电邮这篇文章 Generation of magnetic field waves in celestial bodies by spatially separated sources
- 作者: Popova E.P.1,2
-
隶属关系:
- Skobeltsyn Research Institute of Nuclear Physics
- Schmidt Joint Institute of Physics of the Earth
- 期: 卷 62, 编号 8 (2017)
- 页面: 371-373
- 栏目: Physics
- URL: https://journals.rcsi.science/1028-3358/article/view/191789
- DOI: https://doi.org/10.1134/S1028335817080055
- ID: 191789
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详细
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.
作者简介
E. Popova
Skobeltsyn Research Institute of Nuclear Physics; Schmidt Joint Institute of Physics of the Earth
编辑信件的主要联系方式.
Email: popovaelp@mail.ru
俄罗斯联邦, Moscow, 119991; ul. Bol’shaya Gruzinskaya 10, Moscow, 123242
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