Secular change in atmospheric Ar∕N<sub>2</sub> and its implications for ocean heat uptake and Brewer–Dobson circulation
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Published:2021-02-01
Issue:2
Volume:21
Page:1357-1373
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ISSN:1680-7324
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Container-title:Atmospheric Chemistry and Physics
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language:en
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Short-container-title:Atmos. Chem. Phys.
Author:
Ishidoya ShigeyukiORCID, Sugawara Satoshi, Tohjima Yasunori, Goto Daisuke, Ishijima Kentaro, Niwa Yosuke, Aoki NobuyukiORCID, Murayama Shohei
Abstract
Abstract. Systematic measurements of the atmospheric Ar∕N2
ratio have been made at ground-based stations in Japan and Antarctica since
2012. Clear seasonal cycles of the Ar∕N2 ratio with summertime maxima
were found at middle- to high-latitude stations, with seasonal amplitudes
increasing with increasing latitude. Eight years of the observed Ar∕N2
ratio at Tsukuba (TKB) and Hateruma (HAT), Japan, showed interannual
variations in phase with the observed variations in the global ocean heat
content (OHC). We calculated secularly increasing trends of 0.75 ± 0.30
and 0.89 ± 0.60 per meg per year from the Ar∕N2 ratio observed at
TKB and HAT, respectively, although these trend values are influenced by
large interannual variations. In order to examine the possibility of the
secular trend in the surface Ar∕N2 ratio being modified significantly
by the gravitational separation in the stratosphere, two-dimensional model
simulations were carried out by arbitrarily modifying the mass stream
function in the model to simulate either a weakening or an enhancement of
the Brewer–Dobson circulation (BDC). The secular trend of the Ar∕N2
ratio at TKB, corrected for gravitational separation under the assumption of
weakening (enhancement) of BDC simulated by the 2-D model, was 0.60 ± 0.30 (0.88 ± 0.30) per meg per year. By using a conversion factor of
3.5 × 10−23 per meg per joule by assuming a one-box ocean with a temperature
of 3.5 ∘C, average OHC increase rates of 17.1 ± 8.6 ZJ yr−1 and 25.1 ± 8.6 ZJ yr−1 for the period 2012–2019 were
estimated from the corrected secular trends of the Ar∕N2 ratio for the
weakened- and enhanced-BDC conditions, respectively. Both OHC increase
rates from the uncorrected- and weakened-BDC secular trends of the Ar∕N2
ratio are consistent with 12.2 ± 1.2 ZJ yr−1 reported by ocean
temperature measurements, while that from the enhanced-BDC is outside of the
range of the uncertainties. Although the effect of the actual atmospheric
circulation on the Ar∕N2 ratio is still unclear and longer-term
observations are needed to reduce uncertainty of the secular trend of the
surface Ar∕N2 ratio, the analytical results obtained in the present
study imply that the surface Ar∕N2 ratio is an important tracer for
detecting spatiotemporally integrated changes in OHC and BDC.
Funder
Japan Society for the Promotion of Science Global Environment Bureau
Publisher
Copernicus GmbH
Subject
Atmospheric Science
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