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the earth observation handbook

The Earth Observation Handbook - Key Tables - SEOCA

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Instrument & agency (& any<br />

partners)<br />

ULTRAPAN (Cartosat-3)<br />

Panchromatic sensor<br />

ISRO<br />

Missions Status Type Measurements & applications Technical characteristics<br />

CARTOSAT-3<br />

Being developed High resolution<br />

optical imagers<br />

High resolution images for study of Waveband: Panchromatic VIS: 0.5 - 0.75 µm<br />

topography, urban areas, development of Spatial resolution: 0.3 m<br />

DTM, run-off models etc. Urban sprawl, Swath width: 15 km<br />

forest cover/timber volume, land use change Accuracy:<br />

UV Spectrometer (GACM)<br />

NASA<br />

UV/Vis Near IR Wide Imaging<br />

Spectrometer (Geo-Cape)<br />

NASA<br />

UVAS<br />

UVAS (Ultraviolet Visible and nearinfrared<br />

Atmospheric Sounder)<br />

CDTI<br />

UVN (Sentinel-4)<br />

UV-visible- near infrared imaging<br />

spectrometer (Sentinel-4)<br />

ESA (EC)<br />

GACM Proposed Atmospheric<br />

chemistry<br />

Daytime measurements of O3, NO2, SO2,<br />

CH2O, and aerosols<br />

GEO-CAPE Proposed Imaging multispectral<br />

Measures natural and human-produced<br />

gases and aerosols in <strong>the</strong> atmosphere,<br />

radiometers (vis/IR) including those that react in sunlight to form<br />

polluting low-level ozone.<br />

Ingenio Approved Atmospheric<br />

chemistry<br />

Sentinel-4 A, Sentinel-4 B Proposed<br />

Atmospheric<br />

chemistry<br />

UVNS (post-EPS)<br />

UV-visible-near infrared-shortwave<br />

infrared imaging spectrometer (post-<br />

EPS)<br />

Sentinel-5 Proposed Atmospheric<br />

chemistry<br />

ESA (EC)<br />

UVNS (Sentinel-5 precursor)<br />

UV-visible- near infrared imaging<br />

spectrometer (Sentinel-5 precursor)<br />

ESA (EC, NSO)<br />

VEGETATION<br />

CNES (SNSB, EC)<br />

VFM<br />

Vector Field Magnetometer<br />

ESA<br />

VHRR<br />

Very High Resolution Radiometer<br />

ISRO<br />

VIIRS<br />

Visible/Infrared Imager Radiometer<br />

Suite<br />

NOAA (NASA)<br />

VIRR<br />

Multispectral Visible and Infra-red<br />

Scan Radiometer (10 channels)<br />

NRSCC (CAST)<br />

VIRS<br />

Visible Infra-red Scanner<br />

NASA<br />

Visible imaging spectrometer<br />

(HyspIRI)<br />

NASA<br />

Sentinel-5 precursor Proposed Atmospheric<br />

chemistry<br />

SPOT-4, SPOT-5 Operational Imaging multispectral<br />

radiometers (vis/IR)<br />

Waveband: 305-320 nm and 500-650 nm<br />

Spatial resolution:<br />

Swath width:<br />

Accuracy:<br />

Waveband: 315-600nm<br />

Spatial resolution: 7 km spatial resolution, single<br />

layer vertical resolution, 0.9 nm spectral resolution<br />

Swath width: typically uses 2D data array with 1-D<br />

north to south in space (7 km wide) and 1D for<br />

(oversampled) spectral intervals/bins. The spatial<br />

domain is mechanically scanned for east to west to<br />

cover a continental domain (ei<strong>the</strong>r north or south<br />

America).<br />

Accuracy: ozone precision: 1.3 x 10^16 cm^(-2);NO2<br />

precision: 5 x 10^14 cm^(-2)<br />

The main scientific objectives of <strong>the</strong> UVAS Waveband: NIR 1500-1750 nm O2 A-band 650 to<br />

mission are: - Observe with unprecedented 770 nm UV/VIS 290 to 490 nm<br />

high spatial resolution <strong>observation</strong>s of air Spatial resolution: 20Km nominal, 5Km zoom<br />

quality gases ozone (O3, nitrogen dioxide Swath width:<br />

(NO2), sulphur dioxide (SO2), formaldehyde Accuracy:<br />

(HCHO) and glyoxal (CHO-CHO), and<br />

aerosols over selected urban areas. -<br />

Produce highly-spatially resolved<br />

<strong>observation</strong>s of <strong>the</strong> major greenhouse<br />

gases: carbon dioxide (CO2), methane<br />

(CH4) and water vapor (H2O) over selected<br />

<strong>observation</strong> areas. - Combine high spatial<br />

resolution <strong>observation</strong>s with atmospheric<br />

models to better quantify sources and sinks<br />

of specific gases. - Assimilate <strong>the</strong> remote<br />

sensing measurements into global chemistryclimate<br />

models to examine <strong>the</strong> processes<br />

linking atmospheric composition and climate.<br />

Supporting atmospheric composition and air<br />

quality monitoring services<br />

Supporting atmospheric composition and air<br />

quality monitoring services<br />

Supporting atmospheric composition and air<br />

quality monitoring services<br />

Data of use for crop forecast and monitoring,<br />

vegetation monitoring, and biosphere/<br />

geosphere interaction studies<br />

Waveband: UV-1: 290 - 308 nm, UV-2: 308 - 400 nm,<br />

VIS: 400 - 500 nm, NIR: 750 - 775 nm<br />

Spatial resolution: < 5 km at SSP, possibly relaxed to<br />

50 km for wavelengths < 308 nm<br />

Swath width: FOV E-W: 30°W-45°E @ 40°N, N-S:<br />

30°N-65°N<br />

Accuracy: TBD<br />

Waveband: UV-1: 270 - 300 nm, UV-2: 300-400 nm,<br />

VIS: 400-500 nm, NIR: 710-775 nm, SWIR-1: 1593-<br />

1672 nm, SWIR-2: 1940-2030 nm, SWIR-3: 2305-<br />

2385 nm<br />

Spatial resolution: 5 - 15 km at SSP, possibly relaxed<br />

to 50 km for wavelengths < 300 nm<br />

Swath width: Daily global coverage<br />

Accuracy: TBD<br />

Waveband: UV-1: 270 - 300 nm, UV-2: 300 - 400 nm,<br />

VIS: 400 - 500 nm, NIR: 710 - 775 nm, SWIR-3: 2305<br />

- 2385 nm<br />

Spatial resolution: 5 - 15 km at SSP, possibly relaxed<br />

to 50 km for wavelengths < 300 nm<br />

Swath width: Daily global coverage<br />

Accuracy: TBD<br />

Waveband: Operational mode: VIS: 0.61 - 0.68 µm,<br />

NIR: 0.78 - 0.89 µm, SWIR: 1.58 - 1.75 µm,<br />

Experimental mode: VIS: 0.43 - 0.47 µm<br />

Spatial resolution: 1.15 km at nadir - minimal<br />

variation for off-nadir viewing<br />

Swath width: 2200 km<br />

Accuracy:<br />

Swarm Being developed Magnetic field Magnetic field vector measurments Waveband: N/A<br />

Spatial resolution:

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