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Propagation Characteristics of Electromagnetic Waves in the Magnetosphere

  • D. Jones
  • R. J. L. Grard
Part of the Astrophysics and Space Science Library book series (ASSL, volume 57)

Abstract

The propagation mechanism of electromagnetic waves in the Earth’s magnetosphere and magnetotail is investigated using a ray-tracing technique. The present study makes use of macroscopic models for the magnetic-field topology and electron density distribution. The existence of the bow shock, magnetopause and plasma-pause is taken into account; the distortion of the Earth’s magnetic field by the solar wind is also included in the models. Results are presented in the form of ray paths. This study deals with the penetration of Type-III solar bursts into the magneto- sphere, the trapping of terrestrial nonthermal radiation, and the propagation of auroral kilometric radiation.

Keywords

Solar Wind Plasma Frequency Subsolar Point Auroral Kilometric Radiation Magnetosheath Plasma 
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 1976

Authors and Affiliations

  • D. Jones
    • 1
  • R. J. L. Grard
    • 1
  1. 1.Space Science DepartmentESTECNoordwijkNetherlands

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