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Non-linear Convection with Hexagonal Planform

Published online by Cambridge University Press:  25 April 2016

J. O. Murphy
J. O. Murphy*
Affiliation:
Department of Mathematics, Monash University, Melbourne
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Extract

Observations of the solar surface indicate a cellular structure, photospheric granulation, which, as suggested by Wilson and others, could arise from a shallow convection layer. The basic observed granulation pattern has been likened to a hexagonal cell type structure.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 2 , Issue 1 , July 1971 , pp. 53 - 54
Copyright
Copyright © Astronomical Society of Australia 1971

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References

1 Wilson, P. R., Solar Physics, 9, 303 (1969).Google Scholar
2 Murphy, J. O., Proc. ASA, 2, 51 (1971).Google Scholar
3 Roberts, P. H., ‘Non-Equilibrium Thermodynamics, Variational Techniques and Stability’, University of Chicago Press, Chicago 1966 p. 125.Google Scholar
4 Chandrasekhar, S., ‘Hydrodynamic and Hydromagnetic Stability’, Oxford University Press 1961 p. 47.Google Scholar