Model Output File Format Description
Model output files should be in ASCII text format. Each file size should not exceed 1Mb. Full path name to the input file at your local disk should not contain any blank spaces or quotation marks. On DOS/Windows systems the recommended extension for the input file name is "txt".
The following file formats for model outputs for different metrics studies are expected:
Metrics 1: Magnetic field at geosynchronous orbit
Year Month Day Hour Min Sec XGSE[Re] YGSE[Re] ZGSE[Re] BXGSE[nT] BYGSE[nT] BZGSE[nT]Here BXGSE[nT] BYGSE[nT] BZGSE[nT] are magnetic field components at GOES position (XGSE[Re] YGSE[Re] ZGSE[Re] ) in GSE coordinates.
You can view a sample file here.
Metics 2: Magnetopause crossings by geosynchronous satellite
Year Month Day Hour Min Sec XGSE[Re] YGSE[Re] ZGSE[Re] I/OHere "I" when geosynchronous satellite position XGSE[Re] YGSE[Re] ZGSE[Re] (GOES or LANL) is inside the modeled magnetopshere, "O" when it is outside.
Sample IDL statement | Sample file
Metrics 3: Plasma density and temperature at geosynchronous orbit
Year Month Day Hour Min Sec XGSE[Re] YGSE[Re] ZGSE[Re] DEN [cm^(-3)] TEMP [Kelvin]Here DEN [cm^(-3)] and TEMP [Kelvin] are plasma density and temperature at LANL position (XGSE[Re] YGSE[Re] ZGSE[Re] ).
Metrics 4: Ground magnetic field perturbations
Year Month Day Hour Min Sec GeomagLat [deg] GeomagLon[deg] B_NorthGeomag[nT], B_EastGeomag[nT], B_DownGeomag[nT]Here B_NorthGeomag[nT], B_EastGeomag[nT], B_DownGeomag[nT] are components of magnetic field perturbation (north, east, down) at ground station location (Geomagnetic Latitude, Geomagnetic Longitude). Please note that Geomagnetic Dipole Coordinates (Hapgood, 1992) are used.
References
M.A. Hapgood, Space physics coordinate transformations: A user guide // Planet. Space Sci. 1992. V. 40, P. 711-717.
Sample Fortran statement | Sample IDL statement | Sample file
Metrics 5: Dst index
Year Month Day Hour Min Sec Dst[nT]







