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
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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 |
Ghost Parameter 3
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3 | p4 |
binary float | size: 4 |
Ghost Parameter 4
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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
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8 | n_pelt |
binary int16 | size: 2 |
Number of Peltier filter coefficients used
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9 | fc_pnc |
binary array[100] | size: 400 |
Filter coefficients for Peltier induced dark signal noise correction
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10 | n_leak |
binary int16 | size: 2 |
Number of Leakage Correction Parameter Sets
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11 | noise_arr |
binary array[dim_0, 4101] |
Array Noise, 3 PMD Offsets, PMD Noise and Dark Current
dim_0: int(../n_leak)
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12 | p2p_gain |
binary array[4, 1024] | size: 16384 |
Pixel-to-Pixel Gain
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13 | n_hot |
binary int16 | size: 2 |
Number of Hot Pixel Occurences during this Orbit
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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
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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)
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17 | ind_spec |
binary int16 | size: 2 |
Index into Spectral Calibration Parameters for the following Calibration Parameters and Sun Specific Calibration Records
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18 | icp |
binary array[4, 1024] | size: 16384 |
Intensity Calibration Parameters (Interpolated Radiance Response Function)
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19 | srs_mean |
binary array[4, 1024] | size: 16384 |
Sun Reference Spectrum (Mean Value)
binary float | size: 4 |
unit: "BU"
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20 | prec_srs |
binary array[4, 1024] | size: 16384 |
Relative Radiometric Precision of the Sun Reference Spectrum
binary float | size: 4 |
unit: ""
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21 | pmd_srs |
binary array[3] | size: 12 |
PMD Mean Values of the Sun Reference Spectra
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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"
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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"
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1 | milliseconds |
binary uint32 | size: 4 |
milliseconds since start of day
unit: "1e-3 s"
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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.
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25 | ip_sens |
binary array[dim_0, 2, 1024] |
Interpolated Polarisation Sensitivity and Radiance Response
dim_0: int(../n_ang)
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