Abstract
The positions and motions of solar bursts in the range 20 to 60 MHz have been measured by the means of a sweep-frequency grating interferometer with angular resolution of 5′ arc at 60 MHz decreasing to 15′ arc at 20 MHz. The positional characteristics of the decameter wavelength bursts are discussed in terms of the commonly accepted theories of the origin of radio bursts from plasma and synchrotron radiations.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Kundu, M. R.: 1965, Solar Radio Astronomy, John Wiley-Interscience Publishers, p. 329.
Ramaty, R. and Lingenfelter, R. E.: 1967, J. Geophys. Res. 72, 879.
Smerd, S. F., Wild, J. P. and Sheridan, K. V.: 1962, Australian J. Phys. 15, 180.
Weiss, A. A.: 1963, Australian J. Phys. 16, 526.
Weiss, A. A. and Stewart, R. T.: 1965, Australian J. Phys. 18, 143.
Wild, J. P., Sheridan, K. V., and Neylan, A. A.: 1959, Australian J. Phys. 12, 369.
Zheleznyakov, V. V. and Zaitsev, V. V.; 1968, Soviet Astron.-AJ 12, 14.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Kundu, M.R., Erickson, W.C., Jackson, P.D. et al. Positions and motions of solar bursts at decameter wavelengths. Sol Phys 14, 394–403 (1970). https://doi.org/10.1007/BF00221325
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF00221325