Physics of Magnetic Flux Tubes
This book is the first account of the physics of magnetic flux tubes from their fundamental properties to collective phenomena in an ensembles of flux tubes. The physics of magnetic flux tubes is absolutely vital for understanding fundamental physical pro
- PDF / 23,814,860 Bytes
- 569 Pages / 453.543 x 683.15 pts Page_size
- 106 Downloads / 203 Views
Margarita Ryutova
Physics of Magnetic Flux Tubes
Astrophysics and Space Science Library Volume 417 Editorial Board Chairman W.B. Burton, National Radio Astronomy Observatory, Charlottesville, VA, USA ([email protected]); University of Leiden, The Netherlands ([email protected]) F. Bertola, University of Padua, Italy C.J. Cesarsky, Commission for Atomic Energy, Saclay, France P. Ehrenfreund, Leiden University, The Netherlands O. Engvold, University of Oslo, Norway A. Heck, Strasbourg Astronomical Observatory, France E.P.J. Van Den Heuvel, University of Amsterdam, The Netherlands V.M. Kaspi, McGill University, Montreal, Canada J.M.E. Kuijpers, University of Nijmegen, The Netherlands H. Van Der Laan, University of Utrecht, The Netherlands P.G. Murdin, Institute of Astronomy, Cambridge, UK B.V. Somov, Astronomical Institute, Moscow State University, Russia R.A. Sunyaev, Space Research Institute, Moscow, Russia
More information about this series at http://www.springer.com/series/5664
Margarita Ryutova
Physics of Magnetic Flux Tubes
123
Margarita Ryutova Lawrence Livermore National Laboratory Institute of Geophysics and Planetary Physics Livermore, CA USA
ISSN 0067-0057 ISSN 2214-7985 (electronic) Astrophysics and Space Science Library ISBN 978-3-662-45242-4 ISBN 978-3-662-45243-1 (eBook) DOI 10.1007/978-3-662-45243-1 Library of Congress Control Number: 2014958576 Springer Heidelberg New York Dordrecht London © Springer-Verlag Berlin Heidelberg 2015 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. The use of general descriptive names, registered names, trademarks, service marks, etc. in this publication does not imply, even in the absence of a specific statement, that such names are exempt from the relevant protective laws and regulations and therefore free for general use. The publisher, the authors and the editors are safe to assume that the advice and information in this book are believed to be true and accurate at the date of publication. Neither the publisher nor the authors or the editors give a warranty, express or implied, with respect to the material contained herein or for any errors or omissions that may have been made. Cover illustration: The image is a 3-wavelength composite of solenoidal slinky at the coronal temperatures 2 MK (Fe XV 211 A), 1.5 MK (Fe XII 193 A) and 0.6 MK (Fe IX/X 171A) taken by the SDO/AIA on August 31, 2012. Printed on acid-free paper Springer-Verlag GmbH Berlin Heidelberg is part of Springer Science+Business Media (www.springer.com)
To Dmitri, Alex and Dmitri, Jr.
Preface
The advanced space and ground-based observations show amazing details in the sun’s be