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dc.contributor.authorMeftah, M.
dc.contributor.authorHauchecorne, A
dc.contributor.authorIrbah, A.
dc.contributor.authorCessateur, G.
dc.contributor.authorBekki, S.
dc.contributor.authorDamé, L.
dc.contributor.authorBolsée, D.
dc.contributor.authorPereira, N.
dc.date2016
dc.date.accessioned2016-06-06T09:49:58Z
dc.date.available2016-06-06T09:49:58Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4039
dc.descriptionPicard 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.
dc.languageeng
dc.titleSolar Spectral Irradiance at 782 nm as Measured by the SES Sensor Onboard Picard
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleSolar Physics
dc.source.volume291
dc.source.issue4
dc.source.page1043-1057
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11207-016-0885-2


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