A Preliminary Study of the Calibration for the Rotating Fan-Beam Scatterometer on CFOSAT
The first rotating fan-beam scatterometer (RFSCAT) will be launched onboard the Chinese-French Oceanic Satellite (CFOSAT) in 2018. It provides a set of radar cross-section (σ 0 ) measurements at different azimuth/incidence angles over a wind vector cell (WVC), in order to determine the near-surface...
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Published in | IEEE journal of selected topics in applied earth observations and remote sensing Vol. 8; no. 2; pp. 460 - 470 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
IEEE
01.02.2015
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Subjects | |
Online Access | Get full text |
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Summary: | The first rotating fan-beam scatterometer (RFSCAT) will be launched onboard the Chinese-French Oceanic Satellite (CFOSAT) in 2018. It provides a set of radar cross-section (σ 0 ) measurements at different azimuth/incidence angles over a wind vector cell (WVC), in order to determine the near-surface wind field using the backscatter model, i.e., the so-called geophysical model function (GMF). The accuracy of the retrieved wind vector is a sensitive function of the radiometric accuracy of the σ 0 measurements. Therefore, in-flight calibration, including the loop-back (internal) calibration and the external calibration performed with natural extended-area targets, is studied in this paper. Several homogeneous areas over land are first analyzed to check the stability and azimuthal dependence of the σ 0 over these areas. A new calibration mask of the homogeneous land areas is generated and will be used by RFSCAT calibration. Then a simple method of external calibration is proposed to eliminate the azimuthal-dependent σ 0 errors induced by the insertion loss of the rotating joint, which can be applied to both the rotating pencil-beam scatterometers and the coming RFSCAT. The "observed" σ 0 of RFSCAT is simulated using the SeasatA scatterometer (SASS) measurements and the "perturbed" azimuthal-dependent σ 0 errors. The latter is then tracked by the proposed external calibration. The results show that the accuracy of gain corrections is up to 0.2 dB, ensuring consistency between different azimuthal measurements. |
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ISSN: | 1939-1404 2151-1535 |
DOI: | 10.1109/JSTARS.2014.2333241 |