The solar irradiance is an important parameter for the entire earth climate system since it governs the physical processes at the land surface (i.e., glacier melting, potential evapotranspiration, and diurnal cycling development of the planetary boundary layer (PBL)), and impacts on water and energy balance in the earth atmosphere (Ramanathan et al., 2001;Rosenfeld, 2006aRosenfeld, , 2006b. One objective of the studies focusing on man-made climate change is to quantify the variation of surface solar irradiance directly and indirectly caused by air pollutants from anthropogenic emissions (Jing & Suzuki, 2018;Powers et al., 2017). Additionally, solar irradiance forecast plays a key role in accelerating the ongoing global transition from conventional energy to renewable energy (Jimenez et al., 2016). Therefore, representation of physical processes controlling solar irradiance in the atmospheric models is important to estimate the radiation budget of the earth system, assess climate change, and accelerate the common application of green energy.The accuracy of simulating solar irradiance damping by aerosols, clouds, and light-absorbing gases during the transport from the top of the atmosphere to the earth's surface is usually unsatisfactory (Feng & Wang, 2019). The uncertainty of the solar irradiance simulation in mesoscale and global models is believed to intimately link to cloud radiative effect (CRE) since clouds usually show much higher solar irradiance extinct efficiency and sharper evolution than the gases and aerosols (Paquin-Ricard et al., 2010;Ruiz-Arias et al., 2016). Simulation of cloud-solar irradiance effect consists of two parts: (a) simulating cloud properties and (b) quantifying the solar irradiance extinction in the cloudy atmosphere. Therefore, solar irradiance forecast is determined by three