Ice Dynamics at Dome C, East Antarctica

The University Archives has determined that this item is of continuing value to OSU's history. The temperature distribution in an ice sheet depends on the advective transport of heat in the ice as well as the nature of the boundary conditions at the upper and lower surfaces. This fact is exploi...

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Main Author: Bolzan, John F.
Format: Report
Language:English
Published: Institute of Polar Studies, The Ohio State University. 1984
Subjects:
Online Access:http://hdl.handle.net/1811/38738
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record_format openpolar
spelling ftohiostateu:oai:kb.osu.edu:1811/38738 2023-05-15T13:50:04+02:00 Ice Dynamics at Dome C, East Antarctica Bolzan, John F. 1984 application/pdf http://hdl.handle.net/1811/38738 en_US eng Institute of Polar Studies, The Ohio State University. Report (Ohio State University. Institute of Polar Studies) no. 85 Bolzan, John F. 1984. Ice Dynamics at Dome C, East Antarctica. Institute of Polar Studies, The Ohio State University, 55 pages. 0078-415X http://hdl.handle.net/1811/38738 Dome C Antarctica Ice Sheets -- Antarctica Temperature -- Dome C Technical Report 1984 ftohiostateu 2020-08-22T19:23:46Z The University Archives has determined that this item is of continuing value to OSU's history. The temperature distribution in an ice sheet depends on the advective transport of heat in the ice as well as the nature of the boundary conditions at the upper and lower surfaces. This fact is exploited here in an analysis of an 800 meter temperature profile measured at Dome C, East Antarctica. An ice sheet model is outlined for which the heat equation is solved numerically. Surface boundary conditions are specified in terms of an interpretation of the Dome C oxygen isotope profile, while basal conditions are related to radio-echo sounding data. Two different classes of functions are considered for the longitudinal strain rate, both consisting of simple polynomials that can be characterized by a single parameter. Temperature profile s generated by each function are compared with the measured profile. For the boundary conditions assumed here, the best fit results from a strain rate function proportional to (l-z/H)P, with H the ice thickness and p approximately 2.5. As a result, the vertical velocity decreases rapidly with depth in the upper half of the ice sheet. The corresponding depth-age relation suggests that ice at 1400 m depth could be as old as 80,000 to 90,000 years. National Science Foundation Grant DPP-7823834. Report Antarc* Antarctica East Antarctica Ice Sheet Ohio State University (OSU): Knowledge Bank East Antarctica
institution Open Polar
collection Ohio State University (OSU): Knowledge Bank
op_collection_id ftohiostateu
language English
topic Dome C
Antarctica
Ice Sheets -- Antarctica
Temperature -- Dome C
spellingShingle Dome C
Antarctica
Ice Sheets -- Antarctica
Temperature -- Dome C
Bolzan, John F.
Ice Dynamics at Dome C, East Antarctica
topic_facet Dome C
Antarctica
Ice Sheets -- Antarctica
Temperature -- Dome C
description The University Archives has determined that this item is of continuing value to OSU's history. The temperature distribution in an ice sheet depends on the advective transport of heat in the ice as well as the nature of the boundary conditions at the upper and lower surfaces. This fact is exploited here in an analysis of an 800 meter temperature profile measured at Dome C, East Antarctica. An ice sheet model is outlined for which the heat equation is solved numerically. Surface boundary conditions are specified in terms of an interpretation of the Dome C oxygen isotope profile, while basal conditions are related to radio-echo sounding data. Two different classes of functions are considered for the longitudinal strain rate, both consisting of simple polynomials that can be characterized by a single parameter. Temperature profile s generated by each function are compared with the measured profile. For the boundary conditions assumed here, the best fit results from a strain rate function proportional to (l-z/H)P, with H the ice thickness and p approximately 2.5. As a result, the vertical velocity decreases rapidly with depth in the upper half of the ice sheet. The corresponding depth-age relation suggests that ice at 1400 m depth could be as old as 80,000 to 90,000 years. National Science Foundation Grant DPP-7823834.
format Report
author Bolzan, John F.
author_facet Bolzan, John F.
author_sort Bolzan, John F.
title Ice Dynamics at Dome C, East Antarctica
title_short Ice Dynamics at Dome C, East Antarctica
title_full Ice Dynamics at Dome C, East Antarctica
title_fullStr Ice Dynamics at Dome C, East Antarctica
title_full_unstemmed Ice Dynamics at Dome C, East Antarctica
title_sort ice dynamics at dome c, east antarctica
publisher Institute of Polar Studies, The Ohio State University.
publishDate 1984
url http://hdl.handle.net/1811/38738
geographic East Antarctica
geographic_facet East Antarctica
genre Antarc*
Antarctica
East Antarctica
Ice Sheet
genre_facet Antarc*
Antarctica
East Antarctica
Ice Sheet
op_relation Report (Ohio State University. Institute of Polar Studies)
no. 85
Bolzan, John F. 1984. Ice Dynamics at Dome C, East Antarctica. Institute of Polar Studies, The Ohio State University, 55 pages.
0078-415X
http://hdl.handle.net/1811/38738
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