Turbulence is ubiquitous in astrophysical fluids such as the interstellar medium(ISM) and the intracluster medium(ICM). There are many driving mechanisms which can inject energy into the fluid in variety driving scales, But the plausible driving scale of ISM/ICM turbulence are yet unknown. Therefore, understanding different statistical properties between turbulence with single driving scale and turbulence with double driving scale is required. In this work, we performed 3-dimensional isothermal compressible, magnetohydrodynamic(MHD) turbulence simulations. We drive turbulence in the Fourier space in two ranges, 2<k<3(large scale) and 15<k<26(small scale). We injected different amount of energies by changing the amplitudes of forcing in these ranges. We present time evolution of kinetic and magnetic energy densities and spectra of density, kinetic and magnetic fields. We also examine density probability distribution function(PDF) and make statistical analysis.