A.G. Kosovichev
, S. Basu
,
J. Christensen-Dalsgaard
, A. Eff-Darwich
, D.O. Gough
,
C. A. Iglesias
, F. Pérez-Hernández
, F. Rogers
,
T. Sekii
, H. Shibahashi
W.W. Hansen Experimental Physics Laboratory,
Center for Space Science & Astrophysics
Stanford University,
MC4055, Stanford, CA 94305, U.S.A.
Teoretisk Astrofysik Center, Danmarks Grundforskningsfond, and
Institut for Fysik og Astronomi
Aarhus Universitet, DK-8000 Aarhus C, Denmark
Instituto de Astrofisica de Canarias, 38205, Tenerife, Spain
Institute of Astronomy, and
Department of Applied Mathematics & Theoretical Physics
University of Cambridge, Cambridge CB3 0HA, U.K.
Lawrence Livermore National Laboratory, Livermore, CA 94550, U.S.A.
Department of Astronomy, University of Tokyo,
Bunkyo-ku, Tokyo 113, Japan
ABSTRACT
The paper contains the contributions reported at the Working Group Session `Interior Structure and Inversions'. Discussion at this session has been focused on problems of inversion analyses of current solar oscillation data and future data from the SOHO and GONG projects. New developments in helioseismological inversion techniques and in modeling physical processes in the Sun's interior have been presented.
Keywords: Sun's interior, oscillations, data inversion, equation of state,
opacity, solar models, SOHO, GONG