Abstract:
A solar radio spectrograph has been developed to observe the transient solar radio emissions in the band of 30 MHz at our School of Physics. A non trackable log periodic antenna having beam of 60 degree in E-W and 90 degree in N-S is being used. The recent solar eclipse of October 24, 1995 was observed with maximum obstruction of sun's disc by moon to the tune of 40% using the above radio spectrograph. The initial results have been reported in this paper.