about
The Chicxulub asteroid impact and mass extinction at the Cretaceous-Paleogene boundaryPeak-ring structure and kinematics from a multi-disciplinary study of the Schrödinger impact basinPressure-temperature evolution of primordial solar system solids during impact-induced compactionThe formation of peak rings in large impact cratersAsymmetric distribution of lunar impact basins caused by variations in target properties.How does multiscale modelling and inclusion of realistic palaeobathymetry affect numerical simulation of the Storegga Slide tsunami?Spherule layers, crater scaling laws, and the population of ancient terrestrial impactorsHow big was the Chesapeake Bay impact? Insight from numerical modelingMantle deformation beneath the Chicxulub impact craterDynamic modeling suggests terrace zone asymmetry in the Chicxulub crater is caused by target heterogeneityLunar Net—a proposal in response to an ESA M3 call in 2010 for a medium sized missionChicxulub and the Exploration of Large Peak-Ring Impact Craters through Scientific DrillingAuthor Correction: Rock fluidization during peak-ring formation of large impact structuresRock fluidization during peak-ring formation of large impact structuresPenetrators for in situ subsurface investigations of EuropaResponse--Cretaceous ExtinctionsControls on the Formation of Lunar Multiring BasinsEffect of target properties and impact velocity on ejection dynamics and ejecta depositionMesoscale simulations of shock compaction of a granular ceramic: effects of mesostructure and mixed-cell strength treatmentCombining shock barometry with numerical modeling: Insights into complex crater formation-The example of the Siljan impact structure (Sweden)Evidence for an impact-induced magnetic fabric in Allende, and exogenous alternatives to the core dynamo theory for Allende magnetizationDependence of secondary crater characteristics on downrange distance: High-resolution morphometry and simulationsA numerical assessment of simple airblast models of impact airburstsMesoscale modeling of impact compaction of primitive solar system solidsComparing approaches for numerical modelling of tsunami generation by deformable submarine slidesThe formation of peak-ring basins: Working hypotheses and path forward in using observations to constrain models of impact-basin formationAn improved quantitative measure of the tendency for volcanic ash plumes to form in water: implications for the deposition of marine ash bedsExcavation of the lunar mantle by basin-forming impact events on the MoonRock AvalancheReply to comment on: “Supportive comment on: “Morphology and population of binary asteroid impact craters”, by K. Miljković, G.S. Collins, S. Mannick and P.A. Bland – An updated assessment”The effect of impact obliquity on shock heating in planetesimal collisionsHydrocode simulation of Ganymede and Europa cratering trends – How thick is Europa’s crust?Meso-scopic deformation in brittle granular materialsTerraced Crater Wall (Mass Wasting)Thermal consequences of impacts in the early solar systemQuantifying the attenuation of structural uplift beneath large lunar cratersThe transition from circular to elliptical impact cratersThe early impact histories of meteorite parent bodiesThree-dimensional tsunami propagation simulations using an unstructured mesh finite element modelNumerical modeling of asteroid survivability and possible scenarios for the Morokweng crater-forming impact
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Gareth S Collins
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