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[[File:Mediterranean Cyclone 16 jan 1995 1004Z.jpg|right|thumb|Satellite image of a Medicane from 1995]]
[[File:Mediterranean Cyclone 16 jan 1995 1004Z.jpg|thumb|right|250px|Satellite imagery of a well-documented Mediterranean tropical cyclone at 1004 UTC on 16 January 1995]]
'''Mediterranean tropical cyclones''', sometimes referred to as '''Mediterranean hurricanes''' or '''medicanes''' are a rare meteorological phenomenon observed in the [[Mediterranean Sea]]. Due to the dry nature of the Mediterranean region, formation of [[tropical cyclone]]s is infrequent, with only 99 recorded cyclones between 1948 and 2011. [[Tropical cyclogenesis]] typically occurs within two separate regions of the sea. The first region, encompassing areas of the western Mediterranean, is more conducive for development than the other, the [[Ionian Sea]] to the east. The rough mountainous geography of the region raises additional difficulties despite being favorable for the development of severe weather and convective activity in general, and only with abnormal meteorological circumstances can medicanes form. Numerous studies have been conducted on the impact of [[global warming]] on Mediterranean tropical cyclone formation, with generally concluding that although fewer storms would form, those that did would be of a greater intensity.
A '''Mediterranean tropical cyclone''', sometimes called a '''Medicane''', is a ''subtropical or tropical'' cyclone like storm system that resembles a [[hurricane]]. It occurs in the [[Mediterranean Sea]], and usually does not reach hurricane strength. These storms generate a lot of damage due to highly populated areas in the Mediterranean region.<ref name="ReferenceA">ftp://texmex.mit.edu/pub/emanuel/PAPERS/Romero_Emanuel_2013.pdf</ref> Even though the Mediterranean is not a official tropical cyclone basin, and thus not under the authority of any [[Regional Specialized Meteorological Center]] like the [[National Hurricane Center]], cyclones occasionally form in the mid-latitudes and on very rare occasions in the [[Black Sea]],<ref>http://en.ria.ru/strange/20120127/170988652.html</ref><ref>http://link.springer.com/article/10.3103%2FS1068373908040067#</ref><ref>http://query.nytimes.com/gst/abstract.html?res=F4061EF73B5A12738DDDAF0994DB405B868CF1D3</ref> having properties of a [[tropical cyclone]]. A medicane is small, has an [[Rotational_symmetry|axisymmetric]] cloud structure, generates strong winds, heavy rains and thunderstorms. This phenomenon has often been named Medicane or Tropical-like Mediterranean Storm (T.M.S.).


The development of tropical cyclones in the Mediterranean Sea can usually only occur under somewhat unusual circumstances. Low [[wind shear]] and [[atmosphere|atmospheric]] instability induced by incursions of cold air are often required. A majority of medicanes are also accompanied by upper-level [[trough (meteorology)|trough]]s, providing energy required for intensifying [[atmospheric convection]]—thunderstorms—and heavy [[precipitation]]. The [[baroclinity|baroclinic]] properties of the Mediterranean region, with high temperature gradients, also provides necessary instability for the formation of tropical cyclones. Another factor, rising cool air, provides necessary moisture as well. Warm [[sea surface temperature|sea surface temperatures (SSTs)]] are mostly unnecessary, however, as most medicanes' energy is derived from warmer air temperatures. When these favorable circumstances coincide, the genesis of warm-core Mediterranean tropical cyclones, often from within existing cut-off [[cold-core low]]s, is possible in a conducive environment for formation.
==Climatology==
Tropical cyclone-like systems in the Mediterranean Sea are extremely rare. Sufficient evidence has not been presented to prove these systems are full-fledged tropical systems, as some previously recorded cyclones share more characteristics with [[polar low]]s than regular [[tropical cyclone]]s.<ref name="tfaq">{{cite web|url=http://www.aoml.noaa.gov/hrd/tcfaq/F1.html|title=TCFAQ F1) What regions around the globe have tropical cyclones and who is responsible for forecasting there?|last=Landsea|first=Chris|work=[[Atlantic Oceanographic and Meteorological Laboratory]]|publisher=[[Hurricane Research Division]]|date=2010-05-14|accessdate=2011-11-07}}</ref> A cyclonic system in January 1995 resembled a [[tropical cyclone]] in several aspects — it featured an [[eye (cyclone)|eye]] and a warm core. Experiments revealed that heat and moisture were abundant at the time of formation of the 1995 cyclone, and were vital in its development. However, baroclinic instability did not appear to have been a major factor in its formation, although it formed near a baroclinic zone.<ref name="pytharoulis">{{cite journal|last1=Pytharoulis|last2=Craig|first2=C.G.|last3=Ballard|first3=S.P.|year=1999|title=Study of the Hurricane-like Mediterranean cyclone of January 1995|journal=Physics and Chemistry of the Earth|volume=24|issue=6|pages=627–632|doi=10.1016/S1464-1909(99)00056-8|accessdate=2011-11-07}}</ref>


Several notable and damaging medicanes are known to have occurred. In September 1969, a north African Mediterranean tropical cyclone produced flooding which killed nearly 600&nbsp;individuals, left 250,000&nbsp;homeless, and crippled local economies. A medicane in September&nbsp;1996 which developed in the [[Balearic Islands]] region spawned six tornadoes and inundated parts of the islands. Several medicanes have also been subject to extensive study, such as those of January&nbsp;1982, January&nbsp;1995, September&nbsp;2006, and November&nbsp;2011. The January&nbsp;1995 storm is one of the best-studied Mediterranean tropical cyclones, with its close resemblance to tropical cyclones elsewhere and availability of observations. The medicane of September&nbsp;2006, meanwhile, is well-studied due to availability of existing observations and data. In November&nbsp;2011, the [[National Oceanic and Atmospheric Administration]] officially designated a Mediterranean tropical cyclone for the first time as 01M, also named Tropical Storm Rolf by the [[Free University of Berlin]].
Most Medicanes form in the western [[Mediterranean]] region, and some form in the Ionian region.<ref name="refa">Leone Cavicchia, Hans von Storch and Silvio Gualdi [http://www.academia.edu/4775469/A_long-term_climatology_of_medicanes A long-term climatology of medicanes] ''Climate Dynamics'' August 2013</ref> There is a difference between the two regions: In fall there is a steady increase in Medicane formation in the western Mediterranean region and in January it decreases. In the [[Ionian Sea|Ionian region]] Medicanes are less frequent in fall than in January or February.<ref name="refa"/>


== Climatology ==
==Origins and features==
[[File:Mediterranean Cyclone 07 oct 1996 1202Z.jpg|thumb|right|200px|Visible satellite imagery of a medicane above the Balearic Islands on 7 October 1996]]
A majority of [[Mediterranean Sea|Mediterranean]] [[tropical cyclone]]s form over two separate regions. The first, more conducive for development than the other, encompasses an area of the western Mediterranean bordered by the [[Balearic Islands]], southern [[France]], and the shorelines of the islands of [[Corsica]] and [[Sardinia]]. The second identified region of development, in the [[Ionian Sea]] between [[Sicily]] and [[Greece]] and stretching south to [[Libya]], is less favorable for [[tropical cyclogenesis]]. An additional two regions, in the [[Aegean Sea|Aegean]] and [[Adriatic Sea|Adriatic]] seas, produce fewer medicanes, while activity is minimal in the [[Levant]]ine region. The geographical distribution of Mediterranean tropical cyclones is markedly different than that of other [[cyclone]]s, with the formation of regular cyclones centering on the [[Pyrenees]] and [[Atlas Mountains|Atlas]] mountain ranges, the [[Gulf of Genoa]], and the island of [[Cyprus]] in the [[Ionian Sea]].<ref name="Cavicchia2013-7">Cavicchia et al. 2013, p. 7</ref> Although meteorological factors are most advantageous in the Adriatic and Aegean seas, the closed nature of the region's geography, bordered by land, allows little time for further evolution.<ref name="Cavicchia2013-18">Cavicchia et al. 2013, p. 18</ref>


The geography of mountain ranges bordering the Mediterranean are conducive for severe weather and thunderstorms, with the sloped nature of mountainous regions permitting the development of convective activity.<ref name="Homar2003-1470">Homar et al. 2003, p. 1470</ref> Although the geography of the Mediterranean region, as well as its dry air, typically prevent the formation of tropical cyclones, when [[#Development and characteristics|certain meteorological circumstances arise]], difficulties influenced by the region's geography are overcome.<ref name="Emanuel2005-220">Emanuel 2005, p. 220</ref> The occurrence of tropical cyclones in the Mediterranean Sea is generally extremely rare, with an average of 1.57&nbsp;forming annually and merely 99&nbsp;recorded occurrences discovered between 1948 and 2011 in a modern study, with no definitive trend in activity within that period.<ref name="Cavicchia2013-6">Cavicchia et al. 2013, p. 6</ref> Few medicanes form during the summer season, though activity typically rises in autumn, peaks in January, and gradually decreases from February to May.<ref name="Cavicchia2013-7"/> In the western Mediterranean region of development, approximately 0.75&nbsp;such systems form each year, compared to 0.32&nbsp;in the Ionian Sea region.<ref name="Cavicchia2013-8">Cavicchia et al. 2013, p. 8</ref>
At least once or twice every year,<ref name="ReferenceA"/><ref>http://www.uib.es/depart/dfs/meteorologia/METEOROLOGIA/ANGEL/ProceedingEUMETSAT07.pdf</ref> usually during fall when the [[Mediterranean Sea]] is still warm, a [[Low-pressure area|depression]] takes on the characteristics of a subtropical storm with clouds wrapped around an eye, intense [[thunderstorm]] activity, strong winds at surface winds and warm temperature in the center clouds. In a satellite image such a system can look very similar to a tropical storm, but without having the dimensions or the power. An example for such a cyclonic storm is a Medicane that threatened [[France]] from November 1 to November 9, 2011 and produced up to {{convert|800|mm|in|abbr=on}} of rain.<ref>http://www.meteo.fr/cic/meetings/2012/ERAD/presentations/thursday/13A-4.pdf</ref>


