id | field name | definition |
0 | dsr_time |
binary time | size: 12 |
Start time of the Data Set Record
unit: "s since 2000-01-01"
value: float(./days) * 86400 + float(./seconds) + float(./microseconds) / 1000000
binary record | size: 12 |
ENVISAT binary datetime
id | field name | definition |
0 | days |
binary int32 | size: 4 |
days since January 1st, 2000 (may be negative)
unit: "days since 2000-01-01"
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1 | seconds |
binary uint32 | size: 4 |
seconds since start of day
unit: "s"
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2 | microseconds |
binary uint32 | size: 4 |
microseconds since start of second
unit: "1e-6 s"
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1 | quality_flag |
binary int8 | size: 1 |
Quality Indicator (-1 for blank MDSR, 0 otherwise)
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2 | trans_spectra |
binary array[2336] | size: 9344 |
Full transmission spectra
binary float | size: 4 |
unit: ""
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3 | cov |
binary array[2336] | size: 9344 |
Covariance function of the full transmission
binary float | size: 4 |
unit: ""
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4 | scaled_back |
binary array[2336] | size: 4672 |
Scaled estimated central background
binary uint16 | size: 2 |
unit: "e"
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5 | error_back |
binary array[2336] | size: 4672 |
Error bar for the estimated central background
binary uint16 (double) | size: 2 |
unit: "1e-1 %"
converted unit: "%" (multiply by 1/10)
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6 | fp1_data |
binary array[500] | size: 2000 |
Photometers engineering data (FP1)
binary float | size: 4 |
unit: "e"
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7 | fp2_data |
binary array[500] | size: 2000 |
Photometers engineering data (FP2)
binary float | size: 4 |
unit: "e"
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8 | err_fp1 |
binary array[50] | size: 100 |
Error bar for the photometers engineering data (FP1)
binary uint16 (double) | size: 2 |
unit: "1e-1 %"
converted unit: "%" (multiply by 1/10)
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9 | err_fp2 |
binary array[50] | size: 100 |
Error bar for the photometers engineering data (FP2)
binary uint16 (double) | size: 2 |
unit: "1e-1 %"
converted unit: "%" (multiply by 1/10)
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10 | pcd_spec |
binary array[2336] | size: 4672 |
PCD at sample level (SP) for the spectrometers. Each unsigned short integer is composed of the following bit flags: bit 0: FL_sat(k,L,f) - saturation flag for the lower band (0 = no saturation; 1 = saturated); bit 1: FL_sat(k,C,f) - saturation flag for the central band (0 = no saturation; 1 = saturated); bit 2: FL_sat(k,U,f) - saturation flag for the upper band (0 = no saturation; 1 = saturated); bit 3: FL_bad(k,L) - bad pixel flag for the lower band (0 = no bad pixel in the sample; 1 = at least one bad pixel); bit 4: FL_bad(k,C) - bad pixel flag for the central band (0 = no bad pixel in the sample; 1 = at least one bad pixel); bit 5: FL_bad(k,U) - bad pixel flag for the upper band (0 = no bad pixel in the sample; 1 = at least one bad pixel); bit 6: FL_cr(k,L,f) - cosmic ray detection for lower band (0 = no cosmic ray detected in the sample; 1 = one cosmic ray in the sample); bit 7: Fl_cr(k,C,f) - cosmic ray detection for the central band (0 = no cosmic ray detected in the sample; 1 = one cosmic ray in the sample); bit 8: FL_cr(k,U,f) - cosmic ray detection for the upper band (0 = no cosmic ray detected in the sample; 1 = one cosmic ray in the sample); bit 9-10: FL_bg(k,f) - background data flag (0 = central background computed with no flagged sample; 1 = less than 25% flagged samples; 2 = less than 50% flagged samples; 3 = more than 50% flagged samples); bit 11-12: FL_ft(k,f) - full transmission computation (0 = no problems identified; 1 = reference star spectrum value is zero; 2 = one of the spatial bands is flagged for saturation); bit 13: FL_off(k) - pixel is in an invalid spectral range (0 = pixel is in a valid range; 1 = pixel is in an invalid spectral range); bit 14: FL_rsp(k,f) - pixel has been computed with flagged data during resampling process (0 = no problem; 1 = current data computed with flagged data); bit 15: Not used anymore.
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11 | pcd_fp |
binary array[2] | size: 4 |
PCD at sample level (FP) for the fast photometers. The first integer refers to photometer 1, the second to photometer 2. Each unsigned integer contains the following information: bit 0: FL^FP_sat(fc,f,fp) - photometers saturation flag (0 = no saturation; 1 = saturated sample); bit 1-15: not used.
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