| id | field name | definition |
| 0 | dcf |
| binary int16 | size: 2 |
|
Detector Confidence Flags; Bit 16-12: aways 0, Bit 11: PMD 3, Bit 10: PMD 2, Bit 9: PMD 1, Bit 8-7: Array 4, Bit 6-5: Array 3, Bit 4-3: Array 2, Bit 2-1: Array 1; 0 = detector ok, 1 = detector is dead, 2 = detector has dead pixels (arrays only)
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|
| 1 | bcr |
| binary array[10] | size: 60 |
Sensor Identifier
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| 2 | reb_kdf |
| binary array[4152] | size: 16608 |
Relative Error Budget on KeyData Functions
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|
| 3 | bdsd_fp |
| binary array[11] | size: 44 |
Bi-directional Scattering Distribution Function (BSDF) Parameters
|
|
| 4 | ustray_lev |
| binary array[4] | size: 16 |
Uniform Straylight level
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| 5 | ghst |
| binary array[8] | size: 96 |
Symmetrical and asymmetrical ghost characteristics
| binary record | size: 12 |
| id | field name | definition |
| 0 | p1 |
| binary int16 | size: 2 |
|
Ghost parameter 1
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| 1 | p2 |
| binary int16 | size: 2 |
|
Ghost parameter 2
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| 2 | p3 |
| binary float | size: 4 |
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Ghost Parameter 3
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| 3 | p4 |
| binary float | size: 4 |
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Ghost Parameter 4
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|
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| 6 | tcw_wdt |
| binary int16 | size: 2 |
|
Width of the triangle convolution window used in straylight
|
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| 7 | sf_pnc |
| binary array[5] | size: 20 |
Scale factors for Peltier induced dark signal noise correction
|
|
| 8 | n_pelt |
| binary int16 | size: 2 |
|
Number of Peltier filter coefficients used
|
|
| 9 | fc_pnc |
| binary array[100] | size: 400 |
Filter coefficients for Peltier induced dark signal noise correction
|
|
| 10 | n_leak |
| binary int16 | size: 2 |
|
Number of Leakage Correction Parameter Sets
|
|
| 11 | noise_arr |
| binary array[dim_0, 4101] |
Array Noise, 3 PMD Offsets, PMD Noise and Dark Current
dim_0: int(../n_leak)
|
|
| 12 | p2p_gain |
| binary array[4, 1024] | size: 16384 |
Pixel-to-Pixel Gain
|
|
| 13 | n_hot |
| binary int16 | size: 2 |
|
Number of Hot Pixel Occurences during this Orbit
|
|
| 14 | hot_occ |
| binary array[dim_0, 3] |
Hot Pixel Occurrences: Record, Array, Pixel
dim_0: int(../n_hot)
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|
| 15 | n_spec |
| binary int16 | size: 2 |
|
Number of Spectral Calibration Parameter Sets
|
|
| 16 | spec_par |
| binary array[dim_0, 24] |
Spectral Calibration Parameters (4th order polynomial) and Average Pixel Deviation for each channel
dim_0: int(../n_spec)
|
|
| 17 | ind_spec |
| binary int16 | size: 2 |
|
Index into Spectral Calibration Parameters for the following Calibration Parameters and Sun Specific Calibration Records
|
|
| 18 | icp |
| binary array[4, 1024] | size: 16384 |
Intensity Calibration Parameters (Interpolated Radiance Response Function)
|
|
| 19 | srs_mean |
| binary array[4, 1024] | size: 16384 |
Sun Reference Spectrum (Mean Value)
| binary float | size: 4 |
|
unit: "BU"
|
|
|
| 20 | prec_srs |
| binary array[4, 1024] | size: 16384 |
Relative Radiometric Precision of the Sun Reference Spectrum
| binary float | size: 4 |
|
unit: ""
|
|
|
| 21 | pmd_srs |
| binary array[3] | size: 12 |
PMD Mean Values of the Sun Reference Spectra
|
|
| 22 | wl_pmd_srs |
| binary array[3] | size: 12 |
Wavelength of the PMD Mean Values of the Sun Reference Spectrum
| binary float | size: 4 |
|
unit: "nm"
|
|
|
| 23 | datetime |
| binary time | size: 8 |
Date, time of the Sun Reference Spectrum
unit: "s since 2000-01-01"
value: (float(./days) - 18262) * 86400 + float(./milliseconds) / 1000
| binary record | size: 8 |
GOME binary datetime
| id | field name | definition |
| 0 | days |
| binary int32 | size: 4 |
days since January 1st, 1950 (may be negative)
unit: "days since 1950-01-01"
|
|
| 1 | milliseconds |
| binary uint32 | size: 4 |
milliseconds since start of day
unit: "1e-3 s"
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|
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| 24 | n_ang |
| binary int16 | size: 2 |
|
Number of different scan mirror angles per channel for which the pre-flight calibration parameters 'Interpolated Polarisation Sensitivity' and 'Radiance Response' are calculated.
|
|
| 25 | ip_sens |
| binary array[dim_0, 2, 1024] |
Interpolated Polarisation Sensitivity and Radiance Response
dim_0: int(../n_ang)
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|