Studies have evaluated that [[global warming]] can result in higher observed intensities of tropical cyclones as a result of deviations in the [[flux|surface energy flux]] and atmospheric composition, which both heavily influence the development of medicanes as well. In tropical and subtropical areas, [[sea surface temperature|sea surface temperatures (SSTs)]] rose {{convert|0.2|C|F}} within a 50-year period, and in the [[North Atlantic hurricane|North Atlantic]] and [[typhoon|Western Pacific]] [[tropical cyclone basins]], the potential destructiveness and energy of storms nearly doubled within the same duration, evidencing a clear correlation between global warming and tropical cyclone intensities.<ref name="TousRomero2013-9">Tous & Romero 2013, p. 9</ref> Within a similarly recent 20-year period,<ref name="TousRomero2013-10">Tous & Romero 2013, p. 10</ref> SSTs in the Mediterranean Sea increased by {{convert|0.6|to|1|C|F}},<ref name="TousRomero2013-9"/> though no observable increase in medicane activity has been noted, as of yet.<ref name="Cavicchia2013-6"/> In 2006, a computer-driven [[atmospheric model]] evaluated the future frequency of Mediterranean cyclones between 2071 and 2100, projecting a decrease in autumn, winter, and spring cyclonic activity coinciding with a dramatic increase in formation near [[Cyprus]], with both scenarios attributed to elevated temperatures as a result of [[global warming]].<ref name="Anagnostopoulou2006-13">Anagnostopoulou et al. 2006, p. 13</ref> Other studies, however, have been inconclusive, forecasting both increases and decreases in duration, number, and intensity.<ref name="Gaertner2007-4">Gaertner et al. 2007, p. 4</ref> A third study, conducted in 2013, evaluated that while medicane activity would likely decline between 10 and 40 percent by 2100, a higher percentage of those that formed would be of greater strength.<ref name="RomeroEmanuel2013">Romero & Emanuel 2013, p. 6000</ref>
The origins of Mediterranean tropical cyclones can usually be traced to deep [[block (meteorology)#Cut-off highs and lows|cut-off]] [[cold-core low|cold-core low pressure systems]]. These systems usually featured deep [[atmospheric convection|convection]] and strong winds. In contrast to normal tropical cyclones, Mediterranean storms remain at a minimal size and usually do not exceed a weak intensity. Medicanes usually feature weak rotation at the time of formation, which increases dramatically as they evolve, along with an increase in size. However, of seven cyclones studied, none exceeded {{convert|500|km|mi}} in diameter.<ref name="fita">{{cite web|url=http://hal.archives-ouvertes.fr/docs/00/30/16/76/PDF/nhess-7-41-2007.pdf|title=Analysis of the environments of seven Mediterranean tropical-like storms using an axisymmetric, nonhydrostatic, cloud resolving model|last1=Fita|first1=L.|last2=Romero|first2=R.|last3=Luque|first3=A.|last4=Emanuel|first4=K.|last5=Ramis|first5=C.|date=2007-01-15|work=Grup de Meteorologia; [[Massachusetts Institute of Technology]]|publisher=Natural Hazards and Earth System Sciences|pages=41–56|accessdate=2011-11-07}}</ref>
[[File:Mediterranean Hurricane TLC dic 2005.jpg|right|thumb|Satellite image of a December Medicane from 2005]]


== Development and characteristics ==
Using a simulated cloud model, it has been noted that a slight increase in [[humidity]] can result in a much more intense cyclone. In addition, the formation is accelerated, being reduced from the original simulation of 4 days to 2 days.<ref name="fita" /> It is also proven that unlike regular tropical cyclones, high sea surface temperatures are not vital in medicanes. Medicanes usually evolve under the influence of [[trough (meteorology)|trough]]s in the upper troposphere. The environment in the Mediterranean is usually too dry, although if an upper-level cut-off low moves into the area, the cold air brought with it must rise to keep steady, creating a cool, humid, environment. The high temperatures of the Mediterranean's reaction with the cool air associated with the low creates a situation in which tropical cyclone-like have potential to develop.<ref name="emanuel">{{cite journal|last=Emanuel|first=Kerry|others=Ferraris, L. (editor)|date=2005-06-27|title=Genesis and maintenance of "Mediterranean hurricanes"|journal=Advances in Geosciences|volume=2|pages=217–220|url=http://www.adv-geosci.net/2/217/2005/adgeo-2-217-2005.pdf|doi=10.5194/adgeo-2-217-2005|accessdate=2011-11-08}}</ref>
[[File:Mediterranean tropical cyclone October 27 2005.jpg|thumb|right|200px|A Mediterranean tropical cyclone south of Italy on 27 October 2005]]
Factors required for the formation of medicanes are somewhat different than that normally expected of [[tropical cyclone]]s; known to emerge over regions with [[sea surface temperature|sea surface temperatures (SSTs)]] below {{convert|26|C|F}}, development often requires incursions of colder air inducing atmospheric instability.<ref name="Cavicchia2013-7"/> A majority of medicanes develop above regions of the Mediterranean with temperatures of {{convert|15|to|26|C|F}}, with the upper bound only found in the southernmost reaches of the sea. Despite the low sea surface temperatures, the instability incited by cold atmospheric air within a [[baroclinity|baroclinic]] zone permits the formation of medicanes, while in tropical areas where high baroclinity is absent, raised SSTs are needed.<ref name="TousRomero2013-8">Tous & Romero 2013, p. 8</ref> While significant deviations in air temperature have been noted around the time of Mediterranean tropical cyclones' formation, few anomalies in sea surface temperature coincide with their development, indicating that the development of medicanes is influenced by elevated air temperatures, not by by anomalous SSTs.<ref name="Cavicchia2013-14">Cavicchia et al. 2013, p. 14</ref> Similar to tropical cyclones, minimal [[wind shear]] as well as abundant moisture and vorticity encourages the genesis of tropical cyclone-like systems in the Mediterranean Sea.<ref name="Cavicchia2013-15">Cavicchia et al. 2013, p. 15</ref>


Due to the more confined character of the Mediterranean and the limited capability of [[heat flux]]es, tropical cyclones with a diameter larger than {{convert|300|km|mi|abbr=on}} cannot exist.<ref name="TousRomero2013-3">Tous & Romero 2013, p. 3</ref> Despite being a relatively baroclinic area with high temperature gradients, the primary energy source utilized by Mediterranean tropical cyclones is derived from underlying heat sources generated by the presence of convection in a humid environment, similar to tropical cyclones elsewhere, outside the Mediterranean Sea.<ref name="TousRomero2013-5">Tous & Romero 2013, p. 5</ref> In comparison to other [[tropical cyclone basins]], the Mediterranean Sea is generally presents a dificult environment for development; although the potential energy necessary for development is not abnormally large, its atmosphere is characterized by its lack of moisture, impeding potential formation. The full development of a medicane often necessitates the formation of a large-scale baroclinic disturbance transitioning late in its life cycle into a tropical cyclone-like system, nearly always under the influence of a deep, cut-off, [[cold-core low]] within the middle-to-upper [[troposphere]], frequently resulting from abnormalities in a wide-spreading [[Rossby wave]].<ref name="TousRomero2013-6">Tous & Romero 2013, p. 6</ref>
==Evolution and life cycle==


[[File:Mediterranean tropical cyclone January 28 2010.jpg|thumb|right|200px|A weak and disorganized Mediterranean tropical cyclone on 28 January 2010]]
Medicanes usually have a life cycle between 12 hours and 5 days and travel between {{convert|700|km|abbr=on}} and
{{convert|3000|km|abbr=on}}.<ref>http://www.hvonstorch.de/klima/pdf/cavicchia-2011.pdf</ref> These cyclone like storms are similar to tropical cyclones in the [[Caribbean]] or the [[Atlantic Ocean]], however there are some differences concerning evolution of theses storms. Unlike [[hurricanes]], which often evolve from a [[tropical wave]], medicanes often have developed from a cold upper-level low.<ref>[http://www.uib.es/depart/dfs/meteorologia/METEOROLOGIA/MEDICANES/introduction.html MEDICANES: Mediterranean tropical-like storms - introduction] Grup de Meterologia Department de Fisia, Universitat de les Illes Balears</ref> In the first phase there is a [[Baroclinity|baroclinic]] development, the second phase, however is much more like a convective tropical air-sea interaction<ref group=note>convective tropical-like activity and air-sea interaction</ref> with sea temperatures above 26°C (78.8°F)


The development of medicanes often results from the vertical shift of air in the troposphere, resulting in a decrease in its temperature coinciding with an increase in relative humidity, creating an environment more conducive for tropical cyclone formation. This in turn leads to in an increase in potential energy, producing heat-induced air-sea instability. Moist air prevents the occurrence of convective [[vertical draft|downdrafts]] which often hinder the inception of tropical cyclones,<ref name="TousRomero2013-6"/> and in such a scenario, wind shear remains minimal; overall, cold-core cut-off lows serve well for the later formation of compact [[flux|surface flux]]-influenced warm-core lows such as medicanes. The regular genesis of cold-core upper-level lows and the infrequency of Mediterranean tropical cyclones, however, indicate that additional unusual circumstances are involved the emergence of the latter. Elevated sea surface temperatures, contrasting with cold atmospheric air, encourage atmospheric instability, especially within the troposphere.<ref name="TousRomero2013-8"/>
A study concluded that warmth generated by the ocean were not an essential in the development of a Mediterranean cyclone in September 1996. In addition, it was evaluated that the upper-level trough played a crucial role in the evolution of a cyclone.<ref name="homar">{{cite journal|last1=Homar|first1=V.|last2=Romero|first2=R.|last3=Stensrud|first3=D.J.|last4=Ramis|first4=C.|last5=Alonso|first5=S.|date=April 2003|title=Numerical diagnosis of a small, quasi-tropical cyclone over the western Mediterranean: Dynamical vs. boundary factors|journal=[[Astronomy & Geophysics#Quarterly Journal of the RAS|Quarterly Journal of the Royal Astronomical Society]]|publisher=[[John Wiley & Sons#Wiley Online Library|Wiley Online Library]]|volume=129|issue=590|pages=1469–1490|url=http://onlinelibrary.wiley.com/doi/10.1256/qj.01.91/pdf|issn=1477-870X|doi=10.1256/qj.01.91|accessdate=2011-11-08}}</ref>


