Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/7716
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dc.contributor.authorallWalsh, K.; School of Earth Science Univ. of Melbourneen
dc.contributor.authorallLavander, S.; CSIROen
dc.contributor.authorallScoccimarro, E.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
dc.date.accessioned2012-02-15T12:52:02Zen
dc.date.available2012-02-15T12:52:02Zen
dc.date.issued2013en
dc.identifier.urihttp://hdl.handle.net/2122/7716en
dc.description.abstractDetection of tropical lows is performed in a suite of climate model simulations using objectively-determined detection thresholds that are resolution-dependent. It is found that there is some relationship between model resolution and tropical cyclone formation rate even after the resolution-dependent tropical cyclone detection threshold is applied. The relationship is investigated between model-simulated tropical cyclone formation and a climate-based tropical cyclone Genesis Potential Index (GPI). It is found that coar- ser-resolution models simulate the GPI better than they simulate formation of tropical cyclones directly. As a result, there appears to be little relationship from model to model between model GPI and the directly-simulated cyclone formation rate. Statistical analysis of the results shows that the main advantage of increasing model resolution is to give a considerably better pattern of cyclone formation. Finer resolution models also simulate a slightly better pattern of GPI, and for these models there is some relationship between the pattern of GPI simulated by each model and that model’s pattern of simulated tropical cyclone formation.en
dc.language.isoEnglishen
dc.publisher.nameSpringer Verlag GMBH Germanyen
dc.relation.ispartofClimate dynamicsen
dc.relation.ispartofseries/40 (2013)en
dc.subjecttropical cyclonesen
dc.subjectclimate modelsen
dc.titleResolution dependence of tropical cyclone formation in CMIP3 and finer resolution modelsen
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber585-599en
dc.subject.INGV01. Atmosphere::01.01. Atmosphere::01.01.02. Climateen
dc.identifier.doi10.1007/s00382-012-1298-zen
dc.description.obiettivoSpecifico3.7. Dinamica del clima e dell'oceanoen
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.relation.issn0930-7575en
dc.relation.eissn1432-0894en
dc.contributor.authorWalsh, K.en
dc.contributor.authorLavander, S.en
dc.contributor.authorScoccimarro, E.en
dc.contributor.departmentSchool of Earth Science Univ. of Melbourneen
dc.contributor.departmentCSIROen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Bologna, Bologna, Italiaen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptUniversity of Melbourne-
crisitem.author.deptCSIRO-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Bologna, Bologna, Italia-
crisitem.author.orcid0000-0001-7987-4744-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent01. Atmosphere-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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