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SOLAR ULTRAVIOLET RADIATION AT THE EARTH'S SURFACE
Author(s) -
Frederick J. E.,
Snell H. E.,
Haywood E. K.
Publication year - 1989
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.1751-1097.1989.tb05548.x
Subject(s) - irradiance , atmospheric sciences , ozone depletion , environmental science , radiation , ozone , northern hemisphere , ultraviolet radiation , ozone layer , solar irradiance , ultraviolet , tropospheric ozone , troposphere , meteorology , chemistry , stratosphere , physics , optics , radiochemistry
The biologically effective ultraviolet irradiance at the earth's surface varies with the elevation of the sun, the atmospheric ozone amount, and with the abundance of scatterers and absorbers of natural and anthropogenic origin. Taken alone, the reported decrease in column ozone over the Northern Hemisphere between 1969 and 1986 implies an increase in erythemal irradiance at the ground of four percent or less during summer. However, an increase in tropospheric absorption, arising from polluting gases or particulates over localized areas, could more than offset the predicted enhancement in radiation. Any such extra absorption is likely to be highly regional in nature and does not imply that a decrease in erythemal radiation has occurred on a global basis. The Antarctic ‘ozone hole’ represents a special case in which a portion of the earth has experienced ultraviolet radiation levels during spring that are far in excess of those which prevailed prior to the present decade.