In general, most medicanes maintain a radius of {{convert|70|to|200|km|mi|abbr=on}}, last between 12&nbsp;hours and 5&nbsp;days, travel between {{convert|700|to|3000|km|mi|abbr=on}}, develop an eye for less than 72&nbsp;hours, and feature wind speeds approaching {{convert|144|km/h|mph|abbr=on}};<ref name="CavicchiavonStorch-2012-2273">Cavicchia & von Storch 2012, p. 2276</ref> in addition, a majority are characterized on [[satellite imagery]] by a distinct round [[eye (cyclone)|eye]] encircled by [[atmospheric convection]] in addition to a mostly axisymmetric cloud pattern.<ref name="TousRomero2013-3"/> Weak rotation, similar to that in most tropical cyclones, is usually noted in a medicane's early stages, increasing with intensity;<ref name="Fita2007-43">Fita et al. 2007, p. 43</ref> medicanes, however, often have less time to intensify, remaining weaker than most [[North Atlantic hurricane]]s and only persisting for the duration of a few days.<ref name="Fita2007-53">Fita et al. 2007, p. 53</ref> The maximum achievable intensity of medicanes is equivalent to the lowest classification on the [[Saffir–Simpson hurricane wind scale]], Category&nbsp;1. While the entire lifetime of a cyclone may encompass several days, most will only retain tropical characteristics for less than 24&nbsp;hours.<ref name="Miglietta2013-2402">Miglietta et al. 2013, p. 2402</ref> Circumstances sometimes permit the formation of smaller-scale medicanes, although the required conditions differ even from those needed by other medicanes. The development of abnormally small tropical cyclones in the Mediterranean usually requires upper-level atmospheric cyclones inducing cyclogenesis in the lower atmosphere, leading to the formation of warm-core lows, encouraged by favorable moisture, heat, and other environmental circumstances.<ref name="Homar2003-1469">Homar et al. 2003, p. 1469</ref>
==Notes==
{{reflist|group=note}}


Mediterranean cyclones have been compared to [[polar low]]s for their similarly small size and heat-related instability; however, while medicanes nearly always feature warm-core lows, polar lows are primarily cold-cored. The prolonged life of medicanes and similarity to polar lows is caused primarily by origins as synoptic-scale surface lows and heat-related instability.<ref name="Homar2003-1470"/> Heavy precipitation and convection within a developing Mediterranean tropical cyclone are usually incited by the approach of an upper-level [[trough (meteorology)|trough]], bringing downstream cold air, encircling an existing low-pressure system. After this occurs, however, a considerable reduction in rainfall rates occurs despite visible organization on satellite imagery,<ref name="Claud2010-2211">Claud et al. 2010, p. 2211</ref> coinciding with a decrease in lightning activity, previously high, as well.<ref name="Miglietta2013-2404">Miglietta et al. 2013, p. 2404</ref> Although throughs will often accompany medicanes along their track, separation eventually occurs, usually in the later part of a Mediterranean tropical cyclone's life cycle.<ref name="Claud2010-2211"/> At the same time, moist air, saturated and cooled while rising into the atmosphere, then encounters the medicane and permits further development and evolution into a tropical cyclone. Many of these characteristics are also evident in polar lows.<ref name="Emanuel2005-217">Emanuel 2005, p. 217</ref>
==References==
{{reflist}}


== Known occurrences and impacts ==
==External links==
=== September 1969 ===
* {{official website|http://www.eumetsat.int/}}
[[File:Mediterranean tropical cyclone 23 September 1969 0909Z.png|thumb|right|200px|ESSA-8 visible satellite imagery of the September 1969 cyclone]]
* [http://internationalweatherarchive.org/satellite.aspx EUMETSAT weather satellite viewer]
An unusually severe Mediterranean tropical cyclone developed on 23&nbsp;September 1969 southeast of [[Malta]], producing severe flooding.<ref name="Pytharoulis2000-262"/> Steep pressure and temperature gradients above the [[Atlas Mountains|Atlas mountain range]] were evident on 19&nbsp;September, a result of cool sea air attemtping to penetrate inland; south of the mountains, a lee depression developed. Under the influence of mountainous terrain, the [[low-pressure area]] initially meandered northeastward, but following the entry of cool sea air, it recurved to the southeast before transitioning into a Saharan depression associated with a distinct cold front by 22&nbsp;September. Along the front's path, desert air moved northward while cold air drifted in the opposite direction, and in northern Libya, warm arid air clashed with the cooler [[levant (wind)|levant]] of the Mediterranean. The organization of the disturbance improved slightly further before emerging into the Mediterranean Sea on 23&nbsp;September, upon which the system experienced immediate [[cyclogenesis]],<ref name="Winstanley1970-393">Winstanley 1970, p. 393</ref> rapidly intensifying while southeast of Malta as a cold-core cut-off low,<ref name="Winstanley1970-396">Winstanley 1970, p. 396</ref> and acquiring tropical characteristics.<ref name="Pytharoulis2000-262"/> In western Africa, meanwhile, several disturbances converged toward [[Mauritania]] and [[Algeria]], while the medicane recurved southwestward back toward the coast, losing its closed circulation and later dissipating.<ref name="Winstanley1970-396"/>
* [http://www.cyprus-storms.net/medhurricanes.htm Website monitoring Medicane activity]
* [http://www.nat-hazards-earth-syst-sci.net/10/2199/2010/nhess-10-2199-2010.html Scientific article about Medicanes]


The cyclone produced severe flooding throughout regions of northern Africa. Malta received upward of {{convert|123|mm|in|abbr=on}} of rainfall on 23&nbsp;September, [[Sfax]] measured {{convert|45|mm|in|abbr=on}} on 24&nbsp;September, [[Tizi Ouzou]] collected {{convert|55|mm|in|abbr=on}} on 25&nbsp;September, [[Gafsa]] received {{convert|79|mm|in|abbr=on}} and [[Istanbul]] measured {{convert|46|mm|in|abbr=on}} on 26&nbsp;September, Cap Bengut collected {{convert|43|mm|in|abbr=on}} on 27&nbsp;September, and [[Biskra]] received {{convert|122|mm|in|abbr=on}} on 28&nbsp;September.<ref name="Winstanley1970-392">Winstanley 1970, p. 392</ref> In Malta, a 20000-ton tanker struck a reef and split in two, while in Gafsa, Tunisia, the cyclone flooded [[phosphate]] mines, leaving over 25,000&nbsp;miners unemployed and costing the government over £2&nbsp;million per week. Thousands of camels and snakes, drowned by flood waters, were swept out to sea, and massive [[Roman bridge]]s, which withstood all floods since the [[Decline of the Roman Empire|fall of the Roman Empire]], collapsed. In all, the floods in Tunisia and Algeria killed almost 600&nbsp;individuals, left 250,000&nbsp;homeless, and severely damaged regional economies.<ref name="Winstanley1970-390">Winstanley 1970, p. 390</ref> Due to communication problems, however, flood relief funds and television appeals were not set up until nearly a month later.<ref name="Winstanley1970-392"/>
<!--spacing-->


=== January 1982 ===
{{Portal|Tropical cyclones}}
[[File:Mediterranean tropical storm 26 January 1982 1236Z.png|thumb|right|200px|NOAA-7 visible satellite imagery of a Mediterranean tropical storm at 1236 UTC on 26 January 1982]]
{{Cyclones}}
The unusual Mediterranean tropical storm of January&nbsp;1982 was first detected in waters north of [[Libya]].<ref name="Pytharoulis2000-262"/> The storm likely reached the [[Atlas Mountains|Atlas mountain range]] as a [[low-pressure area]] by 23&nbsp;January 1982, reinforced by an elongated, slowly-drifting trough above the [[Iberian Peninsula]]. Eventually, a closed circulation center developed by 1310&nbsp;[[Coordinated Universal Time|UTC]],<ref name="ErnstMatson1983-333">Ernst & Matson 1983, p. 333</ref> over parts of the Mediterranean with [[sea surface temperature|sea surface temperatures (SSTs)]] of approximately {{convert|12|C|F}}.<ref name="ErnstMatson1983-334">Ernst & Matson 1983, p. 334</ref> A hook-shaped cloud developed within the system shortly thereafter, rotating as it elongated into a {{convert|150|km|mi|abbr=on}}-long comma-shaped apparatus. After looping around Sicily, it drifted eastward between the island and [[Peloponnese]], recurving on its track again,<ref name="Reed2001-187">Reed et al. 2001, p. 187</ref> exhibiting clearly curved spiral banding before shrinking slightly.<ref name="Reed2001-189">Reed et al. 2001, p. 189</ref> The cyclone reached its peak intensity at 1800&nbsp;UTC on the following day, maintaining an [[atmospheric pressure]] of 992&nbsp;[[bar (unit)|mbar]] (29.30&nbsp;[[inch of mercury|inHg]]), and was succeeded by a period of gradual weakening, with the system's pressure eventually rising to 1009&nbsp;mbar (29.80&nbsp;inHg). The system slightly reintensified, however, for a six-hour period on 26&nbsp;January. Ship reports indicated winds of {{convert|93|km/h|mph|abbr=on}} were present in the cyclone at the time, tropical storm-force winds on the [[Saffir–Simpson hurricane wind scale]].<ref name="ErnstMatson1983-333"/>


The Global Weather Center's Cyclone Weather Center of the [[United States Air Force]] initiated "Mediterranean Cyclone Advisories" on the cyclone at six-hour intervals starting at 1800&nbsp;UTC on 27&nbsp;January until 0600&nbsp;UTC the following day.<ref name="ErnstMatson1983-337"/> Although the most intense convection was present in the eastern sector of the cyclone as it drifted east-northeastward, the ship reports containing information on wind speed could have been within the opposite side of the eyewall, which usually features the highest winds in a tropical cyclone. On infrared satellite imagery, the [[eye (cyclone)|eye]] itself was {{convert|58.5|km|mi|abbr=on}} in diameter,<ref name="ErnstMatson1983-334"/> contracting to just {{convert|28|km|mi}} one day prior to making landfall.<ref name="ErnstMatson1983-337">Ernst & Matson 1983, p. 337</ref> The cyclone passed by Malta, Italy, and Greece before dissipating several days later in the extreme eastern Mediterranean. Observations related to the cyclone, however, were inadequate, and although the system maintained numerous tropical characteristics, it is possible it was merely a compact but powerful [[extratropical cyclone]] exhibiting a clear eye, spiral banding, towering cumulonimbi, and high surface winds along the eyewall.<ref name="Pytharoulis2000-262"/>
{{DEFAULTSORT:Tropical Cyclone}}

