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The New SCIAMACHY Reference Solar Spectral Irradiance and Its Validation

Authors :
Slimane Bekki
Dominique Sluse
Ralph Snel
Stefan Noel
J. M. Krijger
Luc Damé
John P. Burrows
Nuno Pereira
Klaus Bramstedt
Mark Weber
David Bolsée
T. Hilbig
Mustapha Meftah
Institute of Environmental Physics [Bremen] (IUP)
University of Bremen
SRON Netherlands Institute for Space Research (SRON)
TNO [Delf]
Radboud university [Nijmegen]
STRATO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
HELIOS - LATMOS
Belgian Institute for Space Aeronomy / Institut d'Aéronomie Spatiale de Belgique (BIRA-IASB)
Source :
Solar Physics, Solar Physics, Springer Verlag, 2018, 293 (8), pp.art. 121. ⟨10.1007/s11207-018-1339-9⟩, Solar Physics, 8, 293
Publication Year :
2018
Publisher :
HAL CCSD, 2018.

Abstract

International audience; This paper describes a new reference solar spectrum retrieved from measurements of the satellite instrument SCIAMACHY in the wavelength region from 0.24 μm to 2.4 μm and its comparison with several other established solar reference spectra. The SCIAMACHY reference spectrum was recorded early in the mission before substantial optical degradation due to the harsh space environment sets in. The radiometric calibration of SCIAMACHY, applied in this study, includes a physical model of the scanner unit. Furthermore, SCIAMACHY’s internal white light source (WLS) is used to correct for on-ground to in-flight changes. The resultant calibrated solar spectrum from SCIAMACHY is in good agreement with several available solar spectral irradiance (SSI) references in the visible spectral range. Strong throughput losses due to detector icing in the near infrared (NIR) are now adequately accounted for. Nevertheless, a deficit with respect to the ATLAS-3 composite and SORCE/SIM SSI is observed in the NIR. However, the SCIAMACHY solar reference spectrum agrees well with the recently re-evaluated SOLAR/SOLSPEC-ISS and recent ground measurements taken at Mauna Loa in the NIR.

Details

Language :
English
ISSN :
00380938 and 1573093X
Database :
OpenAIRE
Journal :
Solar Physics, Solar Physics, Springer Verlag, 2018, 293 (8), pp.art. 121. ⟨10.1007/s11207-018-1339-9⟩, Solar Physics, 8, 293
Accession number :
edsair.doi.dedup.....cfcae6a987f856279ea48bddefb75fe6