Impacts and Ejecta in Natural Granular Material
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arXiv
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| Auteurs principaux: | , , |
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| Format: | Preprint |
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2025
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| _version_ | 1866912484629151744 |
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| author | Wright, Esteban Argueta, Emau Losert, Wolfgang |
| author_facet | Wright, Esteban Argueta, Emau Losert, Wolfgang |
| contents | With laboratory experiments we investigate the ejecta of low-velocity (~m/s) impacts into multi-scale granular media and compare them against ejecta from impacts into mono-scale media. Impacts are into a 50 cm diameter galvanized washtub filled with fine sand that has larger diameter gravel buried below the surface is filmed with two high-speed cameras. The resulting ejecta curtain consists mainly of fine sand, and has a complex asymmetric structure that depends on the location and interaction of the ejecta with the larger gravel grains mixed into the sand. To characterize the highly heterogeneous ejecta curtain we combine three analysis techniques: Particle tracking measures the ejecta velocities and ejecta angles best in low density regions, while particle image velocimetry (PIV) elucidates average motion in dense regions, and histogram of oriented gradients (HOG) which captures directions of motion against a patterned background. We find significant asymmetries in the multi-scale ejecta's velocity distributions and ejection angles compared to the symmetry seen in the ejecta from impacts into mono-scale media. Our experiments show that larger grains under the surface impede and direct ejecta along preferential paths during the impact process. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_11691 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Impacts and Ejecta in Natural Granular Material Wright, Esteban Argueta, Emau Losert, Wolfgang Soft Condensed Matter Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics With laboratory experiments we investigate the ejecta of low-velocity (~m/s) impacts into multi-scale granular media and compare them against ejecta from impacts into mono-scale media. Impacts are into a 50 cm diameter galvanized washtub filled with fine sand that has larger diameter gravel buried below the surface is filmed with two high-speed cameras. The resulting ejecta curtain consists mainly of fine sand, and has a complex asymmetric structure that depends on the location and interaction of the ejecta with the larger gravel grains mixed into the sand. To characterize the highly heterogeneous ejecta curtain we combine three analysis techniques: Particle tracking measures the ejecta velocities and ejecta angles best in low density regions, while particle image velocimetry (PIV) elucidates average motion in dense regions, and histogram of oriented gradients (HOG) which captures directions of motion against a patterned background. We find significant asymmetries in the multi-scale ejecta's velocity distributions and ejection angles compared to the symmetry seen in the ejecta from impacts into mono-scale media. Our experiments show that larger grains under the surface impede and direct ejecta along preferential paths during the impact process. |
| title | Impacts and Ejecta in Natural Granular Material |
| topic | Soft Condensed Matter Earth and Planetary Astrophysics Instrumentation and Methods for Astrophysics |
| url | https://arxiv.org/abs/2507.11691 |