Velocity errors affect diffusion coefficient results more than spatial errors in microscopic simulations of Galactic Cosmic Rays.
The divergence of the curves for small path lengths is due to the absence of trajectory points 4 and the odd transformation of the curves in double logarithmic scales 5
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On the Numerical Stability of the Diffusion Coefficient in Microscopic Simulations
Velocity errors affect diffusion coefficient results more than spatial errors in microscopic simulations of Galactic Cosmic Rays.