In a recent paper ; hereafter called Paper A) the author pointed out that multiple peaks in the Fourier spectra of the 5-rain oscillations as reported by others and discussed in several theoretical papers, do not characterize the average solar atmosphere, but result from insufficient statistical sta
Contribution to the observation of the photospheric oscillations
β Scribed by E. Fossat; G. Ricort
- Publisher
- Springer
- Year
- 1973
- Tongue
- English
- Weight
- 345 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
β¦ Synopsis
Observations of the 300 s photospheric oscillation on large solar surfaces (up to 5 '20" in diameter) using a sodium optical resonance cell seem to show that the power at long horizontal wavelengths is larger than previous results would indicate. In order to get more information about the spatial distribution of the energy, a new observational method has been perfected, which will allow us to obtain the spatiotemporal power spectrum.
In some of our observations, a long-period oscillation (about 40 rain) appears, with an amplitude comparable to that of the 300-s oscillation, and which seems to be correlated with the occurence of chromospheric flares.
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