The chromosphere above a sunspot umbra

Details The chromosphere above a sunspot umbra The chromosphere above a sunspot umbra

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...79...31b&link_type=abstract

Solar Physics, vol. 79, July 1982, p. 31-39. Research supported by the Korean Science and Engineering Foundation, Seoul National

Physics

11

Chromosphere, Solar Atmosphere, Solar Spectra, Spectral Line Width, Sunspots, Umbras, Atmospheric Models, Calcium, H Lines, K Lines, Thermodynamic Equilibrium

Scientific paper

A model representing the chromosphere above part of the observed umbra, presented in this study in tabular form, is able to accurately predict the intensity profiles of the cores of selected strong spectral lines. The model is also consistent with studies of the transmission region above spots. The present selection of a local minimum in brightness is not only found to assist in the spatial registration of the reduced data, but to provide a model of what may be a low temperature extremum.

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