Turbulence and magnetic fields in the large-scale structure of the universe

Science

Volumn 320, Issue 5878, 2008, Pages 909-912

  Ryu, Dongsu ^a   Kang, Hyesung ^b   Cho, Jungyeon ^a   Das, Santabrata ^c  

^a Chungnam National University   (South Korea)

^b Pusan National University   (South Korea)

^c Sejong University   (South Korea)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; COSMOLOGY; MAGNETIC FIELD; MODELING; SOLAR SYSTEM; TURBULENCE; VORTICITY;

ARTICLE; COMPUTER SIMULATION; COSMOS; GRAVITY; MAGNETIC FIELD; MOLECULAR MECHANICS; PRIORITY JOURNAL; TURBULENT FLOW;

EID: 46449128609     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1154923     Document Type: Article

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30. This work was supported by the Korea Foundation for International Cooperation of Science and Technology through grant K20702020016-07E0200-01610 provided by the Ministry of Education, Science and Technology. The work of D.R. was also supported by the Korea Science and Engineering Foundation (KOSEF) through the grant of basic research program R01-2007-000-20196-0. The work of H.K. and S.D. was also supported by KOSEF through the Astrophysical Research Center for the Structure and Evolution of the Cosmos. The work of J.C. was also supported by the Korea Research Foundation, grant KRF-2006-331-C00136, funded by the Korean Government.