dc.date.accessioned
2024-09-30T08:19:06Z
dc.date.available
2024-09-30T08:19:06Z
dc.identifier
https://doi.org/10.35003/KUZHQH
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/45083
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-44795
dc.description
Key Points</br>
- Impact velocity and target properties largely affect simple crater morphology in layered targets</br>
- Lunar regolith thicknesses inferred from crater morphometry deviate up to 80% from previous estimates</br>
- The morphological transition from normal to flat-bottomed craters is the most robust indicator for the thickness of the uppermost layer</br>
dc.subject
Computer and Information Science
dc.subject
Crater Morphology
dc.subject
Regolith Thickness
dc.subject
Morphological Transition
dc.title
Replication Data for: Formation of simple impact craters in layered targets: Implications for lunar crater morphology and regolith thickness.
dcterms.accessRights.openaire
metadata only access
