Marine boundary layer (MBL) clouds cover 30% of the Earth's surface and strongly influence the Earth's radiative budget by reflecting significant amount of solar radiation back to space (Wood, 2012). It is estimated that only 4% change of the low-level clouds amount can offset the warming effect caused by doubling CO 2 concentration (Randall et al., 1984). Thus, an accurate estimation of the MBL clouds feedbacks is essential for the future climate prediction (Bony & Dufresne, 2005;Cess et al., 1990;Stephens, 2005). However, MBL clouds are a delicate, complex system with dynamics and microphysics closely interacts with each other across a wide range of scales from millimeter to thousands of kilometers (Khain & Pinsky, 2018). Several processes that act at small-scales and affect MBL clouds are poorly observed and poorly parameterized in climate models, which leads to large uncertainties in the MBL clouds representation and feedbacks (Glassmeier & Feingold, 2017;Randall, 1989).Turbulence is ubiquitous in MBL clouds and can be generated by surface forcing, cloud top radiative cooling, and wind shear (Mellado, 2017). Turbulence at various scales closely interact with the cloud microphysics and plays an important role on rain formation, cloud dissipation, and Stratocumulus (Sc)-Cumulus (Cu) transition process (Bodenschatz et al., 2010;Grabowski & Wang, 2013). For example, turbulence at small scales is known to enhance the collision-coalescence (C-C) mechanism, broaden the drop size distribution (DSD) and trigger precipitation (Chen et al., 2018;Pinsky et al., 2008;Shaw, 2003). Specifically, it is estimated that in shallow cumulus clouds with eddy dissipation rate (EDR) on the order of 10 −2 m 2 s −3 , the presence of turbulence can enhance the collision efficiency and shorten the drizzle formation time by 40%