Free Delivery Over $100
|
|
|||
|
||||
OverviewThis monograph is devoted to the main problems of cosmic electrodynamics: magnetic field of generation, current sheet formation, turbulence and shocks. It also gives a review of dynamo models and, in more detail, of turbulent dynamo, i.e., magnetic field generation due to turbulent motions in galaxies, stars and the sun. Full Product DetailsAuthor: Samuil Iosifovich Vaĭnshteĭn , Andreĭ Mikhaĭlovich Bykov , Igor Nikolaevich ToptyginPublisher: Gordon & Breach Science Publishers SA Imprint: Gordon & Breach Science Publishers SA Volume: Vol 6 Weight: 0.725kg ISBN: 9782881248771ISBN 10: 2881248772 Pages: 398 Publication Date: 18 October 1993 Audience: College/higher education , Professional and scholarly , Undergraduate , Postgraduate, Research & Scholarly Format: Hardback Publisher's Status: Active Availability: In Print  This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us. Table of ContentsReviewsIt is remarkably comprehensive, covering a wide range of important topics of current interest. -A. M. Soward of University of Newcastle\# upon Tyne, UK The field itself is very extensive. It concerns plasmas in the cosmos and the resulting dynamics of the interstellar medium; it delves deeply into extremely complex questions, including the nature of plasma turbulence, magnetohydrodynamic equilibria and their stability, magnetohydrodynamic shocks and their consequences. The book will therefore become a valuable foundation on which future researchers will rely in developing the field further. -Paul H. Roberts of University of California, Los Angeles It is remarkably comprehensive, covering a wide range of important topics of current interest. <br>-A. M. Soward of University of Newcastle\# upon Tyne, UK <br> The field itself is very extensive. It concerns plasmas in the cosmos and the resulting dynamics of the interstellar medium; it delves deeply into extremely complex questions, including the nature of plasma turbulence, magnetohydrodynamic equilibria and their stability, magnetohydrodynamic shocks and their consequences. The book will therefore become a valuable foundation on which future researchers will rely in developing the field further. <br>-Paul H. Roberts of University of California, Los Angeles <br> Author InformationSamuil Iosifovich Vaĭnshteĭn, Andreĭ Mikhaĭlovich Bykov and Igor Nikolaevich Toptygin Tab Content 6Author Website:Countries AvailableAll regions |
||||