[[Category:Basic meteorological concepts and phenomena]]
=== January 1995 ===
[[Category:Tropical cyclone meteorology|Medicane]]
[[File:Mediterranean Cyclone 15 jan 1995 1015Z.jpg|thumb|right|200px|The 1995 medicane at 1015 UTC on 15&nbsp;January shortly after tropical cyclogenesis]]
[[Category:Tropical cyclones|Medicane]]
Among numerous documented medicanes, the cyclone of January&nbsp;1995 is generally considered to be the best-documented instance. Emerging off of the [[Libya]]n coast into the central [[Mediterranean Sea]] toward the [[Ionian Sea|Ionian]] shoreline of [[Greece]] on 13&nbsp;January as a compact [[low-pressure area]], the precursor low maintained winds reaching up to {{convert|108|km/h|mph|abbr=on}} as it traversed the Ionian Sea,<ref name="CavicchiavonStorch-2012-2280">Cavicchia & von Storch 2012, p. 2280</ref> while the German research ship ''Meteor'' noted winds of {{convert|135|km/h|mph|abbr=on}}.<ref name="Pytharoulis2000-263">Pytharoulis et al. 2000, p. 263</ref> Upon the low's approach near Greece, it began to envelop an area of [[atmospheric convection]]; meanwhile, in the middle [[troposphere]], a [[trough (meteorology)|through]] extended from Russia to the Mediterranean, bringing with it extremely cold temperatures.<ref name="Pytharoulis1999-628">Pytharoulis et al. 1999, p. 628</ref> Two low-pressure areas were present along the path of the trough, with one situated above Ukraine and the other above the central Mediterranean, likely associated with a low-level cyclone over western Greece, which began to weaken on 14&nbsp;January, and a second low, the system which would evolve into the Mediterranean tropical cyclone, developed ''in situ'' on 15&nbsp;January.<ref name="Pytharoulis2000-263"/>
[[Category:Types of cyclone|Medicane]]

[[Category:Vortices|Medicane]]
At the time of formation, high clouds indicated the presence of intense convection,<ref name="Pytharoulis2000-263"/> and the cyclone featured an axisymmetric cloud structure, with a distinct, cloud-free [[eye (cyclone)|eye]] and [[rainband]]s spiraling around the disturbance as a whole.<ref name="Pytharoulis2000-264">Pytharoulis et al. 2000, p. 264</ref> Soon thereafter, the parent low separated from the medicane entirely and continued eastward,<ref name="Pytharoulis1999-628"/> meandering toward the [[Aegean Sea]] and [[Turkey]].<ref name="CavicchiavonStorch-2012-2280"/> Initially remaining stationary between Greece and [[Sicily]] with a minimum [[atmospheric pressure]] of 1002&nbsp;[[bar (unit)|mbar]] (29.59&nbsp;[[inch of mercury|inHg]]), the newly-formed system began to drift southwest-to-south in the following days, influenced by northeasterly flow incited by the initial low, now far to the east, and a [[high-pressure area]] above central and eastern Europe.<ref name="Pytharoulis1999-628"/> The system's atmospheric pressure increased throughout 15&nbsp;January due to the fact it was embedded within a large-scale environment, with its rising pressure due to the general prevalence of higher air pressures throughout the region, and was not a sign of deintensification.<ref name="Pytharoulis2000-264"/>
[[Category:Weather hazards|Medicane]]

[[Category:Global warming and hurricanes|Medicane]]
Initial wind speeds within the young medicane were generally low, with sustained winds of merely {{convert|28|to|46|km/h|mph|abbr=on}}, with the highest recorded value associated with the disturbance being {{convert|63|km/h|mph|abbr=on}} at 0000&nbsp;UTC on 16&nbsp;January, slightly below the threshold for tropical storm on the [[Saffir–Simpson hurricane wind scale]]. Its structure now consisted of a distinct eye encircled by counterclockwise-rotating [[cumulonimbus cloud|cumulonimbi]] with [[cloud top]] temperatures below {{convert|-50|C|F}}, evidencing deep convection and a regular feature observed in most tropical cyclones.<ref name="Pytharoulis2000-265">Pytharoulis et al. 2000, p. 265</ref> Intense convection continued to follow the entire path of the system as it traversed the Mediterranean, and the cyclone made [[landfall (meteorology)|landfall]] in northern Libya at approximately 1800&nbsp;[[Coordinated Universal Time|UTC]] on 17&nbsp;January, rapidly weakening after coming ashore.<ref name="Pytharoulis1999-628"/> As it moved inland, a minimum atmospheric pressure of 1012&nbsp;mbar (29.89&nbsp;inHg) was recorded, accompanied by wind speeds of {{convert|93|km/h|mph|abbr=on}} as it slowed down after passing through the [[Gulf of Sidra]].<ref name="Pytharoulis2000-266">Pytharoulis et al. 2000, p. 266</ref> Although the system retained its strong convection for several more hours, the cyclone's cloud tops began to warm, evidencing lower clouds, before losing tropical characteristics entirely on 17&nbsp;January.<ref name="Pytharoulis2000-267">Pytharoulis et al. 2000, p. 267</ref> Offshore ship reports recorded that the medicane produced intense winds, copious rainfall, and abnormally warm temperatures.<ref name="CavicchiavonStorch-2012-2281">Cavicchia & von Storch 2012, p. 2281</ref>

=== September and October 1996 ===
[[File:Mediterranean Cyclone 07 oct 1996 0603Z.jpg|thumb|right|200px|The last major Mediterranean tropical cyclone of 1996 while west of Italy on 7&nbsp;October]]
Three notable medicanes developed in 1996. The first, in mid-September&nbsp;1996, was a typical Mediterranean tropical cyclone which developed in the [[Balearic Islands]] region, an area conducive to cyclone development.<ref name="CavicchiavonStorch-2012-2282">Cavicchia & von Storch 2012, p. 2282</ref> At the time of the cyclone's formation, a powerful Atlantic [[cold front]] and a [[warm front]] associated with the large-scale low, producing northeasterly winds over the Iberian peninsula, extended eastward into the Mediterranean, while abundant moisture gathered in the lower troposphere over the Balearic channel.<ref name="Homar2003-1473">Homar et al. 2003, p. 1473</ref> On the morning of 12&nbsp;September, a disturbance developed off the coast of [[Valencia|Valencia, Spain]], dropping heavy rainfall on the coast. An eye developed shortly thereafter as the system rapidly traversed across [[Majorca]] and [[Sardinia]] in its eastward trek before making landfall upon the coast of southern Italy on the evening of 13&nbsp;September with a minimum atmospheric pressure of 990&nbsp;mbar (29.24&nbsp;inHg), dissipating shortly after coming ashore,<ref name="CavicchiavonStorch-2012-2283">Cavicchia & von Storch 2012, p. 2283</ref> with a diameter of about {{convert|150|km|mi|abbr=on}}.<ref name="Homar2003-1469"/>

At Valencia and other regions of eastern Spain, the storm generated heavy precipitation, while six tornadoes touched down over the Balearic Islands. While approaching the coast, the warm-core low induced a pressure drop of 11&nbsp;mbar (0.32&nbsp;inHg) at [[Palma, Majorca]] in advance of the tropical cyclone's landfall. Medicanes as small as the one that formed in September&nbsp;1996 are atypical, and often require circumstances different even from those required for regular Mediterranean tropical cyclone formation.<ref name="Homar2003-1469"/> Warm low-level [[advection]] caused by a large-scale low over the western Mediterranean,<ref name="Homar2003-1470"/> in conjunction with the presence of a mid- to upper-level cut-off cold-core low were the two main factors in the rise of strong convection. In addition, interaction between a northeastward-drifting [[trough (meteorology)|trough]], the medicane, and the large-scale also permitted the formation of tornadoes within thunderstorms generated by the cyclone after making landfall.<ref name="Homar2003-1471">Homar et al. 2003, p. 1471</ref>

The second of the three recorded Mediterranean tropical cyclones in 1996 formed between Sicily and [[Tunisia]] on 4&nbsp;October, making landfall on both Sicily and southern Italy. The medicane generated major flooding in Sicily; meanwhile, in [[Calabria]], wind gusts of up to {{convert|108|km/h|mph|abbr=on}} were reported in addition to severe inundation.<ref name="Pytharoulis2000-262">Pytharoulis et al. 2000, p. 262</ref> The third major Mediterranean tropical cyclone of that year formed north of [[Algeria]] and strengthened while sweeping between the Balearic Islands and Sardinia, with a definitive [[eye (cyclone)|eye]]-like feature prominent on satellite. The eye was distorted and disappeared after transiting over southern Sardinia throughout the evening of 8&nbsp;October, with the system weakening as a whole. On the morning of October&nbsp;9, a smaller eye emerged as the system passed over the [[Tyrrhenian Sea]], gradually strengthening, with reports {{convert|100|km|mi|abbr=on}} from the storm's center reporting winds of {{convert|90|km/h|mph|abbr=on}}. Extreme damage was reported in the [[Aeolian Islands]] after the tropical cyclone passed north of Sicily, though the system dissipated while turning southward over Calabria. Overall, the lowest estimated atmospheric pressure in the third medicane was 998&nbsp;mbar (29.47&nbsp;inHg).<ref name="CavicchiavonStorch-2012-2284">Cavicchia & von Storch 2012, p. 2284</ref> Both October systems featured distinctive spiral bands, intense convection, high sustained winds, and abundant precipitation.<ref name="Pytharoulis2000-262"/>

=== September 2006 ===
[[File:Mediterranean tropical cyclone September 26 2006.jpg|thumb|right|200px|The Mediterranean tropical cyclone of 26 September 2006]]
A short-lived medicane developed near the end of September&nbsp;2006 along the coast of Italy. The origins of the medicane can be traced to the alpine [[Atlas Mountains|Atlas mountain range]] on the evening of 25&nbsp;September,<ref name="CavicchiavonStorch-2012-2282"/> likely forming as a normal lee cyclone.<ref name="Claud2010-2203">Claud et al. 2010, p. 2203</ref> At 0600&nbsp;[[Coordinated Universal Time|UTC]] on 26&nbsp;September, [[European Centre for Medium-Range Weather Forecasts|European Centre for Medium-Range Weather Forecasts (ECMWF)]] model analyses indicated the existence of two [[low-pressure area]]s along the shoreline of Italy, one on the west coast, sweeping eastward across the [[Tyrrhenian Sea]], while the other, slightly more intense, low was located over the [[Ionian Sea]].<ref name="Moscatello2008-4374">Moscatello et al. 2008, p. 4374</ref> As the latter low approached the [[Strait of Sicily]], it met an eastward-moving convection-producing [[cold front]], resulting in significant intensification, while the system simultaneously reduced in size.<ref name="Claud2010-2203"/> It then achieved a minimum [[atmospheric pressure]] of approximately 986&nbsp;[[bar (unit)|mbar]] (29.12&nbsp;[[inch of mercury|inHg]]) after transiting north-northeastward across the {{convert|40|km|mi|abbr=on}}-wide [[Salento|Salentine peninsula]] in the course of roughly 30&nbsp;minutes at 0915&nbsp;UTC the same day.<ref name="Moscatello2008-4374"/>

