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Polarization of a periodic solar microwave burst

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Abstract

No fluctuations in polarization have been found during a 7 GHz solar burst showing 17 s periodic pulses in intensity. Polarization effects can be produced by the propagation media in the active centre, which are not affected directly by the burst source, but situated more deeply than the observed heights at that microwave frequency.

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Authors and Affiliations

  1. Centro de Rádio Astronomia e Astrofísica (CRAAM), Universidade Mackenzie, São Paulo, SP, Brasil

    Pierre Kaufmann

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  1. Pierre Kaufmann
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Kaufmann, P. Polarization of a periodic solar microwave burst. Sol Phys 50, 197–199 (1976). https://doi.org/10.1007/BF00206201

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  • DOI: https://doi.org/10.1007/BF00206201

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