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Aiming at portraying the Aegean's water mass structure and identifying Dense Water Formation processes, two winter cruises were conducted in 2005-2006, across the plateaus and depressions of the Aegean Sea. The most prominent feature of the water mass distribution in the basin is a distinct "X-shape" of the Θ-S characteristics, suggesting a complicated coupling of the major Aegean sub-basins. The surface and deep waters are relatively decoupled with diverse origin characteristics, while the intermediate layers act as connectors of the main thermohaline cells. The Central Aegean seems to play a key role due to formation processes of water masses with densities equal and/or higher than 29.2 kg/m3, that take place in the sub-basin and disperses in the North Aegean. On the other hand, the South Aegean appears greatly influenced by the Eastern Mediterranean circulation and water mass distribution, especially under the Eastern Mediterranean Transient status. The Transitional Mediterranean Water monitored in the post-EMT period and characterized by low temperature at 14.2°C, low salinity at 38.92 and low dissolved oxygen at 3.97 ml/l, with its core around 750 m and above the saline (39.06) Cretan Deep Water, altered significantly the South Aegean structure. The pre-EMT thermohaline pattern of the Central and South Aegean deep layers were similar, while the bottom density of the Central basin was higher than that in the South Aegean. Thus, it is possible that the deep waters of the Central Aegean acted as a dense water reserve supply for the deeper part of the Southern basin.
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Distribution of the thermohaline characteristics in the Aegean Sea
related to water mass formation processes
(20052006 winter surveys)
Vassilios D. Vervatis,
1
Sarantis S. Sofianos,
1
and Alexander Theocharis
2
Received 7 December 2010; revised 23 June 2011; accepted 7 July 2011; published 30 September 2011.
[1]Aiming at portraying the Aegeans water mass structure and identifying Dense Water
Formation processes, two winter cruises were conducted in 20052006, across the plateaus
and depressions of the Aegean Sea. The most prominent feature of the water mass
distribution in the basin is a distinct Xshapeof the QS characteristics, suggesting a
complicated coupling of the major Aegean subbasins. The surface and deep waters are
relatively decoupled with diverse origin characteristics, while the intermediate layers act as
connectors of the main thermohaline cells. The Central Aegean seems to play a key role
due to formation processes of water masses with densities equal and/or higher than
29.2 kg/m
3
, that take place in the subbasin and disperses in the North Aegean. On the other
hand, the South Aegean appears greatly influenced by the Eastern Mediterranean circulation
and water mass distribution, especially under the Eastern Mediterranean Transient status.
The Transitional Mediterranean Water monitored in the postEMT period and characterized
by low temperature at 14.2°C, low salinity at 38.92 and low dissolved oxygen at 3.97 ml/l,
with its core around 750 m and above the saline (39.06) Cretan Deep Water, altered
significantly the South Aegean structure. The preEMT thermohaline pattern of the Central
and South Aegean deep layers were similar, while the bottom density of the Central basin
was higher than that in the South Aegean. Thus, it is possible that the deep waters of the
Central Aegean acted as a dense water reserve supply for the deeper part of the Southern
basin.
Citation: Vervatis, V. D., S. S. Sofianos, and A. Theocharis (2011), Distribution of the thermohaline characteristics in the
Aegean Sea related to water mass formation processes (20052006 winter surveys), J. Geophys. Res.,116, C09034,
doi:10.1029/2010JC006868.
1. Introduction
[2] In late 1980s and early 1990s the Aegean Sea drew the
attention of the oceanographic community, due to the dra-
matic shift of the Eastern Mediterranean thermohaline cir-
culation pattern. The abrupt changes in the Eastern
Mediterranean Deep Water (EMDW) posed a series of
questions on the stability of the regional thermohaline cir-
culation. Since then, several authors oriented their work in
the Eastern Mediterranean Transient (EMT) event, empha-
sizing the dynamical implication of the Aegean Sea as a
substantial source of regional deep waters [Roether et al.,
1996, 2007; Theocharis et al., 1999b, 2002; Klein et al.,
1999; Lascaratos et al., 1999; Samuel et al., 1999;
MalanotteRizzolietal., 1999; Zervakis et al., 2000; Wu
et al., 2000; Boscolo and Bryden, 2001; Tsimplis and Josey,
2001; Stratford and Haines, 2002; Tsimplis and Rixen,
2002; Nittis et al., 2003].
[3] In the beginning of the 20th century oceanographic
studies focused in the dense waters masses of the Aegean. In
a process first proposed by Nielsen [1912] North Aegean
Dense Water (NAgDW), a uniform cold and heavy layer
from surface to bottom north of Cyclades plateau,could
flow toward the South Aegean and possibly contribute to the
EMDW. However, Schott [1915] reanalyzing Nielsens
data confirmed his argument but disputed the fact that this is
a dominant process. Furthermore, Pollak [1951], Wüst
[1961] and later Hopkins [1978, 1985] minimized even
more the role of the Aegean Sea as a Dense Water Forma-
tion (DWF) area, as well as a contributor to the EMDW
compared with the Adriatic Sea. Under the same rationale
Plakhin [1971, 1972] did not comment of the Aegean being
a contributor to the EMDW, but made a step forward
describing a thermohaline cell triggered from DWF in Chios
and Cretan basins. Lacombe and Tchernia [1958] and Miller
[1974] did not change the suggested marginal character of
the Aegean Sea with respect to DWF. The only dissonance
comes from ElGindy and ElDin [1986], using cruise data
from 1948 to 1972, suggesting that just outside the Cretan
1
Division of Environmental Physics, University of Athens, Athens,
Greece.
2
Hellenic Center for Marine Research, Institute of Oceanography,
Attiki, Greece.
Copyright 2011 by the American Geophysical Union.
01480227/11/2010JC006868
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 116, C09034, doi:10.1029/2010JC006868, 2011
C09034 1of16
arc straits 40% of the EMDW originated from the Cretan
Deep Water (CDW). The general consensus of the majority
of the authors in the preEMT period, leads to the hypoth-
esis that the Aegean produces occasionally insignificant
amounts of dense waters. On the other hand, in the light of
new evidence, it becomes increasingly more likely that the
Aegean Seas location and atmospheric forcing make the
basin an advantageous DWF area.
