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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.
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.
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