Abstract
We present observations of the ‘quiet’ Sun close to the recent solar minimum (Cycle 22), with the Gauribidanur radioheliograph. Our main conclusion is that coronal streamers also influence the observed radio brightness temperature.
This is a preview of subscription content, log in via an institution to check access.
Similar content being viewed by others
References
Aubier, M., Leblanc, Y., Boischot, A. 1971,Astr. Astrophys.,12, 435.
Borkowski, K. M. 1982,Sol. Phys.,81, 207.
Erickson, W. C., Gergely, T. E., Kundu, M. R., Mahoney, M. J. 1977,Sol. Phys.,54, 57.
Ramesh, R., Subramanian, K. R., Sundararajan, M. S., Sastry, Ch. V. 1998,Sol. Phys.,181, 439.
Ramesh, R. 1999,Ph.D. thesis, Bangalore University.
Riddle, A. C. 1974,Sol. Phys.,36, 375.
Sastry, Ch. V, Dwarakanath, K. S., Shevgaonkar, R. K., Krishnan, V. 1981,Sol. Phys.,73, 363.
Sastry, Ch. V., Shevgaonkar, R. K., Ramanuja, M. N. 1983,Sol. Phys.,87, 391.
Sastry, Ch. V. 1994,Sol. Phys.,150, 285.
Sheridan, K. V. 1970,Proc. Astr. Soc. Australia,1, 304.
Thejappa, G., Kundu, M. R. 1992,Sol. Phys.,140, 19.
Thejappa, G., Kundu, M. R. 1994,Sol. Phys.,149, 31.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Ramesh, R. Low frequency radio emission from the ‘quiet’ Sun. J Astrophys Astron 21, 237–240 (2000). https://doi.org/10.1007/BF02702398
Issue Date:
DOI: https://doi.org/10.1007/BF02702398