Using isprint | Doc home | Madrigal home |
Madrigal administrators can get a quick look print out of a CEDAR Madrigal using the command line tool isprint. This may be more convenient than using the web interface or using an Hdf5 viewer such as Hdfview.
The application isprint is used to display both measured and derived data from one particular Cedar/Madrigal file. The input file can be any valid Cedar format. It will generate a table of user selected parameters subject to user specified filters. The name isprint original referred to "Incoherent scatter print" but the application now generically prints any data file in the Cedar format. The engine underlying isprint is the main method for outputting Madrigal data. This application is located in madroot/bin.
The isprint application:
To use isprint, the user needs to specify:
The full filename
file= path to file (this argument is required)
Example: file=/opt/madrigal/experiments/1998/mlh/20jan98/mlh980120g.001.hdf5
The output file
output=<output file>. If not given, default is text file to stdout. If given and extension is one of
<.hdf5, .h5, .hdf>, then will save as Hdf5 file. If extension is .nc, will be saved as netCDF4. In
all other cases, will be saved as ascii text. If hdf5 or netCDF4, arguments (header, summary, badval,
assumed, and knownbad) ignored if given.
Simply enter the desired parameter mnemonic (case-insensitive). They will be displayed in the order entered. If none given, only the header records will be displayed.The parameters desired to be displayed
Any filters to limit the amount of data shown
Time range
date1=mm/dd/yyyy - starting date to be examined. If time1 not given, defaults to 0 UT.
Example: date1=01/20/1998
time1=hh:mm:ss - starting UT time to be examined. If date1 given, is applied to date1. If not, applies on the first day of the experiment.
Example: time1=13:30:00
date2=mm/dd/yyyy - ending date to be examined. If time2 not given, defaults to 0 UT.
Example: date2=01/21/1998
time2=hh:mm:ss - ending UT time to be examined - If date2 not given, refers to date1. If date1 and date2 not given, refers to 1st day.
Example: time2=15:45:00
In the follow arguments ranges are used. If any range value is not given, it may be used to indicate no lower or upper limit (but the comma is always required). Ranges are inclusive of the end points.
Geodetic altitude
z=lower alt limit1, upper alt limit1 [or lower alt limit2 , upper alt limit2 ...] (km)
Example 1: z=100,500 This would limit the geodetic altitude to 100 to 500 km.
Example 2: z=100,200or300,400 This would limit the geodetic altitude to 100 to 200 km or 300 to 400 km.
Example 3: z=,200or300,400 Since the lower limit of the first range is missing, this would limit the geodetic altitude to anything below 200 km or from 300 to 400 km.
Azimuth (from -180 to 180)
az=lower az limit1, upper az limit1 [or lower az limit2 , upper az limit2 ...] (from -180 to 180 degrees)
Example 1: az=100,120 This would limit the azimuth to 100 to 120 degrees.
Example 2: az=-180,-90or90,180 This would limit the azimuth to between -180 and -90 degrees or to between 90 and 180 degrees. Note this allows a filter to go through 180 degrees.
Elevation (from 0 to 90)
el=lower el limit1, upper el limit1 [or lower el limit2 , upper el limit2 ...] (from 0 to 90)
Example 1: el=0,45 This would limit the elevation from 0 to 45 degrees.
Pulse length (in seconds)
plen=lower pl limit1, upper pl limit1 [or lower pl limit2 , upper pl limit2 ...] (pulse len in sec)
Example 1: plen=,5e-4 This would limit the pulse length to 5e-4 seconds or less.
Free form filters
filter=[mnemonic] or [mnemonic1,[+-*/]mnemonic2] , lower limit1 , upper limit1 [or lower limit2 , upper limit2 ...] (any number of filters may be added)
Example: filter=ti,500,1000or2000,3000 Limits the data to points where Ti is between 500 and 1000 degrees or between 2000 and 3000 degrees. Note that the units are always those of the Cedar standard.
Example: filter=gdalt,-,sdwht,0, This filter implies "gdalt - sdwht" must be greater than 0.0. Since sdwht is shadow height (the distance above any point on the earth where the sun is first visible), this filter implies that only data in direct sunlight will be displayed.
Example: filter=ti,/,Dti,100, Limits the data to points where the ratio Ti/dTi is more than 100.
Format options
header=t or f (defaults to header=t, show headers at the beginning of each record)
Example: header=f
badval=bad value string (defaults to "missing")
Example: badval=n/a
assumed=assumed value string (defaults to "assumed")
Example: assumed=-32766
knownbad=known bad value string (defaults to "knownbad")
Example: knownbad=WARNING-BADVALUE
mxchar=maximum characters per line (defaults to no maximum)
Example: mxchar=80
indSpatialParms=<comma separated list of parms>. Used only if saving to an hdf5 or netCDF4 file. If not given,
the default is to use the independent parms in the original file. Ignored if only 1D parms requested.
Example: isprint file=/opt/madrigal/experiments/1998/mlh/20jan98/mil980120g.003.hdf5 date1=01/20/1998 time1=15:00:00 date2=01/20/1998 time2=16:00:00 z=200,300or500,600 badval=noData filter=gdalt,-,sdwht,0, filter=ti,500,1000 uth gdalt gdlat glon ti te
This example would show data from mil980120g.003.hdf5 between 15 and 16 UT on 01/20/1998 where altitude is either between 200 and 300 km or between 500 and 600 km, and where gdalt-sdwht is greater than 0 (point is in sunlight), and where ti is between 500 and 1000. "noData" would be printed if data was not available.
Command line interface to Madrigal | Doc home | Madrigal home |