Power output of a turbulent current sheet on the sun

Details Power output of a turbulent current sheet on the sun Power output of a turbulent current sheet on the sun

Oct 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..789b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, Oct. 1986, p. 789-794) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, Sept.-Oc

Astronomy and Astrophysics

Astronomy

1

Current Sheets, Energy Dissipation, High Temperature Plasmas, Plasma Turbulence, Solar Wind, Magnetohydrodynamic Stability, Solar Flares

Scientific paper

If high-temperature turbulent current sheets on the sun are experiencing
Parker-Sweet flow, they will be in a quasi-linear turbulence regime or
in an instability-threshold regime. For typical parameters of
active-region plasma, energy would be released in such a sheet at a rate
no higher than 10 to the 26th erg/sec.

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