A numerical simulation of supersonic turbulent convection relating to the formation of the Solar system

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 2, 2003, Pages 644-656

  Prentice, A J R ^a,b   Dyt, C P ^a,c  

^a MONASH UNIVERSITY   (Australia)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c CSIRO   (Australia)

Author keywords

Convection; Solar system: Formation; Sun: Atmospheric motions; Turbulence

Indexed keywords

COMPUTATION THEORY; NUMERICAL METHODS; NUMERICAL MODELS; ORBITS; REYNOLDS NUMBER; SUPERSONIC AIRCRAFT; THERMAL GRADIENTS; TURBULENCE;

ATMOSPHERIC MOTIONS; AUSTRALIA; CONVECTION; DOWNFLOW; LAPLACIANS; PETROLEUM RESOURCES; SOLAR SYSTEM FORMATION; SUN: ATMOSPHERIC MOTION; TURBULENT CONVECTION; WESTERN AUSTRALIA;

HEAT CONVECTION;

EID: 0142104998     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06454.x     Document Type: Article

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