Time scales of expansion and contraction of the auroral oval
Technical Report
·
OSTI ID:5175064
The auroral boundary index calculated on the basis of Defense Meteorological Satellite Program precipitating-electron data is used to examine the dynamics of the auroral oval in the midnight sector. The equatorward boundary of the oval expands equatorward and contracts poleward corresponding to southward and northward turnings, respectively, of the interplanetary magnetic field (IMF). The time scales are found to be on the average, 45 min for the expansion and 8 hours for the contraction. A general empirical formula to predict the oval location for any IMF variation is devised. Physical processes in the magnetosphere consistent with the rapid expansion and slow contraction of the auroral oval are discussed.
- Research Organization:
- Air Force Geophysics Lab., Hanscom AFB, MA (USA)
- OSTI ID:
- 5175064
- Report Number(s):
- AD-A-169410/8/XAB; AFGL-TR-86-0130
- 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
AURORAE
AURORAL OVAL
CHARGED-PARTICLE PRECIPITATION
DYNAMICS
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
ELECTRON PRECIPITATION
INTERPLANETARY SPACE
MAGNETIC FIELDS
MECHANICS
SPACE
Ionospheric
& Magetospheric Phenomena
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
AURORAE
AURORAL OVAL
CHARGED-PARTICLE PRECIPITATION
DYNAMICS
EARTH ATMOSPHERE
EARTH MAGNETOSPHERE
ELECTRON PRECIPITATION
INTERPLANETARY SPACE
MAGNETIC FIELDS
MECHANICS
SPACE