Spectral investigation of the chromosphere. V - Observation and analysis of H beta

Details Spectral investigation of the chromosphere. V - Observation and analysis of H beta Spectral investigation of the chromosphere. V - Observation and analysis of H beta

Jun 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975soph...42..303g&link_type=abstract

Solar Physics, vol. 42, June 1975, p. 303-309.

Physics

5

Chromosphere, H Beta Line, Line Spectra, Solar Spectra, Spectrum Analysis, Correlation Coefficients, Cosmic Dust, Curve Fitting, Data Reduction, Distribution Functions, H Alpha Line, Microdensitometers, Root-Mean-Square Errors, Statistical Distributions

Scientific paper

The results of the analysis of 16 H-beta spectra taken with high spatial resolution are presented. The properties of the line profile in the boundary regions of supergranular cells (SGB) are described by the statistical distribution functions and correlation coefficients of four parameters which determine the shape of a suitable fitting curve. Although some of the line profile properties of both H-beta and H-alpha in the SGB can be interpreted in terms of a model which was recently proposed by Durrant (1975) the agreement between that theory and our observations is not entirely satisfactory.

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