Solar science has evolved rapidly over the past ten years as the
results of a new generation of solar space missions have become
available. This book provides a thorough introduction to the
subject of solar physics, based on those spacecraft observations.
The author introduces the solar corona, which has a temperature of
several million degrees, and sets it in the context of basic plasma
physics before moving on to discuss plasma instabilities and plasma
heating processes. The latest results on coronal heating and
radiation, which are fundamental processes in all stars, are
presented. Spectacular phenomena such as solar flares and coronal
mass ejections are described in detail, together with their
potential effects on the Earth. The author draws together
observations made at many wavelengths from hard X-rays, soft
X-rays, extreme UV and radio wavelengths.
This paperback study edition of Markus Aschwanden s highly
acclaimed Physics of the Solar Corona will include 50 pages of
problems and solutions which will much enhance the value of the
book to students."
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