Understanding how the Sun changes though its 11-year sunspot cycle and
how these changes affect the vast space around the Sun - the
heliosphere - has been one of the principal objectives of space research
since the advent of the space age. This book presents the evolution of
the heliosphere through an entire solar activity cycle. The last solar
cycle (cycle 23) has been the best observed from both the Earth and from
a fleet of spacecraft. Of these, the joint ESA-NASA Ulysses probe has
provided continuous observations of the state of the heliosphere since
1990 from a unique vantage point, that of a nearly polar orbit around
the Sun. Ulysses' results affect our understanding of the heliosphere
from the interior of the Sun to the interstellar medium - beyond the
outer boundary of the heliosphere. Written by scientists closely
associated with the Ulysses mission, the book describes and explains the
many different aspects of changes in the heliosphere in response to
solar activity. In particular, the authors describe the rise in solar
activity from the last minimum in solar activity in 1996 to its maximum
in 2000 and the subsequent decline in activity.