Plasmasphere Plume-associated Storm-Enhanced Densities (SED) as Suppliers of Ionospheric Outflows to the Magnetosphere

Elevated ionospheric density regions which evidently have been convected from the subauroral plasmaspheric region toward the noon sector cleft ionosphere have been reported. Here, the possibility that these so-called Storm Enhanced Density (SED) regions could serve as ionospheric plasma source populations for cleft ion fountain outflows is explored. The UT Arlington Dynamic Fluid Kinetic (DyFK) code is employed to simulate the entry of a high-density ``plasmasphere-like'' flux tube entering the cleft region and subjected to an episode of wave-driven transverse ion heating. Initial comparisons of these modeling results with SED-outflow-plasmasphere plume observations will also be presented.