ASTRONOMY AND ASTROPHYSICS LIBRARY Series Editors: G. Börner, Garching, Germany A. Burkert, München, Germany W. B. Burton, Charlottesville, VA, USA and Leiden, The Netherlands M. A. Dopita, Canberra, Australia A. Eckart, Köln, Germany T. Encrenaz, Meudon, France E. K. Grebel, Heidelberg, Germany B. Leibundgut, Garching, Germany J. Lequeux, Paris, France A. Maeder, Sauverny, Switzerland V.Trimble, College Park, MD, and Irvine, CA, USA Kenneth R. Lang The Sun from Space Second Edition 123 Kenneth R. Lang Department of Physics and Astronomy Tufts University Medford MA 02155 USA
[email protected] Cover image: Solar cycle magnetic variations. These magnetograms portray the polarity and distribution of the magnetism in the solar photosphere. They were made with the Vacuum Tower Telescope of the National Solar Observatory at Kitt Peak from 8 January 1992, at a maximum in the sunspot cycle (lower left) to 25 July 1999, well into the next maximum (lower right). Each magnetogram shows opposite polarities as darker and brighter than average tint. When the Sun is most active, the number of sunspots is at a maximum, with large bipolar sunspots that are oriented in the east–west (left–right) direction within two parallel bands. At times of low activity (top middle), there are no large sunspots and tiny magnetic fields of different magnetic polarity can be observed all over the photosphere. The haze around the images is the inner solar corona. (Courtesy of Carolus J. Schrijver, NSO, NOAO and NSF.) ISBN: 978-3-540-76952-1 e-ISBN: 978-3-540-76953-8 Library of Congress Control Number: 2008933407 c Springer-Verlag Berlin Heidelberg 2009 This work is subject to copyright.