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In the present paper we study instability caused by the velocity shear flowsof the great red spot of Jupiter. For the purpose, we imply the Navier Stokesand the continuity equations, perform the linear analysis of the governingequations and numerically solve them. We have considered two different regimes:exponential and harmonic behaviour of wave vectors. It has been shown that bothscenarios reveal unstable character of flows and the corresponding rate mightbe considerably high. For the case of harmonic time dependence of wave vectorswe also found a beat like solution of sound waves.

On the shear flow instability in the great red spot of Jupiter