大葉大學圖書館 |

Magnetohydrodynamic turbulence /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	538/.6
書名/作者:	Magnetohydrodynamic turbulence // Dieter Biskamp.
作者:	Biskamp, D.,
面頁冊數:	1 online resource (xii, 297 pages) : : digital, PDF file(s).
附註:	Title from publisher's bibliographic system (viewed on 05 Oct 2015).
標題:	Magnetohydrodynamic instabilities.
標題:	Turbulence.
ISBN:	9780511535222 (ebook)
摘要、提要註:	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.
電子資源:	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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