Isotope modeling of nitric acid formation in the atmosphere using ISO-RACM: testing the importance of NO oxidation, heterogeneous reactions, and trace gas chemistry
Item
Title (Dublin Core)
Isotope modeling of nitric acid formation in the atmosphere using ISO-RACM: testing the importance of NO oxidation, heterogeneous reactions, and trace gas chemistry
Description (Dublin Core)
Here we present ISO-RACM, an isotope mass balance model that utilizes the Regional Atmospheric Chemistry Mechanism to predict Δ<sup>17</sup>O values in atmospheric nitrate. A large number of simulations were carried out that varied atmospheric parameters that are important in altering the magnitude and range of Δ<sup>17</sup>O values generated in photochemically produce nitrate. These parameters included temperature, relative humidity, actinic flux, aerosol surface area and chemical speciation, and three different N<sub>2</sub>O<sub>5</sub> uptake parameterizations. Trace gas mixing ratios were also varied including CH<sub>4</sub>, CO, NO<sub>x</sub>, O<sub>3</sub>, volatile organic compounds and biogenic organic compounds. The model predicts that there are seasonal, latitudinal and diurnal variations in Δ<sup>17</sup>O values due to changes in actinic flux with lower values corresponding to higher actinic fluxes. There was also a minor positive correlation between higher Δ<sup>17</sup>O values and increased temperature. There were distinct differences in Δ<sup>17</sup>O depending on which N<sub>2</sub>O<sub>5</sub> parameterization was used, mostly the result of changing relative humidity being a factor in two of the parameterization schemes. Changing CO and CH<sub>4</sub> mixing ratios had negligible impact on Δ<sup>17</sup>O values but significant variation in magnitude and range were predicted with NO<sub>x</sub>, O<sub>3</sub>, and organic loading. High NO<sub>x</sub> and O<sub>3</sub> generated high Δ<sup>17</sup>O with a narrow (10 ‰) range, while high organics led to low Δ<sup>17</sup>O values and a wider range of possible values. Implications for using Δ<sup>17</sup>O to evaluate NO<sub>x</sub>-NO<sub>y</sub> chemistry and aerosol formation processes are discussed, as is needed future research.
Creator (Dublin Core)
Michalski, G.
Xu, F.
Date (Dublin Core)
2018-08-10
Type (Dublin Core)
Text
Format (Dublin Core)
application/pdf
Identifier (Dublin Core)
10.5194/acpd-10-6829-2010
https://acp.copernicus.org/preprints/acp-2010-29/
Source (Dublin Core)
eISSN: 1680-7324
Language (Dublin Core)
eng



