Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue

Halocarbons from oceanic sources contribute to halogens in the troposphere, and can be transported into the stratosphere where they take part in ozone depletion. This paper presents distribution and sources in the equatorial Atlantic from June and July 2011 of the four compounds bromoform (CHBr<s...

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Main Authors: H. Hepach, B. Quack, S. Raimund, T. Fischer, E. L. Atlas, A. Bracher
Format: Article
Language:English
Published: Copernicus Publications 2015-11-01
Series:Biogeosciences
Online Access:http://www.biogeosciences.net/12/6369/2015/bg-12-6369-2015.pdf
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spelling doaj-a7adc03d0150402ca24dfcf79f9e61de2020-11-24T22:20:45ZengCopernicus PublicationsBiogeosciences1726-41701726-41892015-11-0112216369638710.5194/bg-12-6369-2015Halocarbon emissions and sources in the equatorial Atlantic Cold TongueH. Hepach0B. Quack1S. Raimund2T. Fischer3E. L. Atlas4A. Bracher5GEOMAR Helmholtz Centre for Ocean Research Kiel, GermanyGEOMAR Helmholtz Centre for Ocean Research Kiel, GermanyGEOMAR Helmholtz Centre for Ocean Research Kiel, GermanyGEOMAR Helmholtz Centre for Ocean Research Kiel, GermanyRosenstiel School of Marine and Atmospheric Science (RSMAS), University of Miami, Florida, USAHelmholtz-University Young Investigators Group PHYTOOPTICS, Alfred-Wegener-Institute (AWI) Helmholtz Center for Polar and Marine Research, Bremerhaven, GermanyHalocarbons from oceanic sources contribute to halogens in the troposphere, and can be transported into the stratosphere where they take part in ozone depletion. This paper presents distribution and sources in the equatorial Atlantic from June and July 2011 of the four compounds bromoform (CHBr<sub>3</sub>), dibromomethane (CH<sub>2</sub>Br<sub>2</sub>), methyl iodide (CH<sub>3</sub>I) and diiodomethane (CH<sub>2</sub>I<sub>2</sub>). Enhanced biological production during the Atlantic Cold Tongue (ACT) season, indicated by phytoplankton pigment concentrations, led to elevated concentrations of CHBr<sub>3</sub> of up to 44.7 and up to 9.2 pmol L<sup>−1</sup> for CH<sub>2</sub>Br<sub>2</sub> in surface water, which is comparable to other tropical upwelling systems. While both compounds correlated very well with each other in the surface water, CH<sub>2</sub>Br<sub>2</sub> was often more elevated in greater depth than CHBr<sub>3</sub>, which showed maxima in the vicinity of the deep chlorophyll maximum. The deeper maximum of CH<sub>2</sub>Br<sub>2</sub> indicates an additional source in comparison to CHBr<sub>3</sub> or a slower degradation of CH<sub>2</sub>Br<sub>2</sub>. Concentrations of CH<sub>3</sub>I of up to 12.8 pmol L<sup>−1</sup> in the surface water were measured. In contrary to expectations of a predominantly photochemical source in the tropical ocean, its distribution was mostly in agreement with biological parameters, indicating a biological source. CH<sub>2</sub>I<sub>2</sub> was very low in the near surface water with maximum concentrations of only 3.7 pmol L<sup>−1</sup>. CH<sub>2</sub>I<sub>2</sub> showed distinct maxima in deeper waters similar to CH<sub>2</sub>Br<sub>2</sub>. For the first time, diapycnal fluxes of the four halocarbons from the upper thermocline into and out of the mixed layer were determined. These fluxes were low in comparison to the halocarbon sea-to-air fluxes. This indicates that despite the observed maximum concentrations at depth, production in the surface mixed layer is the main oceanic source for all four compounds and one of the main driving factors of their emissions into the atmosphere in the ACT-region. The calculated production rates of the compounds in the mixed layer are 34 ± 65 pmol m<sup>−3</sup> h<sup>−1</sup> for CHBr<sub>3</sub>, 10 ± 12 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>2</sub>Br<sub>2</sub>, 21 ± 24 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>3</sub>I and 384 ± 318 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>2</sub>I<sub>2</sub> determined from 13 depth profiles.http://www.biogeosciences.net/12/6369/2015/bg-12-6369-2015.pdf
