsp/efw/examples/rbsp_load_collection.pro)

## RBSP_LOAD_CONTACT

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     Type: procedure.
     Purpose: Load contact time <remote_dir>/MOC_data_products/RBSPX/contact_plan'.
     Parameters:
       cts, out, dblarr[n,2], req. Contact times in UT second.
       probe, in, 'a' or 'b', opt. Default is 'a'.
     Keywords: none.
     Notes: none.
     Dependence: tdas.
     History:
       2014-04-09, Sheng Tian, create.

(See general/missions/rbsp/efw/examples/rbsp_load_contact.pro)

## RBSP_MAGEIS_EXAMPLE_CRIB_OLD

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     Deprecated, 2020-04-13, jmm

     NAME: rbsp_mageis_example_crib.pro
     SYNTAX:
     PURPOSE: Crib sheet showing how to load MagEIS data
     INPUT:
     OUTPUT:
     KEYWORDS:
     HISTORY: Created by Aaron Breneman
     VERSION:
       $LastChangedBy: nikos $
       $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
       $LastChangedRevision: 28720 $
       $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/rbsp_mageis_example_crib_old.pro $

(See general/missions/rbsp/efw/examples/rbsp_mageis_example_crib_old.pro)

## TWAVPOL_MODIFIED

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     NAME:twavpol

    PURPOSE:To perform polarisation analysis of three orthogonal component time
             series data, using tplot variables.

    EXAMPLE: twavpol,'in_data',prefix='in_data',freqline=fl

    INPUTS: tvarname: the name of the tplot variable upon which it will
    operate

    prefix(optional): the prefix to be assigned to the tplot variables that will be
    output, defaults to tvarname

           Subroutine assumes data are in righthanded fieldaligned
    	coordinate system with Z pointing the direction
           of the ambient magnetic field.

    Keywords:
      nopfft(optional) = Number of points in FFT

      steplength(optional) = The amount of overlap between successive FFT intervals

      bin_freq (optional): No. of bins in frequency domain

    OUTPUTS:
              error(optional): named variable in which to return the
              error state of this procedure call. 1 = success, 0 = failure

              freqline(optional): assign a named variable to this keyword
              to store the frequencies of each y-index

             timeline(optional): assign a named variable to this keyword
             to store the times of each x-index

    The program outputs five spectral results derived from the
             fourier transform of the covariance matrix (spectral matrix)
    This version stores these outputs as tplot variables with the
    specified prefix
             These are follows:

             Wave power: On a linear scale, at this stage no units

             Degree of Polarisation:
    		This is similar to a measure of coherency between the input
    		signals, however unlike coherency it is invariant under
    		coordinate transformation and can detect pure state waves
    		which may exist in one channel only.100% indicates a pure
    		state wave. Less than 70% indicates noise. For more
    		information see J. C. Samson and J. V. Olson 'Some comments
    		on the description of the polarization states
    		of waves' Geophys. J. R. Astr. Soc. (1980) v61 115-130

       Wavenormal Angle:
         The angle between the direction of minimum variance
         calculated from the complex off diagonal elements of the
         spectral matrix and the Z direction of the input ac field data.
         for magnetic field data in field aligned coordinates this is the
         wavenormal angle assuming a plane wave. See:
         Means, J. D. (1972), Use of the three-dimensional covariance
         matrix in analyzing the polarization properties of plane waves,
         J. Geophys. Res., 77(28), 5551-5559,
         doi:10.1029/JA077i028p05551.

       Ellipticity:
         The ratio (minor axis)/(major axis) of the ellipse transcribed
         by the field variations of the components transverse to the
         Z direction (Samson and Olson, 1980). The sign indicates
         the direction of rotation of the field vector in the plane (cf.
         Means, (1972)).
         Negative signs refer to left-handed rotation about the Z
         direction. In the field aligned coordinate system these signs
         refer to plasma waves of left and right handed polarization.

             Helicity:Similar to Ellipticity except defined in terms of the
    	direction of minimum variance instead of Z. Stricltly the Helicity
    	is defined in terms of the wavenormal direction or k.
    	However since from single point observations the
    	sense of k cannot be determined,  helicity here is
    	simply the ratio of the minor to major axis transverse to the
           minimum variance direction without sign.

    NOTES:
    1. Although the input is in the form of a tplot variable, the
    output is currently in the form of arrays

    2. -If one component is an order of magnitude or more  greater than
    	the other two then the polarisation results saturate and erroneously
    	indicate high degrees of polarisation at all times and
    	frequencies.

    3. Time series should be eyeballed before running the program.
    	 For time series containing very rapid changes or spikes
    	 the usual problems with Fourier analysis arise.
    	 Care should be taken in evaluating degree of polarisation results.

    4. For meaningful results there should be significant wave power at the
    	 frequency where the polarisation approaches
    	 100%. Remembercomparing two straight lines yields 100% polarisation.

     $LastChangedBy: nikos $
     $LastChangedDate: 2020-05-21 20:36:46 -0700 (Thu, 21 May 2020) $
     $LastChangedRevision: 28720 $
     $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/general/missions/rbsp/efw/examples/twavpol_modified.pro $

(See general/missions/rbsp/efw/examples/twavpol_modified.pro)