Physics
Scientific paper
Sep 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980a%26a....89...80d&link_type=abstract
Astronomy and Astrophysics, vol. 89, no. 1-2, Sept. 1980, p. 80-87.
Physics
8
Line Spectra, Solar Physics, Solar Spectra, Spectral Shift Control, Spectrum Analysis, Atmospheric Models, Frequency Modulation, High Frequencies
Scientific paper
The effects on spectral line shifts due to velocity-correlated opacity and source function fluctuations in waves are discussed in the context of a simple exponential atmospheric model. These correlations contribute a steady net line shift and, if the velocity amplitude is small enough, a small correction to the fluctuating component of the shift. Also noted are the minor changes in the form of the line shift reflecting height-dependent velocity amplitudes and nonlinear source functions. The results and limitations of the model are discussed with reference to the large-amplitude calculations of Cram et al. (1979) and the estimates of the high frequency power in the sun made by Deubner (1976).
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