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Coronal Expansion and Solar Wind (Paperback, Softcover reprint of the original 1st ed. 1972)
Loot Price: R1,524
Discovery Miles 15 240
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Coronal Expansion and Solar Wind (Paperback, Softcover reprint of the original 1st ed. 1972)
Series: Physics and Chemistry in Space, 5
Expected to ship within 10 - 15 working days
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Little more than ten years have passed since spaceprobe-borne
instruments con clusively demonstrated the existence of the solar
wind. These observations con firmed the basic validity of a
theoretical model, first proposed by E. N. Parker, predicting a
continuous, rapid expansion of the solar corona. The subsequent
decade has seen a tremendous growth in both the breadth and
sophistication of solar wind observations; the properties of the
interplanetary plasma near the orbit of the earth are now known in
great detail. The theory of the coronal ex pansion has also been
highly refilled both in the sense of including additional physical
processes, and of treating more realistic (time-dependent and non
spheri cally-symmetric) coronal boundary conditions. The present
volume is an attempt to synthesize the solar wind observations and
coronal expansion models from this decade of rapid development. The
ultimate goal is, of course, the interpretation of observed solar
wind phenomena as the effects of basic physical processes occurring
in the coronal and interplanetary plasma and as the natural
manifestations of solar properties and structures. This approach
implies an emphasis upon the "large-scale" features revealed by the
observations. It requires extensive use of the concepts and methods
of fluid mechanics."
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