[4] The Aegean Sea is a semienclosed basin character-
ized by an alteration of shelves, sills and bottom depres-
sions. It is a semienclosed basin located in the northeastern
Mediterranean (one of the four major basins of Eastern
Mediterranean Sea), covering an area of 180000 km
2
.Itis
connected to the Marmara and Black Seas through the
Dardanelles Strait in its northern part and connected to
the Levantine and Ionian Seas through several straits at the
southern end. The total volume of the Aegean Sea is about
75000 km
3
with an average depth of 415 m accounting for
the presence of extensive plateaus. Its topography is very
complicated, with over 3000 islands and islets and, in
consequence, introducing fragments of continental shelf
areas divided by numerous bottom depressions between
them. The deepest basins include the North Aegean trough,
encompassing the north Sporades, Athos, Lemnos and Saros
basins, with maximum depths up to 1500 m, the Skyros,
Chios and Ikaria basins in the Central Aegean with maxi-
mum depth of 1100 m, bounded to the south by the broad
Cyclades plateau and sills with depths less than 350 m, and
finally, the much bigger Cretan basin in South Aegean, with
maximum depth of 2500 m (Figure 1).
[5] The dominant winds are primarily from the north,
bringing cold and dry air through the Balkan Peninsula
[May, 1982], contributing to substantial heat fluxes for
surface buoyancy loss. The annual amount of evaporation
over the Aegean is around 1.31.5 m/yr [Jakovides et al.,
1989; da Silva et al., 1994; Drakopoulos et al., 1998] and
exceeds the sum of precipitation and river runoff 0.5 m/yr
and 0.11 m/yr, respectively [Poulos et al., 1997], while the
annual upward net heat flux is estimated at 26 W/m
2
[Poulos
et al., 1997]. The latter implies that the Aegean Sea, on an
average loses heat through its surface. A biased method to
classify a basin as a concentration or dilution is to examine
its density relative to the density of an adjacent basin
[Hopkins, 1978]. Zervakis et al. [2004] suggested that the
Aegean should be classified as a concentration basin, based
on the density distribution below the sills.
[6] The Aegeans water masses and stratification are
subject to strong variability at various timescales [Zervakis
et al., 2004; Skliris et al., 2007], intense circulation pat-
terns [Korres et al., 2002; Olson et al., 2007], water mass
formation [Velaoras and Lascaratos, 2005, 2010; Gertman
et al., 2006; Vervatis et al., 2009] and strong forcing of both
wind and thermohaline character [Theocharis et al., 1999b;
Sofianos et al., 2005]. The combination of this forcing with
the complex subbasin circulation and mesoscale eddy field
render a complicated picture of the regional dynamics. All
observational studies [Gertman et al., 1990; Ovchinnikov
et al., 1990; Theocharis and Georgopoulos, 1993; Theocharis
et al., 1999b; Zervakis et al., 2000; Olson et al., 2007] and
numerical simulations [Wu et al., 2000; Korres et al., 2002;
Nittis et al., 2003; Sofianos et al., 2005], point out a general
cyclonic circulation in the Aegean Sea, while an anticyclonic
pattern dominates the northeastern corner of the basin
[Sofianos et al., 2005]. However, the most active dynamic
features are the mesoscale cyclonic and anticyclonic eddies,
which can extend to several Rossby radii of deformation
(around O(10 km)). Some of these features appear to be
permanent (i.e., cyclonic eddy in south Chios basin, anti-
cyclonic circulation in Lemnos basin), while others have a
transient character and yet the mechanisms responsible for
the formation and decay of these features are not clear
[Olson et al., 2007].
[7] The main water masses and their distribution can be
summarized as follows. The most characteristic feature of
the stratification pattern in the North Aegean is the surface
brackish Black Sea Water (BSW) outflowing from the
Dardanelles Strait. The BSW forms a front with the intru-
sion of the much saltier Levantine Surface Water (LSW)
entering the Aegean through the eastern Cretan arc straits.
The intermediate layers of the NorthCentral Aegean are
occupied by Levantine Water (LW) of Levantine origin and/
or the locally formed Aegean Intermediate Water (AgIW)
[Gertman et al., 2006]. The Levantine Intermediate Water
(LIW) entering through the eastern Cretan arc straits follows
a northward path along the Turkish coast to be modified by
the aforementioned LW. Over the LemnosLesvos plateau
the LW and/or the AgIW get subducted below the BSW
thermohaline front. The vertical structure of the North
Aegean is comprised of a 2070 m modified BSW surface
layer, of an intermediate LW and/or AgIW layer down to
400 m and of the locally formed NAgDW [Zervakis et al.,
2003, 2004; Velaoras and Lascaratos, 2005]. After expe-
riencing strong mixing in the NorthCentral Aegean, and
being modulated by the presence of mesoscale eddies
[Zodiatis, 1994], the water masses appear at the western side
of the South Aegean, along the Evian coast and through the
Kafireas strait, with significantly lower salinities than the
ambient surface water masses. A less saline water mass
present in the subsurface layers of the South Aegean is the
Modified Atlantic Water (MAW). At intermediate depths,
the annually ventilated Cretan Intermediate Water (CIW), a
water mass more saline than the LIW, has often been
Figure 1. Aegean bathymetry and major features (basins,
plateaus and straits).
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
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monitored above the core of Transitional Mediterranean
Water (TMW), a product formed by the mixture of LIW and
EMDW outside the Cretan arc. In the early 1980s, the deep
layers of the Cretan Sea were occupied by a homogenous
water mass similar to the TMW and there was no signal of
CDW type [Zervakis et al., 2000].
[8] Observations after the early 1990s revealed a dra-
matically different structure of the Cretan Seawater column.
During the EMT event, extremely dense and saline waters of
local origin, started filling the deep Cretan basin and over-
flowing through the sills of the Cretan arc straits [Roether
et al., 1996; Kontoyiannis et al., 1999; Theocharis et al.,
1999a, 1999b]. Due to its high density, the CDW dis-
placed water from the deepest parts of the Levantine and
Ionian basins of the Eastern Mediterranean, and as a con-
sequence the TMW masses intruded the Cretan basin.
During the EMT, the hydrography of the Cretan Sea
included a distinctive deep water mass close to the bottom of
the basin (8002500 dbar), possibly formed by convection
in the open sea and/or in the surrounding shelf areas
[Theocharis et al., 1999b; Lykousis et al., 2002]. This
structure was not static but seemed to undergo considerable
changes during the same period. Following the EMT, the
CDW volume in the Cretan Sea has decreased, most probably
due to changes in the DWF processes [Theocharis et al.,
2006; Sofianos et al., 2007; Vervatis et al., 2009].
[9] Aiming at portraying the stratification of the Aegeans
subbasins, as well as locating possible areas of DWF pro-
cesses, two cruises were conducted during the winters of
2005 and 2006 and the basic findings are described in this
paper. In section 2 we provide a brief description of the
cruises and the data collected. In section 3 the basic QS
characteristics of the water masses during both winters are
reviewed and the hydrographic structure observed in the
major concavities of the Aegean is presented. Additionally,
in section 4 DWF structures are presented, under the scope
of potential subbasin coupling mechanisms. Finally, in
section 5 in order to quantify the variability of the water
mass structure, related to the EMT and its phases, an
intercomparison analysis is carried out.
