TAILIEUCHUNG - The Origin and Dynamics of Solar Magnetism

Abstract The year 2008 marked the one hundredth anniversary of the observational discovery by George Ellery Hale of magnetic field in sunspots (Hale in Astrophys. J. 28:315–343, 1908). This observation, the first to suggest a direct link between the best-known variable features on the Sun and magnetism, started a line of research that has widened considerably over the last 100 years and is continuing today. Knowledge about all aspects of the Sun has increased in a remarkable way over the past few decades | SPACE SCIENCES SERIES OF ISSI The Origin and Dynamics of Solar Magnetism MJ. Thompson A. Balogh . Culhane Ẳ. Nordlund s. K. Solanki and . Zahn Eds. INTERNATIONAL SPACB SCIENCE INSTITUTE U 1 . Thompson A. Balogh . Culhane Ả. Nordlund . Solanki . Zahn Editors The Origin and Dynamics of Solar Magnetism Previously published in Space Science Reviews Volume 144 Issues 1-4 2009 4 Springer . Thompson School of Mathematics Statistics University of Sheffield Sheffield UK A. Balogh International Space Science Institute Bern Switzerland . Culhane University College London Mullard Space Science Laboratory Dorking UK Ả. Nordlund Niels Bohr Institute University of Copenhagen Copenhagen Denmark . Solanki Max-Planck-Institut fur Sonnensystemforschung Katlenburg-Lindau Germany . Zahn LUTH Observatoire de Paris Meudon France Cover illustration Continuum image blue and line-of-sight components of the velocity yellow and magnetic field red and enhanced as green obtained from Milne-Eddington inversions of Stokes data observed with the CRisp Imaging Spectropolarimeter CRISP on the Swedish 1-m Solar Telescope SST . Shown is a shortlived active region observed on 22 April 2008 in the Fe I 6302 line. The spatial resolution is close to the diffraction limit of . Courtesy of Tomas Hillberg Gautam Narayan and Goran Scharmer. All rights reserved. Library of Congress Control Number 2009926695 DOI 978-1-4419-0239-9 ISBN-978-1-4419-0238-2 e-ISBN-978-1-4419-0239-9 Printed on acid-free paper. 2009 Springer Science Business Media BV No part of this work may be reproduced stored in a retrieval system or transmitted in any form or by any means electronic mechanical photocopying microfilming recording or otherwise without the written permission from the Publisher with the exception of any material supplied specifically for the purpose of being entered and executed on a computer system for the exclusive use by the purchaser of the work. 1 .

• Vật lý
• Solar Dynamo
• Planetary Dynamos
• Convection Zone
• Emerging Magnetic
• Magnetic Fields
• Sunspot Penumbrae