Log in

Association between gradual hard X-Ray emission and metric continua during large flares

  • Articles
  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

X-ray radiation is used to study coronal phenomena in conjunction with meter wave observations during some large solar flares. It is found that metric flare continua and moving type IV bursts are associated with gradual and long lasting (a few tens of minutes) microwave and hard X-ray emissions. The detailed temporal analysis reveals that although metric and hard X-ray sources are located at very different heights, both kinds of emission result from a common and continuous/repetitive injection of electrons in the corona. The late part of the metric event (stationary type IV burst) is only associated with soft X-ray radiation. This indicates that the mean energy of the radiating electrons is lower during stationary type IV bursts than during the earlier parts of the event.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Subscribe and save

Springer+ Basic
EUR 32.99 /Month
  • Get 10 units per month
  • Download Article/Chapter or Ebook
  • 1 Unit = 1 Article or 1 Chapter
  • Cancel anytime
Subscribe now

Buy Now

Price includes VAT (Germany)

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Anderson, K. A., Kane, S. R., Primbsh, J. H., Weitzman, R. H., Evans, W. D., Klebesadel, R. W., and Aiello, W. P.: 1978, IEEE Trans. GE-16, 157.

    Google Scholar 

  • Frost, K. J.: 1974, in G. Newkirk (ed.), ‘Coronal Disturbances’, IAU Symp. 57, 421.

  • Frost, K. J. and Dennis, B. R.: 1971, Astrophys. J. 165, 655.

    Google Scholar 

  • Hudson, H. S.: 1978, Astrophys. J. 224, 235.

    Google Scholar 

  • Hudson, H. S., Lin, R. P., and Stewart, R. T.: 1982, Solar Phys. 75, 245.

    Google Scholar 

  • Kane, S. R., Pick, M., and Raoult, A.: 1980, Astrophys. J. Letters 241, L113.

    Google Scholar 

  • Kane, S. R., Fenimore, E. E., Klebesadel, R. W., and Laros, J. G.: 1982, Astrophys. J. Letters 254, L53.

    Google Scholar 

  • Kosugi, T.: 1981, Solar Phys. 71, 91.

    Google Scholar 

  • Krüger, A.: 1979, Introduction to Solar Radio Astronomy and Radio Physics, D. Reidel Publ. Co., Dordrecht, Holland.

    Google Scholar 

  • Lantos, P., Kerdraon, A., Rapley, C. G., and Bentley, R. D.: 1981, Astron. Astrophys. 101, 33.

    Google Scholar 

  • Pick, M.: 1961, Ann. Astrophys. 24, 183.

    Google Scholar 

  • Radioheliograph Group: 1977, Solar Phys. 55, 251.

    Google Scholar 

  • Robinson, R. D.: 1978, Australian J. Phys. 31, 553.

    Google Scholar 

  • Stewart, R. T., Wolfson, C. J., and Lemen, J. R.: 1980, New Zealand Journal of Science.

  • Švestka, Z., Dennis, B. R., Pick, M., Raoult, A., Rapley, C. G., Stewart, R. T., and Woodgate, C. E.: 1982, Solar Phys. 80, 143.

    Google Scholar 

  • Vilmer, N., Kane, S. R., and Trottet, G.: 1982, Astron. Astrophys. 108, 306.

    Google Scholar 

  • Wild, J. P.: 1970, Proc. Astron. Soc. Australia 1, 365.

    Google Scholar 

  • Wild, J. P., Smerd, S. F., and Weiss, A. A.: 1963, Ann. Rev. Astron. Astrophys. 1, 291.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Klein, L., Anderson, K., Pick, M. et al. Association between gradual hard X-Ray emission and metric continua during large flares. Sol Phys 84, 295–310 (1983). https://doi.org/10.1007/BF00157463

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00157463

Keywords

Navigation