K. R. Subramanian
Articles written in Journal of Astrophysics and Astronomy
Volume 2 Issue 1 March 1981 pp 59-65
Observations on the pulsation pattern in the time profile of short duration solar radio bursts at decametre wavelengths are presented. The pulsations are found to be present predominantly in the saturation phase of the burst. A tentative physical model based on the non-linear development of the waves interacting in a turbulent medium is invoked to explain the origin of the pulsations.
Volume 9 Issue 4 December 1988 pp 225-229
The low-frequency radio spectrum of the continuum emission from the undisturbed Sun is determined for 24 days during the period 1985 May-September. It is found that the spectral index varied from + 1.6 to +3.6 during this period. It is suggested that the large positive spectral indices are due to the existence of temperature gradients in the outer corona.
Volume 21 Issue 3-4 September 2000 pp 421-422
Volume 40 | Issue 3
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