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Inflation of the Inner Magnetosphere

  • Laurence J. CahillJr.
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 10)

Abstract

Frequently, the inner magnetosphere between L = 2 and L = 6 receives a large influx of energy. In the form of large numbers of charged particles or as an increase in the particle temperature, the energy enters the magnetosphere and it weakens and distorts the magnetic field through diamagnetism and drift motions of the charged particles. Since the effect is to stretch the magnetic field lines of the earth outward, much as the surface of a balloon expands, the process is called ‘inflation’.

Keywords

Magnetic Storm Ring Current Field Magnitude Sudden Commencement Symmetrical Ring 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© D. Reidel Publishing Company, Dordrecht, Holland 1968

Authors and Affiliations

  • Laurence J. CahillJr.
    • 1
  1. 1.Space Science CenterUniversity of MinnesotaMinneapolisUSA

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