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Study on magnetohydrodynamic turbule...

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Study on magnetohydrodynamic turbulence and its astrophysical applications

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Study on magnetohydrodynamic turbulence and its astrophysical applicationsby Siyao Xu.
作者:	Xu, Siyao.
出版者:	Singapore :Springer Singapore :2019.
面頁冊數:	xiii, 157 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Magnetohydrodynamics.
電子資源:	https://doi.org/10.1007/978-981-13-7515-6
ISBN:	9789811375156$q(electronic bk.)

Study on magnetohydrodynamic turbulence and its astrophysical applications
Xu, Siyao.

Study on magnetohydrodynamic turbulence and its astrophysical applications[electronic resource] /by Siyao Xu. - Singapore :Springer Singapore :2019. - xiii, 157 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Turbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence. These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics.

ISBN: 9789811375156$q(electronic bk.)

Standard No.: nam a2200325 a 4500Subjects--Topical Terms:

207822
Magnetohydrodynamics.

LC Class. No.: QC718.5.M36

Dewey Class. No.: 538.6

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520 $a Turbulence and magnetic fields are ubiquitous in the Universe. Their importance to astronomy cannot be overestimated. The theoretical advancements in magnetohydrodynamic (MHD) turbulence achieved during the past two decades have significantly influenced many fields of astronomy. This book provides predictive theories of the magnetic field generation by turbulence and the dissipation of MHD turbulence. These fundamental non-linear problems were believed to be tractable only numerically. This book provides complete analytical descriptions in quantitative agreement with existing numerics, as well as theoretical predictions in physical regimes still unreachable by simulations, and explanations of various related observations. It also discusses and promotes the astrophysical applications of MHD turbulence theories, including (i) the particle acceleration and radiation in high-energy phenomena, e.g., Gamma-Ray Bursts, supernova remnants, cosmic rays; (ii) interstellar density fluctuations and the effect on observations, e.g., Faraday rotation, scattering measurements of Galactic and extragalactic radio sources; (iii) density and magnetic field structure in molecular clouds toward star formation. In closing, this book demonstrates the key role of MHD turbulence in connecting diverse astrophysical processes and unraveling long-standing astrophysical problems, as foreseen by Chandrasekhar, a founder of modern astrophysics.
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