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
- Univ. of Michigan, Ann Arbor (United States)
- NASA Marshall Space Flight Center, Huntsville, AL (United States)
- Lockheed Palo Alto Research Lab., CA (United States)
- Pacific Northwest Lab., Richland, WA (United States)
- Massachusetts Inst. of Technology, Westford (United States)
- 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
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Related Subjects
GENERAL PHYSICS
AURORAE
EMISSION
ELECTRON-ION COLLISIONS
ENERGY TRANSFER
EARTH MAGNETOSPHERE
F REGION
MAGNETOTAIL
OXYGEN IONS
PROTONS
RING CURRENTS
BARYONS
CHARGED PARTICLES
COLLISIONS
CURRENTS
EARTH ATMOSPHERE
ELECTRIC CURRENTS
ELECTRON COLLISIONS
ELEMENTARY PARTICLES
FERMIONS
HADRONS
ION COLLISIONS
IONOSPHERE
IONS
NUCLEONS
PLANETARY IONOSPHERES
661320* - Auroral
Ionospheric
& Magnetospheric Phenomena- (1992-)