Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Tyler Fuchs"'
Publikováno v:
Journal of Physics: Conference Series. 46:370-384
The late stages of stellar evolution have great importance for the synthesis and dispersal of the elements heavier than helium. We focus on the helium shell flash in low mass stars, where incorporation of hydrogen into the convection zone above the h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a104251b705e4b8bed1494d376dc0b51
https://doi.org/10.1088/1742-6596/46/1/052
https://doi.org/10.1088/1742-6596/46/1/052
Autor:
Tyler Fuchs, Anthony Nowatzki, Falk Herwig, Marco Pignatari, David H. Porter, Paul R. Woodward
The evolution of the first generations of stars at zero or extremly low metallicity, and especially some crucial properties like the primary N14 production, is charactarized by convective-reactive mixing events that are mostly absent from similar evo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7f3b7f3add1b89323afc38095d3d36d2
http://arxiv.org/abs/0711.2091
http://arxiv.org/abs/0711.2091
Autor:
Niranjay Ravindran, Tyler Fuchs, Michael Knox, James Hanson, James Greensky, Paul R. Woodward, Alex J. Larson, David H. Porter
Publikováno v:
Applied Parallel Computing. State of the Art in Scientific Computing ISBN: 9783540757542
PARA
PARA
Recent development work at the Laboratory for Computational Science & Engineering (LCSE) at the University of Minnesota aimed at increasing the performance of parallel volume rendering of large fluid dynamics simulation data is reported. The goal of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::a49bcacaf5c034a4673430ad5ae4c5ff
https://doi.org/10.1007/978-3-540-75755-9_80
https://doi.org/10.1007/978-3-540-75755-9_80
Autor:
Paul R. Woodward, Amitkumar Puthenveetil, Tyler Fuchs, Sarah E. Anderson, B. Kevin Edgar, David H. Porter
Publisher Summary The chapter uses the piecewise-parabolic method (PPM) gas dynamics code on large NSF TeraGrid parallel systems as well as on SMP and cluster systems in a lab, to simulate turbulent flows at grid resolutions of 10243 and 20483 cells.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6de8efd6812f34807778fcce9711742c
https://doi.org/10.1016/b978-044452206-1/50010-0
https://doi.org/10.1016/b978-044452206-1/50010-0