The Current-Driven LH Instability and The Formation of Stable Electron Holes

Details The Current-Driven LH Instability and The Formation of Stable Electron Holes The Current-Driven LH Instability and The Formation of Stable Electron Holes

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009agufmsm21a1572c&link_type=abstract

American Geophysical Union, Fall Meeting 2009, abstract #SM21A-1572

Physics

Geophysics

[2721] Magnetospheric Physics / Field-Aligned Currents And Current Systems, [2723] Magnetospheric Physics / Magnetic Reconnection, [2772] Magnetospheric Physics / Plasma Waves And Instabilities, [4455] Nonlinear Geophysics / Nonlinear Waves, Shock Waves, Solitons

Scientific paper

Using particle-in-cell simulations and kinetic theory, we explore the
turbulence that develops during 3D magnetic reconnection with a guide
field. At late time the turbulence is dominated by the Buneman and lower
hybrid instabilities. Both produce stable electron holes that co-exist
but have very different lifetime and propagation speeds.

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