Electron velocity distribution function in a fully ionized plasma slab with a large temperature gradient - Solar flare transition region

Details Electron velocity distribution function in a fully ionized plasma slab with a large temperature gradient - Solar flare transition region Electron velocity distribution function in a fully ionized plasma slab with a large temperature gradient - Solar flare transition region

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jqsrt..44..203l&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 44, July 1990, p. 203-208.

Physics

2

Electron Mobility, Electron Plasma, Solar Flares, Temperature Gradients, Velocity Distribution, Coronal Loops, Crank-Nicholson Method, Vlasov Equations

Scientific paper

The high velocity tail of the electron distribution function has been
calculated by numerically solving the high velocity form of the Landau
equation for a thermal structure representative of a solar flare. The
calculations show an anisotropy and an enhancement of the tail
populations above the Maxwellian value throughout the flaring loop.

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