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Titlebook: MHD Flows in Compact Astrophysical Objects; Accretion, Winds and Vasily S. Beskin Book 2010 Springer-Verlag Berlin Heidelberg 2010 AGN.Accr

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發(fā)表于 2025-3-21 19:49:00 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書(shū)目名稱MHD Flows in Compact Astrophysical Objects
副標(biāo)題Accretion, Winds and
編輯Vasily S. Beskin
視頻videohttp://file.papertrans.cn/621/620155/620155.mp4
概述A didactic approach to understanding accretion flows, winds and jets of Astrophysical Compact Objects.Analytical treatment of the hydrodynamic and magnetohydrodynamic problem reveals physical concepts
叢書(shū)名稱Astronomy and Astrophysics Library
圖書(shū)封面Titlebook: MHD Flows in Compact Astrophysical Objects; Accretion, Winds and Vasily S. Beskin Book 2010 Springer-Verlag Berlin Heidelberg 2010 AGN.Accr
描述.Accretion flows, winds and jets of compact astrophysical objects and stars are generally described within the framework of hydrodynamical and magnetohydrodynamical (MHD) flows. Analytical analysis of the problem provides profound physical insights, which are essential for interpreting and understanding the results of numerical simulations. Providing such a physical understanding of MHD Flows in Compact Astrophysical Objects is the main goal of this book, which is an updated translation of a successful Russian graduate textbook. The book provides the first detailed introduction into the method of the Grad-Shafranov equation, describing analytically the very broad class of hydrodynamical and MHD flows. It starts with the classical examples of hydrodynamical accretion onto relativistic and nonrelativistic objects. The force-free limit of the Grad-Shafranov equation allows us to analyze in detail the physics of the magnetospheres of radio pulsars and black holes, including the Blandford-Znajek process of energy extraction from a rotating black hole immersed in an external magnetic field. Finally, on the basis of the full MHD version of the Grad-Shafranov equation the author discusses
出版日期Book 2010
關(guān)鍵詞AGN; Accretion; Black Hole Magnetospheres; Blandford-Znajek-Process; Grad-Shafranov-Equation; Jets; Magnet
版次1
doihttps://doi.org/10.1007/978-3-642-01290-7
isbn_softcover978-3-642-26177-0
isbn_ebook978-3-642-01290-7Series ISSN 0941-7834 Series E-ISSN 2196-9698
issn_series 0941-7834
copyrightSpringer-Verlag Berlin Heidelberg 2010
The information of publication is updating

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Vasily S. Beskin agieren kann. Thr kommt somit eine hohe gesellschaftspolitische Bedeutung zu. Univ.-Prof. Dr. Peter Weinberg Institut für Konsum-und Verhaltensforschung an der Universit?t des Saarlandes VII Vorwort Vorwort Die Auffassung, da? mit Kultur und Marketing zwei Welten aufeinanderprallen, ist unter Kultu
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,Force-Free Approximation — the Black Hole Magnetosphere,limation mechanism responsible for the jet formation. In other words, to explain the galactic nuclei activity we use the pulsar idea of a unipolar inductor, the work of which is just provided by the regular poloidal magnetic field, the central object rotation (giving rise to the induction electric f
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發(fā)表于 2025-3-23 03:48:15 | 只看該作者
,Full MHD Version — General Properties,l properties in the magnetosphere of compact objects. In particular, it is shown that, within the full MHD approach, the electric current circulating in the magnetosphere is no longer a free parameter but is to be determined from the critical conditions on the singular surfaces. Asymptotic behavior
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發(fā)表于 2025-3-23 08:36:19 | 只看該作者
,Full MHD Version — Particle Acceleration and Collimation, is to take place. The analytical solutions obtained for quasimonopole and parabolic magnetic fields illustrated the general property that the efficient particle acceleration can take place only for the strongly collimated outflows. Two toy solutions for the black hole magnetosphere support the phys
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