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We carry out experiments of 104 m/s velocity oblique impacts into a granularmedium (sand). Impact craters have nearly round rims even at a grazing angle ofabout $10^\circ$, however, the strength of seismic pulses excited by the impactis dependent upon impact angle, and the ratio between uprange and downrangevelocity peaks can be as large as 5, particularly at shallow depths. Craterslope, an offset between crater center and impact site, crater volume,azimuthal variation in ejection angle, seismic pulse shapes and subsurface flowdirection are also sensitive to impact angle, but to a much lower degree thansubsurface pulse strength. Uprange and downrange pulse peak amplitudes can beestimated from the horizontal and vertical components of the momentum impartedto the medium from the projectile

Subsurface pulse, crater and ejecta asymmetry from oblique impacts into granular media