Convection is fundamental to atmospheric energetics and general circulation. While the ultimate energy source for Earth's atmosphere comes from the Sun, most of the solar insolation is directly deposited at the surface. Convection redistributes the energy by transporting it from the surface upward into the atmosphere, balancing atmospheric cooling in the infrared, and driving large-scale circulation (e.g., Hartmann, 2016). In doing so, convection also moves momentum, moisture, and chemically important trace constituents from the planetary boundary layer to the free troposphere. Deep convection can even communicate these influences all the way to the upper troposphere and lower stratosphere (e.g., Fueglistaler et al., 2009). For these reasons, properly representing convection and convective transport has always been a central task of the global climate models (GCMs) (e.g., Arakawa, 2004).