Physics
Scientific paper
Aug 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17.1251c&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 17, Aug. 1990, p. 1251-1254.
Physics
2
Auroral Zones, Auroras, Earth Ionosphere, Earth Magnetosphere, Electron Precipitation, Magnetic Disturbances, Magnetic Fields, Pulsed Radiation
Scientific paper
This paper reports the significant occurrence of pulsating auroras in the high-latitude post-noon auroral oval. Observations of auroras at Davis, Antarctica during the 1988 austral winter indicate pulsating auroral activity peaks at around 14.5 percent in the period 1330-1400 MLT. Postnoon high latitude pulsating aurora is typically a less than 250 R enhancement on a 1 kR background in the O I emission at 558 nm. Pulsation periods tend to be longer at 20-30 s compared to average auroral zone fluctuations of around 2-10 s. Similar to auroral zone stations, the optical fluctuations are always accompanied by Pi(c) magnetic pulsations. Weak Kp and IMF trends are present.
Burns Gary B.
Craven Matthew
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