Some more effects of waves on spectral line analysis

Physics

Scientific paper

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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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