Wind gusts surpassing {{convert|144|km/h|mph|abbr=on}} were recorded as it passed over Salento due to a steep [[pressure gradient]] associated with it, confirmed by regional [[weather radar|radar observations]] denoting the presence of a clear [[eye (cyclone)|eye]].<ref name="Moscatello2008-4374"/> The high winds inflicted moderate damages throughout the peninsula, though specific damage is unknown.<ref name="CavicchiavonStorch-2012-2282"/> Around 1000&nbsp;UTC,<ref name="Moscatello2008-4374"/> both radar and satellite recorded the system's entry into the [[Adriatic Sea]] and its gradual northwestward curve back toward the Italian coast. By 1700&nbsp;UTC, the cyclone made [[landfall (meteorology)|landfall]] in northern [[Apulia]] while maintaining its intensity, with a minimum atmospheric pressure at 988&nbsp;mbar (29.18&nbsp;inHg). The cyclone weakened and eventually dissipated while drifting further inland over the Italian mainland, eventually dissipating as it curved west-southwestward. A later study in 2008 evaluated that the cyclone possessed numerous characteristics seen in tropical cyclones elsewhere, with a spiral appearance, eye-like apparatus, rapid atmospheric pressure decreases in advance of landfall, and intense sustained winds, concentrated near the storm's eyewall;<ref name="Moscatello2008-4375">Moscatello et al. 2008, p. 4375</ref> the apparent eye-like structure in the cyclone, however, was ill-defined.<ref name="CavicchiavonStorch-2012-2281"/> Since then, the medicane has been the subject of significant study as a result of the availability of scientific observations and reports related to the cyclone.<ref name="Moscatello2008-4374"/>

=== Other storms ===
[[File:Tropical-like cyclone 01-M Rolf.2011312.terra.250m.jpg|thumb|right|200px|Tropical Storm Rolf at peak intensity on 8 November 2011]]
Numerous other Mediterranean cyclones have occurred, but few as better-documented as those in 1969, 1982, 1995, 1996, and 2006. On 27&nbsp;September 1983, a medicane was observed at sea between [[Tunisia]] and [[Sicily]], looping around [[Sardinia]] and [[Corsica]], coming ashore twice on the islands, before making landfall at [[Tunis]] early on 2&nbsp;October and dissipating. The development of the system was not encouraged by [[baroclinity|baroclinic]] instability; rather, convection was incited by abnormally high [[sea surface temperature|sea surface temperatures (SSTs)]] at the time of its formation. It also featured a definitive [[eye (cyclone)|eye]], tall [[cumulonimbus cloud]]s, intense sustained winds, and a warm core. For most of its duration, it maintained a diameter of {{convert|200|to|300|km|mi|abbr=on}}, though it shrank just before landfall on [[Ajaccio]] to a diameter of {{convert|100|km|mi|abbr=on}}. Four other notable cyclones occurred in the late twentieth century, on 26&nbsp;March&nbsp;1983, 29–30&nbsp;December&nbsp;1984, 30–31&nbsp;October&nbsp;1997, and 5–8&nbsp;December&nbsp;1997, all exhibiting characteristics closely resembling tropical cyclones elsewhere.<ref name="Pytharoulis2000-262"/> In November&nbsp;2011, the first officially monitored Mediterranean tropical cyclone by the [[National Oceanic and Atmospheric Administration|National Oceanic and Atmospheric Administration (NOAA)]] formed, designated as 01M by the agency and given the name Rolf by the [[Free University of Berlin]].<ref name="NOAA-bulletins">{{cite web|title=2011 Tropical Bulletin Archive|url=http://www.ssd.noaa.gov/PS/TROP/2011/bulletins/archive.html|work=National Oceanic and Atmospheric Administration|publisher=National Environmental Satellite, Data, and Information Service|accessdate=23 February 2014|date=30 December 2011}}</ref><ref name="FUBerlin">{{cite web|author=Ilmer, P.|title=Lebensgeschichte: Tiefdruckgebiet Rolf|url=http://www.met.fu-berlin.de/wetterpate/Lebensgeschichten/Tief_ROLF_04_11_11.htm|work=Freie Universität Berlin|publisher=Institut für Meteorologie|accessdate=23 February 2014|date=12 August 2011}}</ref>

A study performed in 2013 revealed several additional storms and additional information on medicanes forming on 7&nbsp;April&nbsp;1984, 14&nbsp;December&nbsp;1985, 5&nbsp;December&nbsp;1991, 15&nbsp;January&nbsp;1995, 10&nbsp;December&nbsp;1996, 26&nbsp;January&nbsp;1998, 19&nbsp;March&nbsp;1999, and 27&nbsp;May&nbsp;2003.<ref name="TousRomero2013-4">Tous & Romero 2013, p. 4</ref> A second study, conducted in 2007, revealed additional storms forming on 18&nbsp;October&nbsp;2003, 27&nbsp;October&nbsp;2005, and 15&nbsp;December&nbsp;2005.<ref name="Fita2007-45">Fita et al. 2007, p. 45</ref> A third study revealed several other cyclones, of which developed on 13&nbsp;September&nbsp;1999, 10&nbsp;September&nbsp;2000, 9&nbsp;October&nbsp;2000, 19&nbsp;September&nbsp;2004, 3&nbsp;November 2004, 17&nbsp;and 26&nbsp;October&nbsp;2007, 4&nbsp;December&nbsp;2008, and 13&nbsp;April&nbsp;2012.<ref name="Miglietta2013-2402"/>

== See also ==
*[[Tropical cyclone effects in Europe]]
*[[South Atlantic tropical cyclone]]
*[[Tropical cyclone basins]]
*[[Tropical cyclogenesis]]
{{Portal bar|Tropical cyclones|Global warming|Weather|Disasters}}

== Notes ==

=== Footnotes ===
{{reflist|group="nb"}}

=== Citations ===
{{reflist|3}}

=== References ===
*{{cite journal|author1=Anagnostopoulou, C.|author2=Tolika, K.|author3=Flocas, H.|author4=Maheras, P.|title=Cyclones in the Mediterranean region: present and future climate scenarios derived from a general circulation model (HadAM3P)|journal=Advances in Geosciences|publisher=European Geosciences Union|date=January 2006|volume=7|pages=9&ndash;14|doi=10.5194/adgeo-7-9-2006|url=http://www.adv-geosci.net/7/9/2006/adgeo-7-9-2006.pdf|format=PDF}}
*{{cite journal|author1=Cavicchia, L.|author2=von Storch, H.|title=The simulation of medicanes in a high-resolution regional climate model|journal=Climate Dynamics|publisher=Springer Science+Business Media|doi=10.1007/s00382-011-1220-0|url=http://www.hvonstorch.de/klima/pdf/cavicchia-2011.pdf|format=PDF}}
*{{cite journal|author1=Cavicchia, L.|author2=von Storch, H.|author3=Gualdi, S.|title=A long-term climatology of medicanes|journal=Climate Dynamics|publisher=Springer Science+Business Media|date=August 2013|volume=41|issue=3&ndash;4|pages=2273&ndash;2290|doi=10.1007/s00382-013-1893-7|url=http://www.hvonstorch.de/klima/pdf/medicanes_clim.pdf|format=PDF}}
*{{cite journal|author1=Claud, C.|author2=Alhammoud, B.|author3=Funatsu, B.M.|author4=Chaboureau, J.-P.|title=Mediterranean hurricanes: large-scale environment and convective and precipitating areas from satellite microwave observations|journal=Natural Hazards and Earth System Sciences|publisher=European Geosciences Union|date=October 2010|volume=10|issue=10|pages=2199&ndash;2213|doi=10.5194/nhess-10-2199-2010|url=http://www.nat-hazards-earth-syst-sci.net/10/2199/2010/nhess-10-2199-2010.pdf|format=PDF}}
*{{cite journal|author=Emanuel, K.|title=Genesis and maintenance of 'Mediterranean hurricanes'|journal=Advances in Geosciences|publisher=European Geosciences Union|date=June 2005|volume=2|pages=217&ndash;220|doi=10.5194/adgeo-2-217-2005|url=http://www.adv-geosci.net/2/217/2005/adgeo-2-217-2005.pdf|format=PDF}}
*{{cite journal|author1=Ernst, J.A.|author2=Matson, M.|title=A Mediterranean tropical storm?|journal=Weather|publisher=Royal Meteorological Society|date=November 1983|volume=38|issue=11|pages=332&ndash;337|doi=10.1002/j.1477-8696.1983.tb04818.x}}
*{{cite journal|author1=Fita, L.|author2=Romero, R.|author3=Luque, A.|author4=Emanuel, K.|author5=Ramis, C.|title=Analysis of the environments of seven Mediterranean tropical-like storms using an axisymmetric, nonhydrostatic, cloud resolving model|journal=Natural Hazards and Earth System Sciences|publisher=European Geosciences Union|date=January 2007|volume=7|issue=1|pages=41&ndash;56|doi=10.5194/nhess-7-41-2007|url=http://www.nat-hazards-earth-syst-sci.net/7/41/2007/nhess-7-41-2007.pdf|format=PDF}}
*{{cite journal|author1=Gaertner, M.A.|author2=Jacob, D.|author3=Gil, V.|author4=Domínguez, M.|author5=Padorno, E.|author6=Sánchez, E.|author7=Castro, M.|title=Tropical cyclones over the Mediterranean Sea in climate change simulations|journal=Geophysical Research Letters|publisher=American Geophysical Union|date=July 2007|volume=34|issue=14|pages=L14711|doi=10.1029/2007GL029977}}
*{{cite journal|author1=Homar, V.|author2=Romero, R.|author3=Stensrud, D.J.|author4=Ramis, C.|author5=Alonso, S.|title=Numerical diagnosis of a small, quasi-tropical cyclone over the western Mediterranean: Dynamical vs. boundary factors|journal=Quarterly Journal of the Royal Meteorological Society|publisher=Royal Meteorological Society|date=April 2003|volume=129|issue=590|pages=1469&ndash;1490|doi=10.1256/qj.01.91}}
*{{cite journal|author1=Miglietta, M.M.|author2=Laviola, S.|author3=Malvaldi, A.|author4=Conte, D.|author5=Levizzani, V.|author6=Price, C.|title=Analysis of tropical-like cyclones over the Mediterranean Sea through a combined modeling and satellite approach|journal=Geophysical Research Letters|publisher=American Geophysical Union|date=May 2013|volume=40|issue=10|pages=2400&ndash;2405|doi=10.1002/grl.50432}}
*{{cite journal|author1=Moscatello, A.|author2=Miglietta, M.M.|author3=Rotunno, R.|title=Numerical analysis of a Mediterranean 'hurricane' over southeastern Italy|journal=Monthly Weather Review|publisher=American Meteorological Society|date=November 2008|volume=136|issue=11|pages=4373&ndash;4397|doi=10.1175/2008MWR2512.1|url=http://journals.ametsoc.org/doi/pdf/10.1175/2008MWR2512.1|format=PDF}}
*{{cite journal|author1=Pytharoulis, I.|author2=Craig, G.C.|author3=Ballard, S.P.|title=Study of a hurricane-like Mediterranean cyclone of January 1995|journal=Physics and Chemistry of the Earth|publisher=Elsevier B.V.|date=June 1999|volume=24|issue=6|pages=627&ndash;632|doi=10.1016/S1464-1909(99)00056-8}}
*{{cite journal|author1=Pytharoulis, I.|author2=Craig, G.C.|author3=Ballard, S.P.|title=The hurricane-like Mediterranean cyclone of January 1995|journal=Meteorological Applications|publisher=Royal Meteorological Society|date=September 2000|volume=7|issue=3|pages=261&ndash;279|doi=10.1017/S1350482700001511}}
*{{cite journal|author1=Reed, R.J.|author2=Kuo, Y.-H.|author3=Albright, M.D.|author4=Gao, K.|author5=Guo, Y.-R.|author6=Huang, W.|title=Analysis and modeling of a tropical-like cyclone in the Mediterranean Sea|journal=Meteorology and Atmospheric Physics|publisher=Springer Science+Business Media|date=April 2001|volume=76|issue=3&ndash;4|pages=183&ndash;202|doi=10.1007/s007030170029}}
*{{cite journal|author1=Romero, R.|author2=Emanuel, K.|title=Medicane risk in a changing climate|journal=Journal of Geophysical Research: Atmospheres|publisher=American Geophysical Union|date=June 2013|volume=118|issue=12|pages=5992&ndash;6001|doi=10.1002/jgrd.50475|url=http://www.uib.es/depart/dfs/meteorologia/METEOROLOGIA/ROMU/formal/medicane_risk_synthetic/medicane_risk_synthetic.pdf|format=PDF}}
*{{cite journal|author1=Tous, M.|author2=Romero, R.|title=Meteorological environments associated with medicane development|journal=International Journal of Climatology|publisher=Royal Meteorological Society|date=January 2013|volume=33|issue=1|pages=1&ndash;14|doi=10.1002/joc.3428}}
*{{cite journal|author=Winstanley, D.|title=The North African flood disaster, September 1969|journal=Weather|publisher=Royal Meteorological Society|date=September 1970|volume=25|issue=9|pages=390&ndash;403|doi=10.1002/j.1477-8696.1970.tb04128.x}}

