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Faraday Rotation David Le Vine Aquarius Algorithm Workshop March 9-11, 2010.

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Presentation on theme: "Faraday Rotation David Le Vine Aquarius Algorithm Workshop March 9-11, 2010."— Presentation transcript:

1 Faraday Rotation David Le Vine Aquarius Algorithm Workshop March 9-11, 2010

2 Approach Rotation Angle Retrieved from 3 rd Stokes Parameter*: Ω F = 0.5 Atan[ T3 / (Tv – Th) ] * S. Yueh, “Estimation of Faraday Rotation with Passive Microwave Polarimetry for Microwave Remote Sensing of Earth Surfaces”, TGARS, Vol 38 (#5), pp. 2434, Sept. 2000.

3 Example: Aquarius Simulator Antenna temperature for vertical polarization (top), horizontal polarization (middle) and third Stokes parameter (bottom) for the Aquarius middle beam.

4 Retrieved Faraday Rotation Angle (Top) Faraday rotation angle at boresight of the middle radiometer beam. (Bottom) Third Stokes parameter for the same antenna.

5 Plan Test – SMOS “full-pol” data Remove spurious signals – Filter at land/water boundaries – Match to theoretical profile Magnetic field + estimate of TEC Remove bias – Match ground truth (sounder) at selected locations Backup Plan – Use model (data assimilation) – Correct for altitude (SMOS algorithm)

6 Retrieved Faraday Rotation Angle (Top) Faraday rotation angle at boresight of the middle radiometer beam. (Bottom) Third Stokes parameter for the same antenna. Rotation Angle Retrieved from 3 rd Stokes Parameter*: Ω F = 0.5 Atan[ T3 / (Tv – Th) ] * S. Yueh, “Estimation of Faraday Rotation with Passive Microwave Polarimetry for Microwave Remote Sensing of Earth Surfaces”, TGARS, Vol 38 (#5), pp. 2434, Sept. 2000.


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