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dc.contributor.advisorBowman, Kenneth
dc.creatorMurthi, Aditya
dc.date.accessioned2011-08-08T22:47:26Z
dc.date.accessioned2011-08-09T01:32:59Z
dc.date.available2011-08-08T22:47:26Z
dc.date.available2011-08-09T01:32:59Z
dc.date.created2010-05
dc.date.issued2011-08-08
dc.date.submittedMay 2010
dc.identifier.urihttps://hdl.handle.net/1969.1/ETD-TAMU-2010-05-7648
dc.description.abstractIn this study, the space-time relationship of precipitation fields is examined by testing the Taylor's "frozen field" hypothesis (TH). Specifically, the hypothesis supposes that if a spatio-temporal precipitation field with a stationary covariance Cov(r,tau) in both space r and time tau, moves with a constant velocity v, then the temporal covariance at time lag tau is equal to the spatial covariance at space lag v tau, that is, Cov(0;tau) = Cov(v tau, 0). Of specific interest is whether there is a cut-off or decorrelation time scale for which the TH holds for a given mean flow velocity v. The validity of the TH is tested for precipitation fields using high-resolution gridded NEXRAD radar reflectivity data over southeastern United States by employing two different statistical approaches. The first method is based upon rigorous hypothesis testing while the second is based on a simple correlation analysis, which neglects possible dependencies in the correlation estimates. The data-set has an approximate horizontal resolution of 4 km x 4 km and a temporal resolution of 15 minutes, while the time period of study is 4 days. The results of both statistical methods suggest that the TH might hold for the shortest space and time scales resolved by the data (4 km and 15 minutes), but that it does not hold for longer periods or larger spatial scales. The fidelity of global climate models in accurately simulating seasonal mean precipitation in the tropics is investigated by comparisons with satellite observations. Specifically, six-year long (2000-2005) simulations are performed using a high-resolution (36-km) Weather Research Forecast (WRF) model and the Community Atmosphere Model (CAM) at T85 spatial resolution and the results are compared with satellite observations from the Tropical Rainfall Measuring Mission (TRMM). The primary goal is to study the annual cycle of rainfall over four land regions of the tropics namely, the Indian monsoon, the Amazon, tropical Africa and the North American monsoon. The results indicate that the WRF model systematically underestimates the magnitude of monthly mean rainfall over most Tropical land regions but gets the seasonal timing right. On the other hand, CAM produces rainfall magnitudes that are closer to the observations but the rainfall peak leads or lags the observations by a month or two. Some of these regional biases can be attributed to erroneous circulation and moisture surpluses/deficits in the lower troposphere in both models. Overall, the results seem to indicate that employing a higher spatial resolution (36 km) does not significantly improve simulation of precipitation. We speculate that a combination of several physics parameterizations and lack of model tuning gives rise to the observed differences between the models and the observations.en
dc.format.mimetypeapplication/pdf
dc.language.isoen_US
dc.subjectPrecipitationen
dc.subjectclimate modelingen
dc.subjectTaylor Hypothesisen
dc.titleAnalysis of Precipitation Using Satellite Observations and Comparisons with Global Climate Modelsen
dc.typeThesisen
thesis.degree.departmentAtmospheric Sciencesen
thesis.degree.disciplineAtmospheric Sciencesen
thesis.degree.grantorTexas A&M Universityen
thesis.degree.nameDoctor of Philosophyen
thesis.degree.levelDoctoralen
dc.contributor.committeeMemberDaripa, Prabir, and Saravanan, Ramalinga
dc.contributor.committeeMemberNorth, Jerry
dc.type.genrethesisen
dc.type.materialtexten


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