This page was created by the IDL library routine `mk_html_help2`.

Last modified: Fri Sep 26 18:17:39 2025.

# Directory Listing of Routines

# external/developers/solarwind

- OMNI2_LOAD
- SOLARWIND_CRIB
  Crib sheet showing the use and work of the solar wind (SW) processing
- SOLARWIND_LOAD
  Routine provides solar wind (SW) data time-shifted to the bow-shock
- SOLARWIND_LOAD_HRO
  Plug-in subroutine for driver routine solarwind_load.pro provides
- SOLARWIND_LOAD_OMNI1H
  Plug-in subroutine for driver routine solarwind_load.pro provides
- SOLARWIND_LOAD_WIND
  Plug-in subroutine for driver routine solarwind_load.pro provides

# Routine Descriptions

## OMNI2_LOAD

[Next Routine] [List of Routines]

    Procedure: OMNI2_LOAD

    Purpose:  Loads OMNI data

    keywords:
       TRANGE= (Optional) Time range of interest  (2 element array).
       /VERBOSE : set to output some useful info
    Example:
       omni2_load
    Notes:
      This routine is still in development.
     Author: Davin Larson

     $LastChangedBy: bckerr $
     $LastChangedDate: 2008-09-08 13:16:17 -0700 (Mon, 08 Sep 2008) $
     $LastChangedRevision: 3459 $
     $URL: svn+ssh://thmsvn@ambrosia.ssl.berkeley.edu/repos/spdsoft/trunk/external/developers/solarwind/omni2_load.pro $

(See external/developers/solarwind/omni2_load.pro)

## SOLARWIND_CRIB

[Previous Routine] [Next Routine] [List of Routines]

     NAME:
         SOLARWIND_CRIB

     PURPOSE:
    	Crib sheet showing the use and work of the solar wind (SW) processing
    	routine.

     CATEGORY:
    	Crib sheet

     CALLING SEQUENCE:
    	solarwind_crib

     INPUTS:
    	none; the code prompts user to continue by entering .continue on terminal

     KEYWORDS:
    	none

     PARAMETERS: 3 parameters for outlier filtering and convolution are described
    		and set in the code remove_outliers.pro. Another parameter is set in
    		the auxillary routine remove_outliers_repair.pro. Time range for SW data
    		and time resolution of SW data are set in the crib code.

     OUTPUTS:
    	graphics, interactive terminal

     DEPENDENCIES: convolve_gaussian_1d.pro, remove_outliers.pro,
         remove_outliers_repair.pro, wi_swe_load.pro, get_data.pro, xclip.pro,
         xdegap.pro, xdeflag.pro, solarwind_load.pro, omni_hro_load.pro,
         omni2_load.pro, wi_mfi_load.pro, solarwind_load_hro.pro,
    		solarwind_load_omni1h.pro, solarwind_load_wind.pro

     MODIFICATION HISTORY:
    	Written by:	Vladimir Kondratovich 2008/01/16.

(See external/developers/solarwind/solarwind_crib.pro)

## SOLARWIND_LOAD

[Previous Routine] [Next Routine] [List of Routines]

     NAME:
         SOLARWIND_LOAD

     PURPOSE:
    	Routine provides solar wind (SW) data time-shifted to the bow-shock
    	nose. Time resolution of data is variable with 1 minute as finest.
    	SW data sources: OMNI-2, HRO, and WIND. Time shifting of the WIND
    	data is based on the OMNI-2 metodology.
    	Important difference is that we first average and then propagate
    	averaged WIND quantities to the Earth. If there still is a strong
    	irregularity in the SW speed after averaging, the code warns user.
    	In all cases of insufficient data, the code produces nominal static
    	SW parameters, following SPDF standards. Static nominal SW data is
    	default output if no user preferences are specified in the
    	program call.

