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dc.creatorToracinta, Ernest Richard
dc.date.accessioned2012-06-07T22:43:04Z
dc.date.available2012-06-07T22:43:04Z
dc.date.created1995
dc.date.issued1995
dc.identifier.urihttps://hdl.handle.net/1969.1/ETD-TAMU-1995-THESIS-T67
dc.descriptionDue to the character of the original source materials and the nature of batch digitization, quality control issues may be present in this document. Please report any quality issues you encounter to digital@library.tamu.edu, referencing the URI of the item.en
dc.descriptionIncludes bibliographical references.en
dc.descriptionIssued also on microfiche from Lange Micrographics.en
dc.description.abstractThis study compares radar data from the League City, Texas WSR-88D and cloud-to-ground (CG) lightning data for a set of eight mesoscale convective systems (MCSs) which occur at various stages of development along the upper Texas Gulf Coast. Vertical profiles of radar reflectivity (VPRR) as well as plan views and vertical cross sections are constructed to characterize the structure and relative strength of each MCS. The VPRR are also compared with similar profiles from tropical oceanic MCSs. The data show that in all cases the majority of negative CG lightning flashes are located near high reflectivity convective cores (> 35 dBZ) in the mixed phase region (O'C < T >-20'C). Growing or mature MCSs typically had larger negative flash counts and higher percentages of negative lightning (> 80%) associated with convective cores than MCSs at later stages of their life cycle. Comparison of the median VPRR for the various MCSs showed that although each case had high reflectivity cores (45-55 dBZ) in the lowest 2 to 3 km, the more electrically active MCSs were characterized by smaller reflectivity lapse rates (decrease of reflectivity with height) in mixed phase region than the cores in the remaining systems. Based on existing theories of charge separation, the observation of high negative flash counts coincident with convective cores having small reflectivity lapse rates in the mixed phase region is consistent with the presence of large ice particles aloft. Positive CG flashes were mostly located in low reflectivity (< 30 dBZ near the-10C level) stratiform regions, independent of MCS life cycle stage or VPRR type. Several cases with reports of large hail also had high positive flash densities associated with high reflectivity cores. Devlin et al. (1995) compare 85 GHz brightness temperatures from the Special Sensor Microwave/Imager to lightning data for the same set of MCSs examined in this study. The results using radar and 85 GHz data indicate that the presence of large ice particles aloft is the common linkage between MCSs with lightning, with high radar reflectivity aloft, and large 85 GHz temperature depressions.en
dc.format.mediumelectronicen
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.publisherTexas A&M University
dc.rightsThis thesis was part of a retrospective digitization project authorized by the Texas A&M University Libraries in 2008. Copyright remains vested with the author(s). It is the user's responsibility to secure permission from the copyright holder(s) for re-use of the work beyond the provision of Fair Use.en
dc.subjectmeteorology.en
dc.subjectMajor meteorology.en
dc.titleRadar, satellite, and lightning characteristics of select mesoscale convective systems in Texasen
dc.typeThesisen
thesis.degree.disciplinemeteorologyen
thesis.degree.nameM.S.en
thesis.degree.levelMastersen
dc.type.genrethesisen
dc.type.materialtexten
dc.format.digitalOriginreformatted digitalen


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