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Detailed Reference Information |
Uberoi, C. (1988). The Alfvén wave equation for magnetospheric plasmas. Journal of Geophysical Research 93: doi: 10.1029/88JA01029. issn: 0148-0227. |
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It is shown that besides the continuous spectrum which damps away as inverse power of time, the coupled Alfv¿n wave equation, which gives coupling between a shear Alfv¿n wave and a surface wave, can also admit a well behaved harmonic solution in the closed form for a set of initial conditions. This solution, though valid for finite time intervals, points out that the Alfv¿n surface waves can have a band of frequency (instead of a monochromatic frequency for a nonsheared magnetic field) within which the local field line resonance frequency can lie, and thus can excite magnetic pulsations with latitude-dependent frequency. By considering magnetic fields not only varying in magnitude but also in direction, it is shown that the time interval for the validity of the harmonic solution depend upon the angle between the magnetic field directions on either side of the magnetopause. For small values of the angle the time interval can become appreciably large. ¿ American Geophysical Union 1988 |
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BACKGROUND DATA FILES |
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Abstract |
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Keywords
Magnetospheric Physics, MHD waves and instabilities, Magnetospheric Physics, Magnetopause, cusp, and boundary layers, Magnetospheric Physics, Planetary magnetospheres, Magnetospheric Physics, Plasma waves and instabilities |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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