Summary
The Microwave Imagine Radiometer with Aperture Synthesis MIRAS aboard ESAs SMOS satellite measures the Earths surface brightness temperature TB at LBand frequency of 14 GHz NASAs SMAP spacecraft carries a 12 GHz radar and a 14 GHz radiometer that share a single feedhorn and a mesh reflector The synthetic aperture technique of SMOS allows to measure TB at a range of incidence angles while SMAP uses a conical scan geometry and a constant incidence angle at 40 In order to generate a homogeneous SMOSSMAP data product the SMOS TB will be interpolated to the SMAP incidence angle of 40 SMOS and SMAP polarized TBs and their estimated uncertainties will be projected into a common grid eg polar stereographic or EASE Data products will be generated using standard NetCDF format
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