Software for numerical simulation of convection in spherical shells for hybrid CPU/GPU computing systems
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T. V. Gavrilenko | V. A. Galkin | I. V. Bychin | A. V. Gorelikov | A. V. Ryakhovsky | V. Galkin | T. Gavrilenko | A. V. Ryakhovsky
[1] Peter A. Gilman,et al. Three-dimensional Spherical Simulations of Solar Convection. I. Differential Rotation and Pattern Evolution Achieved with Laminar and Turbulent States , 2000 .
[2] S. Patankar. Numerical Heat Transfer and Fluid Flow , 2018, Lecture Notes in Mechanical Engineering.
[3] A. Gosman,et al. Solution of the implicitly discretised reacting flow equations by operator-splitting , 1986 .
[4] Masaru Kono,et al. A numerical dynamo benchmark , 2001 .
[5] A. D. Gosman,et al. The computation of compressible and incompressible recirculating flows by a non-iterative implicit scheme , 1986 .
[6] G. Glatzmaier,et al. A three-dimensional convective dynamo solution with rotating and finitely conducting inner core and mantle , 1995 .
[7] F. Busse. Convective flows in rapidly rotating spheres and their dynamo action , 2002 .
[8] Gary A. Glatzmaier,et al. Geodynamo Simulations—How Realistic Are They? , 2002 .
[9] Paul H. Roberts,et al. A three-dimensional self-consistent computer simulation of a geomagnetic field reversal , 1995, Nature.
[10] Matthew Scarpino. OpenCL in Action: How to Accelerate Graphics and Computations , 2011 .
[11] Akira Kageyama,et al. Formation of current coils in geodynamo simulations , 2008, Nature.
[12] Paul G. Richards,et al. Seismological evidence for differential rotation of the Earth's inner core , 1996, Nature.
[13] Timothy G. Mattson,et al. OpenCL Programming Guide , 2011 .