Tornado-like vortices in the quasi-cyclostrophic regime of coriolis-centrifugal convection

Coriolis-centrifugal convection (C-3) in a cylindrical domain constitutes an idealised model of tornadic storms, where the rotating cylinder represents the mesocyclone of a supercell thunderstorm. We present a suite of C-3 direct numerical simulations, analysing the influence of centrifugal buoyancy on the formation of tornado-like vortices (TLVs). TLVs are self-consistently generated provided the flow is within the quasi-cyclostrophic (QC) regime in which the dominant dynamical balance is between pressure gradient and centrifugal buoyancy forces. This requires the Froude number to be greater than the radius-to-height aspect ratio, Fr greater than or similar to gamma. We show that the TLVs that develop in our C-3 simulations share many similar features with realistic tornadoes, such as azimuthal velocity profiles, intensification of the vortex strength, and helicity characteristics. Further, we analyse the influence of the mechanical bottom boundary conditions on the formation of TLVs, finding that a rotating fluid column above a stationary surface does not generate TLVs if centrifugal buoyancy is absent. In contrast, TLVs are generated in the QC regime with any bottom boundary conditions when centrifugal buoyancy is present. Our simulations bring forth insights into natural supercell thunderstorm systems by identifying properties that determine whether a mesocyclone becomes tornadic or remains non-tornadic. For tornadoes to exist, a vertical temperature difference must be present that is capable of driving strong convection. Additionally, our Fr greater than or similar to gamma predictions dimensionally imply a critical mesocyclone angular rotation rate of (Omega) over tilde (mc) greater than or similar to root g/H-mc. Taking a typical mesocyclone height of H-mc approximate to 12 km, this translates to (Omega) over tilde (mc) 3 x 10(-2) s(-1) for centrifugal buoyancy-dominated, quasi-cyclostrophic tornadogenesis. The formation of the simulated TLVs happens at all heights on the centrifugal buoyancy time scale tau(cb). This implies a roughly 1 minute, height-invariant formation for natural tornadoes, consistent with recent observational estimates.

Automated summary

The study uses C-3 direct numerical simulations in a cylindrical domain to investigate the formation of tornado-like vortices (TLVs) under the influence of centrifugal buoyancy. TLVs are found to be self-consistently generated within the quasi-cyclostrophic regime, and the influence of bottom boundary conditions on TLV formation is analyzed.