2. Data and Methods
[10] Two cruises were carried out on board the R/V Aegaeo,
from 1 to 10 March 2005 and from 3 to 13 February 2006.
During the first cruise a total of 44 hydrographic CTD
stations were occupied while a total of 47 stations were
recorded in the second cruise (Figure 2). The majority of the
stations were concentrated in the deep concavities in order
to identify the dense water characteristics along the main
northsouth axis of the Aegean Sea and locate possible areas
of DWF. A small number of stations where occupied on this
axis across the Aegeans plateaus, in order to identify pos-
sible shelf convection processes and to monitor exchanges
between subbasins.
[11] The profiles of temperature, salinity (conductivity),
and dissolved oxygen concentration were collected using a
SeaBird CTD with a General Oceanics rosette, including
12 Niskin Bottles for the oxygen and salinity calibration.
The data set acquired was quality controlled, the dissolved
oxygen concentration was calculated with the Winkler
method [Carpenter, 1965] and the data set was filtered and
subsampled at 1 dbar vertical resolution. For safety reasons
the maximum depth of each profile was approximately
10 dbar shallower than the stations sea bottom. All the tem-
perature and densities discussed in the present paper are
potential temperatures and potential densities, respectively.
In section 5, in order to compare the stratification of the
Aegean Sea in different phases of the EMT event, a data
set covering the winter of 1987 [MalanotteRizzoli and
Robinson, 1988] has been analyzed together with the data
sets of the 2005 and 2006 winter cruises. From the
aforementioned data sets an averaged profile has been
computed for each Aegean subbasin. Finally, a data set
(MEDATLAS II) was used for analysis of the Aegean deep
Figure 2. Hydrographic CTD stations during the winter cruises of 2005 and 2006; magenta line denotes
cruise trajectory; first cruise station (start): square dot; last cruise station (end): diamond dot; North
Aegean (NAg): blue dots; Central Aegean (CAg): green dots; South Aegean (SAg): red dots; gray lines:
straits boundaries of the three major Aegean subbasins [Gertman et al., 2006].
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
3of16
water properties evolution, during the EMT [MEDAR Group,
2002].
3. Cruises Hydrographic Observations
3.1. QS Characteristics of the Aegean Sea
[12] The temperature and salinity characteristics mea-
sured during the first cruise, in winter 2005, are depicted in
Figure 3. The projected data in a QS diagram revealed a
diversity of the surface and deep layers between the North
(blue dots) and South (red dots) Aegean. The QS char-
acteristics present a distinct Xshape.At the surface, the
low salinity BSW layer and a warm LSW feature are
observed, whereas in the deep layers, locally formed dense
water masses of the NAgDW and CDW are found. The
same QS pattern is also observed in the second cruise in
winter of 2006 (Figure 4). Differences between the two
years data sets are mainly due to surface variability of the
intruded BSW and LSW masses and different locations of
sampling (e.g., Lemnos/Athos basins in North Aegean,
Skyros/Chios basins in Central Aegean, central/eastern
Cretan basins in South Aegean). Spatial differences in the
deep layers across the Aegean subbasins, indicates DWF
variability and/or different QS modification rates inside
the depressions [Zervakis et al., 2003, 2009].
[13] In Figures 3 and 4 the magenta triangle, following
Gertman et al. [2006], represents intermediate layers of the
Aegean, leaving outside the surface and deep waters. The
Xshapeof the QS diagram implicitly suggests a tran-
sition in properties inside the magenta triangle where the
North and South Aegean QS characteristics converge in the
Central Aegean, as clearly depicted in both cruises in
Figures 3 and 4 (green dots, upper panels). The QS trace
indicates possible DWF, since high dissolved oxygen con-
centrations higher than 4.8 ml/L prevail from the surface
down to depths of 400 m (Figures 3 and 4, lower panels). In
general, relatively high dissolved oxygen concentrations
were recorded in intermediate depths across all three Aegean
subbasins.
3.2. Stratification and Circulation
[14] In the North Aegean, observations on a dense grid of
CTD stations from 2005 winter survey, illustrate the water
mass structure of Lemnos basin. A SWNE transect reveals
a strongly stratified water column in the region (Figure 5).
The most prominent water mass feature, characteristic of the
circulation pattern and exchange with the Dardanelles Strait
is the BSW intrusion, with surface temperature minimum
11.5°C, salinity 36.2 and density 27.5 kg/m
3
, in a wedge
like layer with depth changing from 100 m in the NE to 20 m
in the SW ends of section. This salinity minimum is combined
with the dissolved oxygen concentration maximum of the
intruding water. The BSW intrusion from the Dardanelles
Strait into Lemnos basin is divided in two basic branches
Figure 3. QS diagram; winter 2005; North Aegean (NAg): blue dotes; Central Aegean (CAg): green
dots; South Aegean (SAg): red dots; Graycolor bars: intermediate depths (db) and oxygen concentrations
(ml/lt). Q/S/s
Q
boundaries (magenta lines): NAg surface layers (S < 38.7), SAg surface layers (Q> 14.7°C),
Aegean dense waters (s
Q
> 29.2 kg/m
3
)[Gertman et al., 2006].
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
4of16
around the island of Lemnos, depicted also with surface
drifters [Olson et al., 2007]. The first is westward through
Saint Eustratius strait and the second is northward through
Lemnos strait. The second branch influences more the surface
layers of Lemnos basin since the BSW extends to greater
depths (Figure 5). Below the surface layer, a warmer and
more saline layer centered at intermediate depths, extends
down to 400 m in Lemnos basin (Figure 5, Q/S panels). This
denser water mass cannot be formed locally due to presence
of the BSW insulator layer at the surface [Zervakis et al.,
2003, 2004; Velaoras and Lascaratos, 2005; Gertman et al.,
2006] and is most probably advected from the Central
Aegean. This water mass (Figure 5, Qpanel) is a mixture of
LW and/or AgIW formed locally in the Central Aegean
(discussed in section 4), with varying values of temperature
13.914.4°C, salinity 38.739 and density 2929.2 kg/m
3
.
In greater depths, below the main sill level, to the bottom of
Lemnos basin the dissolved oxygen concentration decreases
to 3.7 ml/l. The very low oxygen concentration of the deep
waters inside Lemnos basin indicates possible trapping of
olddense water from the early stages of the EMT. At the
time of the cruises in the deepest parts of Lemnos basin,
below 1000 m, the density was around 29.4 kg/m
3
gaining
buoyancy in comparison with the first stages of the EMT
[Zervakis et al., 2003, 2009].
