On the thermal durability of solar prominences, or how to evaporate a prominence

Details On the thermal durability of solar prominences, or how to evaporate a prominence On the thermal durability of solar prominences, or how to evaporate a prominence

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986nascp2442..225m&link_type=abstract

In NASA. Goddard Space Flight Center Coronal and Prominence Plasmas p 225-228 (SEE N87-20871 13-92)

Physics

3

Induction Heating, Ohmic Dissipation, Plasma Heating, Solar Corona, Solar Prominences, Thermal Conductivity, Magnetic Induction, Solar Physics, Solar Wind, Thermodynamic Equilibrium

Scientific paper

The authors investigate the thermal disappearance of solar prominences under strong perturbations due to wave heating, Ohmic heating, viscous heating or conduction. Specifically, they calculate how large a thermal perturbation is needed to destroy a stable thermal equilibrium, and find that the prominence plasma appears to be thermally very rugged. Its cold equilibrium may most likely be destroyed by either strong magnetic heating or conduction in a range of parameters which is relevant to flares.

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