Solar Physics

, Volume 126, Issue 1, pp 53–67 | Cite as

The large-scale pattern formed by the spatial distribution of granules

  • R. Muller
  • Th. Roudier
  • J. Vigneau
Article

Abstract

The spatial distribution of granule sizes at the surface of the sun is investigated. Granules have been separated into two classes: those larger than 1″.37 and those smaller, where 1″.37 is the critical scale defined by Roudier and Muller (1986). It is found that granules are not distributed at random: large granules appear to be clustered, forming a cellular pattern with a characteristic scale of 7″; small granules form a similar and complementary pattern. These patterns are probably related to the mesogranulation.

Keywords

Spatial Distribution Characteristic Scale Granule Size Small Granule Large Granule 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Bray, R. J., Loughhead, R. E., and Durrant, C. J.: 1984, The Solar Granulation, 2nd edition, Cambridge University Press, Cambridge.Google Scholar
  2. Dialetis, D., Macris, C., Muller, R., and Prokakis, T.: 1988, Astron. Astrophys. 204, 275.Google Scholar
  3. Franck, Z., Muller, R., Roudier, Th., Vigneau, J., Shine, R., Tarbell, T., Title, A., Topka, K., and Simon, G.: 1989, Bull. Am. Astron. Soc. 21, No. 2, 845.Google Scholar
  4. Kawaguchi, I.: 1980, Solar Phys. 65, 207.Google Scholar
  5. Koutchmy, S. and Lebecq, Ch.: 1988, Astron. Astrophys. 169, 323.Google Scholar
  6. Macris, C. J., Muller, R., Rösch, J., and Roudier, Th.: 1984, in S. Keil (ed.), Small-Scale Dynamical Processes in the Solar and Stellar Atmospheres, Sacramento Peak Observatory, Sunspot, New-Mexico, p. 265.Google Scholar
  7. Muller, R.: 1990, in G. Chapman (ed.), Adv. Space Res. (in press).Google Scholar
  8. Muller, R. and Keil, S. L.: 1983, Solar Phys. 87, 243.Google Scholar
  9. November, L. and Simon, G.: 1990, Astrophys. J. (submitted).Google Scholar
  10. November, L., Toomre, J., Gebbie, K., and Simon, G.: 1981, Astrophys. J. 245, L123.Google Scholar
  11. Oda, N.: 1984, Solar Phys. 93, 243.Google Scholar
  12. Roudier, Th. and Muller, R.: 1986, Solar Phys. 107, 11.Google Scholar
  13. Roudier, Th., Coupinot, G., Hecquet, J., and Muller, R.: 1985, J. Optics 16, 107.Google Scholar
  14. Simon, G., Title, A., Topka, K. P., Tarbell, T., Shine, R. A., Ferguson, S. H., Zirin, H., and the SOUP Team: 1988, Astrophys. J. 327, 964.Google Scholar
  15. Title, A., Tarbell, T., Simon, G., and the SOUP Team: 1986, Adv. Space Res. 6, 253.Google Scholar
  16. Title, A., Tarbell, T., Topka, K., Ferguson, S., Shine, R., and the SOUP Team: 1989, Astrophys. J. 336, 475.Google Scholar
  17. Zahn, J. P.: 1987, in E. H. Schröter and M. Schussler (eds.), Solar and Stellar Physics, Lecture Notes in Physics 292, 55.Google Scholar

Copyright information

© Kluwer Academic Publishers 1990

Authors and Affiliations

  • R. Muller
    • 1
  • Th. Roudier
    • 2
  • J. Vigneau
    • 2
  1. 1.Observatoire du Pic du MidiBagnères-de-BigorreFrance
  2. 2.Observatoire du Pic du MidiToulouseFrance

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