Erratum: “Superdiffusion of Cosmic Rays: Implications for Cosmic Ray Acceleration” (2014, ApJ, 784, 38)

An error is found in Table 1 of the published article describing the regimes of diffusion and superdiffusion. For the weak turbulence when the scales s measured along the magnetic field are larger then the turbulence injection scale L, the separation of magnetic field lines increases in a diffusive way with the step LMA4, where MA is the Alfvén Mach number, i.e., MA = VL/VA, where VL is the turbulent injection velocity and VA is the Alfvén velocity. We provide Table 1 with the error corrected here.The separation of magnetic field lines was studied in Lazarian & Vishniac (1999). There it was found there that for the weak turbulence at scales s Gt L, where s is measured along the magnetic field and L is the injection scale of turbulence the separation is growing as a random walk with the step ${{LM}}_{{\rm{A}}}^{4}$, where MA is the Alfvén Mach number. This result was used in further publications, e.g., in Lazarian (2006) to study the propagation of heat in clusters of galaxies. Unfortunately, due to an error the corresponding entry in our published article is incorrect. We provide the corrected version of the Table 1 here describing the separation of magnetic field lines for different regimes of MHD turbulence