| id | field name | definition |
|---|
| 0 | cos_rays_flag |
| binary uint8 | size: 1 |
|---|
|
Cosmic rays processing activation switch
|
|
| 1 | mod_corr_switch |
| binary uint8 | size: 1 |
|---|
|
Modulation correction switch
|
|
| 2 | dark_charge_flag |
| binary uint8 | size: 1 |
|---|
|
Dark charge correction processing activation switch. 0 = no correction; 1 = use DC maps; 2 = use first measurements; 3 = use DC maps from ADF
|
|
| 3 | inter_stray_flag |
| binary uint8 | size: 1 |
|---|
|
Internal straylight correction activation switch. 0 = correction; 1 = no correction
|
|
| 4 | earth_stray_flag |
| binary uint8 | size: 1 |
|---|
|
External earth straylight correction activation switch. 0 = correction; 1 = no correction
|
|
| 5 | sun_stray_flag |
| binary uint8 | size: 1 |
|---|
|
External sun straylight correction activation switch. 0 = correction; 1 = no correction
|
|
| 6 | cen_back_flag |
| binary uint8 | size: 1 |
|---|
|
Central background estimation mode
|
|
| 7 | satu_flag |
| binary uint8 | size: 1 |
|---|
|
SATU data use activation switch
|
|
| 8 | vign_flag |
| binary uint8 | size: 1 |
|---|
|
Vignetting activation switch. 0 = do not perform vignetting; 1 = perform vignetting
|
|
| 9 | flat_flag |
| binary uint8 | size: 1 |
|---|
|
Flat-field correction mode. 0 = no flat-field correction; 1 = flat-field correction active; 2 = use FP data.
|
|
| 10 | flat_field_switch |
| binary array[4] | size: 4 |
|---|
Flat field correction switches
|
|
| 11 | interp_mode_flag |
| binary uint8 | size: 1 |
|---|
|
Interpolation mode for spectra resampling. 0 = cubic spline; 1 = linear interpolation
|
|
| 12 | grid_sel_flag |
| binary uint8 | size: 1 |
|---|
|
Spectral grid selection for transmission computation. 0 = acquisition spectral grid; 1 = nominal spectral grid
|
|
| 13 | cov_flag |
| binary uint8 | size: 1 |
|---|
|
Covariance computation mode
|
|
| 14 | no_lin_correction |
| binary uint8 | size: 1 |
|---|
|
Non-linearity correction activation switch
|
|
| 15 | reflect_activation_sw |
| binary uint8 | size: 1 |
|---|
|
Reflectivity correction activation switch
|
|
| 16 | spare_1 |
| binary bytes | size: 2 |
|---|
|
Spare
|
hidden: true
|
| 17 | earth_mod |
| binary uint8 | size: 1 |
|---|
|
Identifier of Earth model
|
|
| 18 | flat_earth |
| binary float | size: 4 |
|---|
|
Flattening of the Earth
|
|
| 19 | earth_rad |
| binary float | size: 4 |
|---|
Earth equatorial radius
unit: "m"
|
|
| 20 | atm_thick |
| binary float | size: 4 |
|---|
Atmosphere thickness
unit: "m"
|
|
| 21 | earth_ecc |
| binary float | size: 4 |
|---|
|
Earth orbit eccentricity
|
|
| 22 | sun_const |
| binary float | size: 4 |
|---|
Gravitational constant for the sun
unit: "m3/s2"
|
|
| 23 | orbit_angle |
| binary float | size: 4 |
|---|
Angle between the vernal axis and the Earth orbit perihelion direction
unit: "degrees"
|
|
| 24 | semi_axis |
| binary float | size: 4 |
|---|
Earth orbit semi-major axis
unit: "m"
|
|
| 25 | light_c |
| binary uint32 (double) | size: 4 |
|---|
Speed of light
unit: "m/s"
converted unit: "m/s" ()
|
|
| 26 | param_occ_type |
| binary array[8] | size: 32 |
|---|
Parameters for the determination of the occultation type (full dark / bright / twilight / straylight). Only the 5 first values are useful: 1. TGP altitude threshold for bright limb condition (km) - nominal is 50km; 2. TGP sun zenith angle threshold for bright limb condition (deg) - nominal is 97 deg; 3. TGP altitude threshold for twilight condition (km) - nominal is 100km; 4. TGP sun zenith angle threshold for twilight condition (deg) - nominal is 110 deg; 5. Satellite sun zenith angle threshold for straylight condition (deg) - nominal is 120 deg.
