Hostname: page-component-7bb8b95d7b-w7rtg Total loading time: 0 Render date: 2024-09-13T09:33:24.602Z Has data issue: false hasContentIssue false
  • English
  • Français

On the state of the photosphere before the appearance of sunspots

Published online by Cambridge University Press:  14 August 2015

Z. B. Korobova ,
A. K. Tchandaev  and
G. Y. Vassilyeva
Z. B. Korobova
Affiliation:
Tashkent Observatory, U.S.S.R.
A. K. Tchandaev
Affiliation:
Gorki Institute, U.S.S.R.
G. Y. Vassilyeva
Affiliation:
Pulkovo Observatory, U.S.S.R.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

The object of our investigation was to clarify the behavior of the fluctuations in the brightness in photosphere on the scale of the supergranulation 1–2 days before the appearance of sunspots.

Type
Part III: Optical Structure of an Active Region
Information
Symposium - International Astronomical Union , Volume 35: Structure and Development of Solar Active Regions , 1968 , pp. 149 - 160
Copyright
Copyright © Reidel 1968 

References

Beckers, J. M. (1966) ‘The Fine Structure of the Solar Atmosphere’, Colloquium held at the German Solar Observatory, Capri, June 6–8, p. 56.Google Scholar
Bumba, V., Howard, R. (1965) Astrophys. J., 141, 1492.Google Scholar
Harvey, J.W. (1965) Publ. astr. Soc. Pacific, 77, 129.Google Scholar
Iksanov, R.N., Vitinsky, J.I. (1966) Izv. glav. astr. Obs., 180.Google Scholar
Loughhead, R.E., Bray, R.I. (1961) Austr. J. Phys., 14, 347.Google Scholar
Miller, R. A. (1960) J. Brit. Astron. Assoc., 70, 100.Google Scholar