Electron fluxes and correlations with quiet-time auroral arcs. Interim report
Technical Report
·
OSTI ID:7184401
Primary electron fluxes, measured by two satellites as they crossed quiet-time auroral arcs, are presented for times near 14:20 UT on Nov 12, 1972. The DMSP-30 satellite measured the optical intensity at 0.6 to 1.0 Micrometer (FWHM) and precipitated electrons with 0.22 = or < E = or < 19.7 keV near 2100 MLT. The 72-1 satellite crossed the auroral arc system near 2200 MLT and measured 0.36- to 16.5-keV electrons at all pitch angles. A detailed description of the electron morphology that includes comparisons of electron fluxes with optical intensities is presented. (GRA)
- Research Organization:
- Aerospace Corp., El Segundo, Calif. (USA). Space Physics Lab.
- OSTI ID:
- 7184401
- Report Number(s):
- AD-A-013690/3ST
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640201* -- Atmospheric Physics-- Auroral
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANISOTROPY
AURORAE
CHARGED-PARTICLE PRECIPITATION
CORRELATIONS
DISTURBANCES
EARTH ATMOSPHERE
ELECTRON DENSITY
ELECTRON PRECIPITATION
ELECTRONS
ELEMENTARY PARTICLES
ENERGY
ENERGY RANGE
EV RANGE
EV RANGE 100-1000
FERMIONS
IONOSPHERE
KEV RANGE
KEV RANGE 01-10
KEV RANGE 10-100
LEPTONS
MAGNETIC FIELDS
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ANISOTROPY
AURORAE
CHARGED-PARTICLE PRECIPITATION
CORRELATIONS
DISTURBANCES
EARTH ATMOSPHERE
ELECTRON DENSITY
ELECTRON PRECIPITATION
ELECTRONS
ELEMENTARY PARTICLES
ENERGY
ENERGY RANGE
EV RANGE
EV RANGE 100-1000
FERMIONS
IONOSPHERE
KEV RANGE
KEV RANGE 01-10
KEV RANGE 10-100
LEPTONS
MAGNETIC FIELDS