Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apro16002v&link_type=abstract
American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As
Astronomy and Astrophysics
Astrophysics
Scientific paper
We theoretically describe the complex media of the ionospheric resonance system in which we consider longitudinal as well as transverse components of electric and magnetic fields resulting from natural and man-made sources of excitation. The properties of the ionosphere, as a cool, ionized medium, can sustain plasmon and ion acoustic excitation modes, which appear to explain certain of its unique observed properties. These properties involve collective, coherent resonant states that are sustained over long propagation distances and also over relatively long temporal periods with low dispersive losses. Long range and relatively long-lived shock excitation modes are examined which produced by natural and/or man-made phenomena, such as solar flare and other activity.(1) Characteristic frequencies of resonant excitation of the ionospheric layers have been characterized, and we also calculate the speed of some of the unique velocities of signal propagations in these specific ionospheric layers. The characteristics of the micro pulsations in the magnetosphere are also characterized. (1) E.A. Rauscher and W.L Van Bise, Bull. Am. Phys. Soc. EB01, 1300(2002)
Rauscher Elizabeth A.
van Bise W. L.
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