Abstract
The spectral indices of microwave and hard X-ray emissions of a solar flare are found to correlate. Their observed values are in agreement with the expected relation from synchrotron and bremsstrahlung theory. These results are considered as strong evidence for the synchrotron mechanism in the microwave flare, contrary to recent alternative suggestions.
Similar content being viewed by others
References
Aschwanden, M. J., Wiehl, H. J., Benz, A. O., and Kane, S. R.: 1984, submitted toSolar Phys.
Benz, A. O.: 1977,Astrophys. J. 211, 270.
Benz, A. O. and Tarnstrom, G. L.: 1976,Astrophys. J. 204, 597.
Brown, J. C.: 1971,Solar Phys. 18, 689.
Castelli, J. P. and Guidice, D. A.: 1976,Vistas Astron. 19, 355.
Hoyng, P., Brown, J. C., and van Beek, H. F.: 1976,Solar Phys. 58, 197.
Klein, K. L. and Trottet, G.: 1984,Astron. Astrophys., in press.
Mätzler, C.: 1978,Astron. Astrophys. 70, 181.
Smith, D. F. and Spicer, D. C.: 1979,Solar Phys. 62, 359.
Takakura, T.: 1984, in Chen Biao and C. de Jager (eds.),Workshop on Solar Physics and Interplanetary Travelling Phenomena, Kunming, China, in press.
Zaitsev, V. V. and Stepanov, A. V.: 1983,Solar Phys. 88, 297.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Benz, A.O. Synchrotron or plasma emission in solar microwave flares?. Sol Phys 94, 161–163 (1984). https://doi.org/10.1007/BF00154817
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00154817