... Entrainment-zone thickness (EZT), entrainment velocity w e (typically defined as the temporal rate of the ABL growth), and entrainment flux ratio A i (the negative ratio of entrainment to surface heat fluxes) are the three commonly-used parameters to describe entrainment processes in the atmospheric models (e.g., Fedorovich et al., 2004). In the past, most of the relevant entrainment studies were limited to laboratory experiments (e.g., Deardorff et al., 1980;Jonker and Jiménez, 2014), field measurements by using sodar (Beyrich and Gryning, 1998), radar profilers (Angevine et al., 1994;Cohn and Angevine, 2000), LiDAR (Flamant et al., 1997;Steyn et al., 1999;Hägeli et al., 2000;He et al., 2006;Träumner et al., 2011), and in-situ aircraft (Lenschow et al., 1999;de Arellano et al., 2004;Canut et al., 2010;Berkes et al., 2016), as well as numerical simulations with ABL bulk models (Conzemius and Fedorovich, 2006;Liu et al., 2016;Haghshenas et al., 2019) and large-eddy simulations (LESs) (e.g., Sullivan et al., 1998;Huang et al., 2011;Brooks and Fowler, 2012;Liu et al., 2018aLiu et al., , 2018bLiu et al., , 2019. Deardorff et al. (1980) found that the EZT normalized with the ABL height (ABLH) showed a strong relationship with w e normalized with the convective velocity scale (w * = [(g/θ 0 )z i Q s ] 1/3 ) from their laboratory experiments, and both showed a linear dependence on the Richardson number (Ri = (g/θ 0 ) ( Δθz i /w * 2 ) ), where g, θ 0 , Δθ, z i and Q s are gravitational acceleration constant, reference potential temperature value, potential temperature increment across the entrainment zone, the ABLH, and surface heat flux, respectively. ...