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dc.contributor.authorSellers, William D.
dc.date.accessioned2017-06-09T14:00:42Z
dc.date.available2017-06-09T14:00:42Z
dc.date.copyright1985/08/01
dc.date.issued1985
dc.identifier.issn0733-3021
dc.identifier.otherams-10876.pdf
dc.identifier.urihttp://onlinelibrary.yabesh.ir/handle/yetl/4146041
dc.description.abstractA quasi-three-dimensional global climate model is used to study the effect of a transient change in solar radiation on the model's climate. The solar constant is decreased abruptly by 5 percent in the 10th year of a 50-year run. It is then returned to its original value at increments of 1 percent per year. Although significant changes occur during the perturbation including a drop in the average global surface temperature of about 2.6 K, the long-term effects on the model's climate are small.
dc.publisherAmerican Meteorological Society
dc.titleThe Effect of a Solar Perturbation on a Global Climate Model
dc.typeJournal Paper
dc.journal.volume24
dc.journal.issue8
dc.journal.titleJournal of Climate and Applied Meteorology
dc.identifier.doi10.1175/1520-0450(1985)024<0770:TEOASP>2.0.CO;2
dc.journal.fristpage770
dc.journal.lastpage776
dc.treeJournal of Climate and Applied Meteorology:;1985:;Volume( 024 ):;Issue: 008
dc.contenttypeFulltext


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