Fig. 5

Simulated distributions of deposited particles with rotation angles of a γ = 20°, b γ = 40°, c γ = 60°, and d γ = 80°. Numerical simulations were performed with an ejection speed of v _e = 150 m/s, a direction angle of α = 20° from the north, and a drag coefficient of C _D = 0.8. Each simulation used 3000 particles. Black lines are the boundaries of the impact crater zones, as reported by Kaneko et al. (2016) (see the caption of Fig. 4)