Abstract

<strong class="journal-contentHeaderColor">Abstract.</strong> The oxygen (𝛥<sup>17</sup>O) and nitrogen (𝛿<sup>15</sup>N) isotopic compositions of atmospheric nitrate (NO<sub>3</sub>-) are widely used as tracers of its formation pathways, precursor (nitrogen oxides NO<sub>x</sub> = nitric oxide NO + nitrogen NO<sub>2</sub>) emission sources, and physico-chemical processing. However, the critical lack of observations on the multi-isotopic composition of NO<sub>2</sub> maintains significant uncertainties regarding the links between the isotopic composition of NO<sub>x</sub> and NO<sub>3</sub>-, which may bias estimates of the NO<sub>3</sub>- formation processes and the distribution of sources. We report here on the first simultaneous atmospheric observations of 𝛥<sup>17</sup>O and 𝛿<sup>15</sup>N in NO<sub>2</sub> and NO<sub>3</sub>-. The measurements were carried out at sub-daily (ca. 3 h) resolution over two non-consecutive days in an Alpine city in February 2021. Important diurnal variabilities are observed in both NO<sub>2</sub> and NO<sub>3</sub>- multi-isotopic composition. 𝛥<sup>17</sup>O of NO<sub>2</sub> and NO<sub>3</sub>- range from 19.6 to 40.8 &permil; and 18.7 to 26 &permil;, respectively. During both daytime and nighttime, the variability of 𝛥<sup>17</sup>O(NO<sub>2</sub>) is mainly driven by the oxidation of NO by ozone, with a substantial contribution from peroxy radicals in the morning. NO<sub>3</sub>- local mass balance equations, constrained by observed 𝛥<sup>17</sup>O(NO<sub>2</sub>), suggest that during the first day of sampling NO<sub>3</sub>- was formed locally from the oxidation of NO<sub>2</sub> by hydroxyl radicals during the day, and via heterogeneous hydrolysis of dinitrogen pentoxide during the night. For the second day, calculated and observed 𝛥<sup>17</sup>O(NO<sub>3</sub>-) do not match, particularly daytime values. The effects on 𝛥<sup>17</sup>O(NO<sub>3</sub>-) of a Saharan dust event that occurred during the second day and winter boundary layer dynamics are discussed. 𝛿<sup>15</sup>N of NO<sub>2</sub> and NO<sub>3</sub>- ranged from -10.0 to 19.7 &permil; and -4.2 to 14.8 &permil;, respectively. Consistent with theoretical predictions of N isotope fractionation, the important variability of 𝛿<sup>15</sup>N(NO<sub>2</sub>) is explained by significant post-emission equilibrium N fractionation. After accounting for this effect, vehicle exhaust is found to be the primary source of NO<sub>x</sub> emissions at the sampling site. 𝛿<sup>15</sup>N(NO<sub>3</sub>-) is closely linked to 𝛿<sup>15</sup>N(NO<sub>2</sub>) variability, which bring further evidence of fast and local processing, but uncertainties on current N fractionation factors during NO<sub>2</sub> to NO<sub>3</sub>- conversion are underscored. Overall, this detailed investigation highlights the potential and the necessity to use 𝛥<sup>17</sup>O and 𝛿<sup>15</sup>N in NO<sub>2</sub> and NO<sub>3</sub>- to trace quantitatively the sources and formation chemistry of NO<sub>3</sub>-, particularly in urban environments in winter.

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