collection DOAJ
language English
format Article
sources DOAJ
author H. Hepach
B. Quack
S. Raimund
T. Fischer
E. L. Atlas
A. Bracher
spellingShingle H. Hepach
B. Quack
S. Raimund
T. Fischer
E. L. Atlas
A. Bracher
Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
Biogeosciences
author_facet H. Hepach
B. Quack
S. Raimund
T. Fischer
E. L. Atlas
A. Bracher
author_sort H. Hepach
title Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
title_short Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
title_full Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
title_fullStr Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
title_full_unstemmed Halocarbon emissions and sources in the equatorial Atlantic Cold Tongue
title_sort halocarbon emissions and sources in the equatorial atlantic cold tongue
publisher Copernicus Publications
series Biogeosciences
issn 1726-4170
1726-4189
publishDate 2015-11-01
description Halocarbons from oceanic sources contribute to halogens in the troposphere, and can be transported into the stratosphere where they take part in ozone depletion. This paper presents distribution and sources in the equatorial Atlantic from June and July 2011 of the four compounds bromoform (CHBr<sub>3</sub>), dibromomethane (CH<sub>2</sub>Br<sub>2</sub>), methyl iodide (CH<sub>3</sub>I) and diiodomethane (CH<sub>2</sub>I<sub>2</sub>). Enhanced biological production during the Atlantic Cold Tongue (ACT) season, indicated by phytoplankton pigment concentrations, led to elevated concentrations of CHBr<sub>3</sub> of up to 44.7 and up to 9.2 pmol L<sup>−1</sup> for CH<sub>2</sub>Br<sub>2</sub> in surface water, which is comparable to other tropical upwelling systems. While both compounds correlated very well with each other in the surface water, CH<sub>2</sub>Br<sub>2</sub> was often more elevated in greater depth than CHBr<sub>3</sub>, which showed maxima in the vicinity of the deep chlorophyll maximum. The deeper maximum of CH<sub>2</sub>Br<sub>2</sub> indicates an additional source in comparison to CHBr<sub>3</sub> or a slower degradation of CH<sub>2</sub>Br<sub>2</sub>. Concentrations of CH<sub>3</sub>I of up to 12.8 pmol L<sup>−1</sup> in the surface water were measured. In contrary to expectations of a predominantly photochemical source in the tropical ocean, its distribution was mostly in agreement with biological parameters, indicating a biological source. CH<sub>2</sub>I<sub>2</sub> was very low in the near surface water with maximum concentrations of only 3.7 pmol L<sup>−1</sup>. CH<sub>2</sub>I<sub>2</sub> showed distinct maxima in deeper waters similar to CH<sub>2</sub>Br<sub>2</sub>. For the first time, diapycnal fluxes of the four halocarbons from the upper thermocline into and out of the mixed layer were determined. These fluxes were low in comparison to the halocarbon sea-to-air fluxes. This indicates that despite the observed maximum concentrations at depth, production in the surface mixed layer is the main oceanic source for all four compounds and one of the main driving factors of their emissions into the atmosphere in the ACT-region. The calculated production rates of the compounds in the mixed layer are 34 ± 65 pmol m<sup>−3</sup> h<sup>−1</sup> for CHBr<sub>3</sub>, 10 ± 12 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>2</sub>Br<sub>2</sub>, 21 ± 24 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>3</sub>I and 384 ± 318 pmol m<sup>−3</sup> h<sup>−1</sup> for CH<sub>2</sub>I<sub>2</sub> determined from 13 depth profiles.
url http://www.biogeosciences.net/12/6369/2015/bg-12-6369-2015.pdf
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