On the large scale brightness fluctuatio
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V. A. Krat; V. I. Makarov; K. S. Tavastsherna
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Article
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1980
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Springer
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English
⚖ 250 KB
The October 1976 spectroscopic observations of the solar chromosphere with the great coronagraph of the Kislovodsk Station of the Pulkovo Observatory were analysed using the autocorrelation method. The autocorrelation function and the power spectrum were calculated. It was found that the brightness