暂无分享,去创建一个
[2] Sebastian Cygert,et al. Using GPUs for Parallel Stencil Computations in Relativistic Hydrodynamic Simulation , 2013, PPAM.
[3] Devin W. Silvia,et al. ENZO: AN ADAPTIVE MESH REFINEMENT CODE FOR ASTROPHYSICS , 2013, J. Open Source Softw..
[4] Paul Charbonneau,et al. Solar Dynamo Theory , 2014 .
[5] Gerhard W. Zumbusch. Vectorized Higher Order Finite Difference Kernels , 2012, PARA.
[6] P ? ? ? ? ? ? ? % ? ? ? ? , 1991 .
[7] A. Shukurov,et al. The supernova-regulated ISM - II. The mean magnetic field , 2012, 1206.6784.
[8] David A. Patterson,et al. Computer Architecture: A Quantitative Approach , 1969 .
[9] José E. Moreira,et al. Proceedings of the 8th Workshop on High Performance Computational Finance , 2015, WHPCF@SC.
[10] Paulius Micikevicius,et al. 3D finite difference computation on GPUs using CUDA , 2009, GPGPU-2.
[11] The inverse cascade and nonlinear alpha-effect in simulations of isotropic helical hydromagnetic turbulence , 2000, astro-ph/0006186.
[12] Mauricio Araya-Polo,et al. Algorithm 942 , 2014 .
[13] James Demmel,et al. Benchmarking GPUs to tune dense linear algebra , 2008, HiPC 2008.
[14] Evan E. Schneider,et al. CHOLLA: A NEW MASSIVELY PARALLEL HYDRODYNAMICS CODE FOR ASTROPHYSICAL SIMULATION , 2014, 1410.4194.
[15] Frank Mueller,et al. Auto-generation and auto-tuning of 3D stencil codes on GPU clusters , 2012, CGO '12.
[16] Long Wang,et al. Acceleration of a High Order Finite-Difference WENO Scheme for Large-Scale Cosmological Simulations on GPU , 2013, 2013 IEEE International Symposium on Parallel & Distributed Processing, Workshops and Phd Forum.
[17] Juliane Junker,et al. Computer Organization And Design The Hardware Software Interface , 2016 .
[18] Boulder,et al. Multiple dynamo modes as a mechanism for long-term solar activity variations , 2015, 1507.05417.
[19] Chi-kwan Chan,et al. Dynamics of saturated energy condensation in two-dimensional turbulence. , 2011, Physical review. E, Statistical, nonlinear, and soft matter physics.
[20] Julien Demouth,et al. GPU Implementation of Finite Difference Solvers , 2014, 2014 Seventh Workshop on High Performance Computational Finance.
[21] D. O. Astronomy,et al. Interstellar Turbulence I: Observations and Processes , 2004, astro-ph/0404451.
[22] Cosmin Nita,et al. Optimized three-dimensional stencil computation on Fermi and Kepler GPUs , 2014, 2014 IEEE High Performance Extreme Computing Conference (HPEC).
[23] E. Ostriker,et al. Theory of Star Formation , 2007, 0707.3514.
[24] A 3D MHD model of astrophysical flows: Algorithms, tests and parallelisation , 2001, astro-ph/0102068.