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Study on Magnetohydrodynamic Turbulence and Its Astrophysical Applications

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Éditeur :

Springer


Collection :

Springer Theses

Paru le : 2019-04-23

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Description

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.
Pages
157 pages
Collection
Springer Theses
Parution
2019-04-23
Marque
Springer
EAN papier
9789811375149
EAN PDF
9789811375156
Informations sur l'ebook
Nombre pages copiables
1
Nombre pages imprimables
15
Taille du fichier
3052 Ko
Prix
94,94 €
EAN EPUB
9789811375156
Informations sur l'ebook
Nombre pages copiables
1
Nombre pages imprimables
15
Taille du fichier
7608 Ko
Prix
94,94 €

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