This paper presents an assessment of the seasonal variability velocity fields, mean and eddy kinetics, available potential energies, energy conversion rates for basin-scale circulation regimes. The data were obtained through numerical modeling Black Sea 2011 2016. It revealed significant differences in current structure southern central sea parts In 2011, Rim Current was almost continuous cyclo...

Zonal flow on Jupiter and Saturn consists of equatorial super-rotation alternating East–West jet streams at higher latitudes . Interacting with these zonal flows, numerous vortices occur various sizes lifetimes. The Juno mission Cassini’s grand finale have shown that the jets extend deeply into their molecular envelopes. On Jupiter, vast majority low mid-latitude jovian are anticyclonic, wherea...

We present numerical simulations to systematically explore the differences in formation and maintenance of polar vortices under Saturnian (“S-Regime”) Ice Giant (“I-Regime”) dynamical conditions. The wide variation observed on gas giants Jupiter Saturn by Juno Cassini spacecraft, respectively, ice Uranus Neptune ground- space-based telescopes, was recently captured Brueshaber et al. (2019) (her...