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Field-aligned currents associated with substorms in the vicinity of synchronous orbit. 1. The July 5, 1979, substorm observed by SCATHA, GOES 3, and GOES 2

Journal Article · · Journal of Geophysical Research; (United States)
 [1];  [2];  [3];  [4]
  1. Meteorological Research Inst., Ibaraki (Japan)
  2. Air Force Geophysics Lab., Hanscom AFB, MA (United States)
  3. NASA Goddard Space Flight Center, Greenbelt, MD (United States)
  4. Univ. of Alabama, Huntsville (United States)
Magnetic field topology and field-aligned current signatures in the vicinity of synchronous orbit are examined for a substorm on July 5, 1979. Changes from taillike to dipolar field geometry propagate earthward near the midnight meridian during the substorm. The major field-aligned currents producing a negative D perturbation at and around synchronous orbit are downward currents flowing into the auroral ionosphere on L shells greater than the synchronous spacecraft L shell. Although these currents are located initially on higher L shells, they shift toward the lower L shells as the change from taillike to dipolar fields propagates earthward. There may exist upward field-aligned currents located on smaller L shells in the limited longitudinal region near the meridian where mid-latitude D perturbations change their sign.
OSTI ID:
5596693
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