
%0 Journal Article
%A Swarup, G 
%A Parthasarathy, R 
%T Solar Brightness Distribution at a Wavelength of 60 Centimetres. II. Localized Radio Bright Regions
%J Australian Journal of Physics
%D 1958/09/01
%V 11
%N 3
%P 338-349
%K 
%R https://doi.org/10.1071/PH580338
%U https://www.publish.csiro.au/paper/PH580338 
%X The localized radio bright regions on the Sun which give rise to a slowly varying component of the solar radiation were studied at a wavelength of 60 cm, using a 32-aerial interferometer with a beamwidth of 8·7 min of arc. The observations were undertaken during July 1954 to March 1955 and were limited in number due to this being a minimum period of the solar cycle. The low activity, however, provided the advantage of simple interpretation as often only one region was present on the solar disk. 
