<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-09-19T23:51:05Z</responseDate><request verb="GetRecord" identifier="oai:dspace.mit.edu:1721.1/16815" metadataPrefix="dim">https://dspace.mit.edu/server/oai/request</request><GetRecord><record><header><identifier>oai:dspace.mit.edu:1721.1/16815</identifier><datestamp>2026-06-10T12:41:10Z</datestamp><setSpec>com_1721.1_7582</setSpec><setSpec>com_1721.1_7581</setSpec><setSpec>col_1721.1_131022</setSpec></header><metadata><dim:dim xmlns:dim="http://www.dspace.org/xmlns/dspace/dim" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.dspace.org/xmlns/dspace/dim http://www.dspace.org/schema/dim.xsd">
   <dim:field mdschema="dc" element="contributor" qualifier="advisor" lang="en_US">Robert D. van der Hilst.</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="author" lang="en_US">Saltzer, Rebecca Lee</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="other" lang="en_US">Massachusetts Institute of Technology. Dept. of Earth, Atmospheric, and Planetary Sciences.</dim:field>
   <dim:field mdschema="dc" element="contributor" qualifier="department">Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="accessioned">2009-01-26T21:53:27Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="available">2009-01-26T21:53:27Z</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="copyright" lang="en_US">2002</dim:field>
   <dim:field mdschema="dc" element="date" qualifier="issued" lang="en_US">2002</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="uri">http://hdl.handle.net/1721.1/16815</dim:field>
   <dim:field mdschema="dc" element="identifier" qualifier="oclc" lang="en_US">50631570</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">Thesis (Ph.D.)--Massachusetts Institute of Technology, Dept. of Earth, Atmospheric, and Planetary Sciences, 2002.</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">This electronic version was submitted by the student author.  The certified thesis is available in the Institute Archives and Special Collections.</dim:field>
   <dim:field mdschema="dc" element="description" lang="en_US">Includes bibliographical references (p. 111-122).</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="abstract" lang="en_US">Shear-wave splitting measurements of teleseismic shear waves, such as SKS, have been used to estimate the amount and direction of upper-mantle anisotropy worldwide. One of the basic assumptions in making these measurements is that the anisotropy is confined to a single, homogeneous layer. In this thesis, I use both numerical and analytical modeling to examine the validity of this assumption. I find that variability in the orientation of anisotropy with depth causes observable effects, such as frequency dependence in the apparent splitting parameters, and that the measured fast-axis direction is consistently different than the average of the medium. A separate focus of this thesis is how spatial associations between minerals in a thin-section can be used to infer the evolutionary pressure-temperature history of a rock. I present a new method for textural analysis that uses digital images obtained with the electron microprobe. This method is used to characterize nine mantle xenoliths erupted from kimberlite pipes in South Africa and to test whether the pyroxenes are spatially correlated with the garnets. The observed associations can be explained by a model in which harzburgitic residues are produced by large extents of partial melting at shallow depths (-60-90 km) and high temperatures (1300-1400ʻ C) and are then subsequently dragged down to greater depths where garnet and clinopyroxene exsolve, perhaps in an Archean subduction zone. The third focus of this thesis is on the seismological evidence for compositional heterogeneity in the lower mantle. Using reprocessed ISC data, I compare P and S wave tomographic models and find systematic differences between regions that have undergone subduction in the last 120 million years and those that have not below -1500 km.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="abstract" lang="en_US">(cont.) This global study is followed up with a regional study using higher-quality P and S wave differential traveltimes. Beginning at depths of -1000 km down and continuing down to the core-mantle boundary I find variability in Poisson's ratio that is greater than what would be expected by temperature variations alone. A simple explanation is that the variability includes a contribution from compositional effects, such as 2% variability in iron from one region to another.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="statementofresponsibility" lang="en_US">by Rebecca Lee Saltzer.</dim:field>
   <dim:field mdschema="dc" element="description" qualifier="degree" lang="en_US">Ph.D.</dim:field>
   <dim:field mdschema="dc" element="format" qualifier="extent" lang="en_US">122 p.</dim:field>
   <dim:field mdschema="dc" element="language" qualifier="iso" lang="en_US">eng</dim:field>
   <dim:field mdschema="dc" element="publisher" lang="en_US">Massachusetts Institute of Technology</dim:field>
   <dim:field mdschema="dc" element="rights" lang="en_US">M.I.T. theses are protected by 
copyright. They may be viewed from this source for any purpose, but 
reproduction or distribution in any format is prohibited without written 
permission. See provided URL for inquiries about permission.</dim:field>
   <dim:field mdschema="dc" element="rights" qualifier="uri" lang="en_US">http://dspace.mit.edu/handle/1721.1/7582</dim:field>
   <dim:field mdschema="dc" element="subject" lang="en_US">Earth, Atmospheric, and Planetary Sciences.</dim:field>
   <dim:field mdschema="dc" element="title" lang="en_US">The earth's interior from both a seismological and petrological perspective</dim:field>
   <dim:field mdschema="dc" element="type" lang="en_US">Thesis</dim:field>
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   	&lt;Title>The earth&amp;apos;s interior from both a seismological and petrological perspective&lt;/Title>
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   	&lt;PublicationDate>2002&lt;/PublicationDate>
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        	&lt;DisplayName>Saltzer, Rebecca Lee&lt;/DisplayName>
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    &lt;Keyword>Earth, Atmospheric, and Planetary Sciences.&lt;/Keyword>
   	&lt;Abstract>Shear-wave splitting measurements of teleseismic shear waves, such as SKS, have been used to estimate the amount and direction of upper-mantle anisotropy worldwide. One of the basic assumptions in making these measurements is that the anisotropy is confined to a single, homogeneous layer. In this thesis, I use both numerical and analytical modeling to examine the validity of this assumption. I find that variability in the orientation of anisotropy with depth causes observable effects, such as frequency dependence in the apparent splitting parameters, and that the measured fast-axis direction is consistently different than the average of the medium. A separate focus of this thesis is how spatial associations between minerals in a thin-section can be used to infer the evolutionary pressure-temperature history of a rock. I present a new method for textural analysis that uses digital images obtained with the electron microprobe. This method is used to characterize nine mantle xenoliths erupted from kimberlite pipes in South Africa and to test whether the pyroxenes are spatially correlated with the garnets. The observed associations can be explained by a model in which harzburgitic residues are produced by large extents of partial melting at shallow depths (-60-90 km) and high temperatures (1300-1400ʻ C) and are then subsequently dragged down to greater depths where garnet and clinopyroxene exsolve, perhaps in an Archean subduction zone. The third focus of this thesis is on the seismological evidence for compositional heterogeneity in the lower mantle. Using reprocessed ISC data, I compare P and S wave tomographic models and find systematic differences between regions that have undergone subduction in the last 120 million years and those that have not below -1500 km.&lt;/Abstract>
   	&lt;Abstract>(cont.) This global study is followed up with a regional study using higher-quality P and S wave differential traveltimes. Beginning at depths of -1000 km down and continuing down to the core-mantle boundary I find variability in Poisson&amp;apos;s ratio that is greater than what would be expected by temperature variations alone. A simple explanation is that the variability includes a contribution from compositional effects, such as 2% variability in iron from one region to another.&lt;/Abstract>
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