id | field name | definition |
0 | no_valid |
binary uint8 | size: 1 |
No valid data flag. 0 = valid data was found in the Level 0 product; 1 = no valid packets in the Level 0 product.
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1 | no_int_stray |
binary uint8 | size: 1 |
Internal straylight correction flag. 1 = internal straylight correction was not performed; 0 = internal straylight correction was performed.
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2 | no_ext_earth |
binary uint8 | size: 1 |
External earth straylight correction flag. 1 = external earth straylight correction was not performed; 0 = otherwise.
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3 | no_ext_sun |
binary uint8 | size: 1 |
External sun straylight correction flag. 1 = external sun straylight correction was not performed; 0 = otherwise.
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4 | no_slit_trans |
binary uint8 | size: 1 |
Slit transmission correction flag. 1 = slit transmission correction was not performed; 0 = otherwise.
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5 | no_ref_star_comp |
binary uint8 | size: 1 |
PCD flag for reference star spectrum computation. 0 = no problem; 1 = the reference star spectrum was computed with a small number of measurements; 2 = no valid measurements in the occultation to compute the reference star spectrum (see ref_star_db and no_ref_star).
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6 | ref_star_db |
binary uint8 | size: 1 |
PCD flag indicating that the star spectrum has been read from the stellar spectra database. 0 = the reference spectrum is computed from the measurements; 1 = the reference spectrum is read in the database; 2 = the reference spectrum was not found in the stellar spectra data base (see no_ref_star).
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7 | no_ref_star |
binary uint8 | size: 1 |
PCD flag indicating that the reference star spectrum has not been computed. 1 = the reference star spectrum has not been computed; 0 = the reference star spectrum was computed.
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8 | satu_flag |
binary uint8 | size: 1 |
PCD flag indicating that the SATU data have been used for flat field correction. 1 = the SATU data are used; 0 = the SATU data are not used.
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9 | dark_charge_flag |
binary uint8 | size: 1 |
PCD flag for the dark charge computation (photometers). 1 = no DC correction performed; 0 = DC correction performed.
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10 | num_sp_err |
binary uint32 | size: 4 |
Number of source packets containing errors. This value wil equal the number of Transmission MDSRs with their quality flag set to -1.
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11 | lev0_id |
binary uint8 | size: 1 |
Level 0 PCD. 0 = standard occultation; 1 = first part of a tangent occultation; 2 = last part of a tangent occultation
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12 | atm_type |
binary uint8 | size: 1 |
Type of atmosphere file used. 54 = One ECMWF file used. Time recorded is included in the occultation period; 102 = One ECMWF file used. Time recorded before the beginning of the occultation (Delta t <= 24h); 103 = One ECMWF file used. Time recorded after the beginning of the occultation (Delta t <= 24h); 106 = One ECMWF file used. Only one time record in the validity interval (Delta t <= 24h); 155 = Two ECMWF files used; 201 = No ECMWF file available. Use MSIS model alone; 202 = Only old ECMWF files (Delta t >= 24h). Use MSIS model alone; 203 = Only future ECMWF files (Delta t >= 24h). Use MSIS model alone; 206 = No ECMWF file available in the validity interval (Delta t >= 24h). Use MSIS model alone.
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13 | dark_charge_info |
binary uint8 | size: 1 |
Dark charge correction information. 0 = dark charge map used; 1 = first measurements used; 2 = no dark charge correction applied; 11 = first measurements not available - DC corrections with DC maps; 12 = first measurements not available and missing first packet - DC correction with DC maps without temperature dependence; 21 = dark charge map computed from DSA observation has been used.
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14 | dark_limb_cond |
binary uint8 | size: 1 |
Dark/bright limb condition. 0 = dark limb; 1 = bright limb.
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15 | obs_illum_cond |
binary uint8 | size: 1 |
Observation illumination condition. 0 = full dark limb condition; 1 = bright limb condition; 2 = pure twilight condition; 3 = straylight condition; 4 = twilight and straylight condition.
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16 | sdp_extract |
binary uint32 | size: 4 |
SDP extraction processing. Number of invalid measurements during the occultation.
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17 | dat_err |
binary uint32 | size: 4 |
Datation errors. Number of measurements where flags were raised to indicate a datation problem occurred.
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18 | rt_err |
binary uint32 | size: 4 |
Ray tracing errors. Number of measurements with a non-converged ray path.
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19 | geo_err |
binary uint32 | size: 4 |
Geolocation errors. Number of measurements performed outside the atmosphere, set to 1000 if completely performed outside the atmosphere.
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20 | sat_err |
binary uint32 | size: 4 |
Saturation errors. Number of measurements containing saturated samples.
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21 | cr_err |
binary uint32 | size: 4 |
Cosmic ray errors. Number of measurements where cosmic rays have been detected.
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22 | mod_corr_err |
binary uint32 | size: 4 |
Modulation correction errors. Number of measurements where a modulation correction error has been detected.
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23 | vign_err |
binary uint32 | size: 4 |
Vignetting correction. Number of measurements where the vignetting correction was applied.
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24 | num_cent_back |
binary uint32 | size: 4 |
Central Background. Number of measurements where FLAGbg(f) has been raised.
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25 | num_flat |
binary uint32 | size: 4 |
Flat field correction. Number of measurements where the star falls outside the central band.
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26 | num_full_trans_err |
binary uint32 | size: 4 |
Full transmission errors. Number of measurements where a problem has been detected during the full transmission computation.
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27 | num_bad |
binary uint32 | size: 4 |
Bad Pixels. Number of bad pixels per measurement
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28 | num_fp_sat |
binary array[2] | size: 8 |
Photometer saturation. Number of photometers saturated samples. First number is for photometer 1 second is for photometer 2
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29 | back_corr_flag |
binary uint8 | size: 1 |
Background correction flag. 0 = no background correction; 1 = background correction applied (linear interpolation); 2 = background correction applied (exponential interpolation); 3 = background correction applied (general method).
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