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
On the temporal variation of the solar continuous brightness fluctuations
β Scribed by B. Hadjebi
- Publisher
- Springer
- Year
- 1981
- Tongue
- English
- Weight
- 723 KB
- Volume
- 73
- Category
- Article
- ISSN
- 0038-0938
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β¦ Synopsis
From a sequence of white-light photographs of solar granulation at the centre of the disk, obtained by Spectro-Stratoscope on May 17, 1975, two-dimensional spatial power spectra of photospheric intensity fluctuations were deduced. These show periodicities of ~1000 s, 250--450 s (5-min oscillation), and shorter ones in the range 30-120 s. The reality of the shorter periods, however, seems to be questionable.
The weighted mean wavenumber of the spatial power spectra and rms of the intensity fluctuation (/~ms) are also computed, showing the same periodicities as the power.
* Mitteilungen aus dem Kiepenheuer-lnstitut Nr. 188.
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