Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models

<p>A fast-response (10 Hz) chemiluminescence detector for ozone (O<span class="inline-formula"><sub>3</sub></span>) was used to determine O<span class="inline-formula"><sub>3</sub></span> fluxes using the eddy covariance techn...

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Main Authors: D. C. Loades, M. Yang, T. G. Bell, A. R. Vaughan, R. J. Pound, S. Metzger, J. D. Lee, L. J. Carpenter
Format: Article
Language:English
Published: Copernicus Publications 2020-12-01
Series:Atmospheric Measurement Techniques
Online Access:https://amt.copernicus.org/articles/13/6915/2020/amt-13-6915-2020.pdf
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author D. C. Loades
M. Yang
T. G. Bell
A. R. Vaughan
R. J. Pound
S. Metzger
S. Metzger
J. D. Lee
J. D. Lee
L. J. Carpenter
spellingShingle D. C. Loades
M. Yang
T. G. Bell
A. R. Vaughan
R. J. Pound
S. Metzger
S. Metzger
J. D. Lee
J. D. Lee
L. J. Carpenter
Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
Atmospheric Measurement Techniques
author_facet D. C. Loades
M. Yang
T. G. Bell
A. R. Vaughan
R. J. Pound
S. Metzger
S. Metzger
J. D. Lee
J. D. Lee
L. J. Carpenter
author_sort D. C. Loades
title Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
title_short Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
title_full Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
title_fullStr Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
title_full_unstemmed Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
title_sort ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange models
publisher Copernicus Publications
series Atmospheric Measurement Techniques
issn 1867-1381
1867-8548
publishDate 2020-12-01
description <p>A fast-response (10 Hz) chemiluminescence detector for ozone (O<span class="inline-formula"><sub>3</sub></span>) was used to determine O<span class="inline-formula"><sub>3</sub></span> fluxes using the eddy covariance technique at the Penlee Point Atmospheric Observatory (PPAO) on the south coast of the UK during April and May 2018. The median O<span class="inline-formula"><sub>3</sub></span> flux was <span class="inline-formula">−</span>0.132 mg m<span class="inline-formula"><sup>−2</sup></span> h<span class="inline-formula"><sup>−1</sup></span> (0.018 ppbv m s<span class="inline-formula"><sup>−1</sup></span>), corresponding to a deposition velocity of 0.037 cm s<span class="inline-formula"><sup>−1</sup></span> (interquartile range 0.017–0.065 cm s<span class="inline-formula"><sup>−1</sup></span>) – similar to the higher values previously reported for open-ocean flux measurements but not as high as some other coastal results. We demonstrate that a typical single flux observation was above the 2<span class="inline-formula"><i>σ</i></span> limit of detection but had considerable uncertainty. The median 2<span class="inline-formula"><i>σ</i></span> uncertainty of deposition velocity was 0.031 cm s<span class="inline-formula"><sup>−1</sup></span> for each 20 min period, which reduces with the square root of the sample size. Eddy covariance footprint analysis of the site indicates that the flux footprint was predominantly over water (<span class="inline-formula">&gt;</span> 96 %), varying with atmospheric stability and, to a lesser extent, with the tide. At very low wind speeds when the atmosphere was typically unstable, the observed ozone deposition velocity was elevated, most likely because the footprint contracted to include a greater land contribution in these conditions. At moderate to high wind speeds when atmospheric stability was near-neutral, the ozone deposition velocity increased with wind speed and showed a linear dependence with friction velocity. This observed dependence on friction velocity (and therefore also wind speed) is consistent with the predictions from the one-layer model of Fairall et al. (2007), which parameterises the oceanic deposition of ozone from the fundamental conservation equation, accounting for both ocean turbulence and near-surface chemical destruction, while assuming that chemical O<span class="inline-formula"><sub>3</sub></span> destruction by iodide is distributed over depth. In contrast to our observations, the deposition velocity predicted by the recently developed two-layer model of Luhar et al. (2018) (which considers iodide reactivity in both layers but with molecular diffusivity dominating over turbulent diffusivity in the first layer) shows no major dependence of deposition velocity on wind speed and underestimates the measured deposition velocities. These results call for further investigation into the mechanisms and control of oceanic O<span class="inline-formula"><sub>3</sub></span> deposition.</p>
