Earth's surface heat flux

We present a revised estimate of Earth's surface heat flux that is based upon a heat flow data-set with 38 347 measurements, which is 55% more than used in previous estimates. Our methodology, like others, accounts for hydrothermal circulation in young oceanic crust by utilising a half-space co...

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Main Authors: Davies, J, Davies, Rhodri
Format: Article in Journal/Newspaper
Language:unknown
Published: Copernicus GmbH 2015
Subjects:
Online Access:http://hdl.handle.net/1885/65286
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spelling ftanucanberra:oai:digitalcollections.anu.edu.au:1885/65286 2023-05-15T13:36:32+02:00 Earth's surface heat flux Davies, J Davies, Rhodri 2015-12-10T23:17:36Z http://hdl.handle.net/1885/65286 unknown Copernicus GmbH 1869-9510 http://hdl.handle.net/1885/65286 Solid Earth Journal article 2015 ftanucanberra 2015-12-28T23:33:02Z We present a revised estimate of Earth's surface heat flux that is based upon a heat flow data-set with 38 347 measurements, which is 55% more than used in previous estimates. Our methodology, like others, accounts for hydrothermal circulation in young oceanic crust by utilising a half-space cooling approximation. For the rest of Earth's surface, we estimate the average heat flow for different geologic domains as defined by global digital geology maps; and then produce the global estimate by multiplying it by the total global area of that geologic domain. The averaging is done on a polygon set which results from an intersection of a 1 degree equal area grid with the original geology polygons; this minimises the adverse influence of clustering. These operations and estimates are derived accurately using methodologies from Geographical Information Science. We consider the virtually un-sampled Antarctica separately and also make a small correction for hot-spots in young oceanic lithosphere. A range of analyses is presented. These, combined with statistical estimates of the error, provide a measure of robustness. Our final preferred estimate is 47±2 TW, which is greater than previous estimates. Article in Journal/Newspaper Antarc* Antarctica Australian National University: ANU Digital Collections
institution Open Polar
collection Australian National University: ANU Digital Collections
op_collection_id ftanucanberra
language unknown
description We present a revised estimate of Earth's surface heat flux that is based upon a heat flow data-set with 38 347 measurements, which is 55% more than used in previous estimates. Our methodology, like others, accounts for hydrothermal circulation in young oceanic crust by utilising a half-space cooling approximation. For the rest of Earth's surface, we estimate the average heat flow for different geologic domains as defined by global digital geology maps; and then produce the global estimate by multiplying it by the total global area of that geologic domain. The averaging is done on a polygon set which results from an intersection of a 1 degree equal area grid with the original geology polygons; this minimises the adverse influence of clustering. These operations and estimates are derived accurately using methodologies from Geographical Information Science. We consider the virtually un-sampled Antarctica separately and also make a small correction for hot-spots in young oceanic lithosphere. A range of analyses is presented. These, combined with statistical estimates of the error, provide a measure of robustness. Our final preferred estimate is 47±2 TW, which is greater than previous estimates.
format Article in Journal/Newspaper
author Davies, J
Davies, Rhodri
spellingShingle Davies, J
Davies, Rhodri
Earth's surface heat flux
author_facet Davies, J
Davies, Rhodri
author_sort Davies, J
title Earth's surface heat flux
title_short Earth's surface heat flux
title_full Earth's surface heat flux
title_fullStr Earth's surface heat flux
title_full_unstemmed Earth's surface heat flux
title_sort earth's surface heat flux
publisher Copernicus GmbH
publishDate 2015
url http://hdl.handle.net/1885/65286
genre Antarc*
Antarctica
genre_facet Antarc*
Antarctica
op_source Solid Earth
op_relation 1869-9510
http://hdl.handle.net/1885/65286
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