templates/en/rst/ozoneloss_uvi.rst
author Jens-Uwe Grooss <j.-u.grooss@fz-juelich.de>
Tue, 11 Mar 2025 20:42:55 +0100
changeset 1705 a0a2b2974acc
parent 1045 622c19af65a3
permissions -rw-r--r--
eskp plot update from 250311
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UV increase due to ozone loss
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=============================
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The chemical depletion of ozone in the stratosphere causes an increase
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of ultraviolet radiation on the ground. The UV index is a measure of
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the danger of the UV radiation.  It corresponds to the
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sunburn-effective solar irradiance.
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This is a sample calculation [#FN1]_, how the UV index typically
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changes at a certain latitude in winter and spring.  Shown are
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noontime values of the UV index at clear sky for the range of the
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observed ozone columns of the years 2000 and 2012 (black) and
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corresponding values for a given decrease the ozone column (blue). The
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selection of the two values for geographical latitude and ozone loss
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can be altered.  The anthropogenically induced polar ozone depletion
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takes place within the polar vortex, which in winter and spring is
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well separated from the mid-latitudes.  After the breakdown of the
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polar vortex (in the Northern hemisphere typically at the latest in
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early April), ozone-rich air from mid-latitudes will be transported
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back into the polar regions.
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In contrast to the Southern hemisphere, there are typically no
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significant increases to very high UV indices in polar high latitudes
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in the Northern hemisphere in the relevant period until April.
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These graphs show how the maximum UV index (at noontime at clear sky)
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would change due to ozone depletion in the Arctic polar vortex.
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.. [#FN1] The mean values and standard deviations of the ozone columns were calculated from the database of Bodeker-Scientific (http://www.bodekerscientific.com).  Calculation of the UV index for cloudless sky according to the method of Allaart et al. (Meteorological Applications, 11, 59-65, 2004)
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