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Titlebook: Magnetic Fields of Galaxies; A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloff Book 1988 Kluwer Academic Publishers 1988 Variation.cosmic ray.

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发表于 2025-3-21 19:05:55 | 显示全部楼层 |阅读模式
书目名称Magnetic Fields of Galaxies
编辑A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloff
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Magnetic Fields of Galaxies;  A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloff Book 1988 Kluwer Academic Publishers 1988 Variation.cosmic ray.
描述Magnetism, when extended beyond normal frameworks into cosmic space is characterized by an enormous spatial scale. Because of their large sizes the nature of magnets such as the Earth and the Sun is entirely different from the nature of a horseshoe magnet. The source of cosmic magnetism is associated with the hydrodynamic motions of a highly conductive medium. In this aspect, cosmic magnets resemble a dynamo. However, currents in the dynamo flow along properly ordered wires, while chaotic, turbulent motions are dominant inside stars and liquid planetary cores. This makes more intriguing and surprising the fact that these motions maintain a regular magnetic field. Maintenance of magnetic fields is even more impressive in huge magnets, i.e. galaxies. In fact, we are living inside a giant dynamo machine, the Milky Way galaxy. Although the idea of the global magnetic field of our Galaxy was clearly proposed almost 40 years ago, firm observational evidence and definite theoretical concepts of galactic magnetism have been developed only in the last decade. This book is the first attempt at a full and consistent presentation of this problem. We discuss both theoretical views on the origin
出版日期Book 1988
关键词Variation; cosmic ray; galaxies; galaxy; quasars; star; star formation; stars; turbulence
版次1
doihttps://doi.org/10.1007/978-94-009-2835-0
isbn_softcover978-94-010-7776-7
isbn_ebook978-94-009-2835-0Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightKluwer Academic Publishers 1988
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书目名称Magnetic Fields of Galaxies影响因子(影响力)




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Origin of Magnetic Fields,mes of radiogalaxies, in quasars and in other objects. Details of magnetic field configurations and their strengths are not always reliable, but the general result is certainty of the presence in galaxies and galactic-type objects of magnetic fields that cover wide ranges of spatial scales and stren
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Concluding Remarks,gnetic fields at galactic scales. This process of maintenance and generation of the magnetic field is called the hydromagnetic dynamo; the same term is usually applied to the motion itself, which provides the dynamo action. In spiral galaxies, the basic elements of the dynamo are the differential ro
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A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloffbetween a matrix and an embedded wh. Since LF wh movement out of finite complements is blocked in Hindi, an explanation along these lines is obviously not feasible for it. I show that there are two distinct sources for long-distance lists, neither of which require us to compromise locality in scope
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A. A. Ruzmaikin,A. M. Shukurov,D. D. Sokoloffned to IP is coindexed with a DP in the main clause and that this instantiates an operator-variable relation. In this chapter the semantics associated with this relation is made explicit. Treating the relative clause as a generalized quantifier and the main clause DP as a variable, I show how the tw
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