Decay of correlations and the collisionless conductivity in the geomagnetic tail

Details Decay of correlations and the collisionless conductivity in the geomagnetic tail Decay of correlations and the collisionless conductivity in the geomagnetic tail

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17..123h&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Feb. 1990, p. 123-126.

Physics

44

Electrical Resistivity, Geomagnetic Tail, Magnetic Field Reconnection, Collisionless Plasmas, Diurnal Variations, Plasma Heating, Plasma Layers, Polar Substorms, Stochastic Processes

Scientific paper

The collisionless electrical conductivity is calculated for the
geomagnetic tail from the stochastic orbits in the plasma sheet. The new
conductivity formula is important for the stochastic heating of the
plasma sheet and modifies the Galeev-Zelenyi formulas for the
collisionless reconnection growth rate for geomagnetic substorms.

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