Compressible Convection and Subduction: Kinematic and Dynamic Modeling

dc.contributor.authorLee, Changyeolen
dc.contributor.committeechairKing, Scott D.en
dc.contributor.committeemembervan Keken, Peter E.en
dc.contributor.committeememberAngel, Ross J.en
dc.contributor.committeememberWeiss, Chester J.en
dc.contributor.committeememberHole, John A.en
dc.contributor.departmentGeosciencesen
dc.date.accessioned2014-03-14T20:17:20Zen
dc.date.adate2010-10-25en
dc.date.available2014-03-14T20:17:20Zen
dc.date.issued2010-10-05en
dc.date.rdate2011-10-25en
dc.date.sdate2010-10-12en
dc.description.abstractSubduction is a dynamic and time-dependent process which requires time-dependent models for its study. In addition, due to the very high pressures within the Earth's interior, an evaluation of the role of compressibility in subduction studies should be undertaken. However, most subduction studies have been conducted by using kinematic, steady-state, and/or incompressible mantle convection models; these simplifications may miss important elements of the subduction process. In this dissertation, I evaluate the effects of time-dependence and compressibility on the evolution of subduction by using 2-D Cartesian numerical models. The effect of compressibility on the thermal and flow structures of subduction zones is evaluated by using kinematically prescribed slab and steady-state models. The effect of compressibility is primarily expressed as an additional heat source created by viscous dissipation. The heat results in thinner thermal boundary layer on the subducting slab and increases slab temperatures. With that exception, the effect of compressibility is relatively small compared with, for example, the effect of the mantle rheology on the thermal and flow structures of the mantle wedge. Plate reconstruction models show that the convergence rate and age of the incoming plate to trench vary with time, which poses a problem for steady-state subduction models. Thus, I consider the time-dependent convergence rate and age of the incoming plate in the kinematic-dynamic subduction models in order to understand the localization of high-Mg# andesites in the western Aleutians. The results show that the localization of high-Mg# andesites is a consequence of the time-dependent convergence rate and slab age along the Aleutian arc. The influence of mantle and slab parameters as well as compressibility on the slab dynamics is evaluated by using 2-D dynamic subduction models. The results demonstrate that periodic slab buckling in the mantle results in periodic convergence rate and dip of the subducting slab; time-dependence is a natural expression of subduction. The effect of compressibility on the slab dynamics is not significant. The periodic convergence rate and dip of the subducting slab explain time-dependent seafloor spreading at the mid-ocean ridge, convergence rate of the oceanic plate at trench and arc-normal migration of arc volcanoes.en
dc.description.degreePh. D.en
dc.identifier.otheretd-10122010-215256en
dc.identifier.sourceurlhttp://scholar.lib.vt.edu/theses/available/etd-10122010-215256/en
dc.identifier.urihttp://hdl.handle.net/10919/29260en
dc.publisherVirginia Techen
dc.relation.haspartLee_C_D_2010.pdfen
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjectCompressibilityen
dc.subjectNumerical modelen
dc.subjectPeriodic slab bucklingen
dc.subjectSubduction zoneen
dc.subjectAleutian island arcen
dc.subjectViscous dissipationen
dc.subjectHigh-Mg# andesiteen
dc.titleCompressible Convection and Subduction: Kinematic and Dynamic Modelingen
dc.typeDissertationen
thesis.degree.disciplineGeosciencesen
thesis.degree.grantorVirginia Polytechnic Institute and State Universityen
thesis.degree.leveldoctoralen
thesis.degree.namePh. D.en

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