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Meridional overturning circulation conveys fast acidification to the deep Atlantic Ocean

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Since the Industrial Revolution, the North Atlantic Ocean has been accumulating anthropogenic carbon dioxide (CO2) and experiencing ocean acidification, that is, an increase in the concentration of hydrogen ions (a reduction in pH) and a reduction in the concentration of carbonate ions. The latter causes the 'aragonite saturation horizon'-below which waters are undersaturated with respect to a particular calcium carbonate, aragonite-to move to shallower depths (to shoal), exposing corals to corrosive waters. Here we use a database analysis to show that the present rate of supply of acidified waters to the deep Atlantic could cause the aragonite saturation horizon to shoal by 1,000-1,700 metres in the subpolar North Atlantic within the next three decades. We find that, during 1991-2016, a decrease in the concentration of carbonate ions in the Irminger Sea caused the aragonite saturation horizon to shoal by about 10-15 metres per year, and the volume of aragonite-saturated waters to reduce concomitantly. Our determination of the transport of the excess of carbonate over aragonite saturation (xc[CO32-])-an indicator of the availability of aragonite to organisms-by the Atlantic meridional overturning circulation shows that the present-day transport of carbonate ions towards the deep ocean is about 44 per cent lower than it was in preindustrial times. We infer that a doubling of atmospheric anthropogenic CO2 levels-which could occur within three decades according to a 'business-as-usual scenario' for climate change-could reduce the transport of xc[CO32-] by 64-79 per cent of that in preindustrial times, which could severely endanger cold-water coral habitats. The Atlantic meridional overturning circulation would also export this acidified deep water southwards, spreading corrosive waters to the world ocean.
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22 FEBRUARY 2018 | VOL 554 | NATURE | 515
LETTER doi:10.1038/nature25493
Meridional overturning circulation conveys fast
acidification to the deep Atlantic Ocean
Fiz F. Perez1*, Marcos Fontela1*, Maribel I. García-Ibáñez1*, Herlé Mercier2*, Anton Velo1, Pascale Lherminier2, Patricia Zunino2,
Mercedes de la Paz1, Fernando Alonso-Pérez1, Elisa F. Guallart1 & Xose A. Padin1
Since the Industrial Revolution, the North Atlantic Ocean has been
accumulating anthropogenic carbon dioxide (CO2) and experiencing
ocean acidification1, that is, an increase in the concentration
of hydrogen ions (a reduction in pH) and a reduction in the
concentration of carbonate ions. The latter causes the ‘aragonite
saturation horizon’—below which waters are undersaturated with
respect to a particular calcium carbonate, aragonite—to move to
shallower depths (to shoal), exposing corals to corrosive waters2,3.
Here we use a database analysis to show that the present rate of
supply of acidified waters to the deep Atlantic could cause the
aragonite saturation horizon to shoal by 1,000–1,700metres in the
subpolar North Atlantic within the next three decades. We find that,
during 1991–2016, a decrease in the concentration of carbonate
ions in the Irminger Sea caused the aragonite saturation horizon to
shoal by about 10–15metres per year, and the volume of aragonite-
saturated waters to reduce concomitantly. Our determination of
the transport of the excess of carbonate over aragonite saturation
(xc[CO32])—an indicator of the availability of aragonite to
organisms—by the Atlantic meridional overturning circulation
shows that the present-day transport of carbonate ions towards the
deep ocean is about 44 per cent lower than it was in preindustrial
times. We infer that a doubling of atmospheric anthropogenic CO2
levels—which could occur within three decades according to a
‘business-as-usual scenario’ for climate change
4
—could reduce the
transport of xc[CO32] by 64–79 per cent of that in preindustrial
times, which could severely endanger cold-water coral habitats. The
Atlantic meridional overturning circulation would also export this
acidified deep water southwards, spreading corrosive waters to the
world ocean.
Atmospheric CO2 levels have increased from 280 to 400 parts per
million (p.p.m.) since the Industrial Revolution. The global ocean has
captured some 30% of this anthropogenic CO
2
(C
ant
), thereby acting as
a climate regulator
1
. This CO
2
absorption has led to a decrease in sea-
water pH (of about 0.12 units) and in the supersaturation of calcium
carbonate (CaCO3)—effects known collectively as ocean acidification.
Ocean acidification can particularly affect marine calcifiers
1
by favour-
ing the dissolution of CaCO3-based shells and skeletons2. Notably,
deep cold-water coral (CWC) reefs formed by scleractinian corals—
such as the ecosystem engineer Lophelia pertusa—are highly vulner-
able to ocean acidification3. The global distribution of CWC seems
to be partly limited by the depth of the aragonite saturation horizon
(ASH), which marks the boundary between aragonite-stable waters
above and dissolution-prone waters below
5
. In preindustrial times,
more than 95% of CWC locations were found above the ASH6, pro-
viding evidence that environments located below the ASH are hostile
to CWC growth. In the North Pacific Ocean (Fig. 1a), where the ASH
is only 500metres deep
7
, the distribution of aragonitic CWC is patchy
and CWCs do not develop to form the large, deep reef frameworks
that are abundant in the North Atlantic
8
, where the ASH has tended
to occur at depths of more than 2,000metres. However, ocean acifidi-
cation is causing the ASH to shoal, thus exposing CWCs to CaCO
3
undersaturation. Although laboratory experiments suggest that adult
L. pertusa can acclimatize to CaCO
3
undersaturation
9,10
, the long-term
survival of CWC reefs in undersaturated water is questioned, because
L. pertusa skeletons become weaker when exposed yearlong to levels
of ocean acidification that are predicted to occur in the future
10
, and
the dead skeletal framework that supports the reef itself is likely to
dissolve in undersaturated waters11.
