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On the size and structure of bright solar Ca+-network cells depending on the heliographic position

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Abstract

From photographic recordings of some hundred bright Ca+-network cells on the solar disk we find evidence for a smaller size of polar cells as compared to equatorial cells by a factor of about 0.9. We do not find an indication of a dependence of the structure of the cells on the heliographic position.

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References

  • Brune, R.: 1980, Staatsexamensarbeit, Göttingen.

  • Leighton, R. B., Noyes, R. W., and Simon, G. W.: 1961, Astrophys. J. 135, 474.

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  • Rogers, E. H.: 1970, Solar Phys. 13, 57.

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  • Stix, M.: 1980, in R. Dunn (ed.), Solar Instrumentation - What's Next? (in press).

  • Waldmeier, M.: 1941, Ergebnisse und Probleme der Sonnenforschung, Leipzig.

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Brune, R., Wöhl, H. On the size and structure of bright solar Ca+-network cells depending on the heliographic position. Sol Phys 75, 75–78 (1982). https://doi.org/10.1007/BF00153461

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