Influence of heating rate on the condensational instability

Details Influence of heating rate on the condensational instability Influence of heating rate on the condensational instability

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988soph..117...51d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 117, no. 1, 1988, p. 51-56. NASA-Navy-sponsored research.

Physics

22

Magnetic Flux, Plasma Heating, Solar Flux, Thermal Instability, Linear Evolution Equations, Magnetohydrodynamic Stability, Nonlinear Evolution Equations, Solar Atmosphere

Scientific paper

Analysis and numerical simulation are used to determine the effect that various heating rates have on the linear and nonlinear evolution of a typical plasma within a solar magnetic flux tube subject to the condensational instability. It is found that linear stability depends strongly on the heating rate. The results of numerical simulations of the nonlinear evolution of the condensational instability in a solar magnetic flux tube are presented. Different heating rates lead to quite different nonlinear evolutions, as evidenced by the behavior of the global internal energy.

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