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LONG‐TERM VARIATIONS IN ULTRAVIOLET SUNLIGHT REACHING THE BIOSPHERE: . CALCULATIONS FOR THE PAST THREE DECADES
Author(s) -
Frederick J. E.,
Weatherhead E. C.,
Haywood E. K.
Publication year - 1991
Publication title -
photochemistry and photobiology
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 0.818
H-Index - 131
eISSN - 1751-1097
pISSN - 0031-8655
DOI - 10.1111/j.1751-1097.1991.tb02090.x
Subject(s) - sunlight , environmental science , latitude , irradiance , atmospheric sciences , northern hemisphere , southern hemisphere , term (time) , ultraviolet radiation , seasonality , solar irradiance , climatology , meteorology , geography , physics , mathematics , chemistry , geology , statistics , astronomy , geodesy , quantum mechanics , radiochemistry
The long‐term data base on atmospheric ozone combined with a set of radiative transfer calculations provides estimates of the variability in ultraviolet (UV) sunlight that should have occurred over the period1957–1988 under clear, pollution‐free skies. Results refer to the earth's surface at specific locations in the Northern Hemisphere and to averages over collections of sites located in three latitude bands from 30 to 64°N. For any one year the annually integrated solar irradiance, weighted by the action spectrum for erythema, typically lies within3–4% of the 32‐year mean. No statistically significant trends span the entire 32‐year time frame. However, over the shorter time period1970–1988 the annually integrated erythemal irradiance shows an upward trend of +2.1 ± 1.2% per decade based on all ozone data at latitudes from 40 to 52°N. No trends exist in lower (30‐39°N) and higher (53‐64°N) latitude bands. We caution that a trend line provides a very simple index of the variability in UV sunlight, and these results should not necessarily be extrapolated into the future.