[15] In the Central Aegean the locally formed water
masses, as well as the water masses of Black Sea and Le-
vantine origin, undergo strong mixing while being modulated
by the presence of mesoscale eddies [Zodiatis, 1994]. The
modified water masses follow the general cyclonic circula-
tion of the Aegean, exiting the Central Aegean via two main
paths to the South Aegean: a surface path through Kafireas
strait with QS characteristics of 13°C, salinity at 38.1 and
28.8 kg/m
3
and a surface/intermediate path through Myco-
nosIkaria strait. The latter exchange between the Central and
South Aegean is monitored from three stations across the
strait (Figure 6). Warm and saline waters of Levantine origin
(maximum values at 15.4°C and salinity at 39.1, Figure 6,
Q/S panels), enter the Central Aegean at the east end of
the strait with densities of 29 kg/m
3
(Figure 6, s
Q
/O
2
panels),
whereas cool and less saline AgIW egress from surface/
intermediate depths at the west side of the strait (minimum
values at 13.8°C and salinity at 38.7, Figure 6, Q/S panels)
with slightly increased densities of 29.1 kg/m
3
(Figure 6,
s
Q
/O
2
panels).
[16] The vertical water mass structure of the South
Aegean follows a postEMT typical three layer pattern
consisting of a surface, an intermediate and a deep layer,
but in contrast with the North Aegean the stratification is
much weaker (surface density 29 kg/m
3
; 1000 m density
29.18 kg/m
3
). However, none of the layers resemble the
QS characteristics ofthe North Aegean. This can be explained
mainly by the very strong influence from the adjacent basins.
In Figure 7, a NWSE transect during the winter close to
Figure 4. QS diagram; winter 2006; North Aegean (NAg): blue dotes; Central Aegean (CAg): green dots;
South Aegean (SAg): red dots; Graycolor bars: intermediate depths (db) and oxygen concentrations (ml/lt).
Q/S/s
Q
boundaries (magenta lines): NAg surface layers (S < 38.7), SAg surface layers (Q> 14.7°C),
Aegean dense waters (s
Q
> 29.2 kg/m
3
)[Gertman et al., 2006].
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
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Kassos strait, depicts the strong influence of Levantine region
to South Aegean. In contrast with Lemnos basin where the
surface stratification is dominated by the shallow (20100 m
thickness) BSW layer, the South Aegean Mixed Layer Depth
(MLD) extends to 200 m (Figure 7). The horizontal tempera-
ture gradient, ascribed to a permanent cyclone in the eastern
Cretan Sea [Balopoulos et al.,1999;Theocharis et al.,1999b;
Kontoyiannis et al.,1999;Tsimplis et al.,1999;Georgopoulos
et al., 2000], is dominating the region (Figure 7, Q/S panels).
[17] The South Aegean intermediate layers consisted of
several intrusive and locally formed water masses. A mix-
ture of LIW and locally formed Cretan Intermediate Water
(CIW) lies between 200 and 500 m (Figure 7, Q/S panels,
intermittent core of 14.6°C and salinity at 38.98). A second
very distinct intermediate layer in the Cretan Sea is the
TMW, a mixture of LIW and old EMDW with its core
around 750 m, which enters from the adjacent Levantine
basin through Kassos strait at the sill depth. The TMW QS
core characteristics are low temperature 14.2°C, relatively
low salinity 38.92 and low dissolved oxygen concentrations
3.97 ml/l (Figure 7) and had never been recorded inside the
Aegean in the preEMT period. In the first stages of the
EMT, the TMW was present in the Cretan Sea in interme-
diate layers of about 300 m [Theocharis et al., 2006;
Sofianos et al., 2007; Vervatis et al., 2009]. Since 1995 the
EMT event started to decay confirming its transitional char-
acter. As a consequence, the TMW core was continuously
deepening, due to the deflation and outflow of the CDW from
the Cretan to Levantine basin through Kassos strait. At the
time of the cruises, the CDW horizon has dropped in depths
greater than the Kassos sill. The deep layers of Cretan basin
are filled by CDW, locally formed in the Aegean Sea, with
properties of 14°C, salinity of 39.06, 29.32 kg/m
3
and dis-
solved oxygen concentration of 4.2 ml/l, which is larger than
the overlying TMW.
4. DWF Processes
[18] Although the North Aegean is a dilution basin (winter
surface densities of 28 kg/m
3
influenced by the presence of
BSW), the deep layers are filled up to the sills with very
dense waters (29.4 kg/m
3
below a depth of 1000 m). Several
authors in recent studies [Zervakis et al., 2000, 2003;
Tragou et al., 2003; Nittis et al., 2003] suggested that the
northern Aegean can act in some exceptionally rare cases as
a concentration basin, under extremely cold and dry winter
Figure 5. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 6 CTD stations in the
winter of 2005 at Lemnos basin in the North Aegean (NAg); inside map blue large dot denote initial sta-
tion, following a SWNE direction of the magenta section (small blue dots); top axis indicating the code
names of the stations during the cruise; lower axis are in distance (km) from the initial station; major sea-
bed features: Lemnos basin.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
6of16
events such as the EMT. Under this scope two basic scientific
questions arise: Are the Aegean subbasins decoupled or is
there a connecting mechanism? Is the Aegean circulation
controlled by intrusions from adjacent basins or by local
processes?
[19] Investigating the role of the Central Aegean in DWF
processes, a number of stations were occupied during the
cruise of 2006 in Skyros, Chios and Ikaria deep basins,
aiming at capturing open ocean convection events and shelf
convection in LemnosLesvos plateau. In Figures 8 and 9
both eastward and westward transects are depicted, respec-
tively, introducing a winter snapshot of the NorthCentral
Aegean. The most outstanding feature in both transects is
the surface isopycnal layers of 29.1 kg/m
3
and 29.2 kg/m
3
over almost the entire Central Aegean (Figures 8 and 9, s
Q
panel). The physical mechanism which makes this area
favorable for DWF is the combination of extreme saline
LSW, loss of buoyancy through intense winter cooling,
along its northward travel over the depressions and plateaus
of the Central Aegean and finally transformed to the
locally formed AgIW. This buoyancy loss mechanism is
enhanced by the trapping of water in the permanent and
semipermanent cyclonic features in the region (Chios and
Skyros cyclones) over the deep subbasins [Lykousis et al.,
2002; Olson et al., 2007]. Both deep water and shelf
convection processes across the LemnosLesvos plateau
are believed to contribute to DWF in the region. During the
2006 cruise the DWF processes extended to intermediate
depths around 400 m. The densest surface waters masses
observed above LemnosLesvos plateau at 29.3 kg/m
3
, while
in Chios and Skyros depressions the surface density was
measured at 29.2 kg/m
3
.
