File:Polarvortexjan211985.jpg
Polar vortex over Maine on the morning of January 21, 1985

A polar vortex (also known as Polar cyclones, polar vortices, Arctic cyclones, sub-polar cyclones, and the circumpolar whirl) is a persistent, large-scale cyclone located near one or both of a planet's geographical poles. On Earth, the polar vortices are located in the middle and upper troposphere and the stratosphere. They surround the polar highs and lie in the wake of the polar front. These cold-core low-pressure areas strengthen in the winter and weaken in the summer.[1] They usually span 1,000–2,000 kilometers (620–1,240 miles) in which the air is circulating in a counter-clockwise fashion (in the northern hemisphere). The reason for the rotation is the same as any other cyclone, the Coriolis effect.

One center lies near Baffin Island and the other over northeast Siberia.[2] In the southern hemisphere, it tends to be located near the edge of the Ross ice shelf near 160 west longitude.[3] When the polar vortex is strong, the Westerlies increase in strength. When the polar cyclone is weak, the general flow pattern across mid-latitudes buckles and significant cold outbreaks occur.[4] Ozone depletion occurs within the polar vortex, particularly over the Southern Hemisphere, which reaches a maximum in the spring.

Duration and power

File:Polarvortexwinter.jpg
Polar vortex and weather impacts due to stratospheric warming

Polar cyclones are climatological features which hover near the poles year-round. They are weaker during summer and strongest during winter. When the polar vortex is strong, the Westerlies increase in strength. When the polar cyclone is weak, the general flow pattern across mid-latitudes buckles and significant cold outbreaks occur. Extratropical cyclones which occlude and migrate into higher latitudes create cold-core lows within the polar vortex.[5] Volcanic eruptions in the tropics lead to a stronger polar vortex during the winter for as long as two years afterwards.[6] The strength and position of the cyclone shapes the flow pattern across the hemisphere of its influence. An index which is used in the northern hemisphere to gage its magnitude is the Arctic oscillation.[7]

The Antarctic polar vortex is more pronounced and persistent than the Arctic one; this is because the distribution of land masses at high latitudes in the northern hemisphere gives rise to Rossby waves which contribute to the breakdown of the vortex, whereas in the southern hemisphere the vortex remains less disturbed. The breakdown of the polar vortex is an extreme event known as a sudden stratospheric warming, here the vortex completely breaks down and an associated warming of 30-50 degrees Celsius over a few days can occur. The Arctic vortex is elongated in shape, with two centres, one normally located over Baffin Island in Canada and the other over northeast Siberia. In rare events, when the general flow pattern is amplified (or meridional), the vortex can push further south as a result of axis interruption, such as during the Winter 1985 Arctic outbreak.[8]

Ozone depletion

File:Srnhemozoneconcentration.gif
Southern Hemisphere Ozone Concentration, February 22, 2012

The chemistry of the Antarctic polar vortex has created severe ozone depletion. The nitric acid in polar stratospheric clouds reacts with CFCs to form chlorine, which catalyzes the photochemical destruction of ozone.[9] Chlorine concentrations build up during the polar winter, and the consequent ozone destruction is greatest when the sunlight returns in spring.[10] These clouds can only form at temperatures below about -80°C. Since there is greater air exchange between the Arctic and the mid-latitudes, ozone depletion at the north pole is much less severe than at the south.[11] Accordingly, the seasonal reduction of ozone levels over the Arctic is usually characterized as an "ozone dent," whereas the more severe ozone depletion over the Antarctic is considered an "ozone hole." This said, chemical ozone destruction in the 2011 Arctic polar vortex attained, for the first time, a level clearly identifiable as an Arctic "ozone hole".

Ongoing studies

The Australian and US Federal Governments recently awarded funding for a study into how the polar vortex might influence drought in Australia. Scientists hope that the study will glean valuable insight into why droughts in Southern Australia are getting worse, and whether or not there is a direct link between polar climate activity, and weather patterns elsewhere. "One of the big problems we have in planning for drought has to do with understanding whether the drought that we are in right now is a climate-change signal or part of a natural cycle. If we want to understand that we need to understand where the rain is coming from." [12]

See also

Template:Cyclones

Outside earth

File:Mars cyclone.jpg
Hubble view of the colossal polar cloud on Mars

Other astronomical bodies are also known to have polar vortices, including Venus (double vortex - that is, two polar vortices at a pole ), Mars,[13] Jupiter, Saturn and Saturn's moon Titan.

References

  1. Halldór Björnsson. Global circulation. Veðurstofa Íslands. Retrieved on 2008-06-15.
  2. Glossary of Meteorology (June 2000). Polar vortex. American Meteorological Society. Retrieved on 15 June 2008.
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  4. James E. Kloeppel (2001-12-01). Stratosheric polar vortex influences winter cold, researchers say. National Aeronautics and Space Administration. Retrieved on 2008-06-15.
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  7. Todd Mitchell (2004). Arctic Oscillation (AO) time series, 1899 - June 2002. University of Washington. Retrieved on 2009-03-02.
  8. Kevin Myatt (2005-01-17). Cold enough for snow, and more's on the way. Roanoke Times. Retrieved on 2012-02-24.
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  12. Monash University (2007-01-05). "Australian survey into what effects polar cyclones have on drought in Australia". Experts Online. http://www.expertguide.com.au/news/article.aspx?ID=572. Retrieved 2008-05-13.
  13. European Space Agency (2006-06-27). Double vortex at Venus South Pole unveiled! European Space Agency. Retrieved on 2012-02-24

External links

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