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Generation of magnetic field waves in celestial bodies by spatially separated sources

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Abstract

For a plane layer we have analytically shown that in the case of spatially separated magnetic field generation sources, waves with different frequencies dependent on the physical parameters of the sources (dynamo numbers) emerge in a celestial body. Each of the waves interacts mainly with its source, while the degree of mutual overlapping of the waves decreases with increasing distance between the sources.

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Authors and Affiliations

  1. Skobeltsyn Research Institute of Nuclear Physics, Moscow State University, Moscow, 119991, Russia

    E. P. Popova

  2. Schmidt Joint Institute of Physics of the Earth, Russian Academy of Sciences, ul. Bol’shaya Gruzinskaya 10, Moscow, 123242, Russia

    E. P. Popova

Authors
  1. E. P. Popova
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Correspondence to E. P. Popova.

Additional information

Original Russian Text © E.P. Popova, 2017, published in Doklady Akademii Nauk, 2017, Vol. 475, No. 5, pp. 511–513.

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Popova, E.P. Generation of magnetic field waves in celestial bodies by spatially separated sources. Dokl. Phys. 62, 371–373 (2017). https://doi.org/10.1134/S1028335817080055

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  • DOI: https://doi.org/10.1134/S1028335817080055

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