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dc.contributor.advisorGirimaji, Sharath S
dc.creatorDas, Rishita
dc.date.accessioned2022-07-27T16:44:24Z
dc.date.available2023-12-01T09:22:14Z
dc.date.created2021-12
dc.date.issued2021-12-10
dc.date.submittedDecember 2021
dc.identifier.urihttps://hdl.handle.net/1969.1/196392
dc.description.abstractVelocity gradients embody the small-scale behavior of turbulence and hold the key to understanding important phenomena such as small-scale intermittency, local-streamline geometry, scalar-mixing, and material-element-deformation. The goal of this dissertation is to investigate velocity-gradient dynamics using direct numerical simulation (DNS) data of turbulent flows to (i) develop deeper understanding of the small-scale dynamics and turbulence processes and (ii) derive a model for the Lagrangian velocity-gradient dynamics in incompressible turbulent flows. We begin with the proposal that improved insight can be obtained by investigating the internal-structure and the magnitude of the velocity-gradient tensor, individually. This is done by factorizing the velocity-gradient tensor into a bounded normalized velocity-gradient tensor, that represents local-streamline geometry and an intermittent magnitude, that represents the scale of the streamlines. Analysis of the DNS datasets of isotropic turbulence and turbulent channel flow demonstrates that the normalized velocity-gradient geometry exhibits a distinct universality across different Reynolds numbers, while the magnitude grows with Reynolds number. The dynamics of the velocity-gradient geometry and magnitude in turbulence are investigated within the state-space of the normalized velocity-gradient tensor. The effects of different turbulence processes – inertial, pressure, viscous, and large-scale forcing – on velocity-gradient dynamics are clearly identified and explicated. The key findings are that pressure along with inertia drive all flow geometries toward pure-shear, while viscosity not only reduces the velocity-gradient magnitudes but also drives the local-flow towards strain-dominated geometries. The turbulence small-scale dynamics is revisited using a novel velocity-gradient triple decomposition. In this decomposition, the effects of normal-strain and pure-rotation are clearly demarcated from that of shear. The analysis of DNS data reveals that shear constitutes the most dominating contribution toward velocity gradients in a turbulent flow field and may be the most responsible for its intermittent nature. A new Lagrangian velocity-gradient model is derived by modeling the bounded dynamics of the normalized velocity-gradient tensor and the dynamics of intermittent magnitude separately. The nonlocal flow-physics are captured by a data-driven closure in the bounded four-dimensional state-space of normalized velocity gradients, while the magnitude is modeled as a near-lognormal diffusion process. The resulting velocity-gradient model shows improved agreement with the small-scale statistics of DNS.
dc.format.mimetypeapplication/pdf
dc.language.isoen
dc.subjectTurbulence
dc.subjectFluid Dynamics
dc.titleVelocity Gradient Dynamics in Incompressible Turbulent Flows: Data-driven Analysis and Modeling
dc.typeThesis
thesis.degree.departmentAerospace Engineering
thesis.degree.disciplineAerospace Engineering
thesis.degree.grantorTexas A&M University
thesis.degree.nameDoctor of Philosophy
thesis.degree.levelDoctoral
dc.contributor.committeeMemberDonzis, Diego
dc.contributor.committeeMemberKarpetis, Adonios
dc.contributor.committeeMemberPalazzolo, Alan
dc.type.materialtext
dc.date.updated2022-07-27T16:44:25Z
local.embargo.terms2023-12-01
local.etdauthor.orcid0000-0001-9785-5109


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