The microstructure of meteoric ice from Vostok, Antarctica

The 3623 m long, 5G core collected at Vostok station, Antarctica, contains alternating layers of meteoric ice with two distinctly different microstructures. In this paper, we present the microstructure and impurity content of a number of specimens ranging in depth from 97 to 3416 m, describe in deta...

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Published in:Journal of Glaciology
Main Authors: Obbard, Rachel, Baker, Ian
Format: Text
Language:unknown
Published: Dartmouth Digital Commons 2006
Subjects:
Online Access:https://digitalcommons.dartmouth.edu/facoa/63
https://doi.org/10.3189/172756507781833901
https://digitalcommons.dartmouth.edu/context/facoa/article/1062/viewcontent/65.pdf
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spelling ftdartmouthcoll:oai:digitalcommons.dartmouth.edu:facoa-1062 2023-07-16T03:53:02+02:00 The microstructure of meteoric ice from Vostok, Antarctica Obbard, Rachel Baker, Ian 2006-10-01T07:00:00Z application/pdf https://digitalcommons.dartmouth.edu/facoa/63 https://doi.org/10.3189/172756507781833901 https://digitalcommons.dartmouth.edu/context/facoa/article/1062/viewcontent/65.pdf unknown Dartmouth Digital Commons https://digitalcommons.dartmouth.edu/facoa/63 doi:10.3189/172756507781833901 https://digitalcommons.dartmouth.edu/context/facoa/article/1062/viewcontent/65.pdf Dartmouth Scholarship Glaciology text 2006 ftdartmouthcoll https://doi.org/10.3189/172756507781833901 2023-06-28T10:42:43Z The 3623 m long, 5G core collected at Vostok station, Antarctica, contains alternating layers of meteoric ice with two distinctly different microstructures. In this paper, we present the microstructure and impurity content of a number of specimens ranging in depth from 97 to 3416 m, describe in detail the characteristics of the different layers and propose a mechanism for their microstructural development. Digital image analysis, ion chromatography, scanning electron microscopy and energy dispersive X-ray spectroscopy were used to measure texture and the location and type of impurities; electron backscatter diffraction was used to determine crystal orientation. The ice associated with interglacial periods is characterized by relatively coarse grains and a strong preferred orientation of the c axes in a plane encompassing the coring direction, producing a vertical-girdle fabric. In contrast, ice from glacial periods is characterized by a much smaller grain size and a strong single-maximum fabric, where the c axes are clustered around the vertical. Calcium is uniquely present in the grain boundaries of the fine-grained glacial layers, and its effect on grain-boundary mobility and the misorientation dependence of mobility can explain the development of the discontinuous microstructure seen in glacial ice at Vostok station. Text Antarc* Antarctica Dartmouth Digital Commons (Dartmouth College) Vostok Station ENVELOPE(106.837,106.837,-78.464,-78.464) Journal of Glaciology 53 180 41 62
institution Open Polar
collection Dartmouth Digital Commons (Dartmouth College)
op_collection_id ftdartmouthcoll
language unknown
topic Glaciology
spellingShingle Glaciology
Obbard, Rachel
Baker, Ian
The microstructure of meteoric ice from Vostok, Antarctica
topic_facet Glaciology
description The 3623 m long, 5G core collected at Vostok station, Antarctica, contains alternating layers of meteoric ice with two distinctly different microstructures. In this paper, we present the microstructure and impurity content of a number of specimens ranging in depth from 97 to 3416 m, describe in detail the characteristics of the different layers and propose a mechanism for their microstructural development. Digital image analysis, ion chromatography, scanning electron microscopy and energy dispersive X-ray spectroscopy were used to measure texture and the location and type of impurities; electron backscatter diffraction was used to determine crystal orientation. The ice associated with interglacial periods is characterized by relatively coarse grains and a strong preferred orientation of the c axes in a plane encompassing the coring direction, producing a vertical-girdle fabric. In contrast, ice from glacial periods is characterized by a much smaller grain size and a strong single-maximum fabric, where the c axes are clustered around the vertical. Calcium is uniquely present in the grain boundaries of the fine-grained glacial layers, and its effect on grain-boundary mobility and the misorientation dependence of mobility can explain the development of the discontinuous microstructure seen in glacial ice at Vostok station.
format Text
author Obbard, Rachel
Baker, Ian
author_facet Obbard, Rachel
Baker, Ian
author_sort Obbard, Rachel
title The microstructure of meteoric ice from Vostok, Antarctica
title_short The microstructure of meteoric ice from Vostok, Antarctica
title_full The microstructure of meteoric ice from Vostok, Antarctica
title_fullStr The microstructure of meteoric ice from Vostok, Antarctica
title_full_unstemmed The microstructure of meteoric ice from Vostok, Antarctica
title_sort microstructure of meteoric ice from vostok, antarctica
publisher Dartmouth Digital Commons
publishDate 2006
url https://digitalcommons.dartmouth.edu/facoa/63
https://doi.org/10.3189/172756507781833901
https://digitalcommons.dartmouth.edu/context/facoa/article/1062/viewcontent/65.pdf
long_lat ENVELOPE(106.837,106.837,-78.464,-78.464)
geographic Vostok Station
geographic_facet Vostok Station
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Dartmouth Scholarship
op_relation https://digitalcommons.dartmouth.edu/facoa/63
doi:10.3189/172756507781833901
https://digitalcommons.dartmouth.edu/context/facoa/article/1062/viewcontent/65.pdf
op_doi https://doi.org/10.3189/172756507781833901
container_title Journal of Glaciology
container_volume 53
container_issue 180
container_start_page 41
op_container_end_page 62
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