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contributor authorBarchet, W. R.
date accessioned2017-06-09T14:14:44Z
date available2017-06-09T14:14:44Z
date copyright1969/01/01
date issued1969
identifier issn0022-4928
identifier otherams-15556.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4151241
description abstractOn the basis of a general formulation of the Gibbs free energy change for heterogeneously nucleating systems, the difference in the free energy change for the formation of a spherical cap embryo and a sessile drop-shaped embryo is evaluated. This difference represents the error introduced by assuming the embryo is a spherical cap in the presence of a gravitational field. Power series expressions for the volume and surface areas of the sessile drop, based on the work of Bashforth and Adams, are used to arrive at the free energy change. Ratios allowing a comparison of the error for different systems are presented along with numerical values for a hypothetical, unit system. This hypothetical system is compared to water and to mercury with the result that the maximum relative error is 10?6. Based on this value, it is concluded that the spherical cap model is an adequate and useful approximation of the shape of an embryo in heterogeneous nucleation under the action of gravity.
publisherAmerican Meteorological Society
titleThe Validity of the Spherical Cap Approximation in Heterogeneous Nucleation
typeJournal Paper
journal volume26
journal issue1
journal titleJournal of the Atmospheric Sciences
identifier doi10.1175/1520-0469(1969)026<0112:TVOTSC>2.0.CO;2
journal fristpage112
journal lastpage114
treeJournal of the Atmospheric Sciences:;1969:;Volume( 026 ):;issue: 001
contenttypeFulltext


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