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dc.contributor.authorLin, Jim J.en_US
dc.contributor.authorChen, Andrew F.en_US
dc.contributor.authorLee, Yuan T.en_US
dc.date.accessioned2014-12-08T15:30:22Z-
dc.date.available2014-12-08T15:30:22Z-
dc.date.issued2011-07-04en_US
dc.identifier.issn1861-4728en_US
dc.identifier.urihttp://dx.doi.org/10.1002/asia.201100151en_US
dc.identifier.urihttp://hdl.handle.net/11536/21726-
dc.description.abstractThe photochemistry of the ClO dimer (ClOOCl) plays a central role in the catalytic destruction of polar stratospheric ozone. In spite of decades of intense investigations, some of its laboratory photochemical data had not reached the desired accuracy to allow a reliable simulation of the stratospheric ozone loss until recently. Inevitable impurities in ClOOCl samples have obstructed conventional measurements. In particular, an absorption measurement of ClOOCl in 2007, which gave much lower cross sections than previous studies, implied that the formation of the ozone hole cannot be explained with cur-rent chemical models. Scientists have wondered whether the model is insufficient or the data is erroneous. Efforts aiming to resolve this controversy are reviewed in this paper, which emphasizes newly developed experiments to determine two critical photochemical properties of ClOOCl-its absorption cross section and product branching ratio-including the first reported product branching ratio at 351.8 nm photolysis.en_US
dc.language.isoen_USen_US
dc.subjectabsorption cross sectionen_US
dc.subjectatmospheric chemistryen_US
dc.subjectozoneen_US
dc.subjectphotochemistryen_US
dc.subjectphotolysisen_US
dc.titleUV Photolysis of ClOOCl and the Ozone Holeen_US
dc.typeReviewen_US
dc.identifier.doi10.1002/asia.201100151en_US
dc.identifier.journalCHEMISTRY-AN ASIAN JOURNALen_US
dc.citation.volume6en_US
dc.citation.issue7en_US
dc.citation.spage1664en_US
dc.citation.epage1678en_US
dc.contributor.department應用化學系zh_TW
dc.contributor.departmentDepartment of Applied Chemistryen_US
dc.identifier.wosnumberWOS:000293135800005-
dc.citation.woscount4-
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