Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources

The Mackenzie River delta is the second largest Arctic river delta in the world. Thin and destabilizing permafrost coupled with vast natural gas reserves at depth, high organic-content soils, and a high proportion of wetlands create a unique ecosystem conducive to high rates of methane (CH 4 ) emiss...

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Main Authors: Wesley, Daniel, Dallimore, Scott, MacLeod, Roger, Sachs, Torsten, Risk, David
Format: Text
Language:English
Published: 2023
Subjects:
Online Access:https://doi.org/10.5194/egusphere-2022-549
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-549/
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spelling ftcopernicus:oai:publications.copernicus.org:egusphere104809 2024-01-14T10:04:53+01:00 Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources Wesley, Daniel Dallimore, Scott MacLeod, Roger Sachs, Torsten Risk, David 2023-12-13 application/pdf https://doi.org/10.5194/egusphere-2022-549 https://egusphere.copernicus.org/preprints/2022/egusphere-2022-549/ eng eng doi:10.5194/egusphere-2022-549 https://egusphere.copernicus.org/preprints/2022/egusphere-2022-549/ eISSN: Text 2023 ftcopernicus https://doi.org/10.5194/egusphere-2022-549 2023-12-18T17:24:22Z The Mackenzie River delta is the second largest Arctic river delta in the world. Thin and destabilizing permafrost coupled with vast natural gas reserves at depth, high organic-content soils, and a high proportion of wetlands create a unique ecosystem conducive to high rates of methane (CH 4 ) emission from biogenic and thermogenic sources. Hotspots are known to have a significant contribution to summertime CH 4 emissions in the region. Still, little research has been done to determine how often geologic or biogenic CH 4 contributes to hotspots in the Mackenzie River delta. In the present study, stable carbon isotope analysis was used to identify the source of CH 4 at several aquatic and terrestrial sites thought to be hotspots of CH 4 flux to the atmosphere. Walking transects and point samples of atmospheric CH 4 and CO 2 concentrations were measured. Source stable carbon isotope ( δ 13 C-CH 4 ) signatures were derived from keeling plots of point samples and ranged from −42 ‰ to −88 ‰ δ 13 C-CH 4 , identifying both biogenic and thermogenic sources. A CH 4 source was determined for eight hotspots, two of which were thermogenic in origin ( −42.5 ‰ , −44.7 ‰ ), four of which were biogenic in origin ( −71.9 ‰ to −88.3 ‰ ), and two of which may have been produced by the oxidation of biogenic CH 4 ( −53.0 ‰ , −63.6 ‰ ), as evidenced by δ 13 C-CH 4 signatures. This indicates that the largest hotspots of CH 4 production in the Mackenzie River delta are caused by a variety of sources. Text Arctic Mackenzie river permafrost Copernicus Publications: E-Journals Arctic Mackenzie River
institution Open Polar
collection Copernicus Publications: E-Journals
op_collection_id ftcopernicus
language English
description The Mackenzie River delta is the second largest Arctic river delta in the world. Thin and destabilizing permafrost coupled with vast natural gas reserves at depth, high organic-content soils, and a high proportion of wetlands create a unique ecosystem conducive to high rates of methane (CH 4 ) emission from biogenic and thermogenic sources. Hotspots are known to have a significant contribution to summertime CH 4 emissions in the region. Still, little research has been done to determine how often geologic or biogenic CH 4 contributes to hotspots in the Mackenzie River delta. In the present study, stable carbon isotope analysis was used to identify the source of CH 4 at several aquatic and terrestrial sites thought to be hotspots of CH 4 flux to the atmosphere. Walking transects and point samples of atmospheric CH 4 and CO 2 concentrations were measured. Source stable carbon isotope ( δ 13 C-CH 4 ) signatures were derived from keeling plots of point samples and ranged from −42 ‰ to −88 ‰ δ 13 C-CH 4 , identifying both biogenic and thermogenic sources. A CH 4 source was determined for eight hotspots, two of which were thermogenic in origin ( −42.5 ‰ , −44.7 ‰ ), four of which were biogenic in origin ( −71.9 ‰ to −88.3 ‰ ), and two of which may have been produced by the oxidation of biogenic CH 4 ( −53.0 ‰ , −63.6 ‰ ), as evidenced by δ 13 C-CH 4 signatures. This indicates that the largest hotspots of CH 4 production in the Mackenzie River delta are caused by a variety of sources.
format Text
author Wesley, Daniel
Dallimore, Scott
MacLeod, Roger
Sachs, Torsten
Risk, David
spellingShingle Wesley, Daniel
Dallimore, Scott
MacLeod, Roger
Sachs, Torsten
Risk, David
Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
author_facet Wesley, Daniel
Dallimore, Scott
MacLeod, Roger
Sachs, Torsten
Risk, David
author_sort Wesley, Daniel
title Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
title_short Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
title_full Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
title_fullStr Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
title_full_unstemmed Characterization of atmospheric methane release in the outer Mackenzie River Delta from biogenic and thermogenic sources
title_sort characterization of atmospheric methane release in the outer mackenzie river delta from biogenic and thermogenic sources
publishDate 2023
url https://doi.org/10.5194/egusphere-2022-549
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-549/
geographic Arctic
Mackenzie River
geographic_facet Arctic
Mackenzie River
genre Arctic
Mackenzie river
permafrost
genre_facet Arctic
Mackenzie river
permafrost
op_source eISSN:
op_relation doi:10.5194/egusphere-2022-549
https://egusphere.copernicus.org/preprints/2022/egusphere-2022-549/
op_doi https://doi.org/10.5194/egusphere-2022-549
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