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SMOS L2 OS ATBD - ARGANS

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3<br />

ICM-CSIC<br />

LOCEAN/SA/CETP<br />

IFREMER<br />

<strong>SM<strong>OS</strong></strong> <strong>L2</strong> <strong>OS</strong><br />

Algorithm Theoretical<br />

Baseline Document<br />

Doc: SO-TN-ARG-GS-0007<br />

Issue: 3 Rev: 9<br />

Date: 25 January 2013<br />

Page: 3<br />

HH along polarization direction H.<br />

VV along polarization direction V.<br />

HV: one arm set to H, the two others set to V.<br />

VH: one arm set to V, the two others set to H. HV and VH mode<br />

produce complex brightness temperatures that are complex conjugates.<br />

In L1C product, both HV and VH modes feed the HV brightness<br />

temperature data field with real and imaginary parts (see SO-TN-<br />

DME-L1PP-0024 and SO-IS-DME-L1PP-0002).<br />

MIRAS operating mode: MIRAS has two operating modes:<br />

Dual polarization mode: measurement sequence is - HH – VV – HH<br />

– VV –HH – VV -…<br />

Full polarization mode: Measurement cycle is - HH – HV – VV – VH<br />

– HH – HV – VV – VH – HH - … (see SO-TN-DME-L1PP-0024)<br />

Retrieval Polarization mode: to derive SSS, one can use<br />

Stokes 1 parameter, i.e. the sum of brightness temperatures in H and V<br />

polarization directions (Stokes 1 retrieval mode).<br />

Brightness temperatures in H and V polarization directions (dual pol<br />

retrieval mode).<br />

Brightness temperatures in H and V directions and real and imaginary<br />

part in HV (full pol retrieval mode).<br />

Modified Stokes vector: Full polarimetric set of temperatures proportional to<br />

modified Stokes parameters as defined by Ulaby, p. 1086<br />

Prior values: Values of the geophysical parameters, obtained from external sources,<br />

that are introduced, with their uncertainties, in the cost function, as reference<br />

information of the variability range during the iterative retrieval<br />

First guesses: Initial values of the geophysical parameters to be retrieved that are<br />

introduced in the first step of the minimisation process, and that will be successively<br />

modified during the iterations until achieving a retrieved value<br />

See the Software Release Document for a list of acronyms.<br />

1.3 List of variables<br />

The modified Stokes vector in the antenna reference frame is [A1, A2, A3, A4] instead<br />

of [Txx, Tyy, Txy] in level 1, with:<br />

A1 = Txx<br />

A2 = Tyy<br />

A3 = 2 Re(Txy)<br />

A4 = 2 Im(Txy)

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