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Modeling Issues in Asteroid-Generated TsunamisThis report studies tsunamis caused by asteroids, both those that arise from atmospheric blast waves moving across the water surface from airburst asteroids, and those that arise when the asteroid reaches the water and forms a crater. We perform numerical experiments that compare simulations using depth-averaged models (shallow water and several forms of Boussinesq) with linearized Euler (acoustics plus gravity) and ALE hydrocode simulations. We find that neither of the depth-averaged models do a good job of initiating the tsunami, but in some cases can be used to propagate a solution generated by a higher-fidelity method. A list of our conclusions and recommendations for further study is given in Section 5.
Document ID
20180006617
Acquisition Source
Ames Research Center
Document Type
Contractor Report (CR)
Authors
Berger, Marsha J.
(New York Univ. New York, NY, United States)
LeVeque, Randall J.
(Washington Univ. Seattle, WA, United States)
Date Acquired
October 24, 2018
Publication Date
March 1, 2018
Subject Category
Oceanography
Report/Patent Number
ARC-E-DAA-TN53167
NASA/CR-2018-219786
Funding Number(s)
CONTRACT_GRANT: NNA10DF26C
CONTRACT_GRANT: NNA16BD60C
Distribution Limits
Public
Copyright
Public Use Permitted.
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