Development of Magnetospheric Physics

  1. Joseph R. Kan,
  2. Thomas A. Potemra,
  3. Susumu Kokubun and
  4. Takesi Iijima
  1. S.-I. Akasofu

Published Online: 19 MAR 2013

DOI: 10.1029/GM064p0003

Magnetospheric Substorms

Magnetospheric Substorms

How to Cite

Akasofu, S.-I. (1991) Development of Magnetospheric Physics, in Magnetospheric Substorms (eds J. R. Kan, T. A. Potemra, S. Kokubun and T. Iijima), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM064p0003

Author Information

  1. Geophysical Institute, University of Alaska Fairbanks, Fairbanks, Alaska 99775–0800

Publication History

  1. Published Online: 19 MAR 2013
  2. Published Print: 1 JAN 1991

ISBN Information

Print ISBN: 9780875900308

Online ISBN: 9781118663981

SEARCH

Keywords:

  • Magnetospheric substorms—Congresses

Summary

Magnetospheric physics has grown out of classical disciplines, such as geomagnetism, auroral physics, ionospheric physics and cosmic ray physics after 1958 and has had a fascinating history of development. The purpose of this paper is to furnish the general background for those that follow by describing briefly the historical development. It is emphasized that magnetospheric physics and a study of magnetospheric substorms are still in the developmental stage. A new instrumental development, a new analytical finding or a new theoretical progress could lead this discipline to a new era of development far beyond the present generation can conceive of at this time. Many basic processes we reveal in this discipline may be applicable to solar, stellar and interstellar phenomena.