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Titlebook: Solar and Stellar Dynamos; Saas-Fee Advanced Co Paul Charbonneau,Oskar Steiner Book 2013 Springer-Verlag Berlin Heidelberg 2013 Astronomica

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發(fā)表于 2025-3-21 18:11:57 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Solar and Stellar Dynamos
副標題Saas-Fee Advanced Co
編輯Paul Charbonneau,Oskar Steiner
視頻videohttp://file.papertrans.cn/872/871460/871460.mp4
概述Provides a didactic presentation of the theory of stellar magnetic fields.Monographic synthesis of lectures given at Saas-Fee Advanced Course 39.Presents a volume in an internationally highly regarded
叢書名稱Saas-Fee Advanced Course
圖書封面Titlebook: Solar and Stellar Dynamos; Saas-Fee Advanced Co Paul Charbonneau,Oskar Steiner Book 2013 Springer-Verlag Berlin Heidelberg 2013 Astronomica
描述.Astrophysical dynamos are at the heart of cosmic magnetic fields of a wide range of scales, from planets and stars to entire galaxies. This book presents a thorough, step-by-step introduction to solar and stellar dynamos. Looking first at the ultimate origin of cosmic seed magnetic fields, the antagonists of field amplification are next considered: resistive decay, flux expulsion, and flows ruled out by anti-dynamo theorems. Two kinematic flows that can act as dynamos are then studied: the Roberts cell and the CP-flow. Mean-field electrodynamics and derivation of the mean-field dynamo equations lead to the alpha Omega-dynamo, the flux transport dynamo, and dynamos based on the Babcock-Leighton mechanism. Alternatives to the mean-field theory are also presented, as are global MHD dynamo simulations. Fluctuations and grand minima in the solar cycle are discussed in terms of dynamo modulations through stochastic forcing and nonlinear effects. The book concludes with an overview of the major challenges in understanding stellar magnetic fields and their evolution in terms of various dynamo models, global MHD simulations, and fossil fields. Each chapter is accompanied by an annotated bi
出版日期Book 2013
關鍵詞Astronomical Constants; Introductions to Stellar Magnetic Fields; MHD Lectures; Magnetic Fields of Comp
版次1
doihttps://doi.org/10.1007/978-3-642-32093-4
isbn_softcover978-3-642-43047-3
isbn_ebook978-3-642-32093-4Series ISSN 1861-7980 Series E-ISSN 1861-8227
issn_series 1861-7980
copyrightSpringer-Verlag Berlin Heidelberg 2013
The information of publication is updating

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沙發(fā)
發(fā)表于 2025-3-21 20:42:38 | 只看該作者
Solar and Stellar Dynamos978-3-642-32093-4Series ISSN 1861-7980 Series E-ISSN 1861-8227
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發(fā)表于 2025-3-22 04:24:10 | 只看該作者
Saas-Fee Advanced Coursehttp://image.papertrans.cn/s/image/871460.jpg
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Dynamo Models of the Solar Cycle,the chapter is on the sun, simply because the amount of available observational material on the solar magnetic field and its cycle dwarfs anything else in the astrophysical realm, in terms of spatial and temporal resolution, sensitivity, and time span.
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Magnetohydrodynamics, as magnetic energy, helicity, vector potential, flux-freezing and force-free magnetic fields are also introduced and discussed. The chapter closes with a simple example of a mechanical dynamo, and a discussion of the astrophysical dynamo problem in general terms.
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Fluctuations, Intermittency and Predictivity,rities and time delay are considered in turn. The occurrence of intermittency in a subset of these models is then investigated, with an eye on explaining Grand Minima observed in the solar activity record. The chapter closes with a brief discussion of solar cycle prediction schemes based on dynamo models.
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