HR: 1340h
AN: SM33B-0449    [Abstracts]
TI: Observational constraints for plasma sheet ion sources and transports during northward IMF
AU: * Wing, S
EM: simon.wing@jhuapl.edu
AF: The Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
AU: Johnson, J R
EM: jrj@pppl.gov
AF: Princeton University, Princeton, Princeton, NJ 08543 United States
AU: Newell, P T
EM: patrick.newell@jhuapl.edu
AF: The Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
AU: Meng, C
EM: ching.meng@jhuapl.edu
AF: The Johns Hopkins University, 11100 Johns Hopkins Road, Laurel, MD 20723-6099 United States
AB: During periods of northward IMF, plasma sheet ions often have two components: hot (magnetospheric origin) and cold (magnetosheath origin). The temperatures of the cold-component ions are ~30-40 percent higher in the dawn sector compared to the dusk sector, implying the magnetosheath ion heating of ~30-40 percent during the entry process along the plasma sheet dawn flank. As a result, the magnetosheath ions are less distinguishable from the hot-component ions, which have lower temperatures on the dawnside, leading to a higher occurrence of the ions having (apparent) one-component distribution. As the duration of the hourly averaged IMF being northward (Dt) increases from 1 to 10 hours, the occurrence of two-component ions increases from 65 to 83 percent in the dusk flank, but in the dawn flank, it remains relatively stable at around 45 percent. In contrast, the occurrence of ions best characterized by kappa distribution increases from 25 to 35 percent in the dawn flank whereas in the dusk flank it remains relatively insensitive to Dt (10 percent). The occurrence of a one-component Maxwellian distribution appears to be most pronounced in the region of the plasma sheet close to the midnight meridian, and these ions appear to be characteristic of the nominal plasma sheet (hot component) ions. The densification of the plasma sheet, as Dt increases, mainly results from the influx of the magnetosheath ions. However, the cooling of the plasma sheet ions can be attributed not only to the influx of the cold magnetosheath ions, but also the cooling of the nominal plasma sheet ions. The dawn-dusk asymmetries observed in the cold magnetosheath ion profiles should provide constraints that can help determine the roles of various proposed magnetosheath ion entry mechanisms.
DE: 2736 Magnetosphere/ionosphere interactions (2431)
DE: 2740 Magnetospheric configuration and dynamics
DE: 2744 Magnetotail
DE: 2748 Magnetotail boundary layers
DE: 2764 Plasma sheet
SC: SPA-Magnetospheric Physics [SM]
MN: Fall Meeting 2005