Abstract
A Dicke-type microwave radiometer has been developed for daily measurement of solar flux at 2800 MHz. The antenna system, consists of a 5 foot parabolic dish with horn feed, is equatorially mounted and is capable of tracking the sun for about 8 hours each day. The dynamic range of the radiometer is such that even strong solar bursts (flux = 10,000 × 10−22 Watts m−2 Hz−1) can be recorded by using the receiver in the AGC mode.
The calibration procedure and the errors involved in the measurement of the solar flux are briefly discussed. Some sample records of solar bursts made by means of this equipment are presented.
Similar content being viewed by others
References
Kundu, M. R...Solar Radio Astronomy, Interscience Publishers, New York, 1965.
Medd, W. J. and Covington, A. E. “Discussion of 10·7cm solar radio flux measurement and an estimation of the accuracy,”Proc. I.R.E., No. 1, Jan, 1958,46, 112–18.
Kraus, J. D...Radio Astronomy, McGraw-Hill Book Company, New York, 1966.
Bhonsle, B. V., Alurkar, S. K., Narayanan, K. and Mattoo, S. K. “Two-element pha-seswitched interferometer at 110 MHz and 74 MHz,”J. Instn. Telecom. Engrs., No. 6, 1971,17, 217–25.
Kuz’min, A. D. and Salomonovich, A. E.Radio Astronomical Methods of Antenna Measurements, Academic Press, New York, 1966.
Author information
Authors and Affiliations
Additional information
Communicated by Dr. K. R. Ramanathan,f.a.sc.
Rights and permissions
About this article
Cite this article
Narayanan, K., Bhonsle, R.V. Microwave solar radiometer at 2800 MHz. Proc. Indian Acad. Sci. 74, 142–151 (1971). https://doi.org/10.1007/BF03047149
Received:
Issue Date:
DOI: https://doi.org/10.1007/BF03047149