Remote observations of the Auroral Acceleration Region (Invited)

Details Remote observations of the Auroral Acceleration Region (Invited) Remote observations of the Auroral Acceleration Region (Invited)

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm51d..04f&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM51D-04

Physics

[2407] Ionosphere / Auroral Ionosphere, [2431] Ionosphere / Ionosphere/Magnetosphere Interactions, [2704] Magnetospheric Physics / Auroral Phenomena, [2730] Magnetospheric Physics / Magnetosphere: Inner

Scientific paper

The Auroral Acceleration Region (AAR) is the key region of transfer of electromagnetic energy to particle kinetic energy. It is thus important for the dynamic coupling between the magnetosphere as the energy reservoir and the ionosphere as the energy sink. Comprehensive knowledge about the AAR can be obtained by multi-point in-situ measurements but still the whole connection between the magnetosphere, the AAR, and the ionosphere can only be investigated by multi-point in-situ and remote observations. We will discuss several opportunities of combined measurements with Cluster/IMAGE, with THEMIS/Reimei/ground-observations, and THEMIS/FAST/ground-observations and the insight that was obtained by these investigations about the AAR and the M-I-coupling.

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