[20] Evidence of previous occurrences of DWF in the
region is revealed by the deep stagnant layers in Figures 8 and
9. In Skyros and Athos basins, a strong EMT signal seems to
be preserved since the late 1980s period, evidenced by
extreme dense waters trapped in the bottom depressions. In
Figure 9 the EMT signature is emphasized with low dissolved
oxygen at 3.4 ml/l, low temperatures at 13°C and salinities at
39.05, resulting to high densities of 29.4 kg/m
3
.Zervakis
et al. [2003, 2009] suggested a slow renewing of the
deep waters in both Skyros and Athos basins, due to an
internal wave braking mechanism.
[21] Intrusive water masses from adjacent basins, such as
the Levantine and Black Seas can play significant roles in
the Aegean Sea processes. The fact that two different water
Figure 6. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 3 CTD stations in the
winter of 2006 at the north edge of the MyconosIkaria strait in the Central Aegean (CAg); inside map
green large dot denote initial station, following a WE direction of the magenta section (small green dots);
top axis indicating the code names of the stations during the cruise; lower axis are in distance (km) from
the initial station; major seabed features: MyconosIkaria strait, Ikaria basin.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
7of16
masses (with very diverse temperature, salinity and density
characteristics) are intruding from the south and north ends
of the basin does not allow the development of a simple
thermohaline cell. The BSW, with very low density, is
covering big parts of the north region of the Aegean acting
as an insulator and preventing DWF processes [Zervakis
et al., 2004]. Coupling between the basins is achieved
through intermediate (and possibly deep) water mass for-
mation processes in the central part of the basin, creating a
rather complicated thermohaline cell. A replenishing mech-
anism of intermediate layers is introduced, through buoyancy
loss of the saline LSW. A mixture of LW and/or locally
formed AgIW recirculates at intermediate depths across the
Aegean. Convection was monitored in Chios basin during the
winter of 2006 (Figure 10), enhanced by the permanent Chios
cyclone [Sofianos et al., 2005; Olson et al., 2007]. Dense
water masses formed in Chios basin are observed to be
spreading isopycnally at 400 m. The QS characteristics of
the dense water masses at intermediate depths of Chios basin
(Figure 10, Q/S panels) are also found in the North Aegean
(Figures 5, 8 and 9, Qpanel) and in the western side of the
MyconosIkaria strait (Figure 6), flowing into the South
Aegean. The deep layers in different basins are decoupled
from each other due to very irregular seabed topography.
5. Pre/PostEMT State
[22] The stratification monitored during 2005 and 2006
cruises should be discussed in the framework of the EMT
climatic shift. The question is: how typical is this latepost
EMT pattern? In order to answer the latter question, a pre
EMT reference year, namely data from a 1987 cruise
[MalanotteRizzoli and Robinson, 1988], is compared to the
winter cruises of 2005 and 2006 (Figure 11, 19872005
2006 map panels). Zervakis et al. [2000] presented a synoptic
log of the winter survey in the beginning of the EMT during
1987. A severe buoyancy loss took place in midMarch
[Lagouvardos et al., 1998] a few days before the stations
depicted at Lemnos and Chios basin (Figure 11, 1987 map
panel, blue/green dots). Therefore, no significant EMT signal
was yet detected at that time in the deep layers. The stations in
the Cretan basin (Figure 11, 1987 map panel, red dots)
chronologically are placed in lateMarch, but the EMT signal
monitored at least two months later in lateApril. Conse-
Figure 7. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 7 CTD stations in the
winter of 2005 at eastern Cretan basin in the South Aegean (SAg); inside map red large dot denote initial
station, following a NWSE direction of the magenta section (small red dots); top axis indicating the code
names of the stations during the cruise; lower axis are in distance (km) from the initial station; major sea-
bed features: eastern Cretan basin.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
8of16
quently, the 1987 mid/latewinter profiles are considered to
be representative of the preEMT state of the Aegean.
[23] In Figure 11 (Q/S/s
Q
panels for the NorthCentral
South Aegean), an average winter profile is depicted, of the
thermohaline properties during the three years (1987, 2005
and 2006). The North Aegean profiles reveal a threelayer
stratification (Figure 11, top row Q/S/s
Q
panels). Surface
BSW intrusion enhances the stratification, whereas LW and/
or AgIW replenish the intermediate layers. In the deep
layers NAgDW is trapped in the depressions. During 1987
the North Aegean surface waters appear to be more saline,
probably due to reduction of the BSW inflow [Zervakis et al.,
2000] and/or to intrusion of larger amounts of LSW/LIW
[MalanotteRizzoli et al., 1999]. At the time of the cruises,
the typical North Aegean QS characteristics significantly
changed, as the colder and less saline intermediate/deep
layers altered in more saline water masses (Figure 11).
Between the cruises, in late postEMT state, the deep layers
of Lemnos basin indicate a small buoyancy gain due to a
possible internal wave breaking [Zervakis et al., 2003, 2009].
This mechanism introduces a slow evolution of the North
Aegean deep layers in the postEMT period, in contrast to the
uplifting mechanism of the deep layers ventilation during
the EMT period.
[24] The SouthCentral Aegean exhibits a completely
different structure during the pre/postEMT periods. A two
layer stratification in both areas during the preEMT period
changed in a compound mode during the EMT phase. In
Central Aegean warm and saline surface water masses existed
on top of cold and less saline trapped deep layers (Figure 11,
middle row Q/S/s
Q
panels). During the winter cruises of
2005 and 2006 a much weaker stratification was observed,
resulting to an almost uniform dense water column in 2006 of
29.1529.2 kg/m
3
(Figure 11, middle row s
Q
panel). The
DWF processes described in section 4, replenish the inter-
mediate layers of the Aegean subbasins. The evolution of the
deep layer characteristics during the EMT is presented in
Figure 12, where the average deep (below 600 m, extracted
from MEDATLAS II database) temperature, salinity and
density was computed form data obtained during cruises from
1986 to 2006 [MEDAR Group, 2002]. Because the preEMT
temperature/salinity patterns of the deep layers of the Central
and South Aegean basins were similar (Figure 11, middle and
bottom rows Q/S/s
Q
panels, 1987; Figure 12), and the bottom
Figure 8. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 17 CTD stations in
the winter of 2006 at the eastern side of the NorthCentral Aegean (NAgCAg); vertical dashed gray line
in seabed divides NAgCAg regions; inside map blue large dot denote initial station, following a NS
direction of the magenta section (small bluegreen dots for NAgCAg, respectively); top axis indicating
the code names of the stations during the cruise; lower axis are in distance (km) from the initial station;
major seabed features: Lemnos basin, LemnosLesvos plateau, Chios basin, MyconosIkaria strait.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
9of16
density of the Central basin was higher than that in the South
Aegean at that time, it seems likely that the deep waters of the
Central basin acted as a reserve supply of dense water for the
deeper part of the Southern basin. In fact, while salinity
increased at deep layers in both basins, it was compensated by
a temperature increase that resulted in a decrease of deep
water density in the Central Aegean, while there was a
marked increase of density in the Southern Aegean deep
waters compared to preEMT stratification (Figure 11, mid-
dle and bottom rows Q/S/s
Q
panels; Figure 12). Furthermore,
the coupling of the CentralSouth Aegean deep layers is
complicated, due to entrainment phenomena, underlined
from the greater densities in Chios than in Cretan basin,
during the first stages of the EMT (Figure 12).