|
|
| 27 | spare_2 |
| binary bytes | size: 8 |
|---|
|
Spare
|
hidden: true
|
| 28 | ray_param |
| binary array[10] | size: 40 |
|---|
Ray tracing parameters
|
|
| 29 | ray_time_shift |
| binary uint32 (double) | size: 4 |
|---|
Time shift for ray tracing computation
unit: "1e-3 s"
converted unit: "s" (multiply by 1/1000)
|
|
| 30 | min_wl |
| binary uint32 (double) | size: 4 |
|---|
Minimum wavelength value for ray-tracing
unit: "1e-3 nm"
converted unit: "nm" (multiply by 1/1000)
|
|
| 31 | max_wl |
| binary uint32 (double) | size: 4 |
|---|
Maximum wavelength value for ray-tracing
unit: "1e-3 nm"
converted unit: "nm" (multiply by 1/1000)
|
|
| 32 | ref_wl |
| binary uint32 (double) | size: 4 |
|---|
Reference wavelength for the ray tracing
unit: "1e-3 nm"
converted unit: "nm" (multiply by 1/1000)
|
|
| 33 | spare_3 |
| binary bytes | size: 8 |
|---|
|
Spare
|
hidden: true
|
| 34 | spec_sat |
| binary array[4, 4] | size: 32 |
|---|
Spectrometer sample saturation level. One amplitude level is specified for each gain of each spectrometer. Order: SPA1 gains 0,1,2,3 followed by SPA2 gains 0,1,2,3 and then SPB1 and SPB2
| binary uint16 | size: 2 |
|---|
|
unit: "ADU"
|
|
|
| 35 | fp_sat |
| binary array[2] | size: 4 |
|---|
Photometer data saturation level
| binary uint16 | size: 2 |
|---|
|
unit: "ADU"
|
|
|
| 36 | half_meas |
| binary uint8 | size: 1 |
|---|
|
Half-number of measurements for CR detection
|
|
| 37 | half_col |
| binary uint8 | size: 1 |
|---|
|
Half-number of CCD columns for CR detection
|
|
| 38 | cr_thresh_rel |
| binary array[4, 4] | size: 16 |
|---|
Threshold for relative variation of the signal for cosmic rays detection
| binary uint8 | size: 1 |
|---|
|
unit: "%"
|
|
|
| 39 | cr_thresh_abs |
| binary array[4, 4] | size: 32 |
|---|
Threshold for absolute variation of the signal for cosmic rays detection
| binary uint16 | size: 2 |
|---|
|
unit: "ADU"
|
|
|
| 40 | cr_min |
| binary array[4, 4] | size: 32 |
|---|
Threshold for cosmic rays detection activation. Minimum sample value for which the cosmic rays detection processing is applied.
| binary uint16 | size: 2 |
|---|
|
unit: "ADU"
|
|
|
| 41 | f_dark |
| binary uint8 | size: 1 |
|---|
|
Number of frames for dark charge estimation
|
|
| 42 | thr_back_dl |
| binary uint32 | size: 4 |
|---|
Threshold for background correction (dark limb)
unit: "e"
|
|
| 43 | thr_back_bl |
| binary uint32 | size: 4 |
|---|
Threshold for background correction (bright limb)
unit: "e"
|
|
| 44 | delta_h |
| binary uint32 | size: 4 |
|---|
Altitude range used in the estimated central background computation (general method)
unit: "m"
|
|
| 45 | poly_back_order |
| binary uint8 | size: 1 |
|---|
|
Order of the polynomial used in the estimated central background computation (general method)
|
|
| 46 | flat_index |
| binary uint16 | size: 2 |
|---|
|
Photometer index for the scintillation correction in the flat-field correction processing
|
|
| 47 | spare_4 |
| binary bytes | size: 8 |
|---|
|
Spare
|
hidden: true
|
| 48 | num_ref |
| binary uint16 | size: 2 |
|---|
|
Number of measurements to be used for the reference star spectrum computation
|
|
| 49 | max_spectra |
| binary uint16 | size: 2 |
|---|
|
Maximum number of star spectra to be checked for the computation of the reference star spectrum
|
|
| 50 | min_spectra |
| binary uint16 | size: 2 |
|---|
|
Minimum number of star spectra used to compute the reference star spectrum before a flag is raised
|
|
| 51 | thres_ref_star_spec |
| binary array[4] | size: 8 |
|---|
Threshold for the validity of the reference star spectrum
|
|
| 52 | num_pix_flagged |
| binary array[4] | size: 4 |
|---|
Number of pixels flagged if the reference star spectrum is below the validity threshold
|
|
| 53 | thr_error_meas |
| binary uint32 (double) | size: 4 |
|---|
Threshold for MPH error indicator computation
unit: "1e-2 %"
converted unit: "%" (multiply by 1/100)
|
|
| 54 | min_alt_start_spectrum |
| binary array[4] | size: 16 |
|---|
Minimum altitudes for the computation of the reference start spectrum
| binary uint32 | size: 4 |
|---|
|
unit: "m"
|
|
|
| 55 | spare_5 |
| binary bytes | size: 8 |
|---|
|
Spare
|
hidden: true
|