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Common origin for UV and radio fluctuations?

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Abstract

Brightness temperature fluctuations induced by a shock wave transit through the solar transition region are computed at several decimetric wavelengths. A simplified method previously used to reproduce the observed UV line intensity fluctuations is shown to give oscillation amplitudes which are consistent with experimental results. The detectability of shock-induced radio fluctuations is briefly discussed, to check the possibility of a common origin for the observed UV and radio phenomena.

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Authors and Affiliations

  1. Osservatorio Astrofisico di Arcetri, Firenze, Italia

    Giannina Poletto

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  1. Giannina Poletto
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Poletto, G. Common origin for UV and radio fluctuations?. Sol Phys 66, 323–332 (1980). https://doi.org/10.1007/BF00150588

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  • DOI: https://doi.org/10.1007/BF00150588

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