To determine the degree of aragonite saturation of the world ocean
waters, we calculated xc[CO32] (in μmol kg1) by using quality-
controlled global data sets of marine CO
2
system measurements
12,13
.
A positive (or negative) xc[CO32] indicates waters that are supersaturated
(or undersaturated) with aragonite (see Methods). We find that high
positive
xc
[CO
32
] values occur in the North Atlantic while negative
values occur in the North Pacific; this is consistent with the known
distribution of CWC14 below 1,000metres (Fig. 1a). About 61% of
CWCs found below 1,000metres are located in the North Atlantic (this
number rises to 78% at depths below 1,500metres), where
xc
[CO
32
]
is greater than 0, with an average xc[CO32] of 24.5 μmol kg1 below
1,000metres (and 15 μmol kg1 below 1,500metres). These are half the
natural (preindustrial) xc[CO32] values (see Extended Data Table 1).
The Atlantic meridional overturning circulation (AMOC) created the
favourable conditions for CWC growth in the North Atlantic by con-
veying ventilated waters loaded with relatively high pH and positive
xc[CO32] to the deep Atlantic Ocean.
In the centre of the Irminger Sea (Fig. 1b), winter deep convection
recorded during 1991–2016 explains a persistent increase in Cant from
30 to 50 μmol kg
1
and the associated deep injection of ocean acidi-
fication in the ventilated subpolar mode water (Fig. 2a). During the
same period, the atmospheric C
ant
grew from 85 p.p.m. to 123 p.p.m.
A thick layer of low salinity (less than 34.91) traces the strong con-
vection events that occurred during the first half of the 1990s and
during 2014–2016. During those strong convection events, subpolar
mode water was ventilated down to 1,500metres, showing high
temporal variability and no indication of a slowing-down of deep
convection15,16. The present-day surface ocean has about a 30% higher
concentration of H+ ions ([H+]) than the natural (preindustrial)
surface ocean
1
. At the centre of the Irminger Sea, the [H
+
] increase
affects a layer about 1,500metres thick (Fig. 2c)—the deepest signal
yet seen of the direct injection of ocean acidification. Since 2002,
anthropogenic perturbations have caused the isolines that mark 25%
and 30% anthropogenic [H+] to deepen from the surface down to
1,500metres. The isolines that mark xc[CO32] progressively ascend
at about 10–15metres per year (Fig. 2b), with some slightly faster
ascension periods that are related to deep convection events (arrows
in Fig. 2b). The effect of these deep convection events is buffered by
1Instituto Investigaciones Marinas (IIM, CSIC), calle Eduardo Cabello, 6, 36208, Vigo, Spain. 2Centre National de la Recherche Scientifique (CNRS), Ifremer, Université de Brest, Institut de
Recherche pour le Développement, Laboratoire d’Océanographie Physique et Spatiale (LOPS), Centre Ifremer de Bretagne, 29280, Plouzané, France.
*These authors contributed equally to this work.
© 2018 Macmillan Publishers Limited, part of Springer Nature. All rights reserved.
Content courtesy of Springer Nature, terms of use apply. Rights reserved
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This paper presents the overview of the Shared Socioeconomic Pathways (SSPs) and their energy, land use, and emissions implications. The SSPs are part of a new scenario framework, established by the climate change research community in order to facilitate the integrated analysis of future climate impacts, vulnerabilities, adaptation, and mitigation. The pathways were developed over the last years as a joint community effort and describe plausible major global developments that together would lead in the future to different challenges for mitigation and adaptation to climate change. The SSPs are based on five narratives describing alternative socio-economic developments, including sustainable development, regional rivalry, inequality, fossil-fueled development, and middle-of-the-road development. The longterm demographic and economic projections of the SSPs depict a wide uncertainty range consistent with the scenario literature. A multi-model approach was used for the elaboration of the energy, land-use and the emissions trajectories of SSP-based scenarios. The baseline scenarios lead to global energy consumption of 400–1200 EJ in 2100, and feature vastly different land-use dynamics, ranging from a possible reduction in cropland area up to a massive expansion by more than 700 million hectares by 2100. The associated annual CO2 emissions of the baseline scenarios range from about 25 GtCO2 to more than 120 GtCO2 per year by 2100. With respect to mitigation, we find that associated costs strongly depend on three factors: (1) the policy assumptions, (2) the socio-economic narrative, and (3) the stringency of the target. The carbon price for reaching the target of 2.6 W/m2 that is consistent with a temperature change limit of 2 �C, differs in our analysis thus by about a factor of three across the SSP marker scenarios. Moreover, many models could not reach this target from the SSPs with high mitigation challenges. While the SSPs were designed to represent different mitigation and adaptation challenges, the resulting narratives and quantifications span a wide range of different futures broadly representative of the current literature. This allows their subsequent use and development in new assessments and research projects. Critical next steps for the community scenario process will, among others, involve regional and sectoral extensions, further elaboration of the adaptation and impacts dimension, as well as employing the SSP scenarios with the new generation of earth system models as part of the 6th climate model intercomparison project (CMIP6).