Skip to main content
Log in

An analysis of type III burst occurrence in spotless regions

  • Published:
Solar Physics Aims and scope Submit manuscript

Abstract

An analysis has been carried of the correlation of the occurrence of type III bursts and flares in spotless regions over the past ten years. As a comparison, the same study has been performed also for flares covering major sunspot umbrae (i.e. in magnetic conditions presumably opposite to the above).

The results show a very low correlation of the former flares with type III bursts (8%) and a higher than average value for the latter flares (36% against the normally accepted 25%). Thus an important role of the ambient magnetic field on the generation of type III events seems well established.

The effect of the presence of surges and of rapid brightness rises (‘flash-phases’) on the correlation with these bursts has been examined: both features appear to improve the correlation.

Some considerations regarding the results of other researches as compared to this one are outlined.

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

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

References

  • Abrami, A. and Zlobec, P.: 1968, Mem.S.A.It. XXXIX(4), 557.

    Google Scholar 

  • Axisa, F.: 1974, Solar Phys. 35, 207.

    Google Scholar 

  • Benz, A. O., Berney, M., and Santin, P.: 1977, Astron. Astrophys. 56, 123.

    Google Scholar 

  • Bruzek, A.: 1974, in G. Newkirk (ed.), ‘Coronal Disturbances’, IAU Symp. 57, 323.

  • De Jager, C.: 1969, in C. de Jager and Z. Švestka (eds.), Solar Flares and Space Research, COSPAR Symp., North-Holland, p. 1.

  • Dodson, H. W. and Hedeman, R. H.: 1970, Solar Phys. 13, 401.

    Google Scholar 

  • Giovannelli, R. G. and McCabe, M. K.: 1958, Australian J. Phys. 11, 191.

    Google Scholar 

  • Kahler, S. W.: 1973, Solar Phys. 32, 477.

    Google Scholar 

  • Kane, S. R.: 1972, Solar Phys. 27, 174.

    Google Scholar 

  • Kuiper, T. B.: 1973, Solar Phys. 33, 461.

    Google Scholar 

  • Kuiper, T. B. and Pasachoff, J. M.: 1973, Solar Phys. 28, 187.

    Google Scholar 

  • Loughhead, R. E., Roberts, J. A., and McCabe, M. K.: 1957, Australian J. Phys. 10, 483.

    Google Scholar 

  • Malville, J. M.: 1962, Astrophys. J. 135, 834.

    Google Scholar 

  • Moreton, G. E. and Ramsey, H. E.: 1960, Publ. Astron. Soc. Pacific 72, 357.

    Google Scholar 

  • Sakurai, K.: 1971, Solar Phys. 16, 125.

    Google Scholar 

  • Smith, H. J. and Smith, E. V. P.: 1963, Solar Flares, McMillan, New York, U.S.A.

    Google Scholar 

  • Švestka, Z.: 1976, Solar Flares, D. Reidel Publ. Co., Dordrecht, Holland.

    Google Scholar 

  • Swarup, G., Stone, P. H., and Maxwell, A.: 1960, Astrophys. J. 131, 725.

    Google Scholar 

  • Vorpahl, J. A.: 1973, Solar Phys. 29, 447.

    Google Scholar 

  • Vorpahl, J. A. and Zirin, H.: 1970, Solar Phys. 11, 285.

    Google Scholar 

  • Zirin, H.: 1966, The Solar Atmosphere, Blaisdell, Waltham, U.S.A.

    Google Scholar 

  • Zlobec, P.: 1970, Mem.S.A.It. XLI(2), 205.

    Google Scholar 

Download references

Author information

Authors and Affiliations

Authors

Rights and permissions

Reprints and permissions

About this article

Cite this article

Zanelli, C., Zlobec, P. & Koren, U. An analysis of type III burst occurrence in spotless regions. Sol Phys 65, 387–396 (1980). https://doi.org/10.1007/BF00152801

Download citation

  • Received:

  • Revised:

  • Issue Date:

  • DOI: https://doi.org/10.1007/BF00152801

Keywords

Navigation