The Quasi-Biennial Oscillation (QBO) is a pattern of descending and alternating easterly and westerly winds in the tropical stratosphere that influences the atmospheric circulation globally (Gray et al., 2018). The QBO can enhance or suppress tropical convection (Son et al., 2017), change the strength and location of the jet-stream (Wang et al., 2018), and change the velocity of the polar stratospheric wind in the southern (Yamashita et al., 2018) and northern hemispheres (Lu et al., 2020). These large-scale remote atmospheric responses to the QBO are sensitive to its structure, its meridional extent (Hansen et al., 2013), its vertical extent (Andrews et al., 2019), how deep the QBO extends into the lower stratosphere (Collimore et al., 2003), and the phase of its easterly and westerly jets (Gray et al., 2018). Now with the Coupled Model Intercomparison Project 6 (CMIP6) models spontaneously generating the QBO, there is variability in how the models represent its structure (Richter et al., 2020), suggesting that there is variability in how the models represent the QBO teleconnections. This presents an opportunity to use multiple models to study one of the most extensively researched, yet still enigmatic, teleconnections associated with the QBO, the Holton-Tan effect (HTE, Holton & Tan, 1980).During early winter, if QBO westerlies are located in the middle stratosphere (10 hPa) and QBO easterlies in the lower stratosphere (50 hPa), hereafter referred to as QBOE, the polar stratospheric westerlies (polar vortex) are weaker than average (Holton & Tan, 1980). One explanation of how this happens emphasizes the QBO mean meridional circulation (QBO-MMC). The QBO-MMC acts as a residual mean meridional circulation that maintains the dynamically forced temperature response to the QBO against radiative relaxation (Hitchman et al., 2021;Pahlavan et al., 2021;Plumb & Bell, 1982). During QBOE, the westerly vertical wind shear below the 10 hPa QBO westerlies coincides with tropical warming, generated by descending motion.