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                  <gco:CharacterString>The importance of considering depth-resolved photochemistry in snow: A radiative-transfer study of NOâ and OH production in Ny-Ãlesund (Svalbard) snowpacks</gco:CharacterString>
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            <gco:CharacterString>Solar visible radiation can penetrate 2-30 cm (e-folding depth) into snowpacks and photolyse nitrate anions and hydrogen peroxide contained in the snow. Photolysis rate coefficients, J, for NOââ» and HâOâ photolysis are presented for a melting and a fresh snowpack at Ny-Ãlesund, Svalbard. Calculations of (a) transfer velocities, áµ¥, and molecular fluxes of gaseous NOâ from the snowpack and (b) depth-integrated production rates of OH radicals within the snowpack are presented. The results show the importance of considering the depth dependence, i.e. not just the snow surface, when modelling snowpack photochemistry. Neglecting photochemistry under the snow surface can result in an apparent larger molecular flux of NOâ from NOââ» photolysis than the melting snowpack. However, when the depth-resolved molecular fluxes of NOâ within the snowpack are calculated, a larger NOâ flux may be apparent in the melting snowpack than the fresh snowpack. For solar zenith angles of 60Â°, 70Â° and 80Â° the modelled molecular fluxes of NOâ from fresh snowpack are 11.6, 5.6 and 1.7 nmol mâ»Â²hâ»Â¹, respectively, and those for melting snowpack are 19.7, 9.1 and 2.9 nmol mâ»Â²hâ»Â¹, respectively.</gco:CharacterString>
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