[25] The very complicated topography of the Aegean Sea
can also play a role in the evolution of deep water char-
acteristics. The topographic differences between the North
and Central Aegean, highlighted by the hypsographic dia-
grams in Figure 13, can explain the density differences in
the deep layers. Lemnos and Athos basins are very abrupt
with a wide, shallow shelf and contrasting deep depression,
favorable for replenishment by abrupt pulses of DWF on
shelf regions such as the LemnosLesvos plateau. The Chios
basin is more like a Vshaped basin with gradual depth
change (Figure 13), and easier to replace deep water masses
by thermohaline circulation cell. However, in Central
Aegean in Skyros basin the seabed topography is similar with
the North Aegean Athos and Lemnos basins (Figure 13), and
the deep water thermohaline properties deviate from those in
Chios basin (Figures 4 and 9). This effect of topography on
deep water mass renewal can explain the density differences
between the depressions in the North and Central Aegean.
Although temperature, salinity and density increased during
the EMT in all northern deep basins, the density of the Central
Aegean appears lower in the postEMT, where renewal
processes are favored by the local topography.
[26] The EMT signal inside the Cretan Sea has recently
declined [Theocharis et al., 2006; Sofianos et al., 2007;
Vervatis et al., 2009] confirming its transitional character.
However, it is still remaining strong enough to obscure a
Figure 9. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 14 CTD stations in
the winter of 2006 at the western side of the NorthCentral Aegean (NAgCAg); vertical dashed gray line
in seabed divides NAgCAg regions; inside map blue large dot denote initial station, following a NS
direction of the magenta section (small bluegreen dots for NAgCAg, respectively); top axis indicating
the code names of the stations during the cruise; lower axis are in distance (km) from the initial station;
major seabed features: Lemnos basin, Athos basin, Skyros basin, Kafireas strait, MyconosIkaria strait.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
10 of 16
Figure 10. Transects of Q(°C), S, s
Q
(kg/m
3
) and oxygen concentration (ml/lt), of 6 CTD stations in
the winter of 2006 at Chios basin in the Central Aegean (CAg); inside map green large dot denote initial
station, following a SWNE direction of the magenta section (small green dots); top axis indicating the
code names of the stations during the cruise; lower axis are in distance (km) from the initial station; major
seabed features: Chios basin.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
11 of 16
Figure 11. Map panels: Aegean Sea winter hydrographic stations for the years 1987 (preEMT), 2005
and 2006 (postEMT); North Aegean (NAg): blue dots at Lemnos basin; Central Aegean (CAg): green
dots at Chios basin; South Aegean (SAg): red dots at centraleastern Cretan basin. Q/S/s
Q
panels: Aver-
aged profiles of Q(°C), S and s
Q
(kg/m
3
), for all three major subbasins.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
12 of 16
Figure 12. Q/S/s
Q
properties of the Aegean deep layers (averaged data below 600 m) during the pre/
postEMT period (19862006). Lemnos (North AegeanNAg, blue circles), Chios (Central AegeanCAg,
green squares) and eastern Cretan (South AegeanSAg, red diamonds) subbasins.
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
13 of 16
clear understanding of the dynamics of the Aegean, since
the CDW remains extremely dense (29.3229.34 kg/m
3
below 2000 m) and because the TMW evolution masks the
signals of the change in intermediate layers.
6. Summary and Discussion
[27] Two winter cruises in the late postEMT period were
conducted during the winter season of 2005 and 2006
aiming at depicting the distribution of the thermohaline
properties and possible DWF processes in the Aegean Sea.
Previous studies highlighted the dramatic changes that took
place in the region during the EMT [Gertman et al., 1990,
2006; Roether et al., 1996, 2007]. With respect to the last
decade observational studies [Balopoulos et al., 1999;
Kontoyiannis et al., 1999; Tsimplis et al., 1999; Theocharis
et al., 1999a, 1999b; Georgopoulos et al., 2000; Zervakis
et al., 2000, 2003, 2004; Lykousis et al., 2002], the cruises
designed to portray the water mass changes in the deep basins
of the North and South Aegean. The decoupled surface and
deep water masses, unveiled an intermediate conveyor belt
coupling the Aegean subbasins. A distinct XshapeQS
emphasizes that the intermediate layers connects the basins
through a main thermohaline cell. Occasional deep water
formation processes replenish the deep layers while the
intermediate waters serve in their preconditioning.
[28] Intrusive water masses from adjacent basins, such as
the Levantine and Black Seas influence the surface vari-
ability of the region, masking local effects. The deep layers
of the three major bottom depressions of the Aegean Sea are
decoupled from each other due to the very irregular seabed
topography. Intermediate layers are replenished through
buoyancy loss of the saline LSW. Both open ocean (Chios
and Skyros basins) and shelf convection (LemnosLesvos
plateau) DWF processes were monitored in the Central
Aegean. Intermediate dense waters were formed locally as a
mixture of LW and local waters, recirculating at interme-
diate depths across the NorthCentral Aegean. On the other
hand, the South Aegean appears greatly influenced by the
Eastern Mediterranean general circulation and water mass
distribution, especially under the EMT status. The South
Aegean intermediate layers with a core at 750 m are influ-
enced by the TMW intrusion in the Cretan Sea, a mixture of
Figure 13. Hypsographic curves A(z) (km
2
) of crosssectional areas as a function of depth z (m). Merid-
ional crosssectional areas (magenta lines inside maps): Lemnos and Athos basins in North Aegean
(NAg), Skyros and Chios basins in Central Aegean (CAg), central Cretan and eastern Cretan basins in
South Aegean (SAg). Gray areas in transects and gray dashed line in hypsographic diagrams denote
the deepest layers of the basins (below 600 m).
VERVATIS ET AL.: AEGEAN SEA THERMOHALINE CHARACTERISTICS C09034C09034
14 of 16
the LIW and the old EMDW entering at sill depth of the
Kassos strait from the adjacent Levantine basin.
[29] In order to quantify the variability of the water mass
properties related to the EMT and its phases, a preEMT
reference year, 1987, was selected to be compared with data
from the winter cruises of 2005 and 2006. During the winter
of 1987, relatively fresh and less dense waters are monitored
in the deep layers. The BSW from the Dardanelles and the
LSW/LIW intrusion from the Cretan arc straits governed the
Aegean surface layers. However, this status changed dra-
matically during the EMT, due to the abrupt displacement of
the deep Aegean waters, together with the significant TMW
intrusion. In the postEMT period, the TMW layer has
similar characteristics with the dense water masses in pre
EMT period [Zervakis et al., 2000]. Furthermore, those
properties are very much alike to the Central Aegean DWF
properties monitored in the two recent winter cruises during
2005 and 2006. Therefore, the DWF processes in the Cen-
tral Aegean could not only trigger the intermediate conveyor
belt, but also act as an EMT relaxation mechanism inside the
Aegean.
