Physics
Scientist
Geomechanics-Rock Fracture Group, Department of Geological Sciences and Engineering / 172, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, NV 89557, USA
Purdue University, West Lafayette, IN
University of Nevada, Reno, NV, US
Purdue Univ., West Lafayette, Ind.
Nevada, Univ., Reno
Department of Geological Sciences and Engineering, University of Nevada, Reno, NV 89557-0138, USA
Purdue, Univ., Lafayette, Ind.
Department Department of Geological Sciences and Engineering, University of Nevada, Reno, NV 89557
University of Nevada, Reno, Department of Geological Sciences and Engineering MS 172, Reno, NV 89557, USA
University of Nevada, Reno, 1664 N. Virginia St., reno, nv 89557-0138, USA
Geomechanics-Rock Fracture Group, Department of Geological Sciences, Mackay School of Mines / 172, University of Nevada, Reno, NV 89557-0138, USA
Geomechanics-Rock Fracture Group, Department of Geological Sciences, Mackay School of Mines, University of Nevada, Reno, NV 89557-0138, USA
Nevada Univ., Reno
University of Nevada, Department of Geological Sciences and Engineering, University of Nevada, Reno, NV 89557, USA
University of Nevada, Reno, Mackay School of Mines / 172, Reno, NV 89557
University of Nevada, Department of Geol. Sciences Mackay School of Mines, Reno, NV 89557, USA
Geomechanics Rock Fracture Group, Department of Geological Sciences Mackay School of Mines University of Nevada, Reno, NV 89557, USA
Geomechanics-Rock Fracture Group, Department of Geol. Sciences / 172, Mackay School of Earth Sciences and Engineering, University of Nevada, Reno, NV 89557, USA
Department of Geological Sciences and Engineering, University of Nevada, Reno, Nevada, USA
NASA, Goddard Space Flight Center, Greenbelt, MD
Department of Geology, Mackay School
3D Fault Interaction and Depth of Strike-Slip Faulting on Mars
3D Normal Faulting Models of Valles Marineris, Mars: Geodynamic and Tectonic Implications
A Large Pre-Hellas Impact Basin in the Southern Hemisphere of Mars
A method to relate initial elastic stress to fault population strains
A New Flexure-Dominated Lithospheric Stress Model for Mars, Driven by Pressure Differences at the Base of the Lithosphere
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