Response of the auroral oval precipitation and magnetospheric convection to changes in the interplanetary magnetic field

Details Response of the auroral oval precipitation and magnetospheric convection to changes in the interplanetary magnetic field Response of the auroral oval precipitation and magnetospheric convection to changes in the interplanetary magnetic field

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987angeo...5..519d&link_type=abstract

(URSI and High Altitude Observatory, International Symposium on Large-Scale Processes in the Ionospheric-Thermospheric System, B

Physics

1

Auroral Zones, Interplanetary Magnetic Fields, Particle Precipitation, Plasma Dynamics, Polar Substorms, Solar Wind, Boundary Layer Plasmas, Convection, Energy Dissipation, Polar Caps, Satellite Observation

Scientific paper

High-latitude observations on January 18, 1984 during the first GISMOS campaign are examined. An intense substorm occurred after a long period of quiescent geomagnetic activity when the IMF decreased gradually over a 2-hour period from +5 to -8 nT. This present study investigates how the auroral precipitation boundary, the energy flux, and the convection respond to this change from quiet to active conditions.

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