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Theory of the Jovian Radiation Belts

  • F. M. Neubauer
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 44)

Abstract

The present picture of the Jovian radiation belts and magnetosphere is based on radioastronomical observations, i.e., the observations of decametric and decimetric emissions and theoretical concepts, most of which were developed for the terrestrial magnetosphere. Since the terrestrial magnetosphere and radiation belts are far from being understood, a number of surprises can be expected from space missions to Jupiter on Pioneer 10 and 11 and Mariner-Jupiter-Saturn 1977.

Keywords

Solar Wind Radial Diffusion Radiation Belt Loss Cone Cutoff Rigidity 
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 1974

Authors and Affiliations

  • F. M. Neubauer
    • 1
  1. 1.Institut für Geophysik und MeteorologieTechnische UniversitätBraunschweigGermany

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