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U.S. Department of Energy
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Role of hydromagnetic waves in the magnetosphere and the ionosphere. Final report, 1 Feb 88-31 Jan 91

Technical Report ·
OSTI ID:5318811
Four research areas were investigated: (1) the propagation and coupling of hydromagnetic waves in the magnetosphere. The coupled hydromagnetic equations in the dipole model of the magnetosphere were solved numerically. A reconstruction of the long period waves in an actual geomagnetic storm was demonstrated (2) non-linear wave-particle interactions in the magnetosphere. Anomalous cross-field diffusion of trapped energetic protons may result in proton precipitation in the equatorial region; (3) the filamentation instability of large amplitude hydromagnetic waves in the solar wind plasma. This work is relevant to observations of Alven waves and magnetosonic waves in space plasmas; (4) parametric excitation of whistler waves in the high latitude ionosphere by a high frequency heater transmitting from the ground. It has been shown that whistler waves and Langmuir waves can be excited by ionospheric heaters. The instability which produces these waves offers a potential mechanism to generate large amplitude long period waves in the ionosphere.
Research Organization:
Polytechnic Inst. of New York, Brooklyn, NY (United States). Dept. of Electrical Engineering and Computer Science
OSTI ID:
5318811
Report Number(s):
AD-A-248332/9/XAB; CNN: AFOSR-88-0127
Country of Publication:
United States
Language:
English