
Transport and Energy Conversion in the Heliosphere
Lectures Given at the CNRS Summer School on Solar Astrophysics, Oleron, France, 25-29 May 1998
Springer (Publisher)
Published on 4. October 2000
Book
Hardback
IX, 218 pages
978-3-540-67595-2 (ISBN)
Description
The book contains courses taught to a public of Ph.D. students, post-docs and confirmed researchers in all fields of heliospheric plasma physics. It aims at identifying physical issues which are common to two different fields of astronomy: solar and magnetospheric physics. Emphasis is given to basic processes of transport and conversion of energy: magnetic reconnection is discussed in detail from the viewpoints of MHD and kinetic physics. Processes of charged particle acceleration are reviewed and compared with recent observations. The subject is introduced by a summary of MHD, and the basic structures and parameters of the solar atmosphere, terrestrial ionosphere and magnetosphere are reviewed. The book combines a pedagogic and comprehensive presentation of physical issues and raises fully open questions, with the complementary and sometimes conflicting views of geophysicists and solar physicists. The book's focus, while basic, opens new avenues.
More details
Series
Language
English
Place of publication
Heidelberg
Germany
Publishing group
Springer Berlin
Target group
College/higher education
Professional and scholarly
Illustrations
64
64 s/w Abbildungen
64 black & white illustrations, biography
Dimensions
Height: 23.5 cm
Width: 15.5 cm
Weight
440 gr
ISBN-13
978-3-540-67595-2 (9783540675952)
DOI
10.1007/3-540-45166-8
Schweitzer Classification
Other editions
Additional editions

J.-P. Rozelot | L. Klein | J.-C. Vial
Transport and Energy Conversion in the Heliosphere
Lectures Given at the CNRS Summer School on Solar Astrophysics, Oleron, France, 25-29 May 1998
Book
10/2013
Springer
€53.49
Shipment within 7-9 days
Content
to MHD.- Magnetic Reconnection: Classical Aspects.- Structuring of the Solar Plasma by the Magnetic Field.- Structuring of the Magnetospheric Plasma by the Solar Terrestrial Interactions.- Self-Consistent Kinetic Approach for Low Frequency and Quasi-static Electromagnetic Perturbations in Magnetic-Mirror Confined Plasmas.