How does magnetospheric convection relate to the expansion onset of substorms?

Details How does magnetospheric convection relate to the expansion onset of substorms? How does magnetospheric convection relate to the expansion onset of substorms?

Jun 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993jatp...55.1151a&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 55, no. 8, p. 1151-1157.

Physics

4

Convection, Earth Magnetosphere, Magnetic Storms, Magnetospheric Instability, Solar Wind, Auroral Electrojets, Interplanetary Magnetic Fields, Solar Terrestrial Interactions, Steady State

Scientific paper

Magnetospheric convection during the growth stage of isolated substorms is examined to determine conditions leading to instabilities associated with substorm expansions. Persistent patterns of two-celled convection for southward interplanetary magnetic field are discussed in terms of their intensity and scale size. The time derivatives of these patterns are examined, and a typical behavior in the period just before the onset of substorm expansion is discussed.

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