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Uspekhi Fizicheskikh Nauk, 2009, Volume 179, Number 8, Pages 809–835
DOI: https://doi.org/10.3367/UFNr.0179.200908a.0809 (Mi ufn801) 		 
This article is cited in 19 scientific papers (total in 19 papers)

REVIEWS OF TOPICAL PROBLEMS

Magnetospheres of magnetized planets

E. S. Belen'kaya

D. V. Skobeltsyn Institute of Nuclear Physics, M. V. Lomonosov Moscow State University
Full-text PDF (6619 kB) Citations (19)
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DOI: https://doi.org/10.3367/UFNr.0179.200908a.0809
Abstract: This review presents the modern understanding of the physics of magnetized planet magnetospheres in the solar system and of the magnetospheric magnetic field structure. In the interiors of Mercury, the Earth, Jupiter, Saturn, Uranus, and Neptune, their intrinsic magnetic fields are generated under the action of the dynamo mechanism. Their magnetic fields are strong enough to sustain the solar wind flow. The magnetosphere surrounding a planet forms during the interaction of the solar wind with the planetary magnetic field. The magnetospheric dynamics is mainly determined by solar wind variations. The magnetosphere of each planet is unique. In this review, the common and individual magnetic field sources and properties of planetary magnetospheres are discussed.
Received: February 2, 2009
Revised: March 7, 2009
English version:
Physics–Uspekhi, 2009, Volume 52, Issue 8, Pages 765–788
DOI: https://doi.org/10.3367/UFNe.0179.200908a.0809
Bibliographic databases:
Document Type: Article
PACS: 94.20.Ss, 94.30.-d, 94.30.Bg, 94.30.Ch
Language: Russian
Citation: E. S. Belen'kaya, “Magnetospheres of magnetized planets”, UFN, 179:8 (2009), 809–835; Phys. Usp., 52:8 (2009), 765–788
Citation in format AMSBIB
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    • This publication is cited in the following 19 articles:
    Citing articles in Google Scholar: Russian citations, English citations
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