The time variability of absorption lines in the solar spectrum

Details The time variability of absorption lines in the solar spectrum The time variability of absorption lines in the solar spectrum

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991kfnt....7...48k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 7, Sept.-Oct. 1991, p. 48-50. In Russian.

Physics

Absorption Spectra, Fraunhofer Lines, Photosphere, Solar Spectra, Spectral Line Width, Neutral Atoms, Solar Atmosphere, Time Dependence

Scientific paper

The conclusion of Babii (1991) that, up to a certain level (in the region where weak absorption lines are formed), the solar photosphere is in a stationary state and above that level the solar photosphere may be considered as being in a variable state, is called into question. It is argued that the only conclusion that can be drawn from the observations is that moderate Fraunhofer lines are susceptible to strong variations.

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