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    <link>https://repository.kopri.re.kr/handle/201206/11938</link>
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    <pubDate>Thu, 16 Apr 2026 18:45:04 GMT</pubDate>
    <dc:date>2026-04-16T18:45:04Z</dc:date>
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      <title>Microstructure and Crystallographic Preferred Orientations of an Azimuthally Oriented Ice Core from a Lateral Shear Margin: Priestley Glacier, Antarctica</title>
      <link>https://repository.kopri.re.kr/handle/201206/13572</link>
      <description>Title: Microstructure and Crystallographic Preferred Orientations of an Azimuthally Oriented Ice Core from a Lateral Shear Margin: Priestley Glacier, Antarctica
Authors: Thomas, Rilee E.; Negrini, Marianne; Prior, David J.; Mulvaney, Robert; Still, Holly; Bowman, M. Hamish; Craw, Lisa; Fan, Sheng; Hubbard, Bryn; Hulbe, Christina; Kim, Daeyeong; Lutz, Franz
Abstract: A 58 m long azimuthally oriented ice core has been collected from the floating lateral sinistral&#xD;
shear margin of the lower Priestley Glacier, Terra Nova Bay, Antarctica. The crystallographic&#xD;
preferred orientations (CPO) and microstructures are described in order to correlate the&#xD;
geometry of anisotropy with constrained large-scale kinematics. Cryogenic Electron&#xD;
Backscatter Diffraction analysis shows a very strong fabric (c-axis primary eigenvalue ∼0.9)&#xD;
with c-axes aligned horizontally sub-perpendicular to flow, rotating nearly 40° clockwise (looking&#xD;
down) to the pole to shear throughout the core. The c-axis maximum is sub-perpendicular to&#xD;
vertical layers, with the pole to layering always clockwise of the c-axes. Priestley ice&#xD;
microstructures are defined by largely sub-polygonal grains and constant mean grain sizes&#xD;
with depth. Grain long axis shape preferred orientations (SPO) are almost always 1？20°&#xD;
clockwise of the c-axis maximum. A minor proportion of “oddly” oriented grains that are&#xD;
distinct from the main c-axis maximum, are present in some samples. These have horizontal&#xD;
c-axes rotated clockwise from the primary c-axis maximum and may define a weaker secondary&#xD;
maximum up to 30° clockwise of the primary maximum. Intragranular misorientations are&#xD;
measured along the core, and although the statistics are weak, this could suggest&#xD;
recrystallization by subgrain rotation to occur. These microstructures suggest subgrain&#xD;
rotation (SGR) and recrystallization by grain boundary migration recrystallization (GBM) are&#xD;
active in the Priestley Glacier shear margin. Vorticity analysis based on intragranular distortion&#xD;
indicates a vertical axis of rotation in the shear margin. The variability in c-axis maximum&#xD;
orientation with depth indicates the structural heterogeneity of the Priestley Glacier shear margin&#xD;
occurs at the meter to tens of meters scale. We suggest that CPO rotations could relate to rigid&#xD;
rotation of blocks of ice within the glacial shear margin. Rotation either post-dates CPO and SPO&#xD;
development or is occurring faster than CPO evolution can respond to a change in kinematics.</description>
      <pubDate>Fri, 26 Nov 2021 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">https://repository.kopri.re.kr/handle/201206/13572</guid>
      <dc:date>2021-11-26T00:00:00Z</dc:date>
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