Physics
Scientific paper
Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm21a1886l&link_type=abstract
American Geophysical Union, Fall Meeting 2010, abstract #SM21A-1886
Physics
[2483] Ionosphere / Wave/Particle Interactions, [2704] Magnetospheric Physics / Auroral Phenomena, [2712] Magnetospheric Physics / Electric Fields, [2721] Magnetospheric Physics / Field-Aligned Currents And Current Systems
Scientific paper
Recently, we have demonstrated that the long-range parallel electric fields in the downward current region of the aurora are supported by a combination of pressure gradients, mirror force, and anomalous heating (but not anomalous resistivity) due to wave turbulence [1-4]. In this paper, we show examples of auroral passes from the FAST satellite where electrostatic ion cyclotron waves contribute substantially to this turbulence even when other wave modes are present. We show that, by using satellite data as a boundary condition for the model and making a few reasonable assumptions about the distribution of wave activity with altitude, we can predict the parallel electric fields over a range of thousands of kilometers, from the estimated average location of the double layer to altitudes where the dipole approximation starts to break down. [1] J. R. Jasperse et al. (2006), Phys. Plasmas 13, 072903. [2] J. R. Jasperse et al. (2006), Phys. Plasmas 13, 112902. [3] J. R. Jasperse et al. (2010), Phys. Plasmas 17, 062903. [4] J. R. Jasperse et al. (2010), Phys. Plasmas 17, 062904.
Basu Baidyanath
Jasperse John R.
Lund Eric J.
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