Magnetospheric substorms - A newly emerging model

Details Magnetospheric substorms - A newly emerging model Magnetospheric substorms - A newly emerging model

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981p%26ss...29.1069a&link_type=abstract

Planetary and Space Science, vol. 29, Oct. 1981, p. 1069-1078.

Physics

16

Auroras, Geomagnetism, Ionospheric Currents, Magnetic Storms, Magnetospheric Instability, Solar Terrestrial Interactions, Auroral Arcs, Electric Potential, Energy Dissipation, Geomagnetic Tail, Polar Regions, Solar Activity Effects, Solar Wind

Scientific paper

A surge of progress in magnetospheric substorm studies is expected by the following three recent developments: (1) the finding of the solar wind-magnetosphere energy coupling function epsilon, (2) the determination of the Pedersen current distribution over the entire polar region, and (3) a new understanding of the auroral potential structure. In this paper, the significance of the three developments and the newly emerging model of magnetospheric substorms is described.

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