the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Forcing For Varying Boundary Layer Stability Across Antarctica
Abstract. The relative importance of changes in radiative forcing (downwelling longwave radiation) and mechanical mixing (20 m wind speed) in controlling boundary layer stability annually and seasonally at five study sites across the Antarctica continent is presented. From near-neutral to extremely strong near-surface stability, radiative forcing decreases with increasing stability, as expected, and is shown to be a major driving force behind variations in near-surface stability at all five sites. Mechanical mixing usually decreases with increasing near-surface stability for regimes with weak to extremely strong stability. For the cases where near-neutral, very shallow mixed, and weak stability occur, the wind speed in the very shallow mixed case is usually weaker compared to the near-neutral and weak stability cases while radiative forcing is largest for the near-neutral cases. This finding is an important distinguishing factor for the unique case where a very shallow mixed layer is present, indicating that weaker mechanical mixing in this case is likely responsible for the shallower boundary layer that defines the very shallow mixed stability regime. For cases with enhanced stability above a layer of weaker near-surface stability, lower downwelling longwave radiation promotes the persistence of the stronger stability aloft, while stronger near-surface winds act to maintain weaker stability immediately near the surface, resulting in this two-layer boundary layer stability regime.
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Notice on discussion status
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
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Preprint
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Supplement
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The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3626 KB) - Metadata XML
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Supplement
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Journal article(s) based on this preprint
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2023-2062', Anonymous Referee #1, 01 Nov 2023
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CC1: 'Comment on EGUSPHERE-2023-2062', Gabin Urbancic, 20 Nov 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2062/
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AC1: 'Comment on egusphere-2023-2062', Mckenzie Dice, 14 Dec 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2062/egusphere-2023-2062-AC1-supplement.pdf
Interactive discussion
Status: closed
- RC1: 'Comment on egusphere-2023-2062', Anonymous Referee #1, 01 Nov 2023
-
CC1: 'Comment on EGUSPHERE-2023-2062', Gabin Urbancic, 20 Nov 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2062/
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AC1: 'Comment on egusphere-2023-2062', Mckenzie Dice, 14 Dec 2023
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2023/egusphere-2023-2062/egusphere-2023-2062-AC1-supplement.pdf
Peer review completion
Journal article(s) based on this preprint
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Mckenzie J. Dice
John J. Cassano
Gina C. Jozef
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(3626 KB) - Metadata XML
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Supplement
(501 KB) - BibTeX
- EndNote
- Final revised paper