Total Solar Radiation Recorder Observation of Total Solar Radiation

The most important source of many physical, chemical and biological processes on Earth comes from the total solar radiation. For example, the surface heat and moisture are related to the total solar radiation. Therefore, it is very necessary to study and calculate the total solar radiation. The total solar radiation observation data is very limited, and it is still necessary to use indirect calculation methods. First, it reviews the general method for calculating the total solar radiation in modern times, and then supplements some of the data that we believe have been given by more reasonable methods. The total solar radiation recorder has played an important role in the current observation process.

In order to calculate the total solar radiation, statistics are usually taken from stations at the same time for observations of sunlight or cloudiness and total solar radiation. Empirical formulas are derived. Based on empirical formulas, no solar radiation observation sites are calculated from the sunshine or cloud records. Total solar radiation. The principle of total solar radiation recorder is to use this observation method to calculate.

It is undoubtedly reasonable for the total solar radiation recorder to calculate the total solar radiation of the eye, because all factors of the total solar radiation are taken into consideration. When we were studying the heat balance of the ground in Guangdong, we calculated the sunny total solar radiation values between 180 and 180 degrees north latitude. Therefore, we have different atmospheric transparency coefficients for northern latitude 100-55: all the months of the year.

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