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Field-aligned currents and ionospheric electric fields in the vicinity of the dayside polar cleft: observations and simulations

Technical Report ·
OSTI ID:6481705
Correlative observations of solar-wind plasma parameters and IMF (Interplanetary Magnetic Field) from the IMP-8 satellites were studied. These data indicate that the dayside high-latitude ionospheric electric field, which drives the observed F-region plasma convection, responds within about 14 minutes to IMF variations at the magnetopause. There is also an indication that IMF fluctuations of 10 minutes or less do not produce changes in the ionospheric electric-field configuration. It has also been found that use of a very simple model of the polar cleft currents driven by solar wind electric fields is able to explain much of the temporal variations in the ionospheric plasma convection pattern observed using the Sondrestrom radar. Several areas of disagreement will require refinement of the simple model. For example, observations during intervals of northward IMF are not consistent with the simulations. Also, occasionally the convection equatorward of the cleft currents in the model is inconsistently with observations, particularly near local noon. Which suggests that the Region 1 and Region 2 currents near noon may not be modeled properly.
Research Organization:
Stanford Univ., CA (USA). Space, Telecommunications and Radioscience Lab.
OSTI ID:
6481705
Report Number(s):
AD-A-177815/8/XAB; -45
Country of Publication:
United States
Language:
English