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Tan, Eh (2006-05-02) I. Multi-scale dynamics of mantle plumes and II. Compressible thermo-chemical convection and the stability of mantle superplumes. http://resolver.caltech.edu/CaltechETD:etd-05142006-210236


Type of Document Dissertation
Author Tan, Eh
Author's Email Address tan2 AT gps.caltech.edu
URN etd-05142006-210236
Persistent URL http://resolver.caltech.edu/CaltechETD:etd-05142006-210236
Title I. Multi-scale dynamics of mantle plumes and II. Compressible thermo-chemical convection and the stability of mantle superplumes
Degree PhD
Option Geophysics
Advisory Committee
Advisor Name Title
T.J. Ahrens Committee Chair
D.V. Helmberger Committee Member
David John Stevenson Committee Member
Jeroen Tromp Committee Member
Michael Gurnis Committee Member
Keywords
  • thermo-chemical convection
  • solver coupling
  • plumes
  • mantle convection
  • superplumes
  • GeoFramework
Date of Defense 2006-05-02
Availability unrestricted
Abstract
The dynamic interaction of mantle plumes with subducted slabs and plate-scale flow is studied in Part I. We found that plumes preferentially develop on the edge of slabs and that a substantial amount of hot mantle can be trapped beneath slabs over long periods of time, leading to "mega-plume" formation. We used the solver-coupling technique to study the deflection of plume conduits and compare our result with the parameterized approach. The stability of mantle superplumes in compressible thermo-chemical convection is studied in Part II. The depth-dependent chemical density profile, caused by composition-dependent compressibility, is the preferred mechanism to stabilize the superplum
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 28.8 Modem   56K Modem   ISDN (64 Kb)   ISDN (128 Kb)   Higher-speed Access 
  0Thesis.pdf 6.34 Mb 00:29:22 00:15:06 00:13:12 00:06:36 00:00:33
  animation2-1.mov 191.62 Kb 00:00:53 00:00:27 00:00:23 00:00:11 00:00:01
  animation2-2.mov 906.75 Kb 00:04:11 00:02:09 00:01:53 00:00:56 00:00:04
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  animation2-4.mov 274.28 Kb 00:01:16 00:00:39 00:00:34 00:00:17 00:00:01
  animation3-1.mov 6.37 Mb 00:29:29 00:15:10 00:13:16 00:06:38 00:00:33

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