Faraday Rotation

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

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Faraday Rotation. David Le Vine Aquarius Algorithm Workshop March 9-11, 2010. Approach. Rotation Angle Retrieved from 3 rd Stokes Parameter*: Ω F = 0.5 Atan [ T3 / ( Tv – Th ) ]. - PowerPoint PPT Presentation

Transcript of Faraday Rotation

Page 1: Faraday Rotation

Faraday Rotation

David Le VineAquarius Algorithm Workshop

March 9-11, 2010

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Approach

Rotation Angle Retrieved from 3rd Stokes Parameter*: ΩF = 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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Example: Aquarius Simulator

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

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Retrieved Faraday Rotation Angle

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

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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)

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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 3rd Stokes Parameter*: ΩF = 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.