Enviar artigo por via de e-mail Generation of magnetic field waves in celestial bodies by spatially separated sources
- Autores: Popova E.P.1,2
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Afiliações:
- Skobeltsyn Research Institute of Nuclear Physics
- Schmidt Joint Institute of Physics of the Earth
- Edição: Volume 62, Nº 8 (2017)
- Páginas: 371-373
- Seção: Physics
- URL: https://journals.rcsi.science/1028-3358/article/view/191789
- DOI: https://doi.org/10.1134/S1028335817080055
- ID: 191789
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Resumo
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.
Sobre autores
E. Popova
Skobeltsyn Research Institute of Nuclear Physics; Schmidt Joint Institute of Physics of the Earth
Autor responsável pela correspondência
Email: popovaelp@mail.ru
Rússia, Moscow, 119991; ul. Bol’shaya Gruzinskaya 10, Moscow, 123242
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