- rescaling the data to a Sun-satellite distance of 1 AU
- removing the dark current
- correcting the data for the degradation trend
- converting the data in physical units
For more information about any of these steps, please refer to the LYRA instrument paper.
Still present in the calibrated data:
- the flat-field effects (i.e. some of the periodic features observed in the data might be linked to spacecraft maneuvers)
- the slow stabilization from MSM-diamond detectors (only applicable to LYRA channels 1-1, 1-3, 2-1, 2-3, 2-4)
ATTENTION: due to the strong degradation, data acquired by the nominal unit (unit2) in Lyman-alpha and Herzberg channels present a very low signal-to-noise ratio, and solar effects might not be easy to extract from them. These data must be used with caution after mid-2010.
Level2 data consist in daily fits files, updated after each contact with the spacecraft. They contain a primary header and a secondary header (described below), followed by the binary table of data.
KEYWORD | EXAMPLE OF VALUE | COMMENT |
---|---|---|
SIMPLE | T | Written by IDL: Tue Feb 15 09:27:46 2011 |
BITPIX | 8 | |
NAXIS | 0 | |
EXTEND | T | File contains extensions |
ORIGIN | ’ROB-SIDC’ | |
TELESCOP | ’PROBA2 ’ | |
INSTRUME | ’LYRA ’ | |
OBJECT | ’EUV solar irrad’ | |
OBS_MODE | ’standard’ | science data |
DATE | ’2011-02-15’ | |
DATE_OBS | ’2010-05-01T00:00:00.004000’ | UTC start of observation |
DATE_END | ’2010-05-01T21:41:22.150995’ | UTC end of observation |
DATASRC | ’Redu ’ | receiving ground station |
LEVEL | ’2 ’ | calibration level |
ALGOR_V | ’EDG=2.1 BSDG=0.5’ | LYRA calibration S/W version |
FILENAME | ’lyra_20100501-000000_lev2_std.fits’ | name of this FITS file |
END |
KEYWORD | EXAMPLE OF VALUE | COMMENT |
---|---|---|
XTENSION | ’BINTABLE’ | Written by IDL: Tue Feb 15 09:27:46 2011 |
BITPIX | 8 | |
NAXIS | 2 | Binary table |
NAXIS1 | 45 | Number of bytes per row |
NAXIS2 | 7789006 | Number of rows |
PCOUNT | 0 | Random parameter count |
GCOUNT | 1 | Group count |
TFIELDS | 6 | Number of columns |
EXTNAME | ’IRRAD LEVEL 2’ | name of binary table extension |
TFORM1 | ’1D ’ | Real*8 (double precision) |
TTYPE1 | ’TIME ’ | Label for column 1 |
TUNIT1 | ’s ’ | Units of column 1 |
TFORM2 | ’1D ’ | Real*8 (double precision) |
TTYPE2 | ’CHANNEL1’ | Label for column 2 |
TUNIT2 | ’W/m**2 ’ | Units of column 2 |
TFORM3 | ’1D ’ | Real*8 (double precision) |
TTYPE3 | ’CHANNEL2’ | Label for column 3 |
TUNIT3 | ’W/m**2 ’ | Units of column 3 |
TFORM4 | ’1D ’ | Real*8 (double precision) |
TTYPE4 | ’CHANNEL3’ | Label for column 4 |
TUNIT4 | ’W/m**2 ’ | Units of column 4 |
TFORM5 | ’1D ’ | Real*8 (double precision) |
TTYPE5 | ’CHANNEL4’ | Label for column 5 |
TUNIT5 | ’W/m**2 ’ | Units of column 5 |
TFORM6 | ’5A ’ | Character string |
TTYPE6 | ’WARNING ’ | Label for column 6 |
TUNIT6 | ’ ’ | Units of column 6 |
END |
Then follows the binary table containing the data, which consists in 6 columns: the time, the irradiance in the four channels, and an index describing the quality of the calibration and time interpolation on the data.