The time variability of the central residual intensities of solar Fraunhofer lines

Details The time variability of the central residual intensities of solar Fraunhofer lines The time variability of the central residual intensities of solar Fraunhofer lines

Apr 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...16b&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Mar.-Apr. 1991, p. 16-22. In Ukrainian.

Astronomy and Astrophysics

Astronomy

Fraunhofer Lines, Light Scattering, Photosphere, Solar Spectra, Astronomical Photometry, Line Spectra, Solar Activity

Scientific paper

It is shown that, for moderately strong Fraunhofer lines, the scatter of the observed central residual intensity values decreases with an increase in excitation potential. In the case of weak lines, such a dependence is absent. The data suggest that, up to a certain level below its surface, the solar photosphere is nonstationary. Below this level, the undisturbed solar photosphere can already be considered a stationary formation.

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