An Analysis of the Accuracy of Solar Radio Observations at 9375MHz,3653MHz and 2902MHz at Yunnan Observatory from 1981 November to 1982 December

In this paper the correlation analysis is made between the antenna temperature of solar radio burst Observations,at 9375MHz,3653MHz and 2902MHz from November in 1981 to December in 1982 at Yunnan Observatory and that of the Sagamore Hill system of USAF.The results show that the r.m.s.errors of the total flux density at 9375MHz,3653MH^and 2902MHz are ±4.9%,±4.6% and ±4.8% respectively.The burst observations at 9375MHz and 2902 MHz are correlated with those of Purple Mountain Observatory,with the results showing that the r.m.s.errors of the peak flux density of solar radio bursts are ±15.9% and 19.9%,respectively.The time accuracy of the burst pealc is within the limit of ±0^m.l.