Magnetospheric cavity modes and field-line resonances - The effect of radial mass density variation

Details Magnetospheric cavity modes and field-line resonances - The effect of radial mass density variation Magnetospheric cavity modes and field-line resonances - The effect of radial mass density variation

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989p%26ss...37..407a&link_type=abstract

Planetary and Space Science (ISSN 0032-0633), vol. 37, April 1989, p. 407-418.

Mathematics

12

Magnetohydrodynamic Waves, Magnetospheric Electron Density, Plasma Density, Resonance Lines, Mathematical Models, Plasmapause

Scientific paper

A numerical wave coupling model is presented to study the relationship between magnetospheric cavity modes and field-line resonances (FLRs) as a function of the radial plasma mass density distribution in the dayside magnetosphere. It is found that the afternoon sector of MLT is the most favorable time to detect cavity-mode driven FLRs and that FLRs observed at high magnetic latitudes are not driven by global cavity modes. The maximum damping of the fundamental cavity mode by coupling to a FLR is determined and the consequences of including a small plasmapause in the model are discussed.

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