Asymmetries in both structure and ejecta are observed around a number of craters on planetary surfaces. Similar asymmetries have been documented for hypervelocity impact experiments. Such asymmetries arise from the stress front developed around oblique impacts. The onset angle for asymmetric stress
โฆ LIBER โฆ
Modeling of measured target pressure profiles in three hypervelocity impact experiments
โ Scribed by Michel Gerassimenko
- Publisher
- Elsevier Science
- Year
- 2001
- Tongue
- English
- Weight
- 667 KB
- Volume
- 26
- Category
- Article
- ISSN
- 0734-743X
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