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<図書>
Advances in solar system magnetohydrodynamics

責任表示 edited by Eric R. Priest and Alan W. Hood
データ種別 図書
出版情報 Cambridge [England] : Cambridge University Press , 1991
本文言語 英語
大きさ xiii, 435 p. : ill. ; 26 cm
概要 Most of the solar system exists in the plasma state (the fourth state of matter). Its subtle nonlinear interaction with the magnetic field can be described by the equations of magnetohydrodynamics (MH...). Over the past few years this important and complex field of research has been actively pursued and increasingly diversely applied to the fields of geophysics, space physics, and astrophysics. It is, for instance, relevant to the study of many dynamic phenomena such as solar flares, and the origins of magnetic fields in the Sun and the Earth. This book examines basic MHD topics, such as equilibria, waves, instabilities, and reconnection, and examines each in the context of different areas that utilize MHD. Many of the world's leading experts have contributed to this volume, which has been edited by two of the key enthusiasts. It is hoped that it will help researchers to appreciate and understand the common threads among the different branches of magnetohydrodynamics. 続きを見る

所蔵情報



筑紫図 1C 400-449 440.12/P 93 1991
067212000002017

書誌詳細

一般注記 Includes index
著者標目 Priest, E. R. (Eric Ronald), 1943-
Hood, A. W.
件 名 LCSH:Astrophysics -- Congresses  全ての件名で検索
LCSH:Magnetohydrodynamics -- Congresses  全ての件名で検索
LCSH:Solar system -- Congresses  全ての件名で検索
LCSH:Magnetosphere -- Congresses  全ての件名で検索
LCSH:Plasma (Ionized gases) -- Congresses  全ての件名で検索
分 類 LCC:QB460
DC20:523.01/886
書誌ID 1000964085
ISBN 0521403251
NCID BA12903576
巻冊次 ISBN:0521403251
登録日 2009.09.16
更新日 2009.09.16

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