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Large-eddy simulations of compressible convection on massively parallel computersWe report preliminary implementation of the large-eddy simulation (LES) technique in 2D simulations of compressible convection carried out on the CM-2 massively parallel computer. The convective flow fields in our simulations possess structures similar to those found in a number of direct simulations, with roll-like flows coherent across the entire depth of the layer that spans several density scale heights. Our detailed assessment of the effects of various subgrid scale (SGS) terms reveals that they may affect the gross character of convection. Yet, somewhat surprisingly, we find that our LES solutions, and another in which the SGS terms are turned off, only show modest differences. The resulting 2D flows realized here are rather laminar in character, and achieving substantial turbulence may require stronger forcing and less dissipation.
Document ID
19930046735
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Xie, Xin
(NASA Headquarters Washington, DC United States)
Toomre, Juri
(Joint Inst. for Lab. Astrophysics; Colorado Univ. Boulder, United States)
Date Acquired
August 16, 2013
Publication Date
March 10, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 405
Issue: 2
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A30732
Funding Number(s)
CONTRACT_GRANT: NAGW-91
CONTRACT_GRANT: NSG-7511
CONTRACT_GRANT: NAS5-30386
CONTRACT_GRANT: NAS8-31958
CONTRACT_GRANT: NAGW-2980
Distribution Limits
Public
Copyright
Other

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