Calculation of solar radiation atmospheric absorption with different H2O spectral line data banks |
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Authors: | T. Yu. Chesnokova B.A. Voronin A.V. Kozodoev J. Tennyson |
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Affiliation: | a Institute of Atmospheric Optics SB RAS, SB of Russian Academy of Science, 1, Akademicheskii av, 634055 Tomsk, Russian Federation b Department of Physics and Astronomy, University College London, London WC1E 6BT, UK |
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Abstract: | A comparison of the atmospheric absorption calculated with different data banks of water vapour absorption lines is made. The HITRAN database, Barber-Tennyson line list (BT2), calculation of Partridge and Schwenke (PS) are considered. The contribution of H2O lines, absent in HITRAN, to the atmospheric transmission, calculated with 10 cm−1 spectral resolution in the 10 000-20 000 cm−1 spectral region is up to 1.5% for a vertical path and 4% for a solar zenith angle of 70 deg. The highest difference is observed in the 940 nm band. The incoming fluxes of solar radiation, measured by a rotating solar spectroradiometer, were modeled with BT2 and HITRAN database. The difference between measured and calculated fluxes does not exceed the instrumental uncertainties. |
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Keywords: | Atmospheric absorption Water vapour Spectral line |
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