Satellite Sensors

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Revision as of 09:52, 15 April 2011

Inter-comparison Database

The evaluation of passive imager cloud properties retrievals is part of CREW. For CREW-2 five Golden days were selected for which the retrievals of the participating algorithms are inter-compared and compared against reference datasets. This comparison will be continued for CREW-3. Below we will provide information that is relevant for those who plan to upload data for the CREW (inter)-comparison activity.

PRODUCTS

In the CREW inter-comparison following cloud physical properties were compared:

Table: cloud physical properties

GOLDEN DAYS

Table: GOLDEN DAYS of CREW-2 & CREW-3

Note: The data sets are stored on the FTP site of ICARE and is available only for CREW members, see Data_Access.

MSG/SEVIRI

SEVIRI is a 50 cm-diameter aperture, line-by-line scanning radiometer, which provides image data in four Visible and Near-InfraRed (VNIR) channels and eight InfraRed (IR) channels. A key feature of this imaging instrument (Fig. 1) is its continuous imaging of the Earth in 12 spectral channels with a baseline repeat cycle of 15 min. The imaging sampling distance is 3 km at the sub-satellite point for standard channels, and down to 1 km for the High Resolution Visible (HRV) channel. (from www.esa.int)
Data access for the CREW periods here: ./crew/observations/SEVIRI

MODIS

MODIS (Moderate-resolution Imaging Spectroradiometer) is a payload scientific instrument launched into Earth orbit by NASA in 1999 on board the Terra (EOS AM) Satellite, and in 2002 on board the Aqua (EOS PM) satellite. The instruments capture data in 36 spectral bands ranging in wavelength from 0.4 µm to 14.4 µm and at varying spatial resolutions (2 bands at 250 m, 5 bands at 500 m and 29 bands at 1 km). Together the instruments image the entire Earth every 1 to 2 days. (from Wikipedia)
Data access for the CREW periods here: ./crew/observations/MODIS

AVHRR

AVHRR instruments measure the reflectance of the Earth in 5 relatively wide (by today's standards) spectral bands. The first two are centered around the red (0.6 micrometer, 0.5 THz) and near-infrared (0.9 micrometer, 0.3 THz) regions, the third one is located around 3.5 micrometer, and the last two sample the thermal radiation emitted by the planet, around 11 and 12 micrometers, respectively. (from Wikipedia).
Data access for the CREW periods here: ./crew/observations/AVHRR

CALIOP

The Cloud-Aerosol LIdar with Orthogonal Polarization (CALIOP) is the primary instrument on the CALIPSO satellite, which was launched in 2005. CALIOP provides profiles of total backscatter at two wavelengths, from which aerosol and cloud profiles will be derived. The instrument also measures the linear depolarization of the backscattered return, allowing discrimination of cloud phase and the identification of the presence of non-spherical aerosols.
Data access for the CREW periods here: ./crew/observations/CALIOP

CPR

./crew/observations/CPR

AMSR

./crew/observations/AMSR

Synthetic datasets

Simulated satellites scenes can be used to validate retrieval algorithms with a 'know truth'.
Data access for the CREW periods here: ./crew/observations/SYNTHETIC