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A comparison of magnetic signatures and DMSP auroral images at substorm onset: Three case studies

Journal Article · · Journal of Geophysical Research; (United States)
;  [1];  [2]
  1. Boston Univ., MA (United States)
  2. Air Force Geophysics Lab., Hanscom AFB, MA (United States)
The authors explore the relationship between mid-latitude and synchronous orbit magnetic signatures and the location of the auroral surge at the onset of three isolated magnetospheric substorms. Mid-latitude data come from the Air Force Geophysics Laboratory Magnetometer Network, synchronous orbit data form the satellites GOES 2 and 3, and auroral data from Defense Meteorological Satellite Program auroral images and auroral magnetograms. They find that the surge forms with its western edge {approximately} 1 hour west of the longitude where the major axis of the mid-latitude Pi 2 polarization ellipse is along magnetic north and where the D component perturbation of the magnetic bay is near zero. These observations are in qualitative agreement with a current wedge consisting of a localized upward current in the west and a longitudinally distributed current in the east. At synchronous orbit the longitude of the surge head appears to separate a region to the west where the magnetic field becomes more taillike from one to the east where the magnetic field becomes more dipolar.
OSTI ID:
5510682
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 92:A3; ISSN 0148-0227; ISSN JGREA
Country of Publication:
United States
Language:
English