the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Vortex streets to the lee of Madeira in a km-resolution regional climate model
Abstract. Atmospheric vortex streets are a widely studied dynamical effect of isolated mountainous islands. Observational evidence comes from case studies and satellite imagery, but the climatology and annual cycle of vortex shedding are often poorly understood. Using the non-hydrostatic limited-area COSMO model driven by the ERA-Interim reanalysis, we conducted a ten-year-long simulation over a mesoscale domain covering Madeira and Canary Archipelagos at high spatial (grid spacing 1 km) and temporal resolutions. Basic properties of vortex streets were analyzed and validated through a 6-day-long case study in the lee of Madeira Island. The simulation compares well with satellite and aerial observations and with existing literature on idealized simulations. Our results show a strong dependency of vortex shedding on local and synoptic flow conditions, which are to a large extent governed by the location, shape, and strength of the Azores high. As part of the case study, we developed a vortex identification algorithm. The algorithm is based on a set of objective criteria and enabled us to develop a climatology of vortex shedding from Madeira Island for the 10-year simulation period. The analysis shows a pronounced annual cycle with an increasing vortex shedding rate from April to August and a sudden decrease in September. This cycle is consistent with mesoscale wind conditions and local inversion height patterns.
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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
(13633 KB)
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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
(13633 KB) - Metadata XML
- BibTeX
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- Final revised paper
Journal article(s) based on this preprint
Interactive discussion
Status: closed
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RC1: 'Comment on egusphere-2022-965', Anonymous Referee #1, 28 Oct 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-965/egusphere-2022-965-RC1-supplement.pdf
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
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RC2: 'Comment on egusphere-2022-965', Anonymous Referee #2, 15 Dec 2022
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
Interactive discussion
Status: closed
-
RC1: 'Comment on egusphere-2022-965', Anonymous Referee #1, 28 Oct 2022
The comment was uploaded in the form of a supplement: https://egusphere.copernicus.org/preprints/2022/egusphere-2022-965/egusphere-2022-965-RC1-supplement.pdf
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
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RC2: 'Comment on egusphere-2022-965', Anonymous Referee #2, 15 Dec 2022
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
- AC1: 'Author response on egusphere-2022-965', Qinggang Gao, 13 Jan 2023
Peer review completion
Journal article(s) based on this preprint
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Qinggang Gao
Christian Zeman
Jesus Vergara‑Temprado
Daniela Lima
Peter Molnar
Christoph Schär
The requested preprint has a corresponding peer-reviewed final revised paper. You are encouraged to refer to the final revised version.
- Preprint
(13633 KB) - Metadata XML