Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability
The Arctic Ocean cold halocline layer (CHL) separates the cold surface mixed layer (SML) from the underlying warm Atlantic water, and thus provides a precondition for sea ice formation. Here, we introduce a new method in which the CHL base depth is diagnosed from vertical stability and compare it to...
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ftnonlinearchiv:oai:noa.gwlb.de:cop_mods_00065077 2023-05-15T14:58:38+02:00 Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability Metzner, Enrico P. Salzmann, Marc 2023-02 electronic https://doi.org/10.5194/egusphere-2023-106 https://noa.gwlb.de/receive/cop_mods_00065077 https://egusphere.copernicus.org/preprints/egusphere-2023-106/egusphere-2023-106.pdf eng eng Copernicus Publications https://doi.org/10.5194/egusphere-2023-106 https://noa.gwlb.de/receive/cop_mods_00065077 https://egusphere.copernicus.org/preprints/egusphere-2023-106/egusphere-2023-106.pdf https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/restrictedAccess CC-BY article Verlagsveröffentlichung article Text doc-type:article 2023 ftnonlinearchiv https://doi.org/10.5194/egusphere-2023-106 2023-02-27T00:14:44Z The Arctic Ocean cold halocline layer (CHL) separates the cold surface mixed layer (SML) from the underlying warm Atlantic water, and thus provides a precondition for sea ice formation. Here, we introduce a new method in which the CHL base depth is diagnosed from vertical stability and compare it to two existing methods. Vertical stability directly affects vertical mixing and heat exchange. When applied to measurements from ice-tethered profilers, ships, and moorings, the new method for estimating the CHL base depth provides robust results with few artifacts. Comparatively large differences between our new method and two existing methods for detecting the CHL base depth were found in regions which are most prone to a CHL retreat in a warming climate. CHL base depth exhibits a seasonal cycle with a maximum depth in winter and also spring, when the SML depth is also at its maximum, but the amplitude of the CHL base depth's seasonal cycle is lower than for the SML for all three methods as expected. We also propose a novel method for detecting the cold halostad layer and study the seasonal cycle employing conservative assumptions to avoid a misclassification (including a lower bound of 50 m for the thickness). Detection of a cold halostad layer was largely confined to the Canada Basin and to the regions off the eastern coast of Greenland and also Svalbard. Article in Journal/Newspaper Arctic Arctic Ocean canada basin Greenland Sea ice Svalbard Niedersächsisches Online-Archiv NOA Arctic Arctic Ocean Canada Greenland Svalbard |
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Niedersächsisches Online-Archiv NOA |
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ftnonlinearchiv |
language |
English |
topic |
article Verlagsveröffentlichung |
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article Verlagsveröffentlichung Metzner, Enrico P. Salzmann, Marc Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
topic_facet |
article Verlagsveröffentlichung |
description |
The Arctic Ocean cold halocline layer (CHL) separates the cold surface mixed layer (SML) from the underlying warm Atlantic water, and thus provides a precondition for sea ice formation. Here, we introduce a new method in which the CHL base depth is diagnosed from vertical stability and compare it to two existing methods. Vertical stability directly affects vertical mixing and heat exchange. When applied to measurements from ice-tethered profilers, ships, and moorings, the new method for estimating the CHL base depth provides robust results with few artifacts. Comparatively large differences between our new method and two existing methods for detecting the CHL base depth were found in regions which are most prone to a CHL retreat in a warming climate. CHL base depth exhibits a seasonal cycle with a maximum depth in winter and also spring, when the SML depth is also at its maximum, but the amplitude of the CHL base depth's seasonal cycle is lower than for the SML for all three methods as expected. We also propose a novel method for detecting the cold halostad layer and study the seasonal cycle employing conservative assumptions to avoid a misclassification (including a lower bound of 50 m for the thickness). Detection of a cold halostad layer was largely confined to the Canada Basin and to the regions off the eastern coast of Greenland and also Svalbard. |
format |
Article in Journal/Newspaper |
author |
Metzner, Enrico P. Salzmann, Marc |
author_facet |
Metzner, Enrico P. Salzmann, Marc |
author_sort |
Metzner, Enrico P. |
title |
Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
title_short |
Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
title_full |
Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
title_fullStr |
Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
title_full_unstemmed |
Technical note: Determining Arctic Ocean cold halocline and cold halostad layer depths based on vertical stability |
title_sort |
technical note: determining arctic ocean cold halocline and cold halostad layer depths based on vertical stability |
publisher |
Copernicus Publications |
publishDate |
2023 |
url |
https://doi.org/10.5194/egusphere-2023-106 https://noa.gwlb.de/receive/cop_mods_00065077 https://egusphere.copernicus.org/preprints/egusphere-2023-106/egusphere-2023-106.pdf |
geographic |
Arctic Arctic Ocean Canada Greenland Svalbard |
geographic_facet |
Arctic Arctic Ocean Canada Greenland Svalbard |
genre |
Arctic Arctic Ocean canada basin Greenland Sea ice Svalbard |
genre_facet |
Arctic Arctic Ocean canada basin Greenland Sea ice Svalbard |
op_relation |
https://doi.org/10.5194/egusphere-2023-106 https://noa.gwlb.de/receive/cop_mods_00065077 https://egusphere.copernicus.org/preprints/egusphere-2023-106/egusphere-2023-106.pdf |
op_rights |
https://creativecommons.org/licenses/by/4.0/ uneingeschränkt info:eu-repo/semantics/restrictedAccess |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.5194/egusphere-2023-106 |
_version_ |
1766330764610240512 |