Ebook Physics of Solar System Plasmas (Cambridge Atmospheric and Space Science Series)By Thomas E. Cravens
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Physics of Solar System Plasmas (Cambridge Atmospheric and Space Science Series)By Thomas E. Cravens
Ebook Physics of Solar System Plasmas (Cambridge Atmospheric and Space Science Series)By Thomas E. Cravens
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Physics of Solar System Plasmas provides a comprehensive introduction to the plasma physics and magnetohydrodynamics that are needed to study the solar wind and magnetosphere. The text includes a broad introduction to plasma physics, including important discussions of kinetic theory, single particle motion, magnetohydrodynamics, geomagnetically trapped energetic particles and the physics of magnetic reconnection. This leads into a thorough description of the Sun and the solar wind, and, finally, the author addresses magnetospheric physics. Among the topics covered here are magnetospheric morphology, bow shocks, magnetospheric convection and electrical currents, substorms, ionospheric physics, magnetosphere-ionosphere coupling, auroral physics and the interaction of the solar wind with the planets. Problem sets at the end of each chapter make this a useful text for advanced undergraduate students in astrophysics, geophysics, or atmospheric sciences. Graduate students and researchers will also find it a valuable source of information.
- Sales Rank: #2314137 in Books
- Brand: Brand: Cambridge University Press
- Published on: 2004-11-11
- Original language: English
- Number of items: 1
- Dimensions: 9.96" h x .98" w x 6.97" l, 1.93 pounds
- Binding: Paperback
- 496 pages
- Used Book in Good Condition
Review
"This is a well-written introduction to the physics of the solar wind and planetary magnetospheres. Some diverse problems are provided at the end of each chapter. ...this is a good textbook for advanced undergraduate students. Graduate students and researchers will enjoy it as a nice introduction to these fascinating fields." Maarten van Aalst, Space Science Review
About the Author
Tom Cravens is Professor of Physics and Astronomy at the University of Kansas. With more than 200 published papers, he has investigated the sources of X-rays throughout the Solar System as well as the upper atmospheres and ionospheres of most Solar System planets and satellites, including Titan. A fellow of the American Geophysical Union, he is a team member of the Cassini Ion and Neutral Mass Spectrometer and author of the Cambridge University Press textbook Physics of Solar System Plasmas (1997).
Sir John Houghton CBE, FRS is a former Chairman of the Scientific Assessment Working Group of the Intergovernmental Panel on Climate Change, Chairman of the UK's Royal Commission on Environmental Pollution, Vice President of the World Meteorological Organisation, President of the Royal Meteorological Society, and Professor of Atmospheric Physics at Oxford University. He was Chief Executive of the UK Meteorological Office from 1983 to his retirement in 1991. As well as the previous editions of this book, he is author of The Physics of Atmospheres (Cambridge University Press, in three editions), and has published numerous research papers and contributed to many influential research documents.
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