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© 1981

Solar Phenomena in Stars and Stellar Systems

Proceedings of the NATO Advanced Study Institute held at Bonas, France, August 25–September 5, 1980

  • Roger M. Bonnet
  • Andrea K. Dupree
Conference proceedings

Part of the NATO Advanced Study Institutes Series book series (ASIC, volume 68)

Table of contents

  1. Front Matter
    Pages i-x
  2. General Overview

  3. Interiors

    1. Ian W. Roxburgh
      Pages 59-74
    2. Eric Fossat
      Pages 75-98
  4. Chromospheres/Coronae and Convective Phenomena

    1. Jean-Paul Zahn
      Pages 123-136
    2. R. A. Stern, J. H. Underwood, M. C. Zolcinski, S. K. Antiochos
      Pages 137-144
    3. Gary A. Glatzmaier, Peter A. Gilman
      Pages 145-172
    4. Eugene H. Avrett
      Pages 173-198
    5. C. Jordan, A. Brown
      Pages 199-225
    6. J. H. Underwood, S. K. Antiochos, J. F. Vesecky
      Pages 227-233
    7. Randolph H. Levine
      Pages 235-237
    8. Claudio Chiuderi
      Pages 269-288
    9. H. C. Spruit
      Pages 289-300
    10. Jack B. Zirker
      Pages 301-318

About these proceedings

Introduction

This book represents the proceedings of a NATO Advanced Study Institute which was held at Bonas from August 25 till Sep­ tember 5, 1980 and was devoted to the study of "Solar Phenomena in Stars and Stellar Systems". It is intended for a broad audi­ ence. Students and post-doctoral scientists for example can dis­ cover new aspects of astrophysics. The general spirit of the ASI was aimed at presenting a unified aspect of astrophysical phenomena which can be studied intensively on the Sun although they are of a much more general nature. On the other hand, spe­ cialists in solar or stellar physics will find here the latest theoretical developments and/or the most recent observations made in their own field of research. An extensive bibliography will be found throughout the various sections, to which the reader may refer, for more detailed developments in various specific areas. In the past, stellar and solar astrophysics have more or less followed their own independent tracks. However, with the rapid development of modern techniques, in particular artificial satellites like the International Ultraviolet Explorer and the Einstein Observatory, which provide a new wealth of data, it appears that chromospheres, coronae, magnetic fields, mass loss and stellar winds, etc . . . . , are found not only in the Sun but occur also in other stars. Frequently these other stars represent quite different conditions of gravity, lumino~ity, and other parameters from those occurring in the Sun.

Keywords

Chromosphere Corona Photosphere Planet Solar Solar flare Solar wind Sun

Editors and affiliations

  • Roger M. Bonnet
    • 1
  • Andrea K. Dupree
    • 2
  1. 1.Centre National de la Recherche ScientifiqueVerrieres-le-BuissonFrance
  2. 2.Harvard Smithsonian Center for AstrophysicsCambridgeUSA

Bibliographic information

  • Book Title Solar Phenomena in Stars and Stellar Systems
  • Book Subtitle Proceedings of the NATO Advanced Study Institute held at Bonas, France, August 25–September 5, 1980
  • Editors R.M. Bonnet
    A.K. Dupree
  • Series Title NATO Advanced Study Institutes Series
  • DOI https://doi.org/10.1007/978-94-009-8479-0
  • Copyright Information Springer Science+Business Media B.V. 1981
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Hardcover ISBN 978-90-277-1275-2
  • Softcover ISBN 978-94-009-8481-3
  • eBook ISBN 978-94-009-8479-0
  • Series ISSN 1389-2185
  • Edition Number 1
  • Number of Pages X, 591
  • Number of Illustrations 0 b/w illustrations, 0 illustrations in colour
  • Topics Planetology
    Astrophysics and Astroparticles
  • Buy this book on publisher's site