The Solar Spectral Irradiance from 200 to 2400 nm as Measured by the SOLSPEC Spectrometer from the Atlas and Eureca Missions

By G. Thuillier, M. Herse, D. Labs, T. Foujols, W. Peetermans, D. Gillotay, P. Simon, Holger Mandel. 2003

723 citations recorded by the source corpus.

Subfields: Aerospace Engineering, Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/249dd796bece513c79ccb6e2912f6ff9bb4fddd6

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In Aerospace Engineering

1. S. Solanki
2. N. Krivova
3. C. Schmitt
4. A. Bansemer
5. C. Willmer
6. Ping Yang
7. Georges Kaddoum
8. Bryan A. Baum

In Astronomy and Astrophysics

1. S. Solanki
2. N. Krivova
3. J. Haigh
4. C. Fröhlich
5. M. Lockwood
6. Greg Kopp
7. M. Haberreiter
8. W. Schmutz

In Atmospheric Science

1. S. Solanki
2. N. Krivova
3. Bryan A. Baum
4. Ping Yang
5. C. Schmitt
6. C. Willmer
7. J. Haigh
8. Andrew J. Heymsfield

Citations in the corpus

• Optical Communication in Space: Challenges and Mitigation Techniques (2017, background): “Thereafter, the pattern decreases with the increase in the wavelength [141].”
• Semiempirical Models of the Solar Atmosphere. I. The Quiet- and Active Sun Photosphere at Moderate Resolution (2006, background): “In Figure 4 we show the computed and observed (Thuillier et al. 2003) irradiance spectra at 1 AU expressed in brightness temperature units (as described by Fontenla et al. [1999]).”
• Solar Surface Magnetism and Irradiance on Time Scales from Days to the 11-Year Cycle (2009, methodology): “The Solar Spectrum (SOLSPEC) experiment on SOLAR/ISS launched February 2009 (for details see Thuillier et al. 2003; Schmidtke et al. 2006b, and references therein) measures the solar spectral irradiance from 180–3000 nm.”
• Improvements in Shortwave Bulk Scattering and Absorption Models for the Remote Sensing of Ice Clouds (2011, methodology): “In this study, the solar spectrum used for integrating over the spectral response functions is given by Thuillier et al. (2003).”
• SEMIEMPIRICAL MODELS OF THE SOLAR ATMOSPHERE. III. SET OF NON-LTE MODELS FOR FAR-ULTRAVIOLET/EXTREME-ULTRAVIOLET IRRADIANCE COMPUTATION (2009, methodology): “…how the absolute irradiance at 1 AU computed from this improved set of photospheric models compares with recent space-borne measurements by SOLSPEC (Thuillier et al. 2003) and SORCE/ SIM (Harder et al. 2005; Rottman et al. 2005) as well as Total Solar Irradiance (TSI) measurements by SORCE/TIM…”
• The Absolute Magnitude of the Sun in Several Filters (2018, methodology): “Table 2 also compares the colors of the new composite with measurements using the Rieke et al. (2008) solar model which combines the Thuillier et al. (2003) SED with the Engelke (1992) approximation for the near to mid infrared.”
• The ACOS CO 2 retrieval algorithm – Part 1: Description and validation against synthetic observations (2011, methodology): “The solar continuum model is a ninth-order polynomial fit to the near-infrared part of the solar spectrum measured by the SOLSPEC instrument ( Thuillier et al., 2003).”
• Preliminary radiometric calibration assessment of ALOS AVNIR-2 (2007, neutral): “They were visually cloud screened, then, converted to reflectance using the extraterrestrial spectrum in [3].”
• Filling-in of near-infrared solar lines by terrestrial fluorescence and other geophysical effects: simulations and space-based observations from SCIAMACHY and GOSAT (2012, neutral): “…as measured below a long-pass filter blocking wavelengths longer than 665 nm, showing maximum fluorescence ( F max ) after 5 min. of dark adaptation, steady state fluorescence ( F s , achieved in less than 0.5 min after illumination), and a sample solar spectrum from Thuillier et al. (2003, 2004).”
• Solar Irradiance Variability and Climate (2013, methodology): “First observations in the visible and IR were sporadic (e.g., by the SOLar SPECtrum, SOLSPEC and SOSP, instruments flown on space shuttles or on the EUropean REtrieval CArrier platform; Thuillier et al. 2004, 2003); see also overviews by Thuillier et al. (2009) and Ermolli et al. (2012).”
• An improved high-resolution solar reference spectrum for earth's atmosphere measurements in the ultraviolet, visible, and near infrared (2010, methodology): “This will be addressed more fully in the future using the calibration techniques developed for OMPS and the present KPNO recalibration, and will be updated at SAO as space-based solar irradiances [10,19] are improved.”