Computer Science
Scientific paper
Oct 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ssrv...42..399c&link_type=abstract
(URSI, USAF, NASA, et al., International School for Space Simulations, 2nd, Kapaa, HI, Feb. 4-15, 1985) Space Science Reviews (I
Computer Science
48
Dissipation, Earth Magnetosphere, Plasma Diffusion, Space Plasmas, Collisionless Plasmas, Electric Current, Field Aligned Currents, Magnetic Field Reconnection, Particle Precipitation, Plasma Waves, Shock Waves
Scientific paper
A prevalent approach to understanding magnetospheric dynamics is to combine a hydromagnetic description of the large scale magnetic structure and convection flows with a locally determined anomalous dissipation which develops in boundary layers. Three problems (nose and tail reconnection, auroral field-aligned currents, and diffuse auroral precipitation) are critically examined to test the validity of this theoretical philosophy. Although the expected plasma wave turbulence is observed for each case, the concept of local anomalous dissipation fails to provide an adequate or complete description of the phenomenae.
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