HR: 15:10h
AN: SM43D-07 INVITED [Abstracts]
TI: Plasma Heating and Transport at the Magnetopause due to Nonlinear interactions with Kinetic ULF
Waves
AU: * Johnson, J R
EM: jrj@pppl.gov
AF: Princeton University, Princeton University
Plasma Physics Laboratory
PO Box 451
MS #28, Princeton, NJ 08525
United States
AU: Wing, S
EM: simon.wing@jhuapl.edu
AF: The Johns Hopkins University, Applied Physics Laboratory
11100 Johns Hopkins Road, Laurel, MD 20723
United States
AU: Lin, Y
EM: ylin@physics.auburn.edu
AF: Auburn University, Department of Physics
206 Allison Laboratory, Auburn, AL 36849
United States
AU: Cheng, C Z
EM: frankcheng@nspo.org.tw
AF: National Space Program Office, 8F, 9
Prosperity 1st Road
Hsinchu Science Park, Hsinchu, 30078
Taiwan
AB:
The magnetopause and boundary layer are typically characterized by large amplitude transverse ULF wave activity with
frequencies below the ion cyclotron frequency. The wave properties are consistent with a mode conversion process that couples
large-scale surface MHD fluctuations with kinetic Alfvén waves at the magnetopause boundary. We model the waves with
theory and global three-dimensional hybrid simulations, and we discuss the importance of plasma flow for this process along
the flanks. We find that ions and electrons can interact nonlinearly with these waves leading to perpendicular heating of
ions, parallel heating of electrons, and plasma transport across the magnetopause boundary. We compare these theoretical
findings with both in situ GEOTAIL particle observations and remote observations of plasma along the magnetotail flanks
inferred using DMSP and discuss possible causes for dawn-dusk asymmetries in the particle distributions that are manifest in
the global density and temperature profiles.
UR: http://w3.pppl.gov/~jrj/magnetopause.html
DE: 2724 Magnetopause and boundary layers
DE: 7805 Chaos (4420)
DE: 7827 Kinetic and MHD theory
DE: 7839 Nonlinear phenomena (4400, 6944)
DE: 7859 Transport processes
SC: SPA-Magnetospheric Physics [SM]
MN: Fall Meeting 2005