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Reconnection of magnetic fields : magnetohydrodynamics and collisionless theory and observations / edited by J. Birn and E.R. Priest.

Contributor(s): Material type: TextTextPublication details: Cambridge : Cambridge University Press, ©2007.Description: 1 online resource (xii, 342 pages, 8 unnumbered pages of plates) : illustrations (some color)Content type:
  • text
Media type:
  • computer
Carrier type:
  • online resource
ISBN:
  • 9780511261213
  • 0511261217
  • 0511258097
  • 9780511258091
  • 0511259395
  • 9780511259395
  • 0511260040
  • 9780511260049
  • 0511260644
  • 9780511260643
  • 9780511536151
  • 0511536151
  • 1280749229
  • 9781280749223
Subject(s): Genre/Form: Additional physical formats: Print version:: Reconnection of magnetic fields.DDC classification:
  • 538.6 22
LOC classification:
  • QC809.M3 R43 2007eb
Online resources:
Contents:
Cover; Half-title; Title; Copyright; Contents; Contributors; Preface; Acknowledgments; 1 Introduction; 2 Basic theory of MHD reconnection; 3 Basic theory of collisionless reconnection; 4 Reconnection in the magnetosphere; 5 Reconnection in the Sun's atmosphere; Definition of specific notations; References; Index.
Summary: The reconnection of magnetic fields is one of the most fascinating processes in plasma physics, responsible for phenomena such as solar flares and magnetospheric substorms. The concept of reconnection has developed through recent advances in exploring the magnetospheres of the Sun and Earth through theory, computer simulations and spacecraft observations. The great challenge in understanding it stems from balancing the large volumes of plasma and magnetic fields involved with the energy release with the physical mechanism which relies on the strongly localized behavior of charged particles. This book, edited by and with contributions from leading scientists in the field, provides a comprehensive overview of recent theoretical and observational findings concerning the physics of reconnection and the complex structures that may give rise to, or develop from, reconnection. It is intended for researchers and graduate students interested in the dynamics of plasmas.
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Electronic-Books Electronic-Books OPJGU Sonepat- Campus E-Books EBSCO Available

Includes bibliographical references and index.

Cover; Half-title; Title; Copyright; Contents; Contributors; Preface; Acknowledgments; 1 Introduction; 2 Basic theory of MHD reconnection; 3 Basic theory of collisionless reconnection; 4 Reconnection in the magnetosphere; 5 Reconnection in the Sun's atmosphere; Definition of specific notations; References; Index.

Print version record.

The reconnection of magnetic fields is one of the most fascinating processes in plasma physics, responsible for phenomena such as solar flares and magnetospheric substorms. The concept of reconnection has developed through recent advances in exploring the magnetospheres of the Sun and Earth through theory, computer simulations and spacecraft observations. The great challenge in understanding it stems from balancing the large volumes of plasma and magnetic fields involved with the energy release with the physical mechanism which relies on the strongly localized behavior of charged particles. This book, edited by and with contributions from leading scientists in the field, provides a comprehensive overview of recent theoretical and observational findings concerning the physics of reconnection and the complex structures that may give rise to, or develop from, reconnection. It is intended for researchers and graduate students interested in the dynamics of plasmas.

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