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J/A+A/600/A21       Sun UV spectrum (06/06/2008-26/04/2009)      (Bolsee+, 2017)

SOLAR/SOLSPEC mission on ISS: In-flight performance for SSI measurements in the UV Bolsee D., Pereira N., Gillotay D., Pandey P., Cessateur G., Foujols T., Bekki S., Hauchecorne A., Meftah M., Dame L., Herse M., Michel A., Jacobs C., Sela A. <Astron. Astrophys. 600, A21 (2017)> =2017A&A...600A..21B (SIMBAD/NED BibCode)
ADC_Keywords: Sun ; Spectra, ultraviolet Keywords: Sun: general - Sun: UV radiation - instrumentation: detectors - techniques: spectroscopic - space vehicles: instruments Abstract: The SOLar SPECtrum (SOLSPEC) experiment is part of the Solar Monitoring Observatory (SOLAR) payload, and has been externally mounted on the Columbus module of the International Space Station (ISS) since 2008. SOLAR/SOLSPEC combines three absolutely calibrated double monochromators with concave gratings for measuring the solar spectral irradiance (SSI) from 166nm to 3088nm. This physical quantity is a key input for studies of climatology, planetary atmospheres, and solar physics. A general description of the instrument is given, including in-flight operations and performance of the ultraviolet (UV) channel from 175nm to 340nm. We developed a range of processing and correction methods, which are described in detail. For example, methods for correcting thermal behavior effects, instrument linearity, and especially the accuracy of the wavelength and absolute radiometric scales have been validated by modeling the standard uncertainties. The deliverable is a quiet Sun UV reference solar spectrum as measured by SOLAR/SOLSPEC during the minimum of solar activity prior to cycle 24. Comparisons with other instruments measuring SSI are also presented. Description: This file provides the data of the Figure 12 of the paper. It is the average spectral irradiance of the Sun as measured by the space instrument SOLAR/SOLSPEC on ISS during the minimum of solar activity prior to cycle 24. Spectral range: 175nm-340nm by step of 0.5nm. Time interval for averaging: 6th June 2008 - 26th April 2009. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file spectrum.dat 32 331 Sun spectrum
See also: III/238 : Synthetic spectra in the near-IR (Munari+, 2000-2001) J/ApJS/91/461 : EUV spectrum of solar active region (Thomas+, 1994) J/A+A/375/591 : SUMER Spectral Atlas of Solar Disk Features (Curdt+, 2001) J/AJ/135/2245 : Absolute spectrum of Sun and Vega for 0.2-30um (Rieke+, 2008) J/ApJS/181/351 : Solar flux model in 30-1300nm wavelength range (Killen+, 2009) J/A+A/525/A74 : 540-690nm Solar Atlas (Molaro+, 2011) J/A+A/544/A125 : Solar lines from Ceres spectra (Molaro+, 2012) J/ApJS/213/11 : UV spectrum of the quiet Sun above the limb (Warren+, 2014) J/other/ApSS/353.347 : 398-710nm Sun spectral atlases (Fathivavsari+, 2014) J/A+A/581/A26 : Solar Lyman irradiance line profiles (Lemaire+, 2015) J/A+A/587/A65 : Visible and near-infrared solar spectra (Reiners+, 2016) Byte-by-byte Description of file: spectrum.dat
Bytes Format Units Label Explanations
4- 16 E13.8 nm lambda Wavelength 20- 32 E13.8 mW/m2/nm Irr Spectral irradiance
Acknowledgements: David Boisee, David.Bolsee(at)
(End) Patricia Vannier [CDS] 21-Dec-2016
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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