Physics
Scientific paper
Apr 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...77..167w&link_type=abstract
Solar Physics, vol. 77, Apr. 1982, p. 167-175.
Physics
9
Energy Dissipation, Enthalpy, Heat Flux, Radiant Cooling, Solar Corona, Coronal Loops, Emission Spectra, Particle Flux Density, Solar Physics, Solar Temperature, Spicules, Stellar Models
Scientific paper
The differential emission measure profile for quiet and flaring solar regions is considered, among a model in which the principal downflow of heat is due to the enthalpy of downward-flowing material, rather than conduction. It is found that the emission measure profile for quiet solar regions is matched well by a downward particle number flux which decreases with temperature. This would be expected if this particle flux is due to heated spicular material falling back onto the chromosphere. In flaring regions, however, a particle flux which increases with temperature is required to explain the step emission measure profile. This could be a result of mass motions downward out of the flaring loops.
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