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