[30]Acknowledgments. This work was supported by the Office of
Naval Research under contract N000140410524. The authors are deeply
indebted to the Captain and the crew of the HCMR R/V Aegaeo for con-
tinuous support during the whole measurement phase and to the Univer-
sity of Washington for the guidance and scientific suggestions/preparation
in both surveys. The thoughtful comments by the reviewers are gratefully
acknowledged.
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... Finally, an imported dense water mass of EMed origin can be found inside the Cretan Sea. This is called the Transitional Mediterranean Water (TMW) and originates in the layers that separate intermediate and deep waters of the EMed [15,20,45,46]. It is characterized by low salinity and oxygen but high nutrient content, and is actually the remnant of older Eastern Mediterranean Deep Waters (EMDW) that are gradually uplifted into shallower depths as new EMDW masses continuously refresh the abyssal EMed basins. ...
... Thus, during stagnation periods they can only alter their characteristics by diapycnal mixing with overlying intermediate waters [73,74]. This was the case during the stagnation period that followed the peak-EMT phase into the early 2000s decade, when a gradual decrease in deep water density, salinity, and dissolved oxygen was observed in all the north Aegean deep basins [1,46,73,75]. Different relaxation rates between the north Aegean deep basins were observed due to the different mixing dynamics in each of them. Data showed that the most intense mixing took place in the Lemnos Basin, while the weakest one was observed in the north Sporades basin. ...
Chapter
The Aegean Sea’s hydrological and circulation characteristics are as complex as its geomorphological setting. All major Eastern Mediterranean (EMed) water masses can be found inside the basin, while the Aegean Sea is a producer of dense intermediate and in some cases deep water masses that are exported to the EMed. The role of the Aegean Sea as a dense/deep water source for the EMed has been revised following the Eastern Mediterranean Transient event of the 1990s decade. The local dense water production has been recognized as having a strong effect over the EMed overturning circulation. In this chapter, up-to-date information on the Aegean Sea is summarized, open questions are highlighted, and major future research aspects are proposed.
... Regarding the scarcity of the production of NAeDW, it should be noted that the BSW acts as an insulation layer in the North Aegean due to its low salinity and temperature, and, consequently, deep-water formation events take place rather infrequently, during periods of exceptionally cold and dry winters and/or reduced Black Sea Water outflow (Zervakis et al., 2000). The densest waters of the Aegean Sea are produced in the Central /North Aegean Sea, especially the plateau connecting the island of Lemnos and Lesvos (south of the thermohaline front) separating the surface layer of Black-Sea-originated waters to the North and the Levantine-originated surface waters flowing northward along the eastern shores of the Aegean (Zervakis et al., 2000;Gertman et al., 2006;Vervatis et al., 2011). Vervatis et al. (2014) have shown that the reduction of BSW inflow through the Dardanelles facilitates the northward displacement of the thermohaline front and thus enabling higher dense-water formation rates in the region, which subsequently "feeds" the deep layers of the rest of the Aegean. ...
Article
Caesium-137 activity concentrations (¹³⁷Cs) were measured between 2003 and 2014 in the water column of Lemnos and Cretan deep basins of the Aegean Sea. The purpose was to assess water-mass dynamics and mixing processes by combining typical oceanographic data with the activity concentrations of ¹³⁷Cs. The radiological data, combined with dissolved oxygen profiles, provided substantially more information than solely temperature and salinity regarding processes such as water-mass identification, formation and mixing. In each basin it was possible to determine stagnant periods, where turbulent mixing was dominant, as well as periods where replenishment of the deep basins had been taken place. At Lemnos basin, the data profile in 2013 proved evidence of water column ventilation down to 800 m and replenishment of the deep basin by less saline water mass. The ¹³⁷Cs information provided evidence for contribution of water from the Black Sea to the intermediate and deep layers of the South Aegean (Cretan) basin. The profiles of 2013 and 2014 were characterized by the return of ¹³⁷Cs inventories to pre-Chernobyl levels.
... The formation of large volumes of dense waters during the Eastern Mediterranean Transient (EMT) event (Roether et al., 2007) has attracted the attention of the Mediterranean oceanographic community to the processes in the basin. As observational evidence pointed to the North and Central Aegean as the region where the EMT was originally triggered via the production of vast volumes of much denser waters than the south Aegean (Zervakis et al., 2000;Gertman et al., 2006), there have been several studies concentrating on the evolution of the intermediate and deep waters of the above basin (Zervakis et al., 2003;Lascaratos, 2005, 2010;Sayin et al., 2011;Vervatis et al., 2011). All analyses converge to the pivotal role of the Central Aegean as the region of formation of the densest waters of the Aegean Sea. ...
Article
This work examines the impact of coastal upwelling on the exchanges of a semi-enclosed basin with the open sea. Five oceanographic transects were performed with a cross-shore direction relative to the western coast of Lesvos island of the eastern Aegean Sea, a region where coastal upwelling is regularly observed during the sum- mer Etesian northerly winds. Filaments of highly saline water were observed during upwelling incidents, and were attributed to the enhanced transport of Levantine water from the south due to the baroclinic response to upwelling. All our observations, as well as a 9-year hindcast of the phenomenon revealed that the origin of the upwelled isopycnals usually remained above 40 m depth, and never exceeded the depth of 60 m. On the con- trary, the isopycnals hosting the nutricline appear to downwell during upwelling incidents. Our hindcast showed that the secondary geostrophic circulation is comprised both by surface and subsurface longshore currents, which affect the meridional exchanges at the surface and intermediate layers and reduce the residence time of the water in the basin. We conclude that coastal upwelling in a region with longshore temperature and salinity gradients can modify the transport of salt and heat along the coast, possibly affecting the thermohaline functioning of a basin.
