Magnetohydrodynamic turbulence (Record no. 35117)

000 -LEADER
fixed length control field 02068 a2200217 4500
003 - CONTROL NUMBER IDENTIFIER
control field OSt
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20241104150133.0
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 241104b |||||||| |||| 00| 0 eng d
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9780521052535
040 ## - CATALOGING SOURCE
Original cataloging agency ICTS-TIFR
050 ## - LIBRARY OF CONGRESS CALL NUMBER
Classification number QC718.5.M36
100 ## - MAIN ENTRY--PERSONAL NAME
Personal name Dieter Biskamp
245 ## - TITLE STATEMENT
Title Magnetohydrodynamic turbulence
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Name of publisher, distributor, etc. Cambridge University Press,
Place of publication, distribution, etc. Cambridge, U.K. ;
Date of publication, distribution, etc. [c2003]
300 ## - Physical Description
Pages: 297 p.
505 ## - FORMATTED CONTENTS NOTE
Formatted contents note Preface<br/>1. Introduction<br/>2. Magnetohydrodynamics<br/>3. Transition to turbulence<br/>4. Macroscopic turbulence theory<br/>5. Spectral properties and phenomenology<br/>6. Two-point-closure theory<br/>7. Intermittency<br/>8. Two-dimensional turbulence<br/>9. Compressible turbulence and turbulent convection<br/>10. Turbulence in the solar wind<br/>11. Turbulence in accretion disks<br/>12. Interstellar turbulence<br/>References<br/>Index.
520 ## - SUMMARY, ETC.
Summary, etc. 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.--- summary provided by the publisher
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Magnetohydrodynamic instabilities
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Turbulence
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Source of classification or shelving scheme
Koha item type Book
Holdings
Withdrawn status Lost status Damaged status Not for loan Collection code Home library Shelving location Date acquired Inventory number Full call number Accession No. Koha item type
        Physics ICTS Rack No 12 11/04/2024 IN813 Dt.25 Oct 2024 QC718.5.M36 02866 Book