Quiescent prominence threads models

Details Quiescent prominence threads models Quiescent prominence threads models

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985soph...96...53f&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 96, March 1985, p. 53-92.

Physics

28

Conductive Heat Transfer, Heat Balance, Radiative Heat Transfer, Solar Physics, Solar Prominences, Solar Temperature, Continuous Spectra, H Alpha Line, Line Spectra, Lyman Spectra, Solar Atmosphere, Thermal Conductivity

Scientific paper

Prominence thread models are calculated for different values of center temperature and pressure. The radiative transfer, statistical equilibrium and ionization equilibrium equations are simultaneously solved, assuming a three-level atom-plus-continuum. Also computed are the energy balance equation including the hydrogen radiative losses from the present calculations, plus other radiative losses and heat conduction. Some models have been calculated assuming possible variations in thermal conductivity and heating terms. The lines and continua emitted by a number of threads are computed, in order to compare them with the observations and evaluate how the different values of the parameters affect the profiles and absolute intensities of L-alpha, L-beta, H-alpha, and Ly continuum.

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