Entrée : SCARAB - montrer la version 3
URI: https://terra-vocabulary.org/ncl/FAIR-Incubator/earthsciencesensors/c_6ff6c386
The Scanner for Radiation Budget (SCaRaB) is a joint project of France, Germany and Russia and was flown on Russian Meteor-3/7 spacecraft in 1994/1995. The main goal of the ScaRaB instrument is to study the Earth's radiation budget and cloud-radiation interactions. The ScaRaB instrument is a cross-track scanning radiometer with a 60x60 km2 field of view and the pixel spacing is on a square grid of 42.5 km at nadir. The ScaRaB radiometer consist of four parallel telescopes. These are identical except for the optical filters. Each telescope represents one spectral channel: visible, solar, total and atmospheric window. 1 Visible Channel: 0.55 - 0.65 5m 2 Solar Channel(SW): 0.20 - 4 5m 3 Total Channel(TW): 0 20 - 50 5m 4 Window Channel: 10.5 - 12.5 5m Radiation in the Thermal Longwave band (4-50 5m) is determined from the measurements in Channel 2 and 3. The narrower channels 1 and 4 are to be used as a link to operational imager channels and to aid in cloud scene identification.
Métadonnées principales
est un | Concept | Sensor |
modifié le | 1 Dec 2023 10:43:54.415 |
soumis par | Viqui Agazzi |
accepté le | 29 Sep 2022 09:14:26.423 |
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date accepted |
29 Sep 2022 09:14:26.423
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date submitted |
29 Sep 2022 09:11:15.089
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definition |
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item class |
Sensor
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label |
SCARAB
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modified |
1 Dec 2023 10:43:54.415
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notation |
c_6ff6c386
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register |
earthsciencesensors
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status |
status experimental
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submitter |
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register item
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version info |
3
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Définition
broader |
Spectrometers
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definition |
The Scanner for Radiation Budget (SCaRaB) is a joint project of France, Germany and Russia and was flown on Russian Meteor-3/7 spacecraft in 1994/1995. The main goal of the ScaRaB instrument is to study the Earth's radiation budget and cloud-radiation interactions. The ScaRaB instrument is a cross-track scanning radiometer with a 60x60 km2 field of view and the pixel spacing is on a square grid of 42.5 km at nadir. The ScaRaB radiometer consist of four parallel telescopes. These are identical except for the optical filters. Each telescope represents one spectral channel: visible, solar, total and atmospheric window. 1 Visible Channel: 0.55 - 0.65 5m 2 Solar Channel(SW): 0.20 - 4 5m 3 Total Channel(TW): 0 20 - 50 5m 4 Window Channel: 10.5 - 12.5 5m Radiation in the Thermal Longwave band (4-50 5m) is determined from the measurements in Channel 2 and 3. The narrower channels 1 and 4 are to be used as a link to operational imager channels and to aid in cloud scene identification.
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exact match |
e3bb4369 8b1d 4c16 b2f1 5745058bee86
| e1e75346 bf65 de61 3b70 d54549eab90a
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label |
SCARAB
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pref label |
SCARAB
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type |
Concept
| Sensor
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