An analysis of the data of the solar radio observations at 3.2 and 10 CM in the Purple Mountain Observatory

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Astronomical Observatories, Centimeter Waves, Radio Observation, Solar Radio Bursts, Solar Radio Emission, Data Correlation, Electromagnetic Noise Measurement, Error Analysis, Noise Temperature, Superhigh Frequencies, Variance (Statistics)

Scientific paper

Data of total solar radio radiation observations at 3.2 cm since 1966 in the Purple Mountain Observatory have been analyzed. Correlation analysis shows that in the course of one month, the standard variances of the daily solar noise temperature amount to plus or minus (2.2-3.9)%. The corresponding value at 10 cm amounts to plus or minus 4.1% in 1978. A relative rms difference of burst with peak value larger than 200 sfu is plus or minus 34% as compared with those of TYKW. Differences of burst peak times between ours and those of TYKW have been found to be plus or minus 0.2m. The variant error sources have also been analyzed.

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