{{DEFAULTSORT:Mediterranean tropical cyclone}}
[[Category:Tropical cyclone meteorology]]
[[Category:Global warming and hurricanes]]
[[Category:Hurricanes in Europe]]

Revision as of 00:02, 24 February 2014

Satellite imagery of a well-documented Mediterranean tropical cyclone at 1004 UTC on 16 January 1995

Mediterranean tropical cyclones, sometimes referred to as Mediterranean hurricanes or medicanes are a rare meteorological phenomenon observed in the Mediterranean Sea. Due to the dry nature of the Mediterranean region, formation of tropical cyclones is infrequent, with only 99 recorded cyclones between 1948 and 2011. Tropical cyclogenesis typically occurs within two separate regions of the sea. The first region, encompassing areas of the western Mediterranean, is more conducive for development than the other, the Ionian Sea to the east. The rough mountainous geography of the region raises additional difficulties despite being favorable for the development of severe weather and convective activity in general, and only with abnormal meteorological circumstances can medicanes form. Numerous studies have been conducted on the impact of global warming on Mediterranean tropical cyclone formation, with generally concluding that although fewer storms would form, those that did would be of a greater intensity.

The development of tropical cyclones in the Mediterranean Sea can usually only occur under somewhat unusual circumstances. Low wind shear and atmospheric instability induced by incursions of cold air are often required. A majority of medicanes are also accompanied by upper-level troughs, providing energy required for intensifying atmospheric convection—thunderstorms—and heavy precipitation. The baroclinic properties of the Mediterranean region, with high temperature gradients, also provides necessary instability for the formation of tropical cyclones. Another factor, rising cool air, provides necessary moisture as well. Warm sea surface temperatures (SSTs) are mostly unnecessary, however, as most medicanes' energy is derived from warmer air temperatures. When these favorable circumstances coincide, the genesis of warm-core Mediterranean tropical cyclones, often from within existing cut-off cold-core lows, is possible in a conducive environment for formation.

Several notable and damaging medicanes are known to have occurred. In September 1969, a north African Mediterranean tropical cyclone produced flooding which killed nearly 600 individuals, left 250,000 homeless, and crippled local economies. A medicane in September 1996 which developed in the Balearic Islands region spawned six tornadoes and inundated parts of the islands. Several medicanes have also been subject to extensive study, such as those of January 1982, January 1995, September 2006, and November 2011. The January 1995 storm is one of the best-studied Mediterranean tropical cyclones, with its close resemblance to tropical cyclones elsewhere and availability of observations. The medicane of September 2006, meanwhile, is well-studied due to availability of existing observations and data. In November 2011, the National Oceanic and Atmospheric Administration officially designated a Mediterranean tropical cyclone for the first time as 01M, also named Tropical Storm Rolf by the Free University of Berlin.

Climatology

Visible satellite imagery of a medicane above the Balearic Islands on 7 October 1996

A majority of Mediterranean tropical cyclones form over two separate regions. The first, more conducive for development than the other, encompasses an area of the western Mediterranean bordered by the Balearic Islands, southern France, and the shorelines of the islands of Corsica and Sardinia. The second identified region of development, in the Ionian Sea between Sicily and Greece and stretching south to Libya, is less favorable for tropical cyclogenesis. An additional two regions, in the Aegean and Adriatic seas, produce fewer medicanes, while activity is minimal in the Levantine region. The geographical distribution of Mediterranean tropical cyclones is markedly different than that of other cyclones, with the formation of regular cyclones centering on the Pyrenees and Atlas mountain ranges, the Gulf of Genoa, and the island of Cyprus in the Ionian Sea.[1] Although meteorological factors are most advantageous in the Adriatic and Aegean seas, the closed nature of the region's geography, bordered by land, allows little time for further evolution.[2]

The geography of mountain ranges bordering the Mediterranean are conducive for severe weather and thunderstorms, with the sloped nature of mountainous regions permitting the development of convective activity.[3] Although the geography of the Mediterranean region, as well as its dry air, typically prevent the formation of tropical cyclones, when certain meteorological circumstances arise, difficulties influenced by the region's geography are overcome.[4] The occurrence of tropical cyclones in the Mediterranean Sea is generally extremely rare, with an average of 1.57 forming annually and merely 99 recorded occurrences discovered between 1948 and 2011 in a modern study, with no definitive trend in activity within that period.[5] Few medicanes form during the summer season, though activity typically rises in autumn, peaks in January, and gradually decreases from February to May.[1] In the western Mediterranean region of development, approximately 0.75 such systems form each year, compared to 0.32 in the Ionian Sea region.[6]

Studies have evaluated that global warming can result in higher observed intensities of tropical cyclones as a result of deviations in the surface energy flux and atmospheric composition, which both heavily influence the development of medicanes as well. In tropical and subtropical areas, sea surface temperatures (SSTs) rose 0.2 °C (32.4 °F) within a 50-year period, and in the North Atlantic and Western Pacific tropical cyclone basins, the potential destructiveness and energy of storms nearly doubled within the same duration, evidencing a clear correlation between global warming and tropical cyclone intensities.[7] Within a similarly recent 20-year period,[8] SSTs in the Mediterranean Sea increased by 0.6 to 1 °C (33.1 to 33.8 °F),[7] though no observable increase in medicane activity has been noted, as of yet.[5] In 2006, a computer-driven atmospheric model evaluated the future frequency of Mediterranean cyclones between 2071 and 2100, projecting a decrease in autumn, winter, and spring cyclonic activity coinciding with a dramatic increase in formation near Cyprus, with both scenarios attributed to elevated temperatures as a result of global warming.[9] Other studies, however, have been inconclusive, forecasting both increases and decreases in duration, number, and intensity.[10] A third study, conducted in 2013, evaluated that while medicane activity would likely decline between 10 and 40 percent by 2100, a higher percentage of those that formed would be of greater strength.[11]

Development and characteristics

A Mediterranean tropical cyclone south of Italy on 27 October 2005

Factors required for the formation of medicanes are somewhat different than that normally expected of tropical cyclones; known to emerge over regions with sea surface temperatures (SSTs) below 26 °C (79 °F), development often requires incursions of colder air inducing atmospheric instability.[1] A majority of medicanes develop above regions of the Mediterranean with temperatures of 15 to 26 °C (59 to 79 °F), with the upper bound only found in the southernmost reaches of the sea. Despite the low sea surface temperatures, the instability incited by cold atmospheric air within a baroclinic zone permits the formation of medicanes, while in tropical areas where high baroclinity is absent, raised SSTs are needed.[12] While significant deviations in air temperature have been noted around the time of Mediterranean tropical cyclones' formation, few anomalies in sea surface temperature coincide with their development, indicating that the development of medicanes is influenced by elevated air temperatures, not by by anomalous SSTs.[13] Similar to tropical cyclones, minimal wind shear as well as abundant moisture and vorticity encourages the genesis of tropical cyclone-like systems in the Mediterranean Sea.[14]

Due to the more confined character of the Mediterranean and the limited capability of heat fluxes, tropical cyclones with a diameter larger than 300 km (190 mi) cannot exist.[15] Despite being a relatively baroclinic area with high temperature gradients, the primary energy source utilized by Mediterranean tropical cyclones is derived from underlying heat sources generated by the presence of convection in a humid environment, similar to tropical cyclones elsewhere, outside the Mediterranean Sea.[16] In comparison to other tropical cyclone basins, the Mediterranean Sea is generally presents a dificult environment for development; although the potential energy necessary for development is not abnormally large, its atmosphere is characterized by its lack of moisture, impeding potential formation. The full development of a medicane often necessitates the formation of a large-scale baroclinic disturbance transitioning late in its life cycle into a tropical cyclone-like system, nearly always under the influence of a deep, cut-off, cold-core low within the middle-to-upper troposphere, frequently resulting from abnormalities in a wide-spreading Rossby wave.[17]

