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The cooling of flare produced plasmas in the solar corona

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Abstract

Solar flare X-rays, at energies less than 10 keV, are emitted by hot plasmas located in the corona. Three plasma cooling models are examined in detail. The cooling of the electrons by Coulomb collisions with ions at a lower temperature would require the observed material to occupy very large volumes. Cooling could take place by conduction or by radiation and observations are proposed which would allow the dominant cooling mechanism to be established.

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References

  • Batstone, R., Evans, K., Parkinson, J., and Pounds, K. A.: 1970, Solar Phys. 13, 389.

    Google Scholar 

  • Beigman, I. E., Grineva, I., Mandel'stam, S. L., Vainstein, L. A., and Zitnik, I. A.: 1969, Solar Phys. 9, 160.

    Google Scholar 

  • Cox, D. P. and Tucker, W. H.: 1969, Astrophys. J. 157, 1157.

    Google Scholar 

  • Culhane, J. L.: 1969, Monthly Notices Roy. Astron. Soc. 144, 375.

    Google Scholar 

  • Culhane, J. L. and Acton, L. W.: 1970, submitted for publication to Monthly Notices Roy. Astron. Soc.

  • Culhane, J. L. and Phillips, K. J. H.: 1970, Solar Phys. 11, 117.

    Google Scholar 

  • Culhane, J. L., Sanford, P. W., Willmore, A. P., Blades, J., and Nettleship, R.: 1967, IEEE Trans. Nucl. Sci. NS14, 38.

    Google Scholar 

  • De Jager, C.: 1964, Paper presented at IAU Symposium No. 23, Liège.

  • Doschek, G. A. and Meekins, J. F.: 1970, Solar Phys. 13, 220.

    Google Scholar 

  • Freeman, F. F., Gabriel, A. H., Jones, B. B., and Jordan, C.: 1970, to be published by the Royal Society.

  • Frost, K.: 1969, Astrophys. J. 158, L159.

    Google Scholar 

  • Gabriel, A. and Jordan, C.: 1969, Monthly Notices Roy. Astron. Soc. 145, 241.

    Google Scholar 

  • Hudson, H. S., Peterson, L. E., and Schwartz, D. A.: 1969, Astrophys. J. 157, 389.

    Google Scholar 

  • Kane, S.: 1969, Astrophys. J. 157, L139.

    Google Scholar 

  • Karzas, W. J. and Latter, R.: 1961, Astrophys. J. Suppl. Ser. 6, 167.

    Google Scholar 

  • Meekins, J. F., Kreplin, R. W., Chubb, T. A., and Friedman, H.: 1968, Science 162, 891.

    Google Scholar 

  • Neupert, W. M., White, W. A., Gates, W. J., Schwartz, M., and Young, R. M: 1969, Solar Phys. 6, 183.

    Google Scholar 

  • Oster, L. and Sofia, S.: 1966, Astrophys. J. 143, 944.

    Google Scholar 

  • Rugge, H. W. and Walker, A. B. C.: 1968, Space Res. 8, 439.

    Google Scholar 

  • Spitzer, L.: 1962, The Physics of Fully Ionized Gases, 2nd ed., Interscience, New York.

    Google Scholar 

  • Vaiana, G. S., Reidy, W. P., Zehnpfennig, L., Van Speybroeck, L., and Giaconni, R.: 1968, Science 161, 564.

    Google Scholar 

  • Walker, A. B. C., Jr. and Rugge, H. R.: 1970, Astron. Astrophys. 5, 4.

    Google Scholar 

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On leave during a portion of this work as University Research Fellow in Astronomy, University of Leicester, England.

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Culhane, J.L., Vesecky, J.F. & Phillips, K.J.H. The cooling of flare produced plasmas in the solar corona. Sol Phys 15, 394–413 (1970). https://doi.org/10.1007/BF00151847

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  • DOI: https://doi.org/10.1007/BF00151847

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