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Observed intensity of the solar continuum over the range 0.33–2.45 μm

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Abstract

The mean absolute intensity of the solar continuum has been found by averaging the most reliable recent observational data from different authors. We used the modern experimental data on the solar constant, the spectral energy distribution, the limb darkening, and the blanketing effect. The continuum intensity is determined for the center disc and the entire disc. The brightness temperatures are compared with similar temperatures in the model of the photosphere.

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Authors and Affiliations

  1. Sternberg State Astronomical Institute, Moscow

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

Authors
  1. E. A. Makarova
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  2. E. M. Roshchina
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  3. A. P. Sarychev
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Radiofizika, Vol. 39, No. 10, pp. 1230–1233, October, 1996.

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Makarova, E.A., Roshchina, E.M. & Sarychev, A.P. Observed intensity of the solar continuum over the range 0.33–2.45 μm. Radiophys Quantum Electron 39, 825–827 (1996). https://doi.org/10.1007/BF02120965

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  • DOI: https://doi.org/10.1007/BF02120965

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