SH32A-06
Solar Spectral Irradiance Observations from the PICARD/PREMOS Radiometer
Wednesday, 16 December 2015: 11:48
2011 (Moscone West)
Micha Schöll1, Gaël Cessateur2, Werner K Schmutz1, Christoph Wehrli1, Julian Groebner1, Margit Haberreiter1, Matthieu Kretzschmar3, Alexander Shapiro4, Gerard O Thuillier5, Wolfgang Finsterle6, Nigel Fox7, Jean-Francois Hochedez8, Silvio Koller1, Mustapha Meftah9, Stephan Nyeki1, Daniel Pfiffner1, Hansjörg Roth1, Michel Rouze10, Marcel Spescha1, Rinat Tagirov1, Lutz Werner11 and Jules Wyss1, (1)PMOD WRC Physical Meteorological Observatory Davos and World Radiation Center, Davos Dorf, Switzerland, (2)Belgisch Instituut voor Ruimte-Aeronomie, Brussel, Belgium, (3)CNRS - LPCE, orléans, France, (4)Max Planck Institute for Solar System Research, Katlenburg-Lindau, Germany, (5)CNRS, Guyancourt, France, (6)PMOD/WRC, Davos Dorf, Switzerland, (7)National Physical Laboratory, Middlesex, United Kingdom, (8)LATMOS/IPSL/CNRS/UVSQ, Guyancourt, France, (9)LATMOS Laboratoire Atmosphères, Milieux, Observations Spatiales, Paris Cedex 05, France, (10)CNES French National Center for Space Studies, Toulouse Cedex 09, France, (11)PTB Physikalisch-Technische Bundesanstalt, Braunschweig, Germany
Abstract:
Space weather and space climate studies require accurate Solar Spectral Irradiance (SSI) observations. The PREcision Monitoring Sensor (PREMOS) instrument aboard the PICARD satellite acquired solar irradiance measurements in specific spectral windows in the UV, visible and near infrared from October 2010 to March 2014. This contribution aims at presenting the Level 3 data, corrected for non solar features as well as for degradation. These level 3 data has been tested over different scientific cases, such as observations during the Venus transit and the presence of the p-mode signature within high-cadence data. The PREMOS Level 3 data have also been compared to others data sets, namely the SOLSTICE and SIM instruments aboard SORCE, for nearly 3 and half years. An excellent correlation has been found for the UV spectral ranges. We have also found a rather good correlation for visible and near-infrared observations for short-term variations, for which an error of about 200 ppm has been estimated within PREMOS visible and near-infrared observations. The PREMOS data could also be used to address several scientific topics, i.e. for validating semi-empirical models of the solar irradiance. We will emphasize about our new irradiance model, COSIR for Code of Solar Irradiance Reconstruction, which is successful at reproducing the solar modulation as seen in the PREMOS, SoHO/Virgo and SORCE data.
