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Detailed Reference Information |
Laakso, H. and Junginger, H. (1990). Magnetosonic waves above fc(H+) at geostationary orbit: GEOS 2 results. Journal of Geophysical Research 95: doi: 10.1029/90JA00286. issn: 0148-0227. |
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The fast magnetosonic waves in the frequency range 1--11 Hz (i.e., above the proton gyrofrequency &OHgr;p) are considered. The electric wave field ΔE (mostly less than 0.5 mV/m) has an elliptic polarization in the plane perpendicular to B. While the magnetic wave field ΔB is strictly polarized along the ambient magnetic field, the ellipticity and the sense of rotation of the electric field polarization ellipses are crucial parameters for the identification of the wave mode. The waves are right-hand polarized, and the ellipticity is usually 0.2. The main axis of the ellipse is close to the azimuthal direction. The wave vector k is almost parallel to ΔE, and thus the fast magnetosonic waves propagate at small angles to the azimuthal direction. The wavelength are usually between 150 and 300 km. The ΔE/ΔB ratio of the waves is between vA and vA(1+&ohgr;2/&OHgr;p2)1/2, where vA is the Alfv¿n velocity. In one case a burst of pure electrostatic modes near the second harmonic of the proton gyrofrequency was observed. ¿ American Geophysical Union 1990 |
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Abstract |
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Keywords
Interplanetary Physics, Cosmic rays, Interplanetary Physics, MHD waves and turbulence, Solar Physics, Astrophysics, and Astronomy, Energetic particles, Space Plasma Physics, Charged particle motion and acceleration |
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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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