Aerosol fluxes and particle growth above managed grassland

Particle deposition velocities (11–3000 nm diameter) measured above grassland by eddy covariance during the EU GRAMINAE experiment in June 2000 averaged 0.24 and 0.03 mm s<sup>−1</sup> to long (0.75 m) and short (0.07 m) grass, respectively. After fertilisat...

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Bibliographic Details
Main Authors: E. Nemitz, J. R. Dorsey, M. J. Flynn, M. W. Gallagher, A. Hensen, J.-W. Erisman, S. M. Owen, U. Dämmgen, M. A. Sutton
Format: Article
Language:English
Published: Copernicus Publications 2009-08-01
Series:Biogeosciences
Online Access:http://www.biogeosciences.net/6/1627/2009/bg-6-1627-2009.pdf
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Summary:Particle deposition velocities (11–3000 nm diameter) measured above grassland by eddy covariance during the EU GRAMINAE experiment in June 2000 averaged 0.24 and 0.03 mm s<sup>−1</sup> to long (0.75 m) and short (0.07 m) grass, respectively. After fertilisation with 108 kg N ha<sup>−1</sup> as calcium ammonium nitrate, sustained apparent upward fluxes of particles were observed. Analysis of concentrations and fluxes of potential precursor gases, including NH<sub>3</sub>, HNO<sub>3</sub>, HCl and selected VOCs, shows that condensation of HNO<sub>3</sub> and NH<sub>3</sub> on the surface of existing particles is responsible for this effect. A novel approach is developed to derive particle growth rates at the field scale, from a combination of measurements of vertical fluxes and particle size-distributions. For the first 9 days after fertilization, growth rates of 11 nm particles of 7.04 nm hr<sup>−1</sup> and 1.68 nm hr<sup>−1</sup> were derived for day and night-time conditions, respectively. This implies total NH<sub>4</sub>NO<sub>3</sub> production rates of 1.11 and 0.44 μg m<sup>−3</sup> h<sup>−1</sup>, respectively. The effect translates into a small error in measured ammonia fluxes (0.06% day, 0.56% night) and a large error in NH<sub>4</sub><sup>+</sup> and NO<sub>3</sub><sup>−</sup> aerosol fluxes of 3.6% and 10%, respectively. By converting rapidly exchanged NH<sub>3</sub> and HNO<sub>3</sub> into slowly depositing NH<sub>4</sub>NO<sub>3</sub>, the reaction modifies the total N budget, though this effect is small (<1% for the 10 days following fertilization), as NH<sub>3</sub> emission dominates the net flux. It is estimated that 3.8% of the fertilizer N was volatilised as NH<sub>3</sub>, of which 0.05% re-condensed to form NH<sub>4</sub>NO<sub>3</sub> particles within the lowest 2 m of the surface layer. This surface induced process would at least scale up to a global NH<sub>4</sub>NO<sub>3</sub> formation of ca. 0.21 kt N yr<sup>−1</sup> from NH<sub>4</sub>NO<sub>3</sub> fertilisers and potentially 45 kt N yr<sup>−1</sup> from NH<sub>3</sub> emissions in general.
ISSN:1726-4170
1726-4189