HR: 09:15h
AN: SM21B-06    [Abstracts]
TI: A laboratory search for plasma erosion by Alfven waves
AU: * Vincena, S
EM: vincena@physics.ucla.edu
AF: UCLA Department of Physics and Astronomy, 1000 Veteran Avenue Room 15-70, Los Angeles, CA 90095-1696, United States
AU: Gekelman, W
EM: gekelman@physics.ucla.edu
AF: UCLA Department of Physics and Astronomy, 1000 Veteran Avenue Room 15-70, Los Angeles, CA 90095-1696, United States
AU: Pribyl, P
AF: UCLA Department of Physics and Astronomy, 1000 Veteran Avenue Room 15-70, Los Angeles, CA 90095-1696, United States
AB: Obliquely propagating shear Alfven waves with transverse wavelengths on the order of the electron inertial length or even the ion gyro-radius are commonly observed in the earth's low-altitude auroral zones. These regions are also replete with observations of electron beams and transversely heated ions. A kinetic treatment of shear Alfven wave-particle interaction reveals how these waves can be responsible for some of the observed particle acceleration. The auroral plasma environment is further enriched by the presence of field-aligned depletions in plasma density, and it has been suggested* that the Alfven waves may, in fact, be the cause of the erosion of ionospheric density. In this laboratory experiment, shear waves will be launched using a variety of proven antennas, and also allowed to grow spontaneously as Drift-Alfven modes in seeded density depletions**. Detailed measurements of the wave magnetic fields in the perpendicular density gradient regions will be presented which demonstrate the generation of short perpendicular wave scales due to the perpendicular gradient in parallel wave phase speed. Miniature in-situ particle diagnostics will also be used to look for electron and ion acceleration. The waves will also be launched into an increasing region of background magnetic field in an attempt to model the ratios of Alfven speed to electron thermal speed, and density gradient scale length to electron inertial length appropriate to the earth's auroral zone. Preliminary results will be presented on the efficacy of shear Alfven waves to self-generate plasma density depletions, or deepen ambient density inhomogeneities. The experiments are conducted at UCLA's Basic Plasma Science Facility in the Large Plasma Device. *Chaston, et al., "Ionospheric erosion by Alfven Waves," JGR, V 111, A03206, 2006. **Penano, et al., "Drift-Alfven fluctuations associated with a narrow pressure striation," Phys. Plasmas, V 7, Issue 1, pp. 144-157 (2000).
DE: 2439 Ionospheric irregularities
DE: 2471 Plasma waves and instabilities (2772)
DE: 2483 Wave/particle interactions (7867)
DE: 7831 Laboratory studies and experimental techniques
SC: SPA-Magnetospheric Physics [SM]
MN: 2007 Fall Meeting