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Advances in Solar Physics

Proceedings of the Seventh European Meeting on Solar Physics Held in Catania, Italy, 11–15 May 1993

  • Conference proceedings
  • © 1994

Overview

Editors:
  1. G. Belvedere
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  2. M. Rodonò
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  3. G. M. Simnett
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Part of the book series: Lecture Notes in Physics (LNP, volume 432)

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Table of contents (39 papers)

  1. Front Matter

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  2. The Sun today

    • Jean-Claude Pecker
    Pages 1-13

  3. Recent results from helioseismology

    • M. J. Thompson
    Pages 17-28

  4. The structure of the solar core

    • W. A. Dziembowski
    Pages 29-40

  5. New sub-barrier nuclear fusion cross sections as a possible solution to the solar neutrino problem

    • Lucio Paternò, Augusto Scalia
    Pages 41-46

  6. Helioseismic evidence for mixing in the radiative interior

    • A. G. Kosovichev
    Pages 47-52

  7. Microscopic settling and turbulent diffusion induced by rotation in the sun

    • Yves Gaigé, Sylvie Vauclair
    Pages 53-58

  8. Mean-field theory of the solar dynamo

    • Dieter Schmitt
    Pages 59-72

  9. Hydrodynamical simulations of the solar dynamo

    • Axel Brandenburg
    Pages 73-84

  10. The asymmetric behaviour of solar activity

    • M. Carbonell, R. Oliver, J. L. Ballester
    Pages 85-90

  11. On the possibility of supergiant stable flows in the convection zone of the sun

    • Evgeniy Tikhomolov
    Pages 91-94

  12. Stellar dynamos

    • Gaetano Belvedere
    Pages 95-100

  13. On magnetic fields, rossby numbers and dynamo action in late-type stars

    • B. Montesinos, C. Jordan
    Pages 101-106

  14. The magnetic field of the solar corona

    • C. E. Alissandrakis
    Pages 107-120

  15. The control of the corona by the convective zone magnetic fields

    • P. Démoulin
    Pages 121-133

  16. Line-tying in a gravitationally stratified atmosphere

    • R. A. M. Van der Linden, A. W. Hood
    Pages 135-140

  17. Magnetic fields surrounding coronal holes

    • Václav Bumba, Miroslav Klvaňa, Július Sýkora
    Pages 141-145

  18. Coronal heating mechanisms

    • G. Einaudi, M. Velli
    Pages 147-160

  19. Coronal heating via nanoflares

    • Giannina Poletto, Roger Kopp
    Pages 161-166

  20. Magnetic structures of the intermediate corona

    • S. Koutchmy, M. Molodensky
    Pages 167-172
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About this book

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.

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