Identifying enhanced urban heat island convection areas for Indianapolis, Indiana using space-borne thermal remote sensing methods

dc.contributor.advisorJohnson, Daniel P.
dc.contributor.authorBoyd, Kelly D.
dc.contributor.otherWilson, Jeffery S.
dc.contributor.otherMartin, Pamela A.
dc.date.accessioned2015-12-23T20:00:12Z
dc.date.available2015-12-23T20:00:12Z
dc.date.issued2015-04-02
dc.degree.date2015en_US
dc.degree.disciplineDepartment of Geographyen
dc.degree.grantorIndiana Universityen_US
dc.degree.levelM.S.en_US
dc.descriptionIndiana University-Purdue University Indianapolis (IUPUI)en_US
dc.description.abstractHeat is one of the most important factors in our atmosphere for precipitation (thunderstorm) formation. Thermal energy from local urban land-cover is also a common source of heat in the lower atmosphere. This phenomenon is known as the urban heat island effect (UHI) and is identified as a substantial cause to a changing climate in surface weather modification. The proceeding study investigates this connection between the UHI and surface weather using remote sensing platforms A ten-year analysis of the Indianapolis UHI and thunderstorms were studied from the summer months of May, June, July, August and September (MJJAS) from 2002 until 2011. LANDSAT space borne satellite technology and land-surface based weather radar technology was used in this analysis for thunderstorm investigation. Precipitation areas identified from land-based NEXRAD WSR-88D technology were used to identify convection from non-synoptic forcing and non-normal surface diurnal heating scenarios. Only convection appearing from the UHI were studied and analyzed. Results showed twenty-one events over eighteen days with the year 2005 and 2011 having the largest frequency of events. The month of August had the largest concentration with seven events during the late afternoon hours. UHI results showed July had the largest heat island magnitude with April and September having the lowest magnitude in UHI temperatures. Three events of the twenty-one storm paths did not had a significant mean temperature difference in the heat island below the storm reflectivity. The nineteen storm paths that were significant had a warmer area underneath storm path development by an average 6.2°C than surrounding areas. UHI initiation points showed twelve of the twenty-one events having statistically significant differences between 2 km initiation areas and the rest of the study areas. Land-cover results showed low intensity developed areas had the most land-cover type (48%) in the 2km initiation buffer regions.en_US
dc.identifier.urihttps://hdl.handle.net/1805/7821
dc.identifier.urihttp://dx.doi.org/10.7912/C2/786
dc.language.isoen_USen_US
dc.rightsCC0 1.0 Universal
dc.rights.urihttp://creativecommons.org/publicdomain/zero/1.0/
dc.subjectRemote Sensingen_US
dc.subjectThunderstormen_US
dc.subjectWeatheren_US
dc.subjectRadaren_US
dc.subjectGISen_US
dc.subjectUrban Heat Islanden_US
dc.subjectPrecipitationen_US
dc.subject.lcshUrban heat island -- Research -- Indiana -- Indianapolisen_US
dc.subject.lcshRemote sensing -- Atmospheric effectsen_US
dc.subject.lcshThunderstorms -- Researchen_US
dc.subject.lcshRadaren_US
dc.subject.lcshGeographic information systems -- Research -- Measurement -- Evaluationen_US
dc.subject.lcshEarth sciences -- Remote sensingen_US
dc.subject.lcshAtmospheric circulationen_US
dc.subject.lcshHeat -- Convectionen_US
dc.subject.lcshPrecipitation (Meteorology) -- Measurementen_US
dc.subject.lcshTemperatureen_US
dc.titleIdentifying enhanced urban heat island convection areas for Indianapolis, Indiana using space-borne thermal remote sensing methodsen_US
dc.typeThesisen
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