activity
20182021
most citedUpward Overshooting in Turbulent Compressible Convection. III. Calibrate Parameters for One-dimensional Reynolds Stress Model

6 citations · 16 across the 5 of their papers we have counts for

collaborators

7 papers

physics.flu-dyn20213 cited

Large-scale Vortices in Rapidly Rotating Rayleigh-Bénard Convection at Small Prandtl number

Tao Cai

One prominent feature in the atmospheres of Jupiter and Saturn is the appearance of large-scale vortices. However, the sustaining mechanism of these large-scale vortices remains un…

astro-ph.SR20213 cited

Convectively coupled equatorial trapped waves in stars and planets

Tao Cai, Cong Yu, Xing Wei

In this paper, we have studied the convectively coupled equatorially trapped waves in rotating stars, with and without magnetic field. The equatorial trapped HD and MHD Poincaré, R…

astro-ph.EP2021

Deep, Closely-Packed, Long-Lived Cyclones on Jupiter's Poles

Tao Cai, Kwing L. Chan, Hans G. Mayr

Juno Mission to Jupiter has found closely-packed cyclones at the planet's two poles. The observation that these cyclones coexist in very confined space, with outer rims almost touc…

physics.flu-dyn20214 cited

Enhancement of wave transmissions in multiple radiative and convective zones

Tao Cai, Cong Yu, Xing Wei

In this paper, we study wave transmission in a rotating fluid with multiple alternating convectively stable and unstable layers. We have discussed wave transmissions in two differe…

astro-ph.SR20206 cited

Upward Overshooting in Turbulent Compressible Convection. III. Calibrate Parameters for One-dimensional Reynolds Stress Model

Tao Cai

In this paper, we calibrate the coefficients for the one-dimensional Reynolds stress model with the data generated from the three-dimensional numerical simulations of upward oversh…

astro-ph.SR2019

Upward Overshooting in Turbulent Compressible Convection. I.Effects of the relative stability parameter, the Prandtl number, and the Péclet number

Tao Cai

In this paper, we investigate the upward overshooting by three-dimensional numerical simulations. We find that the above convectively stable zone can be partitioned into three laye…