Bulletin of the American Physical Society
63rd Annual Meeting of the APS Division of Plasma Physics
Volume 66, Number 13
Monday–Friday, November 8–12, 2021; Pittsburgh, PA
Session UP11: Poster Session VIII:
Fundamental Plasma Physics - Analytical and Computational Techniques; Magnetic Reconnection; Antimatter Heliospheric, Magnetospheric, and Ionospheric Plasma Phenomena and Their Scaled Laboratory Experiments
MFE - DIII-D Tokamak II, ITER, HBT-EP, and Other Tokamaks
2:00 PM - 5:00 PM
Thursday, November 11, 2021
Room: Hall A
Abstract: UP11.00066 : Effect of Electron Precipitation on E-Region Instabilities: Theoretical Analysis*
Presenter:
Yakov S Dimant
(Boston University)
Authors:
Yakov S Dimant
(Boston University)
George V Khazanov
(NASA Goddard)
Meers M Oppenheim
(Boston University)
During periods of strong geomagnetic activity, intense currents flow from the magnetosphere into the high-latitude E-region ionosphere along the magnetic field. In this region, collisions between the plasma and neutral molecules allow the entire magnetosphere-ionosphere current system to close. These same currents cause strong DC electric fields in the E-region ionosphere where they drive plasma instabilities, including the Farley-Buneman instability (FBI). These instabilities give rise to small-scale plasma turbulence that modifies the large-scale ionospheric conductance that, in turn, affects the evolution of the entire near-Earth plasma environment. Also, during geomagnetic storms, precipitating electrons of high energies, $\gtrsim$~5 keV, frequently penetrate down to the same regions where intense currents and E fields develop. This research examines the effects of precipitating electrons on the generation of the FBI and shows that, under many common conditions, it can easily suppress the FBI in a predictable manner. We expect precipitation to exert a significant feedback on the magnetosphere by preventing the elevated conductivity caused by FBI driven turbulence. This suppression should be taken into account in global modeling of the magnetosphere-ionosphere coupling.
*Work is supported by NASA LWS Grant #80NSSC19K0080 and NSF Grant PHY-1500439.
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