The polar vortex is a persistent, large-scale cyclone located near the
Earth's poles, in the middle and upper troposphere and the
stratosphere. It surrounds the polar highs and is part
of the polar front. The vortex is most powerful in the
hemisphere's winter, when the temperature gradient is steepest, and diminishes or can disappear in the summer. 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 Arctic vortex is elongated in shape, with
two centres, one roughly over Baffin Island in Canada and
the other over northeast Siberia.
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. Chlorine concentrations build up during the winter polar
night, and the consequent ozone destruction is greatest when the sunlight returns in spring (September/October). These clouds can
only form at temperatures below about -80°C, so the warmer Arctic region does not have an ozone
hole.
The Antarctic Polar Vortex typically lasts from August to November
Other astronomical bodies are also known to have polar vortices, including Venus,
Mars, Jupiter, Saturn and Saturn's moon Titan.
References
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