“…It is increasingly recognised that atmospheric wind profiles and vertical wind shear are crucial to better understanding the more frequent extreme rainfall events (Huuskonen et al, 2014;Nash and Oakley, 2001;Weber et al, 1990), the intensification of clear-air turbulence associated with aircraft safety (Williams and Joshi, 2013), complicated aerosolcloud-precipitation interaction (Fan et al, 2009;Guo et al, 2016aGuo et al, , 2019Lee et al, 2016) and persistent particulatepollution episodes (Yang et al, 2019;Zhang et al, 2020). For the wind speed in the planetary boundary layer (PBL), the most striking feature is that the turning of winds with height dominates the whole PBL and beyond, which can be explained in terms of force vectors (drag, pressure gradient force, Coriolis force) at the surface and the top of the PBL (pressure gradient force and Coriolis force) (LeMone et al, 2018). Under the influence of large-scale dynamic forcing and land surface processes, wind speed and direction will dramatically vary (Michelson and Bao, 2008), which poses a great challenge for models to simulate or forecast the variation in wind very well, especially in the PBL (Constantinescu et al, 2009;Guo et al, 2016b;Liu et al, 2017).…”