NASA NTRS · 20170003116
Faraday Rotation Measurement with the SMAP Radiometer
Abstract
Faraday rotation is an issue that needs to be taken into account in remote sensing of parameters such as soil moisture and ocean salinity at L-band. This is especially important for SMAP because Faraday rotation varies with azimuth around the conical scan. SMAP retrieves Faraday rotation in situ using the ratio of the third and second Stokes parameters, a procedure that was demonstrated successfully by Aquarius. This manuscript reports the performance of this algorithm on SMAP. Over ocean the process works reasonably well and results compare favorably with expected values. But over land, the inhomogeneous nature of the scene results in much noisier, and in some cases unreliable estimates of Faraday rotation.
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Le Vine, D. M., Abraham, S.. 2016-07-10. Faraday Rotation Measurement with the SMAP Radiometer. https://ntrs.nasa.gov/citations/20170003116
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