On the origin of the occasional springtime nitrate concentration maximum in Greenland snow
Author:
Geng L., Cole-Dai J., Alexander B.ORCID, Erbland J., Savarino J.ORCID, Schauer A. J., Steig E. J.ORCID, Lin P., Fu Q., Zatko M. C.
Abstract
Abstract. An occasional spring nitrate concentration maximum was observed in ice cores from Central Greenland but its origin is unknown. This study performs a case study on its origin by measuring concentration and isotopic composition of nitrate (δ15N, δ18O and Δ17O) in a snowpit from Summit, Greenland covering three years of snow accumulation. A nitrate concentration maximum was found in the spring of 2005. Isotopic data of nitrate combined with photochemical calculations suggest that the presence of this spring maximum was linked to a significantly weakened stratospheric ozone (O3) layer. This weakened O3 layer resulted in elevated UV-B (Ultraviolet B) radiation on the snow surface, where the productions of OH and NOx from the photolysis of their precursors were enhanced. A concentration maximum was then observed as the result of enhanced local nitrate production due primarily to the increased OH concentrations, as indicated by decreases in δ18O and Δ17O of nitrate associated with the spring maximum. We further examined the nitrate concentration record from a shallow ice core covering the period from 1772 to 2006 and compared this record to satellite observations of springtime O3 column density data from 1979 to 2006. We found 19 spring nitrate maxima after the 1950s. After 1979, all spring concentration maxima appeared with O3 column density near or below the 1979–2006 average. We hypothesize that the presence of the spring nitrate concentration maximum is largely associated with and may be determined by the interannual variability of O3 column density, under the condition of elevated local NOx abundance at Summit after the 1950s resulting from enhanced anthropogenic nitrate deposition, though other factor(s) may dominate in some years. Isotopic data covering additional years of low O3 column density are needed to further examine this hypothesis.
Publisher
Copernicus GmbH
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