Ionospheric convection patterns observed during periods of steady magnetospheric convection

Details Ionospheric convection patterns observed during periods of steady magnetospheric convection Ionospheric convection patterns observed during periods of steady magnetospheric convection

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsm22a0565h&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SM22A-0565

Physics

2463 Plasma Convection, 2740 Magnetospheric Configuration And Dynamics

Scientific paper

We present a study of ionospheric convection patterns observed by the Super Dual Auroral Radar Network (SuperDARN) during two recent steady magnetospheric convection (SMC) events. Our analyses foucus on the region near the Harang discontinuity (HD) and show, in contrast to prevous SMC studies, that the HD is not an uncommon feature during SMC events. Although often observed during these events, the HD appears less extended than during a typical substorm growth phase and often forms at relatively high geomagnetic latitudes.

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