Scaling-law equilibria for calcium in canopy-type models of the solar chromosphere

Details Scaling-law equilibria for calcium in canopy-type models of the solar chromosphere Scaling-law equilibria for calcium in canopy-type models of the solar chromosphere

Aug 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79..279j&link_type=abstract

Solar Physics, vol. 79, Aug. 1982, p. 279-290.

Physics

2

Calcium, Chromosphere, Scaling Laws, Solar Atmosphere, Stellar Models, Equilibrium Equations, Ionization, Nonlinear Equations, Pressure Reduction

Scientific paper

Scaling laws for resonance line formation are used to obtain approximate excitation and ionization equilibria for a three-level model of singly ionized calcium. The method has been developed for and is applied to the study of magnetograph response in the 8542 A infrared triplet line to magnetostatic canopies which schematically model diffuse, nearly horizontal fields in the low solar chromosphere. For this application, the method is shown to be efficient and semi-quantitative, and the results indicate the type and range of effects on calcium-line radiation which result from reduced gas pressure inside the magnetic regions.

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