Simulations of hypervelocity rocky-on-icy impacts show porosity controls crater morphology but not the efficient vaporization of the rocky impactor material.
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3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
years
2026 3verdicts
UNVERDICTED 3representative citing papers
Simulations demonstrate that fast magnetoacoustic waves incident on a localized coronal null undergo mode conversion to produce incompressible energetic Alfvén wave packets along separatrices.
Collisional and dynamical models indicate the Eulalia parent body disruption ~800 Ma near the J3:1 resonance produced an impact shower that accounts for observed lunar craters formed near that time.
citing papers explorer
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Numerical Simulations of Hypervelocity Micrometeoroid Impacts: Rocky Impactors onto Icy Targets and the Role of Porosity
Simulations of hypervelocity rocky-on-icy impacts show porosity controls crater morphology but not the efficient vaporization of the rocky impactor material.
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Interaction of Fast Magnetoacoustic Wave with the Localized Coronal Null and Generation of the Energetic Alfv\'en Wave Packet
Simulations demonstrate that fast magnetoacoustic waves incident on a localized coronal null undergo mode conversion to produce incompressible energetic Alfvén wave packets along separatrices.
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An 800-Million-Year-Old Impact Shower on the Terrestrial Planets from the Breakup of the Eulalia Parent Body
Collisional and dynamical models indicate the Eulalia parent body disruption ~800 Ma near the J3:1 resonance produced an impact shower that accounts for observed lunar craters formed near that time.