Comparing Observed Prominence Spectra with Simple Models Computed Using GHV Code

Details Comparing Observed Prominence Spectra with Simple Models Computed Using GHV Code Comparing Observed Prominence Spectra with Simple Models Computed Using GHV Code

Sep 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010pobeo..90..163m&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 90, pp. 163-165

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Scientific paper

Emission spectra in seven lines have been computed for 980 prominence models using code originally developed by Gouttebrose, Heinzel and Vial. Prominence is treated as isothermal, isobaric, 1-D slab, with five input parameters determining outgoing radiation. Computed emission spectra in Hα have been compared with observations from the Ondřejov large solar spectrograph and some of the results are discussed.

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