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Dayside auroral activity and magnetic flux transfer from the solar wind

Journal Article · · Geophysical Research Letters (American Geophysical Union); (USA)
 [1];  [2];  [3]
  1. Rutherford Appleton Laboratory, Chilton (England)
  2. Univ. of Oslo (Norway)
  3. Imperial College, London (England)
Combined observations by meridian-scanning photometers and the EISCAT radar show that the midday-auroral breakup phenomenon is associated with major increases in ionospheric flow. A sequence of nine events is observed in the early afternoon MLT sector during a period when the IMF is strongly southward with a large positive B{sub y} component. Each auroral structure is seen at both 630 and 557.7nm and initially moves westward, accompanied by an increase in potential of 30-60kV across the north-south dimension of the EISCAT field-of-view. After a few minutes the arc (or arc fragment) moves into the polar cap and fades, and the velocities observed by the radar swing from westward toward northward. The authors conclude that dayside auroral breakup is closely associated with momentum transfer across the magnetopause which occurs in a series of events 5-15 minutes apart. The largest of the observed events has dimensions of about 300km (in the direction of westward motion) by 700km, is bounded on its poleward edge by a 5kR arc and is associated with a potential of at least 80kV.
OSTI ID:
5716571
Journal Information:
Geophysical Research Letters (American Geophysical Union); (USA), Journal Name: Geophysical Research Letters (American Geophysical Union); (USA) Vol. 16:1; ISSN 0094-8276; ISSN GPRLA
Country of Publication:
United States
Language:
English

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