Show simple item record

dc.contributor.advisorYang, Ping
dc.contributor.advisorPanetta, Lee
dc.creatorZhang, Jianing
dc.date.accessioned2016-09-22T19:46:52Z
dc.date.available2018-08-01T05:57:31Z
dc.date.created2016-08
dc.date.issued2016-08-04
dc.date.submittedAugust 2016
dc.identifier.urihttps://hdl.handle.net/1969.1/158040
dc.description.abstractSurface roughness, a fundamental characteristic of atmospheric ice particles, is essential for defining an appropriate particle morphology model to simulate optical properties of atmospheric particles. This dissertation presents a dynamic stochastic parameterization approach based on combining the discrete differential geometry and stochastic partial differential equations to generate particle overall shapes and the degree of surface roughness. The scattering of light by particles modeled as Gaussian spheroids with size parameters up to 300 is simulated with the Invariant Imbedding T-Matrix (II-TM) method to investigate the effect of particle surface roughness on the single-scattering properties, including the phase matrix, single-scattering albedo, and extinction efficiency. It is shown that high-frequency oscillations of the phase matrix with respect to scattering angle are gradually suppressed as the degree of roughness increases. The dissertation presents a more thorough method of roughened particles in light scattering computation than various ad hoc methods reported in the literature. We discuss how surface roughness influences the Muller matrix patterns of ice particles. These results also enable better understanding of microphysics on ice surface and more accurate parameterization of atmospheric ice particles. We show that surface irregularity changes the phase matrix elements dramatically. An analysis of optical modeling of mineral dust aerosols as Gaussian spheroids is presented. The modeling results are compared with experimental measurements of feldspar to validate the applicability of roughened model particles. The Gaussian spheroids shows better data fitting than smooth spheroids. Furthermore, we analyze population density and shape distributions of Gaussian spheroid for different mineral dust species. In addition to the scattering study, we propose a new Monte Carlo method for radiative transfer based on the Metropolis algorithm.en
dc.format.mimetypeapplication/pdf
dc.language.isoen
dc.subjectSpectral methoden
dc.subjectT-Matrixen
dc.subjectSurface roughnessen
dc.subjectRandom fielden
dc.subjectMetropolis algorithmen
dc.titleScattering and Radiation Computation with Spectral Methodsen
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.committeeMemberNorth, Gerald R
dc.contributor.committeeMemberBhattacharya, Anirban
dc.type.materialtexten
dc.date.updated2016-09-22T19:46:52Z
local.embargo.terms2018-08-01
local.etdauthor.orcid0000-0002-6643-0690


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record