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Transition radio emission of mildly relativistic particles

  • Fragmented Solar Emission
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Abstract

We report new calculations of transition radiation spectra which are correct for arbitrary energy of a particle at all frequencies down to plasma frequency. The importance of the emission mechanism for solar flares are discussed.

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References

  • Ginzburg, V.L., Tsytovich, V.N.: 1990,Transition Radiation and Transition Scattering, Adam Hilger

  • Fleishman G.D., Kahler S.W.: 1992,Astrophys. J. 394, 688

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  • Platonov, K.Yu., and Fleishman, G.D.: 1994,Zhurn. Exper. Theor. Fiz., in press (transl.: Sov. Phys. JETP, 1994.)

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Authors and Affiliations

  1. Ioffe Physico-Technical Institute, 194021, St. Petersburg, Russia

    G. D. Fleishman

  2. State Technical University, 195251, St. Petersburg, Russia

    K. Yu. Platonov

Authors
  1. G. D. Fleishman
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  2. K. Yu. Platonov
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Fleishman, G.D., Platonov, K.Y. Transition radio emission of mildly relativistic particles. Space Sci Rev 68, 243–244 (1994). https://doi.org/10.1007/BF00749145

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  • DOI: https://doi.org/10.1007/BF00749145

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