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

Parabolic heavy ion flow in the polar magnetosphere

Journal Article · · Journal of Geophysical Research; (United States)
 [1]
  1. Univ. of Alabama, Huntsville (United States)
Recent observations by the Dynamics Explorer 1 satellite over the dayside polar cap magnetosphere have indicated downward flows of heavy ions (O{sup +}, O{sup ++}, N{sup +}, N{sup ++}) with flow velocities of the order 1 km/s (Lockwood et al., 1985b). These downward flows were interpreted as the result of parabolic flow of these heavy ionospheric ions from a source region associated with the polar cleft topside ionosphere. Here the author utilizes a two-dimensional kinetic model to elicit features of the transport of very low energy O{sup +} ions from the cleft ionosphere. Bulk parameter (density, flux, thermal energies, etc.) distributions in the noon-midnight meridian plane illustrate the effects of varying convection electric fields and source energies. The results illustrate that particularly under conditions of weak convection electric fields and weak ion heating in the cleft region, much of the intermediate altitude polar cap magnetosphere may be populated by downward flowing heavy ions. It is further shown how two-dimensional transport effects may alter the characteristic vertical profiles of densities and fluxes from ordinary profiles computed in one-dimensional steady state models.
OSTI ID:
5940167
Journal Information:
Journal of Geophysical Research; (United States), Journal Name: Journal of Geophysical Research; (United States) Vol. 92:A1; ISSN 0148-0227; ISSN JGREA
Country of Publication:
United States
Language:
English