Physics
Scientific paper
Nov 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984esasp.220..271t&link_type=abstract
In ESA The Hydromagnetics of the Sun p 271-272 (SEE N85-25091 14-92)
Physics
Magnetohydrodynamic Stability, Solar Prominences, Tearing Modes (Plasmas), Current Sheets, Magnetic Flux, Solar Magnetic Field
Scientific paper
A one dimensional current sheet model, where magnetic reconnection takes
place, is considered. The analysis shows how perturbation changes the
balance between magnetic and thermal energy in the thin resistive region
and in the wide ideal one.
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