Genesis and maintenance of "Mediterranean hurricanes"
Cyclonic storms that closely resemble tropical cyclones in satellite images occasionally form over the Mediterranean Sea. Synoptic and mesoscale analyses of such storms show small, warm-core structure and surface winds sometimes exceeding 25ms<sup>-1</sup> over small areas. These analyse...
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Format: | Article |
Language: | English |
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Copernicus Publications
2005-01-01
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Series: | Advances in Geosciences |
Online Access: | http://www.adv-geosci.net/2/217/2005/adgeo-2-217-2005.pdf |
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author | K. Emanuel |
author_facet | K. Emanuel |
author_sort | K. Emanuel |
collection | DOAJ |
description | Cyclonic storms that closely resemble tropical cyclones in satellite images occasionally form over the Mediterranean Sea. Synoptic and mesoscale analyses of such storms show small, warm-core structure and surface winds sometimes exceeding 25ms<sup>-1</sup> over small areas. These analyses, together with numerical simulations, reveal that in their mature stages, such storms intensify and are maintained by a feedback between surface enthalpy fluxes and wind, and as such are isomorphic with tropical cyclones. In this paper, I demonstrate that a cold, upper low over the Mediterranean can produce strong cyclogenesis in an axisymmetric model, thereby showing that baroclinic instability is not necessary during the mature stages of Mediterranean hurricanes. |
first_indexed | 2024-12-11T05:49:07Z |
format | Article |
id | doaj.art-69c5ee7a4a6f4b4ab3d52705677d1ddc |
institution | Directory Open Access Journal |
issn | 1680-7340 1680-7359 |
language | English |
last_indexed | 2024-12-11T05:49:07Z |
publishDate | 2005-01-01 |
publisher | Copernicus Publications |
record_format | Article |
series | Advances in Geosciences |
spelling | doaj.art-69c5ee7a4a6f4b4ab3d52705677d1ddc2022-12-22T01:18:52ZengCopernicus PublicationsAdvances in Geosciences1680-73401680-73592005-01-012217220Genesis and maintenance of "Mediterranean hurricanes"K. EmanuelCyclonic storms that closely resemble tropical cyclones in satellite images occasionally form over the Mediterranean Sea. Synoptic and mesoscale analyses of such storms show small, warm-core structure and surface winds sometimes exceeding 25ms<sup>-1</sup> over small areas. These analyses, together with numerical simulations, reveal that in their mature stages, such storms intensify and are maintained by a feedback between surface enthalpy fluxes and wind, and as such are isomorphic with tropical cyclones. In this paper, I demonstrate that a cold, upper low over the Mediterranean can produce strong cyclogenesis in an axisymmetric model, thereby showing that baroclinic instability is not necessary during the mature stages of Mediterranean hurricanes.http://www.adv-geosci.net/2/217/2005/adgeo-2-217-2005.pdf |
spellingShingle | K. Emanuel Genesis and maintenance of "Mediterranean hurricanes" Advances in Geosciences |
title | Genesis and maintenance of "Mediterranean hurricanes" |
title_full | Genesis and maintenance of "Mediterranean hurricanes" |
title_fullStr | Genesis and maintenance of "Mediterranean hurricanes" |
title_full_unstemmed | Genesis and maintenance of "Mediterranean hurricanes" |
title_short | Genesis and maintenance of "Mediterranean hurricanes" |
title_sort | genesis and maintenance of quot mediterranean hurricanes quot |
url | http://www.adv-geosci.net/2/217/2005/adgeo-2-217-2005.pdf |
work_keys_str_mv | AT kemanuel genesisandmaintenanceofquotmediterraneanhurricanesquot |