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A Lagrangian perspective on deep convective tropical raining systems

dc.contributor.authorDuncan, David Ian, author
dc.contributor.authorKummerow, Christian D., advisor
dc.contributor.authorThompson, David W. J., committee member
dc.contributor.authorReising, Steven C., committee member
dc.date.accessioned2007-01-03T05:00:13Z
dc.date.available2007-01-03T05:00:13Z
dc.date.issued2013
dc.description.abstractDeep convective precipitating systems are categorized, tracked, and analyzed in the Tropical Ocean. Precipitating systems are tracked via an algorithm applied to the high-resolution CPC Morphing technique (CMORPH) precipitation product. Systems are categorized with an objective method, using data from the Tropical Rainfall Measuring Mission (TRMM) Microwave Imager (TMI) and a K-means clustering algorithm that exploits the consistency and similarity of tropical precipitation regimes. Propagation characteristics of these systems are found to be remarkably similar among ocean basins. The raining system's geographic center is calculated at each time step, allowing various ancillary datasets to be co-located with these systems to permit analysis of the effect of deep convective raining systems on local oceanic environments. The ancillary fields examined comprise elements of the water and energy budgets, as well as cloud field information from the International Satellite Cloud Climatology Project (ISCCP). The biggest determinant of a system's environmental impact is its propagation speed. This finding is corroborated by analysis of cloud fields which show that slow-moving systems and their associated deep clouds persist longer in a given location and therefore have a greater impact on the local environment than systems that move through more quickly. In the mean, sea surface temperature (SST) drops by 0.1-0.3°C and total precipitable water (TPW) increases by 5-7kg/m2 due to the passage of a deep convective raining system, with impacts dependent on the ocean basin and system speed. The presence of pervasive, optically thick clouds greatly decreases the net radiative flux at the surface, acting as the key driver of the observed drop in SST. The existence of a possible precipitation feedback based on system propagation speed is also explored.
dc.format.mediumborn digital
dc.format.mediummasters theses
dc.identifierDuncan_colostate_0053N_11684.pdf
dc.identifier.urihttp://hdl.handle.net/10217/79042
dc.languageEnglish
dc.language.isoeng
dc.publisherColorado State University. Libraries
dc.relation.ispartof2000-2019
dc.rightsCopyright and other restrictions may apply. User is responsible for compliance with all applicable laws. For information about copyright law, please see https://libguides.colostate.edu/copyright.
dc.subjectclouds
dc.subjectSST
dc.subjectprecipitation
dc.subjectenergy budget
dc.titleA Lagrangian perspective on deep convective tropical raining systems
dc.typeText
dcterms.rights.dplaThis Item is protected by copyright and/or related rights (https://rightsstatements.org/vocab/InC/1.0/). You are free to use this Item in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights-holder(s).
thesis.degree.disciplineAtmospheric Science
thesis.degree.grantorColorado State University
thesis.degree.levelMasters
thesis.degree.nameMaster of Science (M.S.)

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