A weak and disorganized Mediterranean tropical cyclone on 28 January 2010

The development of medicanes often results from the vertical shift of air in the troposphere, resulting in a decrease in its temperature coinciding with an increase in relative humidity, creating an environment more conducive for tropical cyclone formation. This in turn leads to in an increase in potential energy, producing heat-induced air-sea instability. Moist air prevents the occurrence of convective downdrafts which often hinder the inception of tropical cyclones,[17] and in such a scenario, wind shear remains minimal; overall, cold-core cut-off lows serve well for the later formation of compact surface flux-influenced warm-core lows such as medicanes. The regular genesis of cold-core upper-level lows and the infrequency of Mediterranean tropical cyclones, however, indicate that additional unusual circumstances are involved the emergence of the latter. Elevated sea surface temperatures, contrasting with cold atmospheric air, encourage atmospheric instability, especially within the troposphere.[12]

In general, most medicanes maintain a radius of 70 to 200 km (43 to 124 mi), last between 12 hours and 5 days, travel between 700 to 3,000 km (430 to 1,860 mi), develop an eye for less than 72 hours, and feature wind speeds approaching 144 km/h (89 mph);[18] in addition, a majority are characterized on satellite imagery by a distinct round eye encircled by atmospheric convection in addition to a mostly axisymmetric cloud pattern.[15] Weak rotation, similar to that in most tropical cyclones, is usually noted in a medicane's early stages, increasing with intensity;[19] medicanes, however, often have less time to intensify, remaining weaker than most North Atlantic hurricanes and only persisting for the duration of a few days.[20] The maximum achievable intensity of medicanes is equivalent to the lowest classification on the Saffir–Simpson hurricane wind scale, Category 1. While the entire lifetime of a cyclone may encompass several days, most will only retain tropical characteristics for less than 24 hours.[21] Circumstances sometimes permit the formation of smaller-scale medicanes, although the required conditions differ even from those needed by other medicanes. The development of abnormally small tropical cyclones in the Mediterranean usually requires upper-level atmospheric cyclones inducing cyclogenesis in the lower atmosphere, leading to the formation of warm-core lows, encouraged by favorable moisture, heat, and other environmental circumstances.[22]

Mediterranean cyclones have been compared to polar lows for their similarly small size and heat-related instability; however, while medicanes nearly always feature warm-core lows, polar lows are primarily cold-cored. The prolonged life of medicanes and similarity to polar lows is caused primarily by origins as synoptic-scale surface lows and heat-related instability.[3] Heavy precipitation and convection within a developing Mediterranean tropical cyclone are usually incited by the approach of an upper-level trough, bringing downstream cold air, encircling an existing low-pressure system. After this occurs, however, a considerable reduction in rainfall rates occurs despite visible organization on satellite imagery,[23] coinciding with a decrease in lightning activity, previously high, as well.[24] Although throughs will often accompany medicanes along their track, separation eventually occurs, usually in the later part of a Mediterranean tropical cyclone's life cycle.[23] At the same time, moist air, saturated and cooled while rising into the atmosphere, then encounters the medicane and permits further development and evolution into a tropical cyclone. Many of these characteristics are also evident in polar lows.[25]

Known occurrences and impacts

September 1969

ESSA-8 visible satellite imagery of the September 1969 cyclone

An unusually severe Mediterranean tropical cyclone developed on 23 September 1969 southeast of Malta, producing severe flooding.[26] Steep pressure and temperature gradients above the Atlas mountain range were evident on 19 September, a result of cool sea air attemtping to penetrate inland; south of the mountains, a lee depression developed. Under the influence of mountainous terrain, the low-pressure area initially meandered northeastward, but following the entry of cool sea air, it recurved to the southeast before transitioning into a Saharan depression associated with a distinct cold front by 22 September. Along the front's path, desert air moved northward while cold air drifted in the opposite direction, and in northern Libya, warm arid air clashed with the cooler levant of the Mediterranean. The organization of the disturbance improved slightly further before emerging into the Mediterranean Sea on 23 September, upon which the system experienced immediate cyclogenesis,[27] rapidly intensifying while southeast of Malta as a cold-core cut-off low,[28] and acquiring tropical characteristics.[26] In western Africa, meanwhile, several disturbances converged toward Mauritania and Algeria, while the medicane recurved southwestward back toward the coast, losing its closed circulation and later dissipating.[28]

The cyclone produced severe flooding throughout regions of northern Africa. Malta received upward of 123 mm (4.8 in) of rainfall on 23 September, Sfax measured 45 mm (1.8 in) on 24 September, Tizi Ouzou collected 55 mm (2.2 in) on 25 September, Gafsa received 79 mm (3.1 in) and Istanbul measured 46 mm (1.8 in) on 26 September, Cap Bengut collected 43 mm (1.7 in) on 27 September, and Biskra received 122 mm (4.8 in) on 28 September.[29] In Malta, a 20000-ton tanker struck a reef and split in two, while in Gafsa, Tunisia, the cyclone flooded phosphate mines, leaving over 25,000 miners unemployed and costing the government over £2 million per week. Thousands of camels and snakes, drowned by flood waters, were swept out to sea, and massive Roman bridges, which withstood all floods since the fall of the Roman Empire, collapsed. In all, the floods in Tunisia and Algeria killed almost 600 individuals, left 250,000 homeless, and severely damaged regional economies.[30] Due to communication problems, however, flood relief funds and television appeals were not set up until nearly a month later.[29]

January 1982

NOAA-7 visible satellite imagery of a Mediterranean tropical storm at 1236 UTC on 26 January 1982

The unusual Mediterranean tropical storm of January 1982 was first detected in waters north of Libya.[26] The storm likely reached the Atlas mountain range as a low-pressure area by 23 January 1982, reinforced by an elongated, slowly-drifting trough above the Iberian Peninsula. Eventually, a closed circulation center developed by 1310 UTC,[31] over parts of the Mediterranean with sea surface temperatures (SSTs) of approximately 12 °C (54 °F).[32] A hook-shaped cloud developed within the system shortly thereafter, rotating as it elongated into a 150 km (93 mi)-long comma-shaped apparatus. After looping around Sicily, it drifted eastward between the island and Peloponnese, recurving on its track again,[33] exhibiting clearly curved spiral banding before shrinking slightly.[34] The cyclone reached its peak intensity at 1800 UTC on the following day, maintaining an atmospheric pressure of 992 mbar (29.30 inHg), and was succeeded by a period of gradual weakening, with the system's pressure eventually rising to 1009 mbar (29.80 inHg). The system slightly reintensified, however, for a six-hour period on 26 January. Ship reports indicated winds of 93 km/h (58 mph) were present in the cyclone at the time, tropical storm-force winds on the Saffir–Simpson hurricane wind scale.[31]

The Global Weather Center's Cyclone Weather Center of the United States Air Force initiated "Mediterranean Cyclone Advisories" on the cyclone at six-hour intervals starting at 1800 UTC on 27 January until 0600 UTC the following day.[35] Although the most intense convection was present in the eastern sector of the cyclone as it drifted east-northeastward, the ship reports containing information on wind speed could have been within the opposite side of the eyewall, which usually features the highest winds in a tropical cyclone. On infrared satellite imagery, the eye itself was 58.5 km (36.4 mi) in diameter,[32] contracting to just 28 kilometres (17 mi) one day prior to making landfall.[35] The cyclone passed by Malta, Italy, and Greece before dissipating several days later in the extreme eastern Mediterranean. Observations related to the cyclone, however, were inadequate, and although the system maintained numerous tropical characteristics, it is possible it was merely a compact but powerful extratropical cyclone exhibiting a clear eye, spiral banding, towering cumulonimbi, and high surface winds along the eyewall.[26]

January 1995

The 1995 medicane at 1015 UTC on 15 January shortly after tropical cyclogenesis

Among numerous documented medicanes, the cyclone of January 1995 is generally considered to be the best-documented instance. Emerging off of the Libyan coast into the central Mediterranean Sea toward the Ionian shoreline of Greece on 13 January as a compact low-pressure area, the precursor low maintained winds reaching up to 108 km/h (67 mph) as it traversed the Ionian Sea,[36] while the German research ship Meteor noted winds of 135 km/h (84 mph).[37] Upon the low's approach near Greece, it began to envelop an area of atmospheric convection; meanwhile, in the middle troposphere, a through extended from Russia to the Mediterranean, bringing with it extremely cold temperatures.[38] Two low-pressure areas were present along the path of the trough, with one situated above Ukraine and the other above the central Mediterranean, likely associated with a low-level cyclone over western Greece, which began to weaken on 14 January, and a second low, the system which would evolve into the Mediterranean tropical cyclone, developed in situ on 15 January.[37]

At the time of formation, high clouds indicated the presence of intense convection,[37] and the cyclone featured an axisymmetric cloud structure, with a distinct, cloud-free eye and rainbands spiraling around the disturbance as a whole.[39] Soon thereafter, the parent low separated from the medicane entirely and continued eastward,[38] meandering toward the Aegean Sea and Turkey.[36] Initially remaining stationary between Greece and Sicily with a minimum atmospheric pressure of 1002 mbar (29.59 inHg), the newly-formed system began to drift southwest-to-south in the following days, influenced by northeasterly flow incited by the initial low, now far to the east, and a high-pressure area above central and eastern Europe.[38] The system's atmospheric pressure increased throughout 15 January due to the fact it was embedded within a large-scale environment, with its rising pressure due to the general prevalence of higher air pressures throughout the region, and was not a sign of deintensification.[39]

Initial wind speeds within the young medicane were generally low, with sustained winds of merely 28 to 46 km/h (17 to 29 mph), with the highest recorded value associated with the disturbance being 63 km/h (39 mph) at 0000 UTC on 16 January, slightly below the threshold for tropical storm on the Saffir–Simpson hurricane wind scale. Its structure now consisted of a distinct eye encircled by counterclockwise-rotating cumulonimbi with cloud top temperatures below −50 °C (−58 °F), evidencing deep convection and a regular feature observed in most tropical cyclones.[40] Intense convection continued to follow the entire path of the system as it traversed the Mediterranean, and the cyclone made landfall in northern Libya at approximately 1800 UTC on 17 January, rapidly weakening after coming ashore.[38] As it moved inland, a minimum atmospheric pressure of 1012 mbar (29.89 inHg) was recorded, accompanied by wind speeds of 93 km/h (58 mph) as it slowed down after passing through the Gulf of Sidra.[41] Although the system retained its strong convection for several more hours, the cyclone's cloud tops began to warm, evidencing lower clouds, before losing tropical characteristics entirely on 17 January.[42] Offshore ship reports recorded that the medicane produced intense winds, copious rainfall, and abnormally warm temperatures.[43]

