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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/tags/spedas_3_2/external/developers/solarwind/omni2_load.pro $
(See external/developers/solarwind/omni2_load.pro)
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)
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)
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)
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)
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)