Vats, H. O; Deshpande, M. R; Mehta, M; Shah, C. R; Shah, K. J
(Astronomical Society of India, 1999)
The time series of solar radio emission at 2.8 GHz is analysed using correlation methods. The analysis showed that this type of time series can be used to infer the rotation period of the source (in this case solar corona). ...