url https://amt.copernicus.org/articles/13/6915/2020/amt-13-6915-2020.pdf
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spelling doaj-5004798d40494e80ae6d3af1abe1d0442020-12-18T14:22:14ZengCopernicus PublicationsAtmospheric Measurement Techniques1867-13811867-85482020-12-01136915693110.5194/amt-13-6915-2020Ozone deposition to a coastal sea: comparison of eddy covariance observations with reactive air–sea exchange modelsD. C. Loades0M. Yang1T. G. Bell2A. R. Vaughan3R. J. Pound4S. Metzger5S. Metzger6J. D. Lee7J. D. Lee8L. J. Carpenter9Wolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, University Road, York, YO10 5DD, UKPlymouth Marine Laboratory, Prospect Place, Plymouth, PL1 3DH, UKPlymouth Marine Laboratory, Prospect Place, Plymouth, PL1 3DH, UKWolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, University Road, York, YO10 5DD, UKWolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, University Road, York, YO10 5DD, UKNational Ecological Observatory Network Program, Battelle, 1685 38th Street, Boulder, CO 80301, USADepartment of Atmospheric and Oceanic Sciences, University of Wisconsin-Madison, 1225 West Dayton Street, Madison, WI 53706, USAWolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, University Road, York, YO10 5DD, UKNational Centre for Atmospheric Science, University of York, University Road, York, YO10 5DD, UKWolfson Atmospheric Chemistry Laboratories, Department of Chemistry, University of York, University Road, York, YO10 5DD, UK<p>A fast-response (10 Hz) chemiluminescence detector for ozone (O<span class="inline-formula"><sub>3</sub></span>) was used to determine O<span class="inline-formula"><sub>3</sub></span> fluxes using the eddy covariance technique at the Penlee Point Atmospheric Observatory (PPAO) on the south coast of the UK during April and May 2018. The median O<span class="inline-formula"><sub>3</sub></span> flux was <span class="inline-formula">−</span>0.132 mg m<span class="inline-formula"><sup>−2</sup></span> h<span class="inline-formula"><sup>−1</sup></span> (0.018 ppbv m s<span class="inline-formula"><sup>−1</sup></span>), corresponding to a deposition velocity of 0.037 cm s<span class="inline-formula"><sup>−1</sup></span> (interquartile range 0.017–0.065 cm s<span class="inline-formula"><sup>−1</sup></span>) – similar to the higher values previously reported for open-ocean flux measurements but not as high as some other coastal results. We demonstrate that a typical single flux observation was above the 2<span class="inline-formula"><i>σ</i></span> limit of detection but had considerable uncertainty. The median 2<span class="inline-formula"><i>σ</i></span> uncertainty of deposition velocity was 0.031 cm s<span class="inline-formula"><sup>−1</sup></span> for each 20 min period, which reduces with the square root of the sample size. Eddy covariance footprint analysis of the site indicates that the flux footprint was predominantly over water (<span class="inline-formula">&gt;</span> 96 %), varying with atmospheric stability and, to a lesser extent, with the tide. At very low wind speeds when the atmosphere was typically unstable, the observed ozone deposition velocity was elevated, most likely because the footprint contracted to include a greater land contribution in these conditions. At moderate to high wind speeds when atmospheric stability was near-neutral, the ozone deposition velocity increased with wind speed and showed a linear dependence with friction velocity. This observed dependence on friction velocity (and therefore also wind speed) is consistent with the predictions from the one-layer model of Fairall et al. (2007), which parameterises the oceanic deposition of ozone from the fundamental conservation equation, accounting for both ocean turbulence and near-surface chemical destruction, while assuming that chemical O<span class="inline-formula"><sub>3</sub></span> destruction by iodide is distributed over depth. In contrast to our observations, the deposition velocity predicted by the recently developed two-layer model of Luhar et al. (2018) (which considers iodide reactivity in both layers but with molecular diffusivity dominating over turbulent diffusivity in the first layer) shows no major dependence of deposition velocity on wind speed and underestimates the measured deposition velocities. These results call for further investigation into the mechanisms and control of oceanic O<span class="inline-formula"><sub>3</sub></span> deposition.</p>https://amt.copernicus.org/articles/13/6915/2020/amt-13-6915-2020.pdf