Anomalous resistivity from Buneman instability: Theory and simulation

Details Anomalous resistivity from Buneman instability: Theory and simulation Anomalous resistivity from Buneman instability: Theory and simulation

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010agufmsm33e..08y&link_type=abstract

American Geophysical Union, Fall Meeting 2010, abstract #SM33E-08

Physics

Plasma Physics

[7829] Space Plasma Physics / Kinetic Waves And Instabilities, [7839] Space Plasma Physics / Nonlinear Phenomena, [7863] Space Plasma Physics / Turbulence, [7867] Space Plasma Physics / Wave/Particle Interactions

Scientific paper

Buneman or strong ion-electron streaming instability may be a source of anomalous resistivity in reconnection regions or tangential discontinuities in space plasmas. Kinetic effects arising from the excitation of Buneman instability can be coupled to macroscopic models by means of anomalous resistivity in the generalized Ohm's law. The present paper discusses a nonlinear turbulence theory for Buneman instability, which is compared against Vlasov simulation. We also discuss how the anomalous resistivity computed theoretically can be coupled to the macroscopic models.

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