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Numerical modelling of astrophysical flow on hybrid architecture supercomputers. / Kulikov, I.; Chernykh, I.; Snytnikov, A. et al.

Mathematical Research Summaries. Vol. 2 Nova Science Publishers, Inc., 2017.

Research output: Chapter in Book/Report/Conference proceedingChapterResearchpeer-review

Harvard

Kulikov, I, Chernykh, I, Snytnikov, A, Protasov, V, Tutukov, A & Glinsky, B 2017, Numerical modelling of astrophysical flow on hybrid architecture supercomputers. in Mathematical Research Summaries. vol. 2, Nova Science Publishers, Inc.

APA

Kulikov, I., Chernykh, I., Snytnikov, A., Protasov, V., Tutukov, A., & Glinsky, B. (2017). Numerical modelling of astrophysical flow on hybrid architecture supercomputers. In Mathematical Research Summaries (Vol. 2). Nova Science Publishers, Inc..

Vancouver

Kulikov I, Chernykh I, Snytnikov A, Protasov V, Tutukov A, Glinsky B. Numerical modelling of astrophysical flow on hybrid architecture supercomputers. In Mathematical Research Summaries. Vol. 2. Nova Science Publishers, Inc. 2017

Author

Kulikov, I. ; Chernykh, I. ; Snytnikov, A. et al. / Numerical modelling of astrophysical flow on hybrid architecture supercomputers. Mathematical Research Summaries. Vol. 2 Nova Science Publishers, Inc., 2017.

BibTeX

@inbook{f7df8cba31a540d1a2e6683d002d7b55,
title = "Numerical modelling of astrophysical flow on hybrid architecture supercomputers",
abstract = "This chapter describes a comprehensive computer technology of numerical modeling of astrophysical flows on hybrid supercomputer equipped with computations accelerators (NVIDIA and/or Intel accelerators). The design of parallel computing algorithms for modeling the gas-dynamic, magnetic gas dynamic, collisionless component of astrophysical objects with consideration of chemical processes is presented. There are three software packages described in this chapter: GPUPEGAS code designed for simulation of astrophysics objects on hybrid supercomputers; AstroPhi code which is used for the dynamics of stars and molecular clouds simulation on hybrid supercomputers equipped with Intel Xeon Phi accelerators; PADME code for simulation of planetary systems formation on hybrid supercomputers.",
author = "I. Kulikov and I. Chernykh and A. Snytnikov and V. Protasov and A. Tutukov and B. Glinsky",
year = "2017",
month = jan,
day = "1",
language = "English",
isbn = "9781536120226",
volume = "2",
booktitle = "Mathematical Research Summaries",
publisher = "Nova Science Publishers, Inc.",

}

RIS

TY - CHAP

T1 - Numerical modelling of astrophysical flow on hybrid architecture supercomputers

AU - Kulikov, I.

AU - Chernykh, I.

AU - Snytnikov, A.

AU - Protasov, V.

AU - Tutukov, A.

AU - Glinsky, B.

PY - 2017/1/1

Y1 - 2017/1/1

N2 - This chapter describes a comprehensive computer technology of numerical modeling of astrophysical flows on hybrid supercomputer equipped with computations accelerators (NVIDIA and/or Intel accelerators). The design of parallel computing algorithms for modeling the gas-dynamic, magnetic gas dynamic, collisionless component of astrophysical objects with consideration of chemical processes is presented. There are three software packages described in this chapter: GPUPEGAS code designed for simulation of astrophysics objects on hybrid supercomputers; AstroPhi code which is used for the dynamics of stars and molecular clouds simulation on hybrid supercomputers equipped with Intel Xeon Phi accelerators; PADME code for simulation of planetary systems formation on hybrid supercomputers.

AB - This chapter describes a comprehensive computer technology of numerical modeling of astrophysical flows on hybrid supercomputer equipped with computations accelerators (NVIDIA and/or Intel accelerators). The design of parallel computing algorithms for modeling the gas-dynamic, magnetic gas dynamic, collisionless component of astrophysical objects with consideration of chemical processes is presented. There are three software packages described in this chapter: GPUPEGAS code designed for simulation of astrophysics objects on hybrid supercomputers; AstroPhi code which is used for the dynamics of stars and molecular clouds simulation on hybrid supercomputers equipped with Intel Xeon Phi accelerators; PADME code for simulation of planetary systems formation on hybrid supercomputers.

UR - http://www.scopus.com/inward/record.url?scp=85034994071&partnerID=8YFLogxK

M3 - Chapter

AN - SCOPUS:85034994071

SN - 9781536120226

VL - 2

BT - Mathematical Research Summaries

PB - Nova Science Publishers, Inc.

ER -

ID: 10065902