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A model for drift pair and hook burst emission from the solar corona

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Abstract

Combination scattering of the Cerenkov plasma waves generated by a fast electron beam on the electron density fluctuations in a magnetoactive plasma is assumed to be the cause of the emission of the drift pair (or the hook burst) from the solar corona. The features of the combination emission are studied numerically with parameters appropriate to the solar corona condition. It is found that the major properties of the drift pair and the hook burst can be accounted for.

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References

  • Allen, C. W.: 1947, Monthly Notices Roy. Astron. Soc. 107, 426.

    Google Scholar 

  • Ellis, G. R. A.: 1969, Australian J. Phys. 22, 177.

    Google Scholar 

  • Ellis, G. R. A. and McCulloch, P. M.: 1967, Australian J. Phys. 20, 583.

    Google Scholar 

  • Ginzburg, V. L.: 1964, The Propagation of Electromagnetic Waves in Plasmas, Pergamon, New York.

    Google Scholar 

  • Ginzburg, V. L. and Zheleznyakov, V. V.: 1958, Soviet Astron. AJ2, 653.

    Google Scholar 

  • Fokker, A. D.: 1964, Solar System Radio Astronomy (ed. by J. Aarons), Plenum Press, New York, p. 171.

    Google Scholar 

  • Fung, P. C. W. and Yip, W. K.: 1966, Australian J. Phys. 19, 759.

    Google Scholar 

  • Newkirk, G.: 1967, Ann. Rev. Astron. Astrophys. 5, 213.

    Google Scholar 

  • Noë, J. De La, and Møller Pedersen, B.: 1971, Astron. Astrophys. 12, 371.

    Google Scholar 

  • Roberts, J. A.: 1958, Australian J. Phys. 11, 215.

    Google Scholar 

  • Smerd, S. F., Wild, J. P., and Sheridan, K. V.: 1962, Australian J. Phys. 15, 180.

    Google Scholar 

  • Shafranov, V. D.: 1967, Reviews of Plasma Physics, Consultants Bureau, New York, 3, 1.

    Google Scholar 

  • Sitenko, A. G. and Kirochkin, Yu. A.: 1966, Soviet Phys. Usp. 9, 430.

    Google Scholar 

  • Yip, W. K.: 1970a, Planetary Space Sei. 18, 479.

    Google Scholar 

  • Yip, W. K.: 1970b, Australian J. Phys. 23, 161.

    Google Scholar 

  • Yip, W. K.: 1970c, Planetary Space Sei. 18, 867.

    Google Scholar 

  • Zheleznyakov, V. V.: 1965, Soviet Astron. AJ 9, 191.

    Google Scholar 

  • Zheleznyakov, V. V. and Zaitsev, V. V.: 1970a, Soviet Astron. AJ 14, 47.

    Google Scholar 

  • Zheleznyakov, V. V. and Zaitsev, V. V.: 1970b, Soviet Astron. AJ 14, 250.

    Google Scholar 

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Authors and Affiliations

  1. Dept. of Physics, University of Otago, Dunedin, New Zealand

    W. K. Yip

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  1. W. K. Yip
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Yip, W.K. A model for drift pair and hook burst emission from the solar corona. Sol Phys 24, 197–209 (1972). https://doi.org/10.1007/BF00231096

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  • DOI: https://doi.org/10.1007/BF00231096

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