Resistive instabilities in coronal conditions

Details Resistive instabilities in coronal conditions Resistive instabilities in coronal conditions

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...97..309b&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 97, June 1985, p. 309-320. Research supported by the Ministero della Pubblica Istruzione.

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Coronal Loops, Magnetohydrodynamic Stability, Solar Corona, Solar Magnetic Field, Computational Astrophysics, Equilibrium Equations, Hydrodynamic Equations

Scientific paper

Resistive instabilities in a context referring to the solar corona are rigorously investigated. Various equilibrium configurations are considered, differing, among other things, by their behavior with respect to fast, ideal instabilities. The computations presented cover in a unified scheme all known regimes of resistive modes and make it possible to determine the fastest timescale over which resistivity can play a role. Comparisons with previous work as well as possible extensions are presented.

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