Speaking about heat flow, ice fusion and temperature alterations

Heat flow density measurements are difficult to obtain in Antarctica and Greenland due to climate and ice thickness in those regions. The works published about that subject shows that spatial distribution of the heat flux values is highly heterogeneous. Maximum and minimum values of heat flux vary w...

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Main Author: Duque, Maria Rosa
Format: Lecture
Language:English
Published: 2018
Subjects:
Online Access:http://hdl.handle.net/10174/24127
id ftunivevora:oai:dspace.uevora.pt:10174/24127
record_format openpolar
spelling ftunivevora:oai:dspace.uevora.pt:10174/24127 2023-09-05T13:12:50+02:00 Speaking about heat flow, ice fusion and temperature alterations Duque, Maria Rosa 2018-09 http://hdl.handle.net/10174/24127 eng eng Duque, M. R. (2018). Speaking about heat flow, ice fusion and temperature alterations.WMESS2018 ( World Multidisciplinary Earth Sciences Symposium), Praga, República Checa, 3 a 7 de Setembro de 2018.(C. Oral) http://hdl.handle.net/10174/24127 sim nao mrad@uevora.pt 393 restrictedAccess Heat flow density Fusion of the ice Antartida lecture 2018 ftunivevora 2023-08-14T17:43:33Z Heat flow density measurements are difficult to obtain in Antarctica and Greenland due to climate and ice thickness in those regions. The works published about that subject shows that spatial distribution of the heat flux values is highly heterogeneous. Maximum and minimum values of heat flux vary with different authors and method used, but all of them say that East Antarctic is characterized by low heat flux values (45-85 mW m-2) with the lowest values found especially in the central part. The values obtained in West Antarctic (65-180 mW m-2) and in the Antarctic Peninsula (maximum of 170 mW m-2). In the work whose data is used high values were obtained in the West Antarctic Rift system ( maximum value of 130 mW m-2). Some local geothermal anomalies have been reported such as Lake Wilhams (285 mW m-2) or Siple Dome (69 mW m-2). Elevated heat flux values are obtained in volcanic regions and in regions with relatively recent tectonic activity, in West Antarctic. The east Antarctic is characterized by low values, however the Coastal part of Queen Mary Land, the Lambert Rift and Victoria Land, show higher values, suggesting Cenozoic processes in the region, including volcanism or extension. Ice fusion occurs near the base of the ice sheet. In order to study this phenomenon 13 places were chosen from two profiles in WA and EA ( Martos, Y. et al, 2017) with data related to heat flux, sub glacial topography and ice thickness. An average thermal conductivity of 2.35 W K-1 m-1 and density of 917.5 Kg m-3 were used for the ice. Relations between the amount of molten ice per year due to the heat flux, the altitude and the thickness of the ice were obtained. The effect of temperature alteration at the surface in the temperature of the ice was calculate considering different modes of temperature variation, using an average value of 1.3 X 10-6 m2 s-1 for the thermal diffusivity of the ice. The results obtained show differences in the two regions studied but the heat flow values used were found from “Curie Depth Temperature” ... Lecture Antarc* Antarctic Antarctic Peninsula Antarctica Greenland Ice Sheet Queen Mary land Victoria Land Repositório Científico da Universidade de Évora Antarctic Antarctic Peninsula Greenland Queen Mary Land ENVELOPE(96.000,96.000,-68.000,-68.000) Siple ENVELOPE(-83.917,-83.917,-75.917,-75.917) Siple Dome ENVELOPE(-148.833,-148.833,-81.667,-81.667) The Antarctic Victoria Land
institution Open Polar
collection Repositório Científico da Universidade de Évora
op_collection_id ftunivevora
language English
topic Heat flow density
Fusion of the ice
Antartida
spellingShingle Heat flow density
Fusion of the ice
Antartida
Duque, Maria Rosa
Speaking about heat flow, ice fusion and temperature alterations
topic_facet Heat flow density
Fusion of the ice
Antartida
description Heat flow density measurements are difficult to obtain in Antarctica and Greenland due to climate and ice thickness in those regions. The works published about that subject shows that spatial distribution of the heat flux values is highly heterogeneous. Maximum and minimum values of heat flux vary with different authors and method used, but all of them say that East Antarctic is characterized by low heat flux values (45-85 mW m-2) with the lowest values found especially in the central part. The values obtained in West Antarctic (65-180 mW m-2) and in the Antarctic Peninsula (maximum of 170 mW m-2). In the work whose data is used high values were obtained in the West Antarctic Rift system ( maximum value of 130 mW m-2). Some local geothermal anomalies have been reported such as Lake Wilhams (285 mW m-2) or Siple Dome (69 mW m-2). Elevated heat flux values are obtained in volcanic regions and in regions with relatively recent tectonic activity, in West Antarctic. The east Antarctic is characterized by low values, however the Coastal part of Queen Mary Land, the Lambert Rift and Victoria Land, show higher values, suggesting Cenozoic processes in the region, including volcanism or extension. Ice fusion occurs near the base of the ice sheet. In order to study this phenomenon 13 places were chosen from two profiles in WA and EA ( Martos, Y. et al, 2017) with data related to heat flux, sub glacial topography and ice thickness. An average thermal conductivity of 2.35 W K-1 m-1 and density of 917.5 Kg m-3 were used for the ice. Relations between the amount of molten ice per year due to the heat flux, the altitude and the thickness of the ice were obtained. The effect of temperature alteration at the surface in the temperature of the ice was calculate considering different modes of temperature variation, using an average value of 1.3 X 10-6 m2 s-1 for the thermal diffusivity of the ice. The results obtained show differences in the two regions studied but the heat flow values used were found from “Curie Depth Temperature” ...
format Lecture
author Duque, Maria Rosa
author_facet Duque, Maria Rosa
author_sort Duque, Maria Rosa
title Speaking about heat flow, ice fusion and temperature alterations
title_short Speaking about heat flow, ice fusion and temperature alterations
title_full Speaking about heat flow, ice fusion and temperature alterations
title_fullStr Speaking about heat flow, ice fusion and temperature alterations
title_full_unstemmed Speaking about heat flow, ice fusion and temperature alterations
title_sort speaking about heat flow, ice fusion and temperature alterations
publishDate 2018
url http://hdl.handle.net/10174/24127
long_lat ENVELOPE(96.000,96.000,-68.000,-68.000)
ENVELOPE(-83.917,-83.917,-75.917,-75.917)
ENVELOPE(-148.833,-148.833,-81.667,-81.667)
geographic Antarctic
Antarctic Peninsula
Greenland
Queen Mary Land
Siple
Siple Dome
The Antarctic
Victoria Land
geographic_facet Antarctic
Antarctic Peninsula
Greenland
Queen Mary Land
Siple
Siple Dome
The Antarctic
Victoria Land
genre Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Greenland
Ice Sheet
Queen Mary land
Victoria Land
genre_facet Antarc*
Antarctic
Antarctic Peninsula
Antarctica
Greenland
Ice Sheet
Queen Mary land
Victoria Land
op_relation Duque, M. R. (2018). Speaking about heat flow, ice fusion and temperature alterations.WMESS2018 ( World Multidisciplinary Earth Sciences Symposium), Praga, República Checa, 3 a 7 de Setembro de 2018.(C. Oral)
http://hdl.handle.net/10174/24127
sim
nao
mrad@uevora.pt
393
op_rights restrictedAccess
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