September and October 1996

The last major Mediterranean tropical cyclone of 1996 while west of Italy on 7 October

Three notable medicanes developed in 1996. The first, in mid-September 1996, was a typical Mediterranean tropical cyclone which developed in the Balearic Islands region, an area conducive to cyclone development.[44] At the time of the cyclone's formation, a powerful Atlantic cold front and a warm front associated with the large-scale low, producing northeasterly winds over the Iberian peninsula, extended eastward into the Mediterranean, while abundant moisture gathered in the lower troposphere over the Balearic channel.[45] On the morning of 12 September, a disturbance developed off the coast of Valencia, Spain, dropping heavy rainfall on the coast. An eye developed shortly thereafter as the system rapidly traversed across Majorca and Sardinia in its eastward trek before making landfall upon the coast of southern Italy on the evening of 13 September with a minimum atmospheric pressure of 990 mbar (29.24 inHg), dissipating shortly after coming ashore,[46] with a diameter of about 150 km (93 mi).[22]

At Valencia and other regions of eastern Spain, the storm generated heavy precipitation, while six tornadoes touched down over the Balearic Islands. While approaching the coast, the warm-core low induced a pressure drop of 11 mbar (0.32 inHg) at Palma, Majorca in advance of the tropical cyclone's landfall. Medicanes as small as the one that formed in September 1996 are atypical, and often require circumstances different even from those required for regular Mediterranean tropical cyclone formation.[22] Warm low-level advection caused by a large-scale low over the western Mediterranean,[3] in conjunction with the presence of a mid- to upper-level cut-off cold-core low were the two main factors in the rise of strong convection. In addition, interaction between a northeastward-drifting trough, the medicane, and the large-scale also permitted the formation of tornadoes within thunderstorms generated by the cyclone after making landfall.[47]

The second of the three recorded Mediterranean tropical cyclones in 1996 formed between Sicily and Tunisia on 4 October, making landfall on both Sicily and southern Italy. The medicane generated major flooding in Sicily; meanwhile, in Calabria, wind gusts of up to 108 km/h (67 mph) were reported in addition to severe inundation.[26] The third major Mediterranean tropical cyclone of that year formed north of Algeria and strengthened while sweeping between the Balearic Islands and Sardinia, with a definitive eye-like feature prominent on satellite. The eye was distorted and disappeared after transiting over southern Sardinia throughout the evening of 8 October, with the system weakening as a whole. On the morning of October 9, a smaller eye emerged as the system passed over the Tyrrhenian Sea, gradually strengthening, with reports 100 km (62 mi) from the storm's center reporting winds of 90 km/h (56 mph). Extreme damage was reported in the Aeolian Islands after the tropical cyclone passed north of Sicily, though the system dissipated while turning southward over Calabria. Overall, the lowest estimated atmospheric pressure in the third medicane was 998 mbar (29.47 inHg).[48] Both October systems featured distinctive spiral bands, intense convection, high sustained winds, and abundant precipitation.[26]

September 2006

The Mediterranean tropical cyclone of 26 September 2006

A short-lived medicane developed near the end of September 2006 along the coast of Italy. The origins of the medicane can be traced to the alpine Atlas mountain range on the evening of 25 September,[44] likely forming as a normal lee cyclone.[49] At 0600 UTC on 26 September, European Centre for Medium-Range Weather Forecasts (ECMWF) model analyses indicated the existence of two low-pressure areas along the shoreline of Italy, one on the west coast, sweeping eastward across the Tyrrhenian Sea, while the other, slightly more intense, low was located over the Ionian Sea.[50] As the latter low approached the Strait of Sicily, it met an eastward-moving convection-producing cold front, resulting in significant intensification, while the system simultaneously reduced in size.[49] It then achieved a minimum atmospheric pressure of approximately 986 mbar (29.12 inHg) after transiting north-northeastward across the 40 km (25 mi)-wide Salentine peninsula in the course of roughly 30 minutes at 0915 UTC the same day.[50]

Wind gusts surpassing 144 km/h (89 mph) were recorded as it passed over Salento due to a steep pressure gradient associated with it, confirmed by regional radar observations denoting the presence of a clear eye.[50] The high winds inflicted moderate damages throughout the peninsula, though specific damage is unknown.[44] Around 1000 UTC,[50] both radar and satellite recorded the system's entry into the Adriatic Sea and its gradual northwestward curve back toward the Italian coast. By 1700 UTC, the cyclone made landfall in northern Apulia while maintaining its intensity, with a minimum atmospheric pressure at 988 mbar (29.18 inHg). The cyclone weakened and eventually dissipated while drifting further inland over the Italian mainland, eventually dissipating as it curved west-southwestward. A later study in 2008 evaluated that the cyclone possessed numerous characteristics seen in tropical cyclones elsewhere, with a spiral appearance, eye-like apparatus, rapid atmospheric pressure decreases in advance of landfall, and intense sustained winds, concentrated near the storm's eyewall;[51] the apparent eye-like structure in the cyclone, however, was ill-defined.[43] Since then, the medicane has been the subject of significant study as a result of the availability of scientific observations and reports related to the cyclone.[50]

Other storms

Tropical Storm Rolf at peak intensity on 8 November 2011

Numerous other Mediterranean cyclones have occurred, but few as better-documented as those in 1969, 1982, 1995, 1996, and 2006. On 27 September 1983, a medicane was observed at sea between Tunisia and Sicily, looping around Sardinia and Corsica, coming ashore twice on the islands, before making landfall at Tunis early on 2 October and dissipating. The development of the system was not encouraged by baroclinic instability; rather, convection was incited by abnormally high sea surface temperatures (SSTs) at the time of its formation. It also featured a definitive eye, tall cumulonimbus clouds, intense sustained winds, and a warm core. For most of its duration, it maintained a diameter of 200 to 300 km (120 to 190 mi), though it shrank just before landfall on Ajaccio to a diameter of 100 km (62 mi). Four other notable cyclones occurred in the late twentieth century, on 26 March 1983, 29–30 December 1984, 30–31 October 1997, and 5–8 December 1997, all exhibiting characteristics closely resembling tropical cyclones elsewhere.[26] In November 2011, the first officially monitored Mediterranean tropical cyclone by the National Oceanic and Atmospheric Administration (NOAA) formed, designated as 01M by the agency and given the name Rolf by the Free University of Berlin.[52][53]

A study performed in 2013 revealed several additional storms and additional information on medicanes forming on 7 April 1984, 14 December 1985, 5 December 1991, 15 January 1995, 10 December 1996, 26 January 1998, 19 March 1999, and 27 May 2003.[54] A second study, conducted in 2007, revealed additional storms forming on 18 October 2003, 27 October 2005, and 15 December 2005.[55] A third study revealed several other cyclones, of which developed on 13 September 1999, 10 September 2000, 9 October 2000, 19 September 2004, 3 November 2004, 17 and 26 October 2007, 4 December 2008, and 13 April 2012.[21]

See also

Notes

Footnotes

Citations

  1. ^ a b c Cavicchia et al. 2013, p. 7
  2. ^ Cavicchia et al. 2013, p. 18
  3. ^ a b c Homar et al. 2003, p. 1470
  4. ^ Emanuel 2005, p. 220
  5. ^ a b Cavicchia et al. 2013, p. 6
  6. ^ Cavicchia et al. 2013, p. 8
  7. ^ a b Tous & Romero 2013, p. 9
  8. ^ Tous & Romero 2013, p. 10
  9. ^ Anagnostopoulou et al. 2006, p. 13
  10. ^ Gaertner et al. 2007, p. 4
  11. ^ Romero & Emanuel 2013, p. 6000
  12. ^ a b Tous & Romero 2013, p. 8
  13. ^ Cavicchia et al. 2013, p. 14
  14. ^ Cavicchia et al. 2013, p. 15
  15. ^ a b Tous & Romero 2013, p. 3
  16. ^ Tous & Romero 2013, p. 5
  17. ^ a b Tous & Romero 2013, p. 6
  18. ^ Cavicchia & von Storch 2012, p. 2276
  19. ^ Fita et al. 2007, p. 43
  20. ^ Fita et al. 2007, p. 53
  21. ^ a b Miglietta et al. 2013, p. 2402
  22. ^ a b c Homar et al. 2003, p. 1469
  23. ^ a b Claud et al. 2010, p. 2211
  24. ^ Miglietta et al. 2013, p. 2404
  25. ^ Emanuel 2005, p. 217
  26. ^ a b c d e f g Pytharoulis et al. 2000, p. 262
  27. ^ Winstanley 1970, p. 393
  28. ^ a b Winstanley 1970, p. 396
  29. ^ a b Winstanley 1970, p. 392
  30. ^ Winstanley 1970, p. 390
  31. ^ a b Ernst & Matson 1983, p. 333
  32. ^ a b Ernst & Matson 1983, p. 334
  33. ^ Reed et al. 2001, p. 187
  34. ^ Reed et al. 2001, p. 189
  35. ^ a b Ernst & Matson 1983, p. 337
  36. ^ a b Cavicchia & von Storch 2012, p. 2280
  37. ^ a b c Pytharoulis et al. 2000, p. 263
  38. ^ a b c d Pytharoulis et al. 1999, p. 628
  39. ^ a b Pytharoulis et al. 2000, p. 264
  40. ^ Pytharoulis et al. 2000, p. 265
  41. ^ Pytharoulis et al. 2000, p. 266
  42. ^ Pytharoulis et al. 2000, p. 267
  43. ^ a b Cavicchia & von Storch 2012, p. 2281
  44. ^ a b c Cavicchia & von Storch 2012, p. 2282
  45. ^ Homar et al. 2003, p. 1473
  46. ^ Cavicchia & von Storch 2012, p. 2283
  47. ^ Homar et al. 2003, p. 1471
  48. ^ Cavicchia & von Storch 2012, p. 2284
  49. ^ a b Claud et al. 2010, p. 2203
  50. ^ a b c d e Moscatello et al. 2008, p. 4374
  51. ^ Moscatello et al. 2008, p. 4375
  52. ^ "2011 Tropical Bulletin Archive". National Oceanic and Atmospheric Administration. National Environmental Satellite, Data, and Information Service. 30 December 2011. Retrieved 23 February 2014.
  53. ^ Ilmer, P. (12 August 2011). "Lebensgeschichte: Tiefdruckgebiet Rolf". Freie Universität Berlin. Institut für Meteorologie. Retrieved 23 February 2014.
  54. ^ Tous & Romero 2013, p. 4
  55. ^ Fita et al. 2007, p. 45

References