Brian D. Kaplinger, Ph.D.
Affiliations: | 2013 | Aerospace Engineering | Iowa State University, Ames, IA, United States |
Area:
Aerospace Engineering, Applied MathematicsGoogle:
"Brian Kaplinger"Parents
Sign in to add mentorBong Wie | grad student | 2013 | Iowa State | |
(Physical modeling and high-performance GPU computing for characterization, interception, and disruption of hazardous near-Earth objects.) |
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Publications
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Wagner S, Wie B, Kaplinger B. (2015) Computational solutions to Lambert's problem on modern graphics processing units Journal of Guidance, Control, and Dynamics. 38: 1305-1310 |
Kaplinger B, Wie B, Dearborn D. (2013) Nuclear fragmentation/dispersion modeling and simulation of hazardous near-Earth objects Acta Astronautica. 90: 156-164 |
Kaplinger BD, Wie B. (2012) High-performance computing for optimal disruption of hazardous NEOs Aiaa/Aas Astrodynamics Specialist Conference 2012 |
Pitz A, Kaplinger B, Vardaxis G, et al. (2012) Conceptual design of a Hypervelocity Asteroid Intercept Vehicle (HAIV) and its flight validation mission Aiaa/Aas Astrodynamics Specialist Conference 2012 |
Kaplinger BD, Wie B. (2012) Comparison of fragmentation/dispersion models for asteroid nuclear disruption mission design Advances in the Astronautical Sciences. 142: 37-52 |
Kaplinger BD, Wie B. (2011) Optimized GPU simulation of a disrupted Near-Earth Object including self gravity Advances in the Astronautical Sciences. 140: 2329-2342 |
Kaplinger BD, Wie B. (2011) Parameter variation in Near-Earth Object disruption simulations using GPU acceleration Advances in the Astronautical Sciences. 140: 2343-2356 |
Kaplinger BD, Wiey B, Dearbornz D. (2010) Preliminary results for high-fidelity modeling and simulation of orbital dispersion of asteroids disrupted by nuclear explosives Aiaa/Aas Astrodynamics Specialist Conference 2010 |
Kaplinger BD, Wie B, Dearborn D. (2010) Efficient parallelization of nonlinear perturbation algorithms for orbit prediction with applications to asteroid deflection and fragmentation Advances in the Astronautical Sciences. 136: 1845-1860 |