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Table of contents

  1. Front Matter
  2. Jean-Claude Pecker
    Pages 1-13
  3. M. J. Thompson
    Pages 17-28
  4. W. A. Dziembowski
    Pages 29-40
  5. Dieter Schmitt
    Pages 59-72
  6. Axel Brandenburg
    Pages 73-84
  7. M. Carbonell, R. Oliver, J. L. Ballester
    Pages 85-90
  8. Gaetano Belvedere
    Pages 95-100
  9. C. E. Alissandrakis
    Pages 107-120
  10. R. A. M. Van der Linden, A. W. Hood
    Pages 135-140
  11. Václav Bumba, Miroslav Klvaňa, Július Sýkora
    Pages 141-145
  12. G. Einaudi, M. Velli
    Pages 147-160
  13. Giannina Poletto, Roger Kopp
    Pages 161-166
  14. S. Koutchmy, M. Molodensky
    Pages 167-172
  15. B. Roberts, P. S. Joarder
    Pages 173-178
  16. G. Peres, F. Reale, L. Golub
    Pages 179-184
  17. N. Vilmer, G. Trottet, C. Barat, J. P. Dezalay, R. Talon, R. Sunyaev et al.
    Pages 197-202
  18. J. -C. Hénoux, K. P. Dere
    Pages 203-215
  19. V. V. Zaitsev
    Pages 217-224
  20. D. A. Biesecker, J. M. Ryan, G. J. Fishman
    Pages 225-230
  21. Sergey Yu. Bogdanov, Anna G. Frank, Natalya P. Kyrie
    Pages 231-236
  22. A. C. -L. Chian, J. R. Abalde, M. V. Alves, S. R. Lopes
    Pages 237-240
  23. J. M. Ryan, E. Bennett, M. A. Lee
    Pages 273-278
  24. M. Messerotti, M. T. Gomez, G. Severino
    Pages 279-284
  25. Franz Ludwig Deubner
    Pages 285-296
  26. P. Lemaire
    Pages 297-309
  27. R. D. Bentley, Yohkoh Team
    Pages 311-314
  28. E. Landi Degl'Innocenti, J. Rayrole, P. Mein
    Pages 315-318
  29. Carole Jordan
    Pages 319-335
  30. Back Matter

About these proceedings

Introduction

This book begins with a very readable survey "The Sun Today" by J.-C. Pecker. It is followed by thorough reviews from leading experts covering theory and observations. The focus shifts from the solar core, studied via neutrino emissions and helioseismology, through the interface regions where it is believed the large-scale magnetic fields are generated, to the corona, where most of the high temperature phenomena characteristic of this region may be studied directly. As energetic particles play such a vigorous role in this part of the sun, a separate session was devoted to their transport and storage in the corona.

Keywords

Neutrino helioseismology solar physics sun

Bibliographic information

  • DOI https://doi.org/10.1007/3-540-58041-7
  • Copyright Information Springer-Verlag 1994
  • Publisher Name Springer, Berlin, Heidelberg
  • eBook Packages Springer Book Archive
  • Print ISBN 978-3-540-58041-6
  • Online ISBN 978-3-540-48420-2
  • Series Print ISSN 0075-8450
  • Series Online ISSN 1616-6361
  • Buy this book on publisher's site