Surface pressure is one of the basic meteorological variables in atmospheric science. Differing from other surface physical quantities such as temperature and humidity, surface pressure is a comprehensive product of the deep structure of the upper air column, and its change reflects the adjustment and evolution of the vertical arrangement of the atmosphere (Mass & Madaus, 2014). For some synoptic-scale systems, such as tropical cyclones (TCs), explosive cyclones (ECs), and anticyclones (ACs), the evolution of central surface pressure marks the development of systems, while for meso-scale systems such as supercells and squall lines, the surface pressure tendency provides coherent mesoscale structural information, with cold pools closely relating to the growth of convection for instance (Wheatley & Stensrud, 2010). Uncovering the mechanisms leading to surface pressure change can offer in-depth insights into a diverse set of weather systems. According to the definition of air pressure, the surface pressure depends on the mass of the air column above the unit area assuming hydrostatic balance, so mass divergence is the direct cause of the change of surface pressure implied by thermodynamic processes such as density advection and temperature advection (Lynch, 2003). The surface pressure tendency equation (SPTE), as