Gareth S. Collins
Gareth S. Collins
Earth Science and Engineering, Imperial College London
Verified email at - Homepage
TitleCited byYear
The Chicxulub asteroid impact and mass extinction at the Cretaceous-Paleogene boundary
P Schulte, L Alegret, I Arenillas, JA Arz, PJ Barton, PR Bown, TJ Bralower, ...
Science 327 (5970), 1214-1218, 2010
Earth Impact Effects Program: A Web‐based computer program for calculating the regional environmental consequences of a meteoroid impact on Earth
GS Collins, HJ Melosh, RA Marcus
Meteoritics & planetary science 40 (6), 817-840, 2005
A strain-based porosity model for use in hydrocode simulations of impacts and implications for transient crater growth in porous targets
K WŁnnemann, GS Collins, HJ Melosh
Icarus 180 (2), 514-527, 2006
Modeling damage and deformation in impact simulations
GS Collins, HJ Melosh, BA Ivanov
Meteoritics & Planetary Science 39 (2), 217-231, 2004
Hydrocode simulations of Chicxulub crater collapse and peak-ring formation
GS Collins, HJ Melosh, JV Morgan, MR Warner
Icarus 157 (1), 24-33, 2002
Peak-ring formation in large impact craters: Geophysical constraints from Chicxulub
JV Morgan, MR Warner, GS Collins, HJ Melosh, GL Christeson
Earth and Planetary Science Letters 183 (3), 347-354, 2000
Validation of numerical codes for impact and explosion cratering: Impacts on strengthless and metal targets
E Pierazzo, N Artemieva, E Asphaug, EC Baldwin, J Cazamias, R Coker, ...
Meteoritics & Planetary Science 43 (12), 1917-1938, 2008
Numerical modelling of impact melt production in porous rocks
K WŁnnemann, GS Collins, GR Osinski
Earth and Planetary Science Letters 269 (3), 530-539, 2008
Impact structures: What does crater diameter mean?
EP Turtle, E Pierazzo, GS Collins, GR Osinski, HJ Melosh, JV Morgan, ...
Geological Society of America Special Papers 384, 1-24, 2005
Scaling of oblique impacts in frictional targets: Implications for crater size and formation mechanisms
D Elbeshausen, K WŁnnemann, GS Collins
Icarus 204 (2), 716-731, 2009
How big was the Chesapeake Bay impact? Insight from numerical modeling
GS Collins, K WŁnnemann
Geology 33 (12), 925-928, 2005
Acoustic fluidization and the extraordinary mobility of sturzstroms
GS Collins, HJ Melosh
Journal of Geophysical Research: Solid Earth 108 (B10), 2003
Dynamic modeling suggests terrace zone asymmetry in the Chicxulub crater is caused by target heterogeneity
GS Collins, J Morgan, P Barton, GL Christeson, S Gulick, J Urrutia, ...
Earth and Planetary Science Letters 270 (3), 221-230, 2008
Constraining the size of the South Pole-Aitken basin impact
RWK Potter, GS Collins, WS Kiefer, PJ McGovern, DA Kring
Icarus 220 (2), 730-743, 2012
Improvements to the ɛ-α porous compaction model for simulating impacts into high-porosity solar system objects
GS Collins, HJ Melosh, K WŁnnemann
International Journal of Impact Engineering 38 (6), 434-439, 2011
The formation of peak rings in large impact craters
JV Morgan, SPS Gulick, T Bralower, E Chenot, G Christeson, P Claeys, ...
Science 354 (6314), 878-882, 2016
Numerical modelling of heating in porous planetesimal collisions
TM Davison, GS Collins, FJ Ciesla
Icarus 208 (1), 468-481, 2010
Mid‐sized complex crater formation in mixed crystalline‐sedimentary targets: Insight from modeling and observation
GS Collins, T Kenkmann, GR Osinski, K WŁnnemann
Meteoritics & Planetary Science 43 (12), 1955-1977, 2008
Pressure–temperature evolution of primordial solar system solids during impact-induced compaction
PA Bland, GS Collins, TM Davison, NM Abreu, FJ Ciesla, AR Muxworthy, ...
Nature communications 5, 2014
Planetary science: Meteor Crater formed by low-velocity impact
HJ Melosh, GS Collins
Nature 434 (7030), 157-157, 2005
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