Hostname: page-component-745bb68f8f-5r2nc Total loading time: 0 Render date: 2025-01-12T21:09:41.405Z Has data issue: false hasContentIssue false
  • English
  • Français

Granulation and Supergranulation as a Diagnostic Test of Solar Structure

Published online by Cambridge University Press:  25 April 2016

R. Van der Borght  and
P. Fox
R. Van der Borght
Affiliation:
Monash University
P. Fox
Affiliation:
Monash University
Get access Rights & Permissions [Opens in a new window]

Extract

One of the most difficult tasks facing theoretical astrophysics today is to find a satisfactory model for the convective transport of energy in regions where the temperature gradient is superadiabatic. A number of such models have been proposed, such as the mixing-length theory and its extensions (Vitense 1953, Böhm-Vitense 1958, Spiegel 1963, Travis and Matsushima 1973 a, b, Parson 1969), to take into account the combined effects of convection and turbulence but it is generally agreed that, to-date, no satisfactory theory has been put forward.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 168 - 169
Copyright
Copyright © Astronomical Society of Australia 1983

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Beckers, J. M., IAU Colloq. #51, ‘Stellar Turbulence’, Ed. Gray, D. F., and Linsky, J. L., p 85 (1979).Google Scholar
Böhm, K. H., IAU Colloq. #38, ‘Problems of Stellar Convection’, Ed. Spiegel, E. A., and Zahn, J. P., p 103 (1977).CrossRefGoogle Scholar
Böhm-Vitense, E., Z. f. Astrophys., 46, 108 (1958).Google Scholar
Bray, R. J., and Loughhead, R. E., ‘Solar granulation’, (Chapman and Hall, Lond.) (1967).Google Scholar
Canfield, R. C., Solar Phys., 50, 329 (1976).CrossRefGoogle Scholar
Deubner, F. L., and Mattig, W., Astron. Astrophys., 45, 167 (1975).Google Scholar
Dravins, D., Solar Phys., 40, 53 (1975).CrossRefGoogle Scholar
Durrant, C. J., Mattig, W., Nesis, A., Reiss, G., and Schmidt, W., Solar Phys., 61, 251 (1979).CrossRefGoogle Scholar
Gibson, E., ‘The Quiet Sun’ (NASA SP-303, Washington, D.C.) (1973).Google Scholar
Graham, E., and Moore, D. R., Oon. Not. R. Astron. Soc., 183, 617 (1978).CrossRefGoogle Scholar
Keil, S., Astrophys. J., 237, 1024 (1980).CrossRefGoogle Scholar
Keil, S., and Canfield, R., Astron. Astrophys., 70, 169 (1978).Google Scholar
Norlund, A., Astron. Astrophys., 32, 407 (1974).Google Scholar
Parsons, S. B., Astophys. J. Suppl., 18, 127 (1969).CrossRefGoogle Scholar
Spiegel, E. A., Astrophys. J., 138, 216 (1963).CrossRefGoogle Scholar
Travis, L. D., and Matsushima, S., Astrophys. J., 180, 975 (1973a).CrossRefGoogle Scholar
Travis, L. D., and Matsushima, S., Astrophys. J., 182, 189 (1973b).CrossRefGoogle Scholar
Vitense, E., Z. f. Astrophys., 32, 135 (1953).Google Scholar
Zahn, J. P., ‘Solar Phenomena in Stars and Stellar Systems’, (D. Reidel Pub. Co.) p 123 (1981).CrossRefGoogle Scholar