Radiative dominated cooling of the flare corona and transition region

Details Radiative dominated cooling of the flare corona and transition region Radiative dominated cooling of the flare corona and transition region

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979stin...7932145a&link_type=abstract

Unknown

Computer Science

Sound

Radiative Heat Transfer, Solar Cooling, Solar Corona, Solar Flares, Line Spectra, Mathematical Models, Solar Wind, Supersonic Speed, Temperature Dependence, Temperature Profiles

Scientific paper

Models in which radiation dominates cooling flare loops are investigated. The radiative models are found to predict a differential emission measure (Q) proportional to T to the (l+1) power, where l measures the dependence of the radiative loss coefficient on temperature, lamda (T) approximately T to the (-l) power. It is concluded that the radiative models are incapable of explaining the observed temperature dependence of Q for flare coronal and transitional plasma. The models suggest that large mass motions (velocities of the order of the sound speed) may be required.

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