SCORe ’96: Solar Convection and Oscillations and their Relationship

  • F. P. Pijpers
  • J. Christensen-Dalsgaard
  • C. S. Rosenthal

Part of the Astrophysics and Space Science Library book series (ASSL, volume 225)

Table of contents

  1. Front Matter
    Pages i-vii
  2. Global Structure

    1. Front Matter
      Pages 1-1
    2. JøRgen Christensen-Dalsgaard
      Pages 3-22
    3. Ian W. Roxburgh
      Pages 23-50
    4. Vladimir A. Baturin, Sergey V. Ayukov
      Pages 55-58
    5. Hans-Günter Ludwig, Bernd Freytag, Matthias Steffen
      Pages 59-64
    6. Helmut Schlattl, Achim Weiss, Hans-Günter Ludwig, Jan Bernkopf
      Pages 65-68
    7. Michael Stix, Michael Kiefer
      Pages 69-72
    8. Regner Trampedach, Jørgen Christensen-Dalsgaard, Åke Nordlund, Robert F. Stein
      Pages 73-76
  3. Basic Properties of Convection

    1. Front Matter
      Pages 77-77
    2. Åke Nordlund, Bob Stein
      Pages 79-103
    3. V. M. Canuto
      Pages 105-125
  4. Convective Effects on Oscillations

    1. Front Matter
      Pages 143-143
    2. Colin S. Rosenthal
      Pages 145-160

About this book

Introduction

This volume contains the reviews and poster papers presented at the workshop Solar Convection and Oscillations and their Relationship: SCORe '96, held in Arhus, Denmark, May 27 - 31, 1996. The aim of this workshop was to bring together experts in the fields of convection and helioseismology, and to stimulate collaborations and joint research. The participation to this workshop was purposely kept limited in order to provide optimal conditions for informal discussions. In autumn of 199,5 the long-awaited GONG network of solar telescopes became fully operational and the first data already show significant improvement over existing datasets on solar oscillations. Furthermore, in December of 1995 the satellite SOHO was launched which, together with GONG, provides a major step forward in both the quantity and the quality of available solar oscillation data. It is with this in mind that we decided to organize the workshop to prepare for the optimal use of this wealth of data, with which to deepen our understanding of solar structure and specifically, of one of the longest-standing problems in solar and stellar modelling: the treatment of convection.

Keywords

3D Chromosphere Photosphere Sun Sunspot helioseismology simulation solar

Editors and affiliations

  • F. P. Pijpers
    • 1
  • J. Christensen-Dalsgaard
    • 1
  • C. S. Rosenthal
    • 1
  1. 1.Theoretical Astrophysics Center, Institute of AstronomyAarhus UniversityÅrhusDenmark

Bibliographic information

  • DOI https://doi.org/10.1007/978-94-011-5167-2
  • Copyright Information Kluwer Academic Publishers 1997
  • Publisher Name Springer, Dordrecht
  • eBook Packages Springer Book Archive
  • Print ISBN 978-94-010-6172-8
  • Online ISBN 978-94-011-5167-2
  • Series Print ISSN 0067-0057
  • About this book