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A theory of nonlocal mixing-length convection. I - The moment formalismA flexible and potentially powerful theory of convection, based on the mixing length picture, is developed to make unbiased self-consistent predictions about overshooting and other complicated phenomena in convection. The basic formalism is set up, and the method's power is demonstrated by showing that a simplified version of the theory reproduces all the standard results of local convection. The second-order equations of the theory are considered in the limit of a steady state and vanishing third moments, and it is shown that they reproduce all the standard results of local mixing-length convection. There is a particular value of the superadiabatic gradient, below which the only possible steady state of a fluid is nonconvecting. Above this critical value, a fluid is convectively unstable. Two distinct regimes of convection, which are identified as efficient and inefficient convection, are determined.
Document ID
19930050726
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Grossman, Scott A.
(Steward Observatory Tucson, AZ, United States)
Narayan, Ramesh
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Arnett, David
(Steward Observatory Tucson, AZ, United States)
Date Acquired
August 16, 2013
Publication Date
April 10, 1993
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 407
Issue: 1
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
93A34723
Funding Number(s)
CONTRACT_GRANT: NAGW-2450
CONTRACT_GRANT: NSF AST-91-48279
CONTRACT_GRANT: NSF AST-90-15976
Distribution Limits
Public
Copyright
Other

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