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These proceedings bring together ideas from solar and stellar
physics. The sun is near enough for rather detailed observations
and one chapter is devoted to the more recent experimental data
from observations from space. On the other hand the multitude of
stars provides a wide range of physical parameters to test
hypotheses in solar and stellar astrophysics. The reader will find
an illuminating overview of these fields ranging from the dynamo in
the convection zone to the stellar envelopes and winds in the outer
regions. In particular the importance of small-scale
magnetohydrodynamic processes for the activity phenomena plays an
important role in the contributions to this volume. For both
students and researchers the general introduction by N. O. Weiss
makes an excellent guide to this very active field of research.
(See also Lecture Notes in Physics Vol. 291.)
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