Potential genesis and implications of calcium nitrate in Antarctic snow
Among the large variety of particulates in the atmosphere, calcic mineral dust particles have highly reactive surfaces that undergo heterogeneous reactions with atmospheric acids contiguously. The association between nssCa<sup>2+</sup>, an important proxy indicator of mineral dust, and N...
Main Authors: | , |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2016-04-01
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Series: | The Cryosphere |
Online Access: | http://www.the-cryosphere.net/10/825/2016/tc-10-825-2016.pdf |
Summary: | Among the large variety of particulates in the atmosphere, calcic mineral
dust particles have highly reactive surfaces that undergo heterogeneous
reactions with atmospheric acids contiguously. The association between
nssCa<sup>2+</sup>, an important proxy indicator of mineral dust, and
NO<sub>3</sub><sup>−</sup>, a dominant anion in the Antarctic snowpack, was analysed.
A total of 41 snow cores ( ∼ 1 m each) that represent snow
deposited during 2008–2009 were studied along coastal–inland transects from
two different regions in East Antarctica – the Princess Elizabeth Land (PEL) and central
Dronning Maud Land (cDML). Correlation statistics showed
a strong association (at 99 % significance level) between NO<sub>3</sub><sup>−</sup>
and nssCa<sup>2+</sup> at the near-coastal sections of both PEL (<i>r</i> = 0.74) and
cDML (<i>r</i> = 0.82) transects. Similarly, a strong association between these
ions was also observed in snow deposits at the inland sections of PEL
(<i>r</i> = 0.73) and cDML (<i>r</i> = 0.84). Such systematic associations between
nssCa<sup>2+</sup> and NO<sub>3</sub><sup>−</sup> are attributed to the interaction between
calcic mineral dust and nitric acid in the atmosphere, leading to the
formation of calcium nitrate (Ca(NO<sub>3</sub>)<sub>2</sub>) aerosol. Principal component
analysis revealed common transport and depositional processes for
nssCa<sup>2+</sup> and NO<sub>3</sub><sup>−</sup> both in PEL and cDML. Forward- and back-trajectory analyses using HYSPLIT model v. 4 revealed that southern South
America (SSA) was an important dust-emitting source to the study region,
aided by the westerlies. Particle size distribution showed that over 90 %
of the dust was in the range < 4 µm, indicating that these
dust particles reached the Antarctic region via long-range transport from the
SSA region. We propose that the association between nssCa<sup>2+</sup> and
NO<sub>3</sub><sup>−</sup> occurs during the long-range transport due to the formation of
Ca(NO<sub>3</sub>)<sub>2</sub> rather than to local neutralisation processes. However,
the influence of local dust sources from the nunataks in cDML and the contribution
of high sea salt in coastal PEL evidently mask such association in the
mountainous and coastal regions respectively. Ionic balance calculations
showed that 70–75 % of NO<sub>3</sub><sup>−</sup> in the
coastal sections was associated with nssCa<sup>2+</sup> (to form Ca(NO<sub>3</sub>)<sub>2</sub>).
However, in the inland sections,
50–55 % of NO<sub>3</sub><sup>−</sup> was present as HNO<sub>3</sub>. The study indicates that the
input of dust-bound NO<sub>3</sub><sup>−</sup> contributes a significant fraction of the
total NO<sub>3</sub><sup>−</sup> deposited in coastal Antarctic snow. |
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ISSN: | 1994-0416 1994-0424 |