Abstract
Numerical solution of the interaction of evolutionary electron beam with coronal plasma shows that the velocity of packet of the generated Langmuir's waves increases with the increase of coronal temperature. This effect can be manifested by a dependence of the drift of type III bursts on the coronal temperature.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Kane, S. R. and Anderson, K. A.: 1970, Astrophys. J. 162, 1003.
Lin, R. P.: 1974, Space Sci. Rev. 16, 189.
Magelssen, G. R. and Smith, D. F.: 1977, Solar Phys. 55, 211.
Takakura, T. and Shibahashi, H.: 1976, Solar Phys. 46, 323.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Karlický, M. Type III bursts and coronal temperature. Sol Phys 71, 381–384 (1981). https://doi.org/10.1007/BF00167559
Received:
Revised:
Issue Date:
DOI: https://doi.org/10.1007/BF00167559