The total solar irradiance (TSI) refers to the sum of the solar electromagnetic radiation energy of all wavebands reaching the top of the earth's atmosphere per unit area in unit time at the average distance between the sun and the earth (Biktash & Lilia, 2017). Although the solar radiation energy received by the earth is only one in two billion of the total radiation energy from the sun to the space, but it is the main energy source of the earth's atmospheric movement, it is the most important energy source of the earth's atmospheric movement and an important external driving factor of global climate change (Haigh, 2007;Kren, 2015;Solanki et al., 2013). Before Hickey-Frieden cavity radiator (HF) was used to observe the solar radiation in October 1978, TSI was regarded as a constant due to the low accuracy of ground observation equipment, so it was called "solar constant." Since HF was launched, TSI has been continuously observed by several radiometers. Due to the high accuracy of these space radiometers, it is recognized that the solar radiation varies from several minutes to several decades (Kopp, 2016). TSI produces the earth's radiation environment and affects the earth's temperature and atmosphere, even a small change in TSI will have a profound impact on the earth's climate (