We present results from a number of 2D high-resolution hydrodynamical simulations of asteroids striking the atmosphere of Venus. These cover a wide range of impact parameters (velocity, size, and incidence angle), but the focus is on 2-3 km diameter asteroids, as these are responsible for most of th
✦ LIBER ✦
The structural control of venusian polygonal impact craters
✍ Scribed by M. Aittola; T. Öhman; J.J. Leitner; V.-P. Kostama; J. Raitala
- Publisher
- Elsevier Science
- Year
- 2010
- Tongue
- English
- Weight
- 701 KB
- Volume
- 205
- Category
- Article
- ISSN
- 0019-1035
No coin nor oath required. For personal study only.
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