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Possible long-period oscillations in solar radio emission at microwaves

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Abstract

Long-enduring bursts in the Sun at microwaves can occur in a succession, and rare examples of 41-min periodic structure are shown. The experimental difficulties for identifying such phenomena are discussed; their possible association with oscillations in quiescent prominences is suggested.

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Authors and Affiliations

  1. Centro de Radio Astronomia e Astrofisica, Universidade Mackenzie, São Paulo, Brasil

    Pierre Kaufmann

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  1. Pierre Kaufmann
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Kaufmann, P. Possible long-period oscillations in solar radio emission at microwaves. Sol Phys 23, 178–182 (1972). https://doi.org/10.1007/BF00153901

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  • DOI: https://doi.org/10.1007/BF00153901

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