SWE is analyzing the Sun Brightness Temperature in L-Band and the Stokes polarization parameters from the ESA SMOS Mission in collaboration with Deimos Space and funded by ESA. Complementary measurements used in the analysis include the soft X-ray flux from GOES mission, radio emission from space and ground-based observatories, LASCO and STEREO coronagraphs images and solar disk images from SDO mission. The project will also issue recommendations for the operational use of SMOS data as an asset to SWE monitoring and the possibility of continuing missions in this regard.
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Welcome to the Space Weather research group at the University of Alcala
