Plasma convection in the magnetosphere and the SuperDARN network

Details Plasma convection in the magnetosphere and the SuperDARN network Plasma convection in the magnetosphere and the SuperDARN network

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..131c&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

The SuperDARN (Dual Auroral Radar Network) coherent HF radars monitor the large-scale ionospheric convection from the Doppler shift affecting the signal coherently backscattered by electron density irregularities frozen in the ionospheric plasma. A network of 15 radars with a field of view covering the northern and southern auroral zones and polar caps provides in real time a global view of the response of the magnetosphere to variations of the parameters of the interplanetary medium. The principle of the radars and their diagnostic potential are reviewed.

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