Anomalous Magnetic Diffusion in Coronal Current Layers

Details Anomalous Magnetic Diffusion in Coronal Current Layers Anomalous Magnetic Diffusion in Coronal Current Layers

Oct 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995soph..161..197v&link_type=abstract

Solar Physics, Volume 161, Issue 1, pp.197-200

Physics

12

Scientific paper

The current-driven kinetic Alfvén instability is proposed as an anomalous transport mechanism for regions of concentrated, field-aligned currents in the solar corona. Anomalous magnetic diffusivity (η e f f ≤ 109cm2s-1), produced by kinetic Alfvén turbulence in the vicinity of the saturation level, provides fast magnetic energy release with a local inflow Alfvén Mach numberM in ≤ 0.1.

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