     CATEGORY:
    	Data Processing

     CALLING SEQUENCE:
    	solarwind_load,swdata,dstout,trange, resol=resol, wind=wind, hro=hro, min5=min5, h1=h1, dst=dst

     INPUTS:
    	trange : [tstart, tend] - time range (at the magnetopause) for SW data
    		Times tstart and tend need to be one of types supported by TDAS
    		(specifically, by the time_double.pro routine), in part:
    		double seconds since 1970 (internal TDAS format)
    		string format: 'YYYY-MM-DD/hh:mm:ss'
     OPTIONAL INPUT:
    	resol  : desired time resolution of the output data in seconds
    		- if not set, SW data are provided in original time resolution

     KEYWORDS:
    	wind - WIND observations used (they are convolved to desired resolution and
    		then time-shifted to the bow-shock nose using OMNI-2 methodology. The
    		code checks if the SW speed irregularities are too large and warns
    		user when more sophisticated processing may be needed.
    	hro - HRO data are used (most consistent approach up-to-date). The data are
    		already propagated, so they are just convolved to desired resolution.
    	min5 - use 5 min HRO merged database (default is to use 1 min HRO merged data)
    	h1 - use OMNI-2 1 hour SW database. No convolution employed and parameter
    		resol is ignored
    	dst - get Dst index from the OMNI-2 database. This switch works independently
    		on the other data keywords (for example, it provides Dst output even
    		if HRO or WIND data are ordered). Dst is interpolated onto the time grid
    		od requested data, if any.

     PARAMETERS: 3 parameters for outlier filtering are described and set at the
    			beginning of the code.

     OUTPUTS:
    	swdata: | t | Dp | Bz | of IMF at the bow-shock nose
    		- 2D double array (ntpoints,3)
    	dstout: | Dst | - Dst index on the 1-hour OMNI-2 time grid
    		- double array (ntpoints)

     DEPENDENCIES: convolve_gaussian_1d.pro, remove_outliers.pro, repair.pro,
         wi_swe_load.pro, wi_mfi_load.pro, omni_hro_load.pro, omni2_load.pro,
         get_data.pro, xclip.pro, xdegap.pro, xdeflag.pro, cotrans.pro. The code
         is a lowest-level part of LMN transform package.

     MODIFICATION HISTORY:
    	Written by:	Vladimir Kondratovich 2007/12/28.
    	Modified by Vladimir Kondratovich 2008/03/31. Mods do not change call syntax. The code
    		is made modular with plug-in subroutines for each data source, so it became easy
    		to add a new one. Existing ingest modules provide a template.

(See external/developers/solarwind/solarwind_load.pro)

## SOLARWIND_LOAD_HRO

[Previous Routine] [Next Routine] [List of Routines]

     NAME:
         SOLARWIND_LOAD_HRO

     PURPOSE:
    	Plug-in subroutine for driver routine solarwind_load.pro provides
    	solar wind (SW) data time-shifted to the bow-shock
    	nose. Time resolution of data is variable with 1 minute as finest.
    	SW data source: High Resolution OMNI. It is already time-shifted.
    	In all cases of insufficient data, the code produces nominal static
    	SW parameters, following SPDF standards.

     CATEGORY:
    	Data Processing

     CALLING SEQUENCE:
    	solarwind_load_hro,ishro,times,timee,swdata, resol=resol, min5=min5

     INPUTS:
    	times : - start time (at the magnetopause) for SW data (double UNIX time or
    		any other TDAS time format)
    	timee : - end time, formatted as above
     OPTIONAL INPUT:
    	resol  : desired time resolution of the output data in seconds (double)
    		- if not set, SW data are provided in original time resolution

     KEYWORDS:
    	min5 - use 5 min HRO merged database (default is to use 1 min HRO merged data)

     PARAMETERS: fill values taken from HRO web site

     OUTPUTS:
    	ishro - 1 if HRO data are found and 0 otherwise
    	swdata: | t | Dp | Bz | of IMF at the bow-shock nose
    		- 2D double array (ntpoints,3)

     DEPENDENCIES: convolve_gaussian_1d.pro, omni_hro_load.pro, get_data.pro,
    		xclip.pro, xdegap.pro, xdeflag.pro. The code is a
    		lowest-level part of LMN transform package.

