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On the Isotropic Hydromagnetic Waves in the Exosphere

Journal Article · · Journal of Geomagnetism and Geoelectricity (Tokyo)
DOI:https://doi.org/10.5636/jgg.14.49· OSTI ID:4782644
The propagation of weak hydromagnetic waves in the exosphere between l x 103 and 5 x 104 km height levels from the Earth's surface is studied, using simplified models. In the upper atmosphere, the steady magnetic field is a dipole one, and it is, in general, difficult to discuss the wave propagation in such a field. But, in some special regions, an approximate treatment can be permitted. An attempt is made to describe two-dimensional wave fronts in the regions near the geomagnetic equatorial plane and high above the geomagnetic pole, using an approximate height-variation of the Alfven wave velocity, and it is found that: (1) For the isotropic wave, the shape of wave fronts is the same for both the equatorial and the polar regions. (2) In the upper region above Va (Alfven wave velocity) maximum height level, the incident waves with large pitch angle to the zenith are almost reflected, but in the region below Va maximum height level, the incident waves with any pitch angle have tendency to propagate almost Earthward. Equations for the drift velocity and rate of heating of each component of an ohmically heated multicomponent plasma are derived using the Fokker-Planck equation. The results are applied to a plasma containing two types of positive ion.
Research Organization:
Kyoto Univ.
Sponsoring Organization:
USDOE
NSA Number:
NSA-17-002378
OSTI ID:
4782644
Journal Information:
Journal of Geomagnetism and Geoelectricity (Tokyo), Journal Name: Journal of Geomagnetism and Geoelectricity (Tokyo) Journal Issue: 1 Vol. 14; ISSN 0022-1392
Country of Publication:
Country unknown/Code not available
Language:
English

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