skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: The role of ring current nose events in producing stable auroral red arc intensifications during the main phase: Observations during the September 19--24, 1984, equinox transition study

Journal Article · · Journal of Geophysical Research; (United States)
DOI:https://doi.org/10.1029/92JA02554· OSTI ID:6200401
 [1];  [2]; ;  [3];  [4];  [5];  [6]
  1. Univ. of Michigan, Ann Arbor (United States)
  2. NASA Marshall Space Flight Center, Huntsville, AL (United States)
  3. Lockheed Palo Alto Research Lab., CA (United States)
  4. Pacific Northwest Lab., Richland, WA (United States)
  5. Massachusetts Inst. of Technology, Westford (United States)
  6. Phillips Lab., Hanscom AFB, MA (United States)

This article reports on a study of the characteristics of stable auroral red (SAR) arcs. These arcs are characterized by 6300-[angstrom] emission which normally appears near F region heights. In particular the authors study observations made in September, 1984. These studies showed that oxygen ion collisions in the ring current were responsible for the recovery phase enhancement of the SAR. Satellite observations showed and enhanced 15 to 25 keV proton component in the ring current during the main phase of the SAR which is responsible for the enhancement during this phase of the event. This enhanced high energy proton flux appears to have come from ion injection into the inner magnetosphere in response to an abrupt change in the electric field across the magnetotail.

DOE Contract Number:
AC06-76RL01830
OSTI ID:
6200401
Journal Information:
Journal of Geophysical Research; (United States), Vol. 98:A6; ISSN 0148-0227
Country of Publication:
United States
Language:
English