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Magnetohydrodynamic turbulence /
~
Biskamp, D.,
Magnetohydrodynamic turbulence /
纪录类型:
书目-语言数据,印刷品 : Monograph/item
[NT 15000414] null:
538/.6
[NT 47271] Title/Author:
Magnetohydrodynamic turbulence // Dieter Biskamp.
作者:
Biskamp, D.,
面页册数:
1 online resource (xii, 297 pages) : : digital, PDF file(s).
附注:
Title from publisher's bibliographic system (viewed on 05 Oct 2015).
标题:
Magnetohydrodynamic instabilities.
标题:
Turbulence.
ISBN:
9780511535222 (ebook)
[NT 15000229] null:
This book presents an introduction to, and modern account of, magnetohydrodynamic (MHD) turbulence, an active field both in general turbulence theory and in various areas of astrophysics. The book starts by introducing the MHD equations, certain useful approximations and the transition to turbulence. The second part of the book covers incompressible MHD turbulence, the macroscopic aspects connected with the different self-organization processes, the phenomenology of the turbulence spectra, two-point closure theory, and intermittency. The third considers two-dimensional turbulence and compressible (in particular, supersonic) turbulence. Because of the similarities in the theoretical approach, these chapters start with a brief account of the corresponding methods developed in hydrodynamic turbulence. The final part of the book is devoted to astrophysical applications: turbulence in the solar wind, in accretion disks, and in the interstellar medium. This book is suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.
电子资源:
http://dx.doi.org/10.1017/CBO9780511535222
Magnetohydrodynamic turbulence /
Biskamp, D.,
Magnetohydrodynamic turbulence /
Dieter Biskamp. - 1 online resource (xii, 297 pages) :digital, PDF file(s).
Title from publisher's bibliographic system (viewed on 05 Oct 2015).
Introduction --1.
This book presents an introduction to, and modern account of, magnetohydrodynamic (MHD) turbulence, an active field both in general turbulence theory and in various areas of astrophysics. The book starts by introducing the MHD equations, certain useful approximations and the transition to turbulence. The second part of the book covers incompressible MHD turbulence, the macroscopic aspects connected with the different self-organization processes, the phenomenology of the turbulence spectra, two-point closure theory, and intermittency. The third considers two-dimensional turbulence and compressible (in particular, supersonic) turbulence. Because of the similarities in the theoretical approach, these chapters start with a brief account of the corresponding methods developed in hydrodynamic turbulence. The final part of the book is devoted to astrophysical applications: turbulence in the solar wind, in accretion disks, and in the interstellar medium. This book is suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.
ISBN: 9780511535222 (ebook)Subjects--Topical Terms:
383749
Magnetohydrodynamic instabilities.
LC Class. No.: QC718.5.M36 / B55 2003
Dewey Class. No.: 538/.6
Magnetohydrodynamic turbulence /
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Introduction --
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This book presents an introduction to, and modern account of, magnetohydrodynamic (MHD) turbulence, an active field both in general turbulence theory and in various areas of astrophysics. The book starts by introducing the MHD equations, certain useful approximations and the transition to turbulence. The second part of the book covers incompressible MHD turbulence, the macroscopic aspects connected with the different self-organization processes, the phenomenology of the turbulence spectra, two-point closure theory, and intermittency. The third considers two-dimensional turbulence and compressible (in particular, supersonic) turbulence. Because of the similarities in the theoretical approach, these chapters start with a brief account of the corresponding methods developed in hydrodynamic turbulence. The final part of the book is devoted to astrophysical applications: turbulence in the solar wind, in accretion disks, and in the interstellar medium. This book is suitable for graduate students and researchers working in turbulence theory, plasma physics and astrophysics.
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http://dx.doi.org/10.1017/CBO9780511535222
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