Observational Constraints on Numerical Models of Peak-Ring Formation
Abstract
We compare observational data from the IODP-ICDP cores of the Chicxulub peak ring with predictions from numerical impact simulations. Our results are remarkably consistent, demonstrating the predictive capabilities of numerical impact models.
- Publication:
-
Large Meteorite Impacts and Planetary Evolution VI
- Pub Date:
- September 2019
- Bibcode:
- 2019LPICo2136.5059R