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The brightness of the solar disk in the continuum in the region 1.0–2.4 µm

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Abstract

From the results of a critical analysis of some absolute solar radiance measurements, we determine two of the most reliable series for the range 1.0–2.4µm. The absolute scale for both series are corrected using modern experimental data. The resulting data show the presence of an unknown source of absorption in the region 2.0–2.4µm in the photosphere.

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Authors and Affiliations

  1. Sternberg State Astronomical Institute, Moscow State University, Universitetsky prospect, 13, 119899, Moscow, RUSSIA

    E. A. Makarova, E. M. Roshchina & A. P. Sarychev

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  1. E. A. Makarova
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  2. E. M. Roshchina
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  3. A. P. Sarychev
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Makarova, E.A., Roshchina, E.M. & Sarychev, A.P. The brightness of the solar disk in the continuum in the region 1.0–2.4 µm. Sol Phys 152, 47–52 (1994). https://doi.org/10.1007/BF01473182

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  • DOI: https://doi.org/10.1007/BF01473182

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