Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

IMF B/sub y/-dependent plasma flow and Birkeland currents in the dayside magnetosphere. 1. Dynamics Explorer observations

Technical Report ·
OSTI ID:6182267
Plasma, magnetic-field, and dc electric-field observations from Dynamics Explorers 1 and 2 are used to investigate the morphology of solar-wind ion injection, Birkeland currents, and plasma convection in the morning sector for both positive and negative interplanetary magnetic field (IMF) B/sub y/ components. The results of the study are used to construct a B/sub y/-dependent global-convection model for southward IMF. A significant element of the model is the coexistence of three types of convection cells (merging cells, viscous cells, and lobe cells). This model can account for observations of a nearly stationary (in local time) convection throat, a sunward-antisunward convection reversal zone at the polar-cap boundary in both the morning and afternoon quadrants, the morphology of solar-wind ion injection and transport in the mid-altitude polar cusp, and the B/sub y/-dependent dawn-dusk asymmetry of polar-cap electron fluxes.
Research Organization:
Southwest Research Inst., San Antonio, TX (USA). Dept. of Space Sciences
OSTI ID:
6182267
Report Number(s):
AD-A-160499/0/XAB
Country of Publication:
United States
Language:
English