Abstract
Assumptions inherent in the determination of coronal temperature from the decay rate of type III radio bursts are examined. It is suggested that no reliable temperature estimates can yet be made.
Similar content being viewed by others
References
Alvarez, H. and Haddock, F. T.: 1973, Solar Phys. 30, 175.
Aubier, M. and Boischot, A.: 1972, Astron. Astrophys. 19, 343.
Caroubalos, C., Aubier, M., Leblanc, Y., and Steinberg, J. L.: 1972, Astron. Astrophys. 16, 374.
Chambe, C. and Lantos, P.: 1971, Solar Phys. 17, 197.
Ginzburg, V. L. and Zheleznyakov, V. V.: 1958, Soviet Astron. AJ 2, 653.
Haddock, F. G. and Graedel, T. F.: 1970, Astrophys. J. 160, 273.
Hartz, T. R.: 1969, Planetary Space Sci. 17, 267.
Harvey, C. C. and Aubier, M. G.: 1973, Astron. Astrophys. 22, 1.
Hirshberg, J.: 1973, Rev. Geophys. Space Phys. 11, 115.
Lin, P., Evans, L., and Fainberg, J.: 1973, Astrophys. Letters 14, 191.
Riddle, A. C.: 1974, submitted to Solar Phys.
Scheuer, P. G.: 1960, Monthly Notices Roy. Astron. Soc. 120, 231.
Smith, D. F.: 1970, Adv. Astron. Astrophys. 7, 147.
Steinberg, J. L., Aubier, G. M., Leblanc, Y., and Boischot, A.: 1971, Astron. Astrophys. 10, 362.
Sturrock, P. A.: 1964, in W. N. Hess (ed.), Physics of Solar Flares, AAS-NASA Symp., Washington: NASA SP-50, p. 357.
Tarnstrom, G. L. and Philip, K. W.: 1972, Astron. Astrophys. 17, 267.
Wolff, C. L., Brandt, J. C., and Southwick, R. G.: 1971, Astrophys. J. 165, 18.
Zaitsev, V. V., Mityakov, N. A., and Rapoport, V. O.: 1972, Solar Phys. 24, 444.
Zheleznyakov, V. V. and Zaitsev, V. V.: 1970, Soviet Astron. AJ 14, 250.
Author information
Authors and Affiliations
Additional information
Exchange visitor from Division of Radiophysics, CSIRO, P.O. Box 76, Epping, N.S.W., 2121, Australia.
Rights and permissions
About this article
Cite this article
Riddle, A.C. On the determination of coronal temperature from the decay of type III radio bursts. Sol Phys 34, 181–184 (1974). https://doi.org/10.1007/BF00149609
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00149609