Abstract
We point out that in the case of sunspots, when Coulomb collisions are included, the reduction in lundqvist number due to anisotropic conductivity is several orders of magnitude less than the reduction estimated by De. This result suggests that, contrary to De's conclusion, sunspot conditions do permit efficient MHD wave propagation.
References
Alfvén, H. and Fälthammar, C.-G.: 1963,Cosmical Electrodynamics, Clarendon Press, Oxford, pp. 100, 179, 180.
Dalgarno, A. and Lane, N. F.: 1966,Astrophys. J. 145, 623.
De, Bibhas R.: 1976,Astrophys. Space Sci. 39, L43.
Mullan, D. J.: 1974,Astrophys. J. 187, 621.
Oster, L.: 1968,Solar Phys. 3, 543.
Parker, E. N.: 1974,Solar Phys. 36, 249.
Rouse, C. S.: 1968,Tables of Ionization Equilibrium Equation of State at Stellar Temperatures and Densities, Naval Res. Lab. Report 6756.
Spitzer, L.: 1962,Physics of Fully Ionized Gases, Interscience, New York, p. 133.
Wilson, P. R.: 1975,Solar Phys. 42, 333.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Mullan, D.J. A comment on ‘A comment on the damping of magnetohydrodynamic waves’ by Bibhas R. De. Astrophys Space Sci 44, L9–L11 (1976). https://doi.org/10.1007/BF00650489
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00650489