Supporting evidence of micro-nonequilibrium on the simulated magnetopause - Further predictions and suggestions

Details Supporting evidence of micro-nonequilibrium on the simulated magnetopause - Further predictions and suggestions Supporting evidence of micro-nonequilibrium on the simulated magnetopause - Further predictions and suggestions

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988angeo...6..305w&link_type=abstract

Annales Geophysicae (ISSN 0980-8752), vol. 6, June 1988, p. 305-308.

Physics

Atmospheric Models, Daytime, Magnetopause, Solar Terrestrial Interactions, Diurnal Variations, Interplanetary Magnetic Fields, Solar Simulation, Solar Wind

Scientific paper

A laboratory experiment, performed in 1966 by Kawashima and Mori, suggests the existence of a micro-nonequilibrium on the dawn-side of the magnetopause. This magnetosphere-solar wind simulation indicates that the plasma intrudes into the simulated magnetosphere via the morning side of the magnetopause. This has been predicted by a micro-nonequilibrium theory. More predictions and suggestions are made to accommodate further laboratory tests on the micro-nonequilibrium theory.

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