Articles | Volume 10, issue 9
https://doi.org/10.5194/amt-10-3375-2017
https://doi.org/10.5194/amt-10-3375-2017
Research article
 | 
15 Sep 2017
Research article |  | 15 Sep 2017

The high-resolution extraterrestrial solar spectrum (QASUMEFTS) determined from ground-based solar irradiance measurements

Julian Gröbner, Ingo Kröger, Luca Egli, Gregor Hülsen, Stefan Riechelmann, and Peter Sperfeld

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Cited articles

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Bolsée, D., Pereira, N., Decuyper, W., Gillotay, D., Yu, H., Sperfeld, P., Pape, S., Cuevas, E., Redondas, A., Hernandéz, Y., and Weber, M.: Accurate determination of the TOA Solar Spectral NIR irradiance using a primary standard source and the Bouguer-Langley technique, Sol. Phys., 289, 2433–2457, https://doi.org/10.1007/s11207-014-0474-1, 2014.
Bolsée, D., Pereira, N., Gillotay, D., Pandey, P., Cessateur, G., Foujols, T., Bekki, S., Hauchecorne, A., Meftah, M., Damé, L., Hersé, M., Michel, A., Jacobs, C., and Sela, A.: SOLAR/SOLSPEC mission on ISS: in-flight performance for SSI measurements in the UV, Astron. Astrophys., 600, A21, https://doi.org/10.1051/0004-6361/201628234, 2017.
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Short summary
We have produced a benchmark high-resolution solar extraterrestrial spectrum from ground-based measurements of direct solar irradiance in the wavelength range 300 to 500 nm. This spectrum can be used for model calculations and for validating solar spectra measured in space. The metrological traceability of this solar spectrum to the International System of Units (SI) is assured by an unbroken chain of calibrations traceable to the primary spectral irradiance standard of PTB.