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Electric field variations during substorms: OGO-6 measurementsThe OGO-6 electric field measurements make it clear that the general pattern of high latitude electric fields in magnetic time-invariant latitude coordinates is not highly variable and that when unusual variations, or field distributions, occur they are relatively isolated in time and spatial extent. Thus, electric field changes on a global scale cannot, in general, be evoked as a direct cause of substorms. Polar traverses along the 18(h) to 6(h) magnetic time meridian show that the sum of potential drops across the evening auroral belt and morning auroral belt approximately equals the potential drop across the polar cap. The integrated polar cap potential drop ranges from 20 to 100 keV and values in the center of this range are most common under conditions of moderate magnetic disturbance. Roughly near 18(h) magnetic local time, a latitudinally narrow strip at the transition between auroral belt and polar cap fields exhibits unusually large field fluctuations immediately following the sudden onset of a negative bay at later magnetic local times. It appears likely that this spatially isolated correlation is related to an effect rather than a cause of substorm enhancement.
Document ID
19720007674
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Heppner, J. P.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
September 2, 2013
Publication Date
January 1, 1972
Subject Category
Geophysics
Report/Patent Number
X-645-72-10
NASA-TM-X-65801
Report Number: X-645-72-10
Report Number: NASA-TM-X-65801
Meeting Information
Meeting: Symp. on Morphol. and Phys. of Magnetospheric Substorms, 15th IUGG Gen. Assembly
Location: Moscow
Start Date: January 1, 1971
Accession Number
72N15324
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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