On Estimation of the Optical Thickness of Solar Prominences

Details On Estimation of the Optical Thickness of Solar Prominences On Estimation of the Optical Thickness of Solar Prominences

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009pobeo..86..283m&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 86, pp. 283-286

Astronomy and Astrophysics

Astronomy

Scientific paper

A method for rough estimation of the optical thickness of solar prominences in Hα line is presented. The method is based on the fitting of observed profiles with the synthetic ones computed by using the model of an isobaric 1-D slab with constant source function under the assumption of complete redistribution. The method was applied on 52 prominences observed with the Ondřejov HSFA2 spectrograph from April 2007 to March 2008.

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