A dataset provided by the European Space Agency

Name SolACES, SOLAR Auto-Calibrating EUV, UV Spectrophotometers
Mission SOLAR-ISS
URL http://isssolac.esac.esa.int/iss-solaces/ and http://www.solaces.eu/
DOI https://doi.org/10.5270/esa-24m92t6
Abstract SolACES (SOLAR Auto-Calibrating EUV/UV Spectrophotometers) was designed to monitor (quasi) continuously the Extreme UV (EUV) and UV radiation of the Sun in the wavelength range between 16 and 220 nm on-board the International Space Station (ISS). A novel feature of the instrument is its capability to auto-calibrate the instrument repeatedly during the whole mission via absolute flux detection inside two ionization chambers. SolACES is part of the SOLAR space science instrument package which was mounted into a Coarse Pointing Device (CPD) on the External Payload Facility of the ESA Columbus module. The CPD compensates for the ISS orbital orientation changes, and points SolACES to the Sun together with another solar science payload: the Solar Spectrum measurement instrument or SOLSPEC. This enables simultaneous and complementary measurements of the two instruments for the spectral irradiance between 16 nm and 3 μm.
Description SolACES dataset provides spectral solar irradiance in W.m-2.nm-1 covered by four spectrophotometer channels
SP1: 16-58 nm
SP2: 32-100 nm
SP3: 40-150 nm
SP4: 115-226 nm
Publication Schäfer, R., G. Schmidtke, R. Brunner, T. Strahl, M. Pfeifer, EUV data processing methods of the Solar Auto-Calibrating EUV Spectrometers (SolACES) aboard the International Space Station, Adv. Space Res., 59, 9, 2207-2228, 2017; https://doi.org/10.1016/j.asr.2017.02.036

Schmidtke, G., B. Nikutowski, C. Jacobi, R. Brunner, C. Erhardt, S. Knecht, J. Scherle, J. Schlagenhauf, Solar EUV Irradiance Measurements by the Auto-Calibrating EUV Spectrometers (SolACES) Aboard the International Space Station (ISS), Solar Phys., 289, 1863-1883, 2014; https://doi.org/10.1007/s11207-013-0430-5

Thuillier, G., D. Bolsée, G. Schmidtke, T. Foujols, B. Nikutowski, A.I. Shapiro, R. Brunner, M. Weber, C. Erhardt, M. Hersé, D. Gillotay, W. Peetermans, W. Decuyper, N. Pereira, M. Haberreiter, H. Mandel, W. Schmutz, The Solar Irradiance Spectrum at Solar Activity Minimum Between Solar Cycles 23 and 24, Solar Phys., 289, 1931-1958, 2014; https://doi.org/10.1007/s11207-013-0461-y

Schmidtke, G., R. Brunner, D. Eberhard, B.Halford, U.Klocke, M.Knothe, W.Konz, W.-J.Riedel, H.Wolf, SOL–ACES: Auto-calibrating EUV/UV spectrometers for measurements onboard the International Space Station, Adv. Space Res., 37, 273-282, 2006; https://doi.org/10.1016/j.asr.2005.01.112
Temporal Coverage 01-04-2008 - 15-02-2017
Mission Description The SOLAR monitoring observatory (SOLAR) was an ESA science observatory mounted externally on the Columbus Laboratory, a module of the International Space Station. The primary goal of SOLAR is the (quasi-) continuous measurement of the solar "constant" in order to separate solar effects from human influence on climatology (in progress). SOLAR was launched on February 2008 aboard STS-122. It was originally composed of three scientific instruments: SOVIM (Solar Variability and Irradiance Monitor), SOLSPEC (Solar Spectral Irradiance Measurements), and SolACES. SOLSPEC and SolACES provided detailed measurements of the Sun's spectral irradiance from April 2008 to mid-February 2017 from 16 nm to 3 microns.

Schmidtke, G., Fröhlich, C., Thuillier, G., ISS-SOLAR: Total (TSI) and spectral (SSI) irradiance measurements, Adv. Space Res., 37, 2, 255-264, 2006; https://doi.org/10.1016/j.asr.2005.01.009
Creator Contact Raimund Brunner, Principal Investigator, Fraunhofer IPM, Germany, Raimund.Brunner@ipm.fraunhofer.de
Publisher And Registrant European Space Agency
Credit Guidelines When publishing any works related to this experiment, please cite the DOI found herein.