Consequences of hydromagnetic waves on magnetospheric particle dynamics

Details Consequences of hydromagnetic waves on magnetospheric particle dynamics Consequences of hydromagnetic waves on magnetospheric particle dynamics

Oct 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...42..515g&link_type=abstract

(URSI, USAF, NASA, et al., International School for Space Simulations, 2nd, Kapaa, HI, Feb. 4-15, 1985) Space Science Reviews (I

Physics

5

Magnetohydrodynamic Waves, Magnetospheric Instability, Plasma-Particle Interactions, Space Plasmas, Geomagnetic Pulsations, Ion Cyclotron Radiation, Magnetoelastic Waves, Particle Acceleration, Power Spectra, Very Low Frequencies

Scientific paper

Wave particle interactions which involve electromagnetic ultra low frequency (ULF) waves in the equatorial region of the magnetosphere are studied. The three-dimensional structure and origin of long period pulsations (3-50 mHz, Pc-3,4,5) are analyzed. The properties of 1-10 Hz magnetosonic waves are described; these emissions correlate with features of the energetic particle population. The linear amplification, quasi-linear diffusion, generation of suprathermal electrons, and nonresonant acceleration of the ion cyclotron waves (0.1-2 Hz, Pc-1,2) are investigated. The propagation characteristics and generation mechanism for Jovian ULF emissions in the Io torus region are examined.

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