arXiv (All)
open access
Low Speed Oblique Impact Behavior On Granular Media Across Gravitational Conditions; The role of cohesion
Analyses of impact provide rich insights from the evolution of granular bodies to their structural properties of the surface and subsurface layers of celestial bodies. Although chemical cohesive bonding has been observed in asteroid samples, and low-speed impact has been a subject of many studies, o
Conceptio Open Archive
Analyze & explore related research in Conceptio
Connect this record directly into your research workflow or AI agent. Explore citations across open repositories, query full text, and export structured proof bundles.
This document is indexed with metadata only: full text is not available in the archive for this record. Open the official source ↗
Related documents
- Self-limited stacking of non-Euclidean colloidal shells: From saddles to caps#1051892
- Planet formation in chemically diverse and evolving discs II. Chemical fingerprints in planetary atmospheres#985159
- N-Body Dynamics as a Mechanism for Mean Motion Resonance Formation in the Post-Gas Era#1105802
- Observations of highly inclined disks with ALMA#1146302
- Across and along-strike crustal structure variations of the western Afar margin and adjacent plateau: Insights from receiver functions analysis#382965
Record · ID 1076736
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Retrieved via Conceptio: every document is proof-bundled with source, license, and retrieval metadata.
Bring this data into your agent: Connect via MCP or API · 20 free credits to start · no card required
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive
Read the Docs → · View CLI source on GitHub · Conceptio Open Knowledge Archive