Email this article Generation of magnetic field waves in celestial bodies by spatially separated sources
- Authors: Popova E.P.1,2
-
Affiliations:
- Skobeltsyn Research Institute of Nuclear Physics
- Schmidt Joint Institute of Physics of the Earth
- Issue: Vol 62, No 8 (2017)
- Pages: 371-373
- Section: Physics
- URL: https://journals.rcsi.science/1028-3358/article/view/191789
- DOI: https://doi.org/10.1134/S1028335817080055
- ID: 191789
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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.
About the authors
E. P. Popova
Skobeltsyn Research Institute of Nuclear Physics; Schmidt Joint Institute of Physics of the Earth
Author for correspondence.
Email: popovaelp@mail.ru
Russian Federation, Moscow, 119991; ul. Bol’shaya Gruzinskaya 10, Moscow, 123242
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