Interplanetary magnetohydrodynamics
Author(s)
Bibliographic Information
Interplanetary magnetohydrodynamics
(International series on astronomy and astrophysics, 3)
Oxford University Press, 1995
Available at 15 libraries
  Aomori
  Iwate
  Miyagi
  Akita
  Yamagata
  Fukushima
  Ibaraki
  Tochigi
  Gunma
  Saitama
  Chiba
  Tokyo
  Kanagawa
  Niigata
  Toyama
  Ishikawa
  Fukui
  Yamanashi
  Nagano
  Gifu
  Shizuoka
  Aichi
  Mie
  Shiga
  Kyoto
  Osaka
  Hyogo
  Nara
  Wakayama
  Tottori
  Shimane
  Okayama
  Hiroshima
  Yamaguchi
  Tokushima
  Kagawa
  Ehime
  Kochi
  Fukuoka
  Saga
  Nagasaki
  Kumamoto
  Oita
  Miyazaki
  Kagoshima
  Okinawa
  Korea
  China
  Thailand
  United Kingdom
  Germany
  Switzerland
  France
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  United States of America
Note
Includes bibliographical references and indexes
Description and Table of Contents
Description
Spacecraft have explored the interplanetary medium between the orbits of Mercury and Pluto, revealing the exotic and beautiful nature of the environment of our planet and sun. This book summarizes the principle results of these historic expeditions. Magnetohydrodynamics provides the framework for interpreting the observations, and the observations have greatly enriched the subject of magnetohydrodynamics. Numerous figures in the book illustrate the essential
observations and fundamental concepts. Simple equations summarize basic physical and phenomenological relations observed in the interplanetary medium. Fundamental objects observed in the interplanetary medium include various types of MHD shocks, tangenital and rotational discontinuities, and force-free field
configurations. Fundamental processes observed in the interplanetary medium include the interaction among shocks (which can be classified using catastrophic theory), the formation of merged interaction region regions associated with various types of flows, the destruction of flows, the growth of the Kelvin-Helmholtz instability and formation of a heliospheric vortex street, the development of multifractal fluctuations on various scales, and the evolution of multifractal intermittent turbulence.
These physical objects and processes are of fundamental interest in themselves. The knowledge about them derived from interplanetary investigations has applications to magnetospheric physics, solar physics, cosmic ray physics and astrophysics. The book contains an extensive set of reference that
gives the readers access to the detailed results in the literature.
Table of Contents
- Introduction
- 1. Large-Scale Magnetic Field
- 2. Large-Scale Plasma
- 3. Pressure Balanced Structures
- 4. Shocks
- 5. Magneic Clouds and Force-Free Magnetic Fields
- 6. Corotating Streams and Interaction Regions
- 7. Merged Interaction Regions
- 8. Large-Scale Fluctuations
- 9. Heliospheric Vortex Street
by "Nielsen BookData"