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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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 |
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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 |
_version_ |
1771548275182141440 |