Abstract
The expansion of the solar corona, with the aid of hydrodynamic blast wave theory using the concept of the Roche model, is studied here when both the solar gravity and radiation heat flux are taken into consideration.
Similar content being viewed by others
References
Carrus, P. A., Fox, P. A., Haas, F. and Kopal, Z.: 1951,Astrophys. J. 113, 193.
Deb Ray, G.: 1966,Bull. Nat. Inst. Sci. 31A (No. 3), 55.
Deb Ray, G. and Bhowmick, J. B.: 1976,Indian J. Pure Appl. Math. 7 (No. 1).
Parker, E. N.: 1961,Astrophys. J. 133, 1014.
Taylor, G. I.: 1950,Proc. Roy. Soc. A201, 159.
Wang, K. C.: 1966,Phys. Fluids 9, 1922.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Bhowmick, J.B. A study of the expansin of the solar corona with radiation heat flux. Astrophys Space Sci 70, 433–439 (1980). https://doi.org/10.1007/BF00639567
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00639567