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Acceleration, Containment and Emission of High Energy Flare Particles: Radio Evidence

Published online by Cambridge University Press:  25 May 2016

A. Boischot
A. Boischot*
Affiliation:
Observatoire de Meudon, France

Abstract

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The existence of non thermal radio bursts provide evidences for the acceleration of electrons in the solar atmosphere.

It is shown, from the characteristics of the bursts, that the electrons are accelerated in at least four different phases:

  1. (1) An impulsive phase which gives μib and III bursts.

  2. (2) A gradual phase which gives μIV and S1IV bursts.

  3. (3) A quasi-continuous phase which gives S2IV bursts and noise storms.

  4. (4) An acceleration by shock waves gives type II bursts.

  5. (5) Eventually, another shock-wave acceleration giving the moIV burst.

Type
Part IV Acceleration, Containement and Emission of High-Energy Flare Particles
Information
Symposium - International Astronomical Union , Volume 57: Coronal Disturbances , 1974 , pp. 423 - 435
Copyright
Copyright © Reidel 1974 

References

Akinyan, S. T., Mogilevsky, E. I., Bohme, A., and Krüger, A.: 1971, Solar Phys. 20, 112.CrossRefGoogle Scholar
Anderson, K. A.: 1969, Solar Phys. 6, 111.Google Scholar
Axisa, F.: 1974, Solar Phys. 35, 207.Google Scholar
Bohme, A.: 1972, Solar Phys. 25, 478.CrossRefGoogle Scholar
Boischot, A. and Clavelier, B.: 1968, Ann. Astrophys. 31, 445.Google Scholar
Boischot, A., De la Noë, J., Du Chaffaut, M., and Rosolen, C.: 1971, Compt. Rend. Acad. Sci. 272, 166.Google Scholar
Boischot, A., De la Noë, J., and Pedersen, B. M.: 1970, Astron. Astrophys. 4, 159.Google Scholar
De Feiter, L. D.: 1972, Space Sci. Rev. 13, 827.Google Scholar
De la Noë, J. and Boischot, A.: 1972, Astron. Astrophys. 20, 55.Google Scholar
Kane, S. R.: 1972, Solar Phys. 27, 174.Google Scholar
Krüger, A.: 1972, Physics of Solar Continuum Radiobursts, Academic Verlag, Berlin.Google Scholar
Kundu, M. R.: 1959, Ann. Astrophys. 22, 1.Google Scholar
Kundu, M. R.: 1965, Solar Radio Astronomy, Interscience Publ., New York.Google Scholar
Lacombe, C. and Mangeney, A.: 1969, Astron. Astrophys. 1, 325.Google Scholar
Leblanc, Y., Kuiper, T. B. H., and Hansen, S.: 1974, this volume, p. 227.Google Scholar
Lin, R. P.: 1972, in Ramaty, R. and Stone, R. G. (eds.), Proc. of High Energy Phenomena on the Sun, GSFC Preprint X-693–73–193, p. 439.Google Scholar
Lin, R. P., Evans, L. G., and Fainberg, J.: 1973, Astrophys. Letters 14, 191.Google Scholar
Mangeney, A.: 1974, this volume, p. 387.Google Scholar
McDonald, F. B.: 1970, in Manno, and Page, (eds.), Intercorrelated Satellite Observations Related to Solar Events, D. Reidel Publ. Co., Dordrecht, Holland, p. 34.Google Scholar
Peterson, L. E., Datlowe, D. W., and McKenzie, D. L.: 1973, in Ramaty, R. and Stone, R. G. (eds.), Proc. of High Energy on the Sun, GSFC Preprint X-693–73–193, p. 132.Google Scholar
Pick, M.: 1961, Ann. Astrophys, 24, 183.Google Scholar
Ramaty, R. and Petrosian, D.: 1972, Astrophys. J. 178, 241.Google Scholar
Schmahl, E. J.: 1972, Proc. Astron. Soc. Australia 2, 95.CrossRefGoogle Scholar
Slottje, C.: 1972, Solar Phys. 25, 210.Google Scholar
Smerd, S. F. and Dulk, G. A.: 1971, in Howard, R. (ed.), ‘Solar Magnetic Fields’, IAU Symp. 49, 616.Google Scholar
Smith, D. F. and Pneuman, G. W.: 1972, Solar Phys. 25, 461.Google Scholar
Stewart, R. T. and Labrum, N. R.: 1972, Solar Phys. 27, 192.Google Scholar
Stone, R. G. and Fainberg, J.: 1973, in Ramaty, R. and Stone, R. G. (eds.), Proc. of High Energy Phenomena on the Sun, GSFC Preprint X-693–73–193, p. 519.Google Scholar
Sturrock, P. A.: 1972, Solar Phys. 23, 438.Google Scholar
Takakura, T.: 1967, Solar Phys. 1, 304.Google Scholar
Takakura, T.: 1972, Solar Phys. 26, 151.Google Scholar
Takakura, T.: 1973, in Ramaty, R. and Stone, R. G. (eds.), Proc. of High Energy Phenomena on the Sun, GSFC Preprint X-693–73–193, p. 179.Google Scholar
Warwick, J. W.: 1968, Solar Phys. 5, 111.Google Scholar
Wild, J. P. and Smerd, S. F.: 1972, Ann. Rev. Astron. Astrophys. 10, 169.Google Scholar
Wild, J. P., Smerd, S. F., and Weiss, A. A.: 1963, Ann. Rev. Astron. Astrophys. 1, 291.Google Scholar