Granule Lifetimes and Dimensions as Function of Distance from a Solar Pore Region

  • Tron Andre Darvann
  • Ulf Kusoffsky
Part of the NATO ASI Series book series (ASIC, volume 263)

Abstract

The lifetimes of photospheric granules have been determined from cross-correlation of granulation images (von der Lühe 1983, Andreassen et al 1984, Darvann 1986). The measurements were carried out on a 19 minute long time series of solar granulation obtained with the Swedish 50 cm Vacuum Tower Telescope at La Palma (Wyller and Scharmer 1985). A rapid decrease of the granule lifetimes, from about 12 minutes close to a pore region to 5 minutes at a distance of about 10 arcseconds from the pores, is found. A morphological study of the granulation (i.e. measurement of the average granule size, number density and fractal dimension) in the same pore region has been carried out, and the results are discussed.

Keywords

Fractal Dimension Cross Correlation Granule Size Pore Region Magnetic Region 
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.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Andreassen, Ø., Engvold O., Müller, R.: 1984, High Resolution in Solar Physics, Proc., Toulouse, France, Ed.: R. Müller, p. 91.Google Scholar
  2. Alissandrakis, C.E., Dialetis, D., Tsiropoula, G.: 1987, Astron. Astrophys. 174, 275.ADSGoogle Scholar
  3. Bray, R.J., Loughhead, R.E., Durrant, C.J.: 1984, The solar granulation. Cambridge University Press, 2nd. edition, p.49, p.86.Google Scholar
  4. Darvann, T.A.: 1986, Proc. of the Inaugural Workshop at Tenerife, Oct. 1986.Google Scholar
  5. Dialetis, D., Macris, C., Muller, R., Prokakis, Th.: 1989a, (this volume).Google Scholar
  6. Dialetis, D., Macris, C., Muller, R., Prokakis, Th.: 1989b, (this volume), also submitted to Astron. Astrophys.Google Scholar
  7. Collados, M., Marco, J., Del Toro, J.C., Vazquez, M.: 1986, Solar. Phys. 105, 17. Koutchmy, S.: 1989, (this volume).Google Scholar
  8. Macris, C., Prokakis, Th., Dialetis, D.: 1989, (this volume).Google Scholar
  9. Mehltretter, J.P.: 1978, Astron. Astrophys. 62, 311.ADSGoogle Scholar
  10. Müller, R., Roudier, Th., Vigneau: 1989, (this volume).Google Scholar
  11. Roudier, Th., Muller, R.: 1986, Solar Phys. 107, 11.ADSCrossRefGoogle Scholar
  12. Schroter, E.H.: 1962, Z. Astrophys. 56, 183.ADSGoogle Scholar
  13. Schmidt, W., Grossmann-Doerth, U., Schroter, E.H.: 1988, Astron. Astrophys.197, 306.ADSGoogle Scholar
  14. Solar Geophysical Data prompt reports, September 1986.Google Scholar
  15. Title, A.M., Tarbell, T., and the SOUP team.: 1986, Proceedings, Boulder, Colorado 1986.Google Scholar
  16. Title, A.M., Tarbell, T.D., Topka, K.P.: 1987, Ap.J. 317, 892.ADSCrossRefGoogle Scholar
  17. von der Liihe, O.: 1983, Astron. Astrophys. 119, 85.ADSGoogle Scholar
  18. Wittmann, A.: 1978, Small scale motions on the Sun, Mitteilungen aus den Kiepenheuer-InstitutNr. 179, 1979.Google Scholar
  19. Wyller, A.A., Scharmer, G.B.: 1985, Vistas in Astronomy 28, 467ADSCrossRefGoogle Scholar

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • Tron Andre Darvann
    • 1
  • Ulf Kusoffsky
    • 2
  1. 1.Institute of Theoretical AstrophysicsUniversity of OsloOslo 3Norway
  2. 2.Grupo SuecoObservatorio del Roque de los Muchachos Apartado 66Santa Cruz de La Palma Islas CanariasSpain

Personalised recommendations