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Can Measurements of the Near‐Infrared Solar Spectral Irradiance be Reconciled? A New Ground‐Based Assessment Between 4,000 and 10,000 cm −1
Author(s) -
Elsey Jonathan,
Coleman Marc D.,
Gardiner Tom,
Shine Keith P.
Publication year - 2017
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1002/2017gl073902
Subject(s) - irradiance , solar irradiance , spectral line , monte carlo method , infrared , environmental science , remote sensing , physics , consistency (knowledge bases) , radiation , computational physics , atmospheric sciences , optics , geology , astronomy , mathematics , statistics , geometry
The near‐infrared solar spectral irradiance (SSI) is of vital importance for understanding the Earth's radiation budget, and in Earth observation applications. Differences between previously published solar spectra (including the commonly used ATLAS3 spectrum) reach up to 10% at the low wavenumber end of the 4,000–10,000 cm −1 (2.5–1 μm) spectral region. The implications for the atmospheric sciences are significant, since this spectral region contains 25% of the incoming total solar irradiance. This work details an updated analysis of the CAVIAR SSI, featuring additional analysis techniques and an updated uncertainty budget using a Monte Carlo method. We report good consistency with ATLAS3 in the 7,000–10,000 cm −1 region where there is confidence in these results due to agreement with other spectra, but ~7% lower in the 4,000–7,000 cm −1 region, in general agreement with several other analyses.