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Physical Processes in Hot Cosmic Plasmas (Paperback, Softcover reprint of the original 1st ed. 1990)
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Physical Processes in Hot Cosmic Plasmas (Paperback, Softcover reprint of the original 1st ed. 1990)
Series: NATO Science Series C, 305
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Gas at temperatures exceeding one million degrees is common in the
Universe. Indeed it is likely that most of the gas in the Universe
exists in intergalactic space in this form. Such highly-ionized
gas, or plasma, is not restricted to the rarefied densities of
intergalactic space, but is also found in clusters of galaxies, in
galaxies themselves, in the expanding remnants of exploded stars
and at higher densities in stars and the collapsed remains of stars
up to the highest densities known, which occur in neutron stars.
The abundant lower-Z elements, at least, in such gas are completely
ionized and the gas acts as a highly conducting plasma. It is
therefore subject to many cooperative phenomena, which are often
complicated and ill-understood. Many of these processes are,
however, well-studied (if not so well-understood) in laboratory
plasmas and in the near environment of the Earth. Astronomers
therefore have much to learn from plasma physicists working on
laboratory and space plasmas and the parameter range studied by the
plasma physicists might in turn be broadened by contact with
astronomers. With that in mind, a NATO Advanced Research Workshop
on Physical Processes in Hot Cosmic Plasmas was organized and took
place in the Eolian Hotel, Vulcano, Italy on May 29 to June 2 1989.
This book contains the Proceedings of that Workshop.
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