Evaporative cooling of flare plasma

Details Evaporative cooling of flare plasma Evaporative cooling of flare plasma

Nov 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7714971a&link_type=abstract

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Computer Science

Sound

Acoustic Velocity, Evaporative Cooling, Flares, Magnetohydrodynamic Flow, Chromosphere, Conductive Heat Transfer, Heat Flux, X Ray Analysis

Scientific paper

A one-dimensional loop model for the evaporative cooling of the coronal flare plasma was investigated. Conductive losses dominated radiative cooling, and the evaporative velocities were small compared to the sound speed. The profile and evolution of the temperature were calculated. The model was in agreement with soft X-ray observations on the evolution of flare temperatures and emission measures. The effect of evaporation was to greatly reduce the conductive heat flux into the chromosphere and to enhance the EUV emission from the coronal flare plasma.

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