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    <link>https://repository.kopri.re.kr/handle/201206/5499</link>
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        <rdf:li rdf:resource="https://repository.kopri.re.kr/handle/201206/11996" />
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    <dc:date>2026-04-18T22:25:34Z</dc:date>
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  <item rdf:about="https://repository.kopri.re.kr/handle/201206/11996">
    <title>Intercrystalline Stable Isotope Exchange in Refractory Minerals of Ca-Al-rich Inclusions</title>
    <link>https://repository.kopri.re.kr/handle/201206/11996</link>
    <description>Title: Intercrystalline Stable Isotope Exchange in Refractory Minerals of Ca-Al-rich Inclusions
Authors: Park, Changkun</description>
    <dc:date>2017-12-29T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repository.kopri.re.kr/handle/201206/8268">
    <title>Modeling for intercrystalline isotope diffusion</title>
    <link>https://repository.kopri.re.kr/handle/201206/8268</link>
    <description>Title: Modeling for intercrystalline isotope diffusion
Authors: Park, Changkun
Abstract: Stable isotope exchange between coexisting minerals can take place during cooling of a closed system, followed by&#xD;
isotopic diffusion through minerals. The result of stable isotope diffusion depends on the temperature, time, diffusion&#xD;
coefficients, fractionation factors, grain sizes and abundances of mineral phases. Since these factors can be determined&#xD;
by experiments and petrological studies, the cooling history of the system can be modeled.&#xD;
To model isotopic exchange between minerals and retrograde intra-crystalline diffusion in a closed system, it is&#xD;
assumed that 1) isotope concentration at grain boundaries is considered to be homogeneous at any points of grain&#xD;
boundaries, 2) mass flux of isotope is preserved (thus, net flux is zero), 3) concentration gradient at the grain surfaces&#xD;
leads to a solid-state isotope diffusion through individual grains, and 4) diffusion coefficients of minerals and isotopic&#xD;
concentrations at grain boundaries are changed with decreasing temperature (Eiler et al., 1994; Jenkin et al., 1994).&#xD;
This process continues until the system cools down to the diffusive closure temperatures of minerals.&#xD;
Results of modeling well reproduce concentration profiles observed in terrestrial rocks (e.g., Bonamici et al., 2011).&#xD;
The model is applied to refractory inclusions in extraterrestrial rocks to reproduce isotopic distributions in coexisting&#xD;
minerals, which could constrain cooling history of the inclusions in the early Solar System.</description>
    <dc:date>2017-01-01T00:00:00Z</dc:date>
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