Solar Spectral Irradiance at 782 nm as Measured by the SES Sensor Onboard Picard

Mustapha Meftah 1, * Alain Hauchecorne 1 Abdanour Irbah 1 Gaël Cessateur 2 Slimane Bekki 1 Luc Damé 3 David Bolsée 2 Nuno Pereira 2
* Auteur correspondant
1 SHTI - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
3 HEPPI - LATMOS
LATMOS - Laboratoire Atmosphères, Milieux, Observations Spatiales
Abstract : Picard is a satellite dedicated to the simultaneous measurement of the total and solar spectral irradiance, the solar diameter, the solar shape, and to the Sun’s interior through the methods of helioseismology. The satellite was launched on June 15, 2010, and pursued its data acquisitions until March 2014. A Sun Ecartometry Sensor (SES) was developed to provide the stringent pointing requirements of the satellite. The SES sensor produced an image of the Sun at 782±2.5 nm. From the SES data, we obtained a new time series of the solar spectral irradiance at 782 nm from 2010 to 2014. During this period of Solar Cycle 24, the amplitude of the changes has been of the order of ± 0.08 %, corresponding to a range of about 2×10−3 Wm−2nm−1. SES observations provided a qualitatively consistent evolution of the solar spectral irradiance variability at 782 nm. SES data show similar amplitude variations with the semi-empirical model Spectral And Total Irradiance REconstruction for the Satellite era (SATIRE-S), whereas the Spectral Irradiance Monitor instrument (SIM) onboard the SOlar Radiation and Climate Experiment satellite (SORCE) highlights higher amplitudes.
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Mustapha Meftah, Alain Hauchecorne, Abdanour Irbah, Gaël Cessateur, Slimane Bekki, et al.. Solar Spectral Irradiance at 782 nm as Measured by the SES Sensor Onboard Picard. Solar Physics, Springer Verlag, 2016, 291 (4), pp.1043-1057. 〈10.1007/s11207-016-0885-2〉. 〈insu-01299636〉

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