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The main aim of this submission is to investigate the effects of someparameters like wave number, shear velocity, magnetic field and temperature forthe growth rate of the magnetized Kelvin-Helmholtz instability (KHI) withincessant profiles through interface of two viscous fluid layer occurred in thesolar atmosphere using the model of Hoshoudy, Cavus and Mahdy (2019). In thisexamination, the presence of KHI is identified for the various cases of wavenumber, magnetic field, shear velocity and temperature in the solar atmosphere.The sensible values of these parameters were acquired.

A viscous magnetohydrodynamic Kelvin Helmholtz instability in the interface of two fluid layer Part II An application to the atmosphere of the Sun