Dayside auroral dynamics

Details Dayside auroral dynamics Dayside auroral dynamics

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.1695e&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, March 1, 1984, p. 1695-1700.

Physics

25

Auroras, Daytime, Plasma Dynamics, Cameras, Electron Precipitation, Geomagnetism, Kp Index, Picosecond Pulses

Scientific paper

Keogram cameras operated at the South Pole during 1980 and 1981 have monitored the position, intensity, color, and dynamic behavior of the dayside aurora. The position of the midday aurora for very quiet magnetic conditions is some 5 deg further poleward than was previously recognized. The average energy of dayside electron precipitation (approximately 100 eV) does not change as magnetic activity increases. Rapid latitudinal movements of discrete dayside aurora structures and pulsating structures with Pc 5 periodicities are regularly observed and have no obvious explanation in terms of interplanetary field conditions.

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