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contributor authorGoody, Richard
date accessioned2017-06-09T16:53:49Z
date available2017-06-09T16:53:49Z
date copyright2007/07/01
date issued2007
identifier issn0022-4928
identifier otherams-76150.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4218565
description abstractR. D. Lorenz et al. claim that recent data on Mars and Titan show that planetary atmospheres are in unconstrained states of maximum entropy production (MEP). Their model as it applies to Venus, Earth, Mars, and Titan is reexamined, and it is shown that their claim is not justified. This does not necessarily imply that MEP is incorrect, and inapplicable to atmospheres, but it does mean that the difficult and unexplored problem of dynamical constraints on the MEP solution must be understood if it is to be of value for climate research.
publisherAmerican Meteorological Society
titleMaximum Entropy Production in Climate Theory
typeJournal Paper
journal volume64
journal issue7
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/JAS3967.1
journal fristpage2735
journal lastpage2739
treeJournal of the Atmospheric Sciences:;2007:;Volume( 064 ):;issue: 007
contenttypeFulltext


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