Nonlinear excitation of magnetic undular instability by convective motion

Details Nonlinear excitation of magnetic undular instability by convective motion Nonlinear excitation of magnetic undular instability by convective motion

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apj...358..698k&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 358, Aug. 1, 1990, p. 698-709.

Astronomy and Astrophysics

Astrophysics

21

Convective Flow, Current Sheets, Magnetohydrodynamic Stability, Solar Atmosphere, Solar Magnetic Field, Boundary Conditions, Buoyancy, Magnetic Flux, Nonlinear Equations, Photosphere

Scientific paper

The influence of convective motions on the stabilty of a Parker stable magnetic flux sheet is numerically investigated. The general characteristics of the Parker instability with convective motions in the nonlinear stage are studied. The possibility that a destabilization of stable flux can be realized by either horizontal photospheric shearing motions and/or by vertical convective flows is examined.

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