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Physics of space plasma activity /

Schindler, Karl, (1931-)

Physics of space plasma activity /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	523.01
書名/作者:	Physics of space plasma activity // Karl Schindler.
作者:	Schindler, Karl,
面頁冊數:	1 online resource (xxiii, 508 pages) : : digital, PDF file(s).
附註:	Title from publisher's bibliographic system (viewed on 05 Oct 2015).
標題:	Space plasmas.
ISBN:	9780511618321 (ebook)
摘要、提要註:	Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity events observed in the solar system occur on the Sun, when coronal mass ejections expel several billion tons of plasma mass into space. This book provides a coherent and detailed treatment of the physical background of large plasma eruptions in space. It provides the background necessary for dealing with space plasma activity, and allows the reader to reach a deeper understanding of this fascinating natural event. The book employs both fluid and kinetic models, and discusses the applications to magnetospheric and solar activity. This will form an interesting reference for graduate students and academic researchers in the fields of astrophysics and plasma physics.
電子資源:	http://dx.doi.org/10.1017/CBO9780511618321

Physics of space plasma activity /
Schindler, Karl,1931-

Physics of space plasma activity /Karl Schindler. - 1 online resource (xxiii, 508 pages) :digital, PDF file(s).

Title from publisher's bibliographic system (viewed on 05 Oct 2015).

Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity events observed in the solar system occur on the Sun, when coronal mass ejections expel several billion tons of plasma mass into space. This book provides a coherent and detailed treatment of the physical background of large plasma eruptions in space. It provides the background necessary for dealing with space plasma activity, and allows the reader to reach a deeper understanding of this fascinating natural event. The book employs both fluid and kinetic models, and discusses the applications to magnetospheric and solar activity. This will form an interesting reference for graduate students and academic researchers in the fields of astrophysics and plasma physics.

ISBN: 9780511618321 (ebook)Subjects--Topical Terms:

467797
Space plasmas.

LC Class. No.: QC809.P5 / S35 2007

Dewey Class. No.: 523.01

Physics of space plasma activity /
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245 1 0 $a Physics of space plasma activity / $c Karl Schindler.
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500 $a Title from publisher's bibliographic system (viewed on 05 Oct 2015).
520 $a Space plasma is so hot that the atoms break up into charged particles which then become trapped and stored in magnetic fields. When critical conditions are reached the magnetic field breaks up, releasing a large amount of energy and causing dramatic phenomena. The largest space plasma activity events observed in the solar system occur on the Sun, when coronal mass ejections expel several billion tons of plasma mass into space. This book provides a coherent and detailed treatment of the physical background of large plasma eruptions in space. It provides the background necessary for dealing with space plasma activity, and allows the reader to reach a deeper understanding of this fascinating natural event. The book employs both fluid and kinetic models, and discusses the applications to magnetospheric and solar activity. This will form an interesting reference for graduate students and academic researchers in the fields of astrophysics and plasma physics.
650 0 $a Space plasmas. $3 467797
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856 4 0 $u http://dx.doi.org/10.1017/CBO9780511618321

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