Investigation of the non-linear magnetic reconnection in solar chromosphere

In order to see the occurrence of magnetic reconnection in the solar chromosphere, we investigate the behavior of nonlinear perturbations on the magneto hydro dynamic (MHD) equations. Numericalstudy of the resistive tearing instability in a current sheet is presented by considering the MHD framework.To do this, the four field model is applied. It is shown based on the simulation that the nonlinear terms make the reconnection occur faster during the spicule life time in the chromosphere.