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Transient magnetic disturbances from solar flare explosions and associated pulsations of type IV radio bursts

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Abstract

We have proposed a mechanism of arise of transient magnetic disturbances from solar flare explosion which can lead to understanding of observed pulsations of type IV radio emission with period of 0.3–3.0 s. According to the proposed mechanism the pulsation activity of the radio emission results from MHD waves accompanying the expanding diamagnetic plasma produced by the explosive flare material.

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Authors and Affiliations

  1. Geophysical Institute of the Slovak Academy of Sciences, Hurbanovo, Czechoslovakia

    Stephen Pintér

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  1. Stephen Pintér
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Pintér, S. Transient magnetic disturbances from solar flare explosions and associated pulsations of type IV radio bursts. Astrophys Space Sci 123, 209–211 (1986). https://doi.org/10.1007/BF00649136

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  • DOI: https://doi.org/10.1007/BF00649136

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