     MODIFICATION HISTORY:
    	Written by:	Vladimir Kondratovich 2007/12/28.
    	Modified by Vladimir Kondratovich 2008/03/31.

(See external/developers/solarwind/solarwind_load_hro.pro)

## SOLARWIND_LOAD_OMNI1H

[Previous Routine] [Next Routine] [List of Routines]

     NAME:
         SOLARWIND_LOAD_OMNI1H

     PURPOSE:
    	Plug-in subroutine for driver routine solarwind_load.pro provides
    	solar wind (SW) data time-shifted to the bow-shock
    	nose. Time resolution of data is fixed: 1 hour. SW data source:
    	OMNI-2. Data is already time-shifted.
    	In all cases of insufficient data, the code produces nominal static
    	SW parameters, following SPDF standards.

     CATEGORY:
    	Data Processing

     CALLING SEQUENCE:
    	solarwind_load_omni1h,isomni1h,times,timee,swdata,dstout

     INPUTS:
    	times : - start time (at the magnetopause) for SW data (double UNIX time or
    		any other TDAS time format)
    	timee : - end time, formatted as above

     KEYWORDS: None

     PARAMETERS: fill values taken from OMNI-2 web site

     OUTPUTS:
    	isomni1h - 1 if OMNI-2 data are found and 0 otherwise
    	swdata: | t | Dp | Bz | of IMF at the bow-shock nose
    		- 2D double array (ntpoints,3)
    	dst_out: | Dst | - Dst index on the 1-hour OMNI-2 time grid
    		- double array (ntpoints)

     DEPENDENCIES: omni2_load.pro, get_data.pro,
    		xclip.pro, xdegap.pro, xdeflag.pro, cotrans.pro. The code is a
    		lowest-level part of LMN transform package.

     MODIFICATION HISTORY:
    	Written by:	Vladimir Kondratovich 2007/12/28.
    	Modified by Vladimir Kondratovich 2008/03/31.

(See external/developers/solarwind/solarwind_load_omni1h.pro)

## SOLARWIND_LOAD_WIND

[Previous Routine] [List of Routines]

     NAME:
         SOLARWIND_LOAD_WIND

     PURPOSE:
    	Plug-in subroutine for driver routine solarwind_load.pro provides
    	solar wind (SW) data time-shifted to the bow-shock
    	nose. Time resolution of data is variable with 1 minute as finest.
    	SW data sources: WIND SWE and MFI. Time shifting of the WIND
    	data is based on the OMNI-2 metodology.
    	Important difference is that we first average and then propagate
    	averaged WIND quantities to the Earth. If there still is a strong
    	irregularity in the SW speed after averaging, the code warns user.
    	In all cases of insufficient data, the code produces nominal static
    	SW parameters, following SPDF standards.

     CATEGORY:
    	Data Processing

     CALLING SEQUENCE:
    	solarwind_load_wind,iswind,times,timee,swdata,resol

     INPUTS:
    	times : - start time (at the magnetopause) for SW data (double UNIX time or
    		any other TDAS time format)
    	timee : - end time, formatted as above
    	resol : desired time resolution of the output data in seconds
    		- if not set, SW data are provided in original time resolution

     KEYWORDS: None

     PARAMETERS: 3 parameters for outlier filtering are propagated through the
    		common block from the main driver solarwind_load.

     OUTPUTS:
    	iswind - 1 if WIND data are found and 0 otherwise
    	swdata: | t | Dp | Bz | of IMF at the bow-shock nose
    		- 2D double array (ntpoints,3)

     DEPENDENCIES: convolve_gaussian_1d.pro, remove_outliers.pro, repair.pro,
         wi_swe_load.pro, wi_mfi_load.pro, get_data.pro,
    		xclip.pro, xdegap.pro, xdeflag.pro, cotrans.pro. The code is a
    		lowest-level part of LMN transform package.

     MODIFICATION HISTORY:
    	Written by:	Vladimir Kondratovich 2007/12/28.
    	Modified by Vladimir Kondratovich 2008/03/31.

(See external/developers/solarwind/solarwind_load_wind.pro)