Article
This study examines the impact of different turbidity products on the Aegean Sea surface physical characteristics, by performing twin-experiment simulations using a high-resolution regional ocean model. The turbidity products used include an in-situ based diffuse attenuation coefficient dataset at 490 nm (kd490, in m− 1) and a satellite derived kd490 product. Satellite turbidity products are broadly used in ocean simulations due to their spatiotemporal coverage and algorithm universality. Their validation and empirical components are trained mainly in phytoplankton driven regions and this may cause systematic differences in oligotrophic areas of variable optical properties’ composition. In the Aegean Sea, the in-situ based turbidity product accounts for the contribution of suspended particles in the solar heating profile, having further implications in the surface characteristics. The Aegean Sea upper-ocean thermohaline characteristics and general circulation patterns, reveal distinct differences between the twin-experiment simulations, showcasing mesoscale to locally induced impact of the turbidity variations. The turbidity impact on the air-sea interaction fluxes affects both thermodynamic processes i.e., solar radiation penetration and absorption in the water column, as well as dynamic processes i.e., momentum fluxes due to changes of the sea surface temperature and subsequently to the momentum drag coefficient. The Aegean Sea surface characteristics in the in-situ based turbidity product simulation, show a stronger decoupling between the North and the South Aegean Sea, when compared with the satellite derived turbidity product simulation. These results highlight the importance of incorporating more realistic turbidity products in ocean models, especially for optically complex regions such as the Aegean Sea.
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The evolution and drivers of dense water formation (DWF) in the North–Central Aegean Sea (NCAeg) during winter 2021–2022 are studied using observations from two Argo floats and the output of an operational data-assimilating model. Dense water with σθ>29.1 kgm−3 was produced over most of the NCAeg, except for the northeastern part covered by Black Sea water (BSW), where the maximum surface density was <29 kgm−3. The highest density waters were produced over the central and southern parts of the Lemnos Plateau and in the shallow coastal areas between Chios Island and the Edremit Gulf. Atmospherically driven transformation to the east of Lesvos Island resulted in the production of waters with anomalously high density and salinity, which flowed inside Skiros Basin, thus partly explaining its historically higher density and salinity compared to the rest of the NCAeg subbasins. The Skiros and Athos Basins were ventilated down to σθ∼29.35 kgm−3 horizons. The 29.1 kgm−3 isopycnal rose by ∼200 m, and the 29.25 kgm−3 isopycnal overflowed above the ∼400 m sill depth filling the southern depressions of the NCAeg. Combining data from Argo floats, vessel casts, gliders, and a fixed-point observatory, the dense water produced in the NCAeg was observed spreading in the deep layer of the Central Cretan Sea for at least one and a half years after the formation. The cyclonic circulation of the newly formed water in the NCAeg has been observed directly for the first time using deep-drifting floats. The Eastern Mediterranean warming and salinification signal has propagated below the NCAeg sill depth. The winter average buoyancy loss was comparable to that of the peak of the Eastern Mediterranean transient (EMT) and other known years of DWF in the NCAeg; however, the high temperature of the upper layers due to long-term warming prevented the widespread formation of denser water.
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This overview presents the different water masses present in the various primary and secondary marine regions of the Mediterranean Sea and Black Sea, providing information on their main physical characteristics (i.e., temperature, salinity, density), the water depths at which they have been observed and the processes involved in their formation. There is a characteristic difference in the overall hydrology of the Mediterranean Sea compared to the Black Sea, in terms of the number and characteristics of water masses and their formation processes, although they form a single (integrated) marine system. This difference is explained by the limited communication between the two seas through the Sea of Marmara and its straits (the Dardanelles and Bosporus) and by the fact that the Mediterranean Sea is a condensation basin while the Black Sea is a dilution basin; therefore, the deficit of water in the former is compensated by the inflow of Atlantic waters, while the surplus in the latter outflows to the Aegean Sea. In total, 21 different water masses have been identified in the Mediterranean Sea (excluding the Straits of Gibraltar and the Sea of Marmara) compared to the 5 water masses identified in the Black Sea (excluding the Sea of Azov). This large number of water masses is attributed to coastal morphology (i.e., presence of straits) and submarine relief (i.e., deep basin separated by shallow sills) and different formation processes.
Article
The neodymium isotopic composition (εNd) of seawater is one of the most important geochemical tracers to investigate water mass provenance, which can also serve as a proxy to reconstruct past variations in ocean circulation. Nd isotopes have recently also been used to reconstruct past circulation changes in the Mediterranean Sea on different time scales. However, the modern seawater εNd dataset for the Mediterranean Sea, which these reconstructions are based on, is limited and up to now only 160 isotopic measurements are available for the entire basin. The lack of present-day data also limits our understanding of the processes controlling the Nd cycle and Nd isotopic distribution in this semi-enclosed basin. Here we present new εNd data from 24 depth profiles covering all Mediterranean sub-basins, which significantly increases the available dataset in the Mediterranean Sea. The main goal of our study is to better characterize the relationship between the dissolved Nd isotope distributions and major water masses in the Mediterranean Sea and to investigate the impact and relative importance of local non-conservative modifications, which include input of riverine particles and waters, aeolian-derived material and exchange with the sediments at continental margins. This comprehensive εNd data set reveals a clear εNd – salinity correlation and a zonal and depth gradient with εNd systematically increasing from the western to the eastern Mediterranean basin (average εNd = -8.8±0.8 and -6.7±1 for the entire water column, respectively), reflecting the large-scale basin circulation. We have evaluated the conservative εNd behaviour in the Mediterranean Sea and quantified the non-conservative components of the εNd signatures by applying an Optimum Multiparameter (OMP) analysis and results from the Parametric Optimum Multiparameter (POMP) analysis of Jullion et al. (2017). The results of the present study combined with previously published Nd isotope values indicate that dissolved εNd behaves overall conservatively in the open Mediterranean Sea and show that its water masses are clearly distinguishable by their Nd isotope signature. However, misfits between measured and OMP- and POMP-derived εNd values exist in almost all sub-basins, especially in the eastern Levantine Basin and Alboran Sea at intermediate-deep depths, which can be explained by the influence of detrital lithogenic εNd signatures through interaction with highly radiogenic Nile sourced volcanic fractions and unradiogenic sediments, respectively. The radiogenic signature acquired in the eastern Levantine Basin is carried by the Levantine Intermediate Water and transferred conservatively to the entire Mediterranean at intermediate depths. Our measured εNd values and OMP- and POMP-derived results indicate that non-conservative contributions originating from sediment sources are then propagated by water mass circulation (with distinct preformed εNd) along the Mediterranean Sea through advection and conservative mixing. Mediterranean εNd effectively traces the mixing between the different water masses in this semi-enclosed basin and is a suitable water mass tracer.
Article
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The circulation of the Eastern Mediterranean Sea is characterized by numerous recurrent or permanent anticyclonic structures, which modulate the pathway of the main currents and the exchange of the water masses in the basin. This work aims to describe the main circulation structures and thermohaline properties of the Eastern Mediterranean with particular focus on two anticyclones, the Pelops and the Cyprus gyres, using in-situ (drifters and Argo floats) and satellite (altimetry) data. The Pelops gyre is involved in the circulation and exchange of Levantine origin surface and intermediate waters and in their flow toward the Ionian and the Adriatic Sea. The Cyprus Gyre presents a marked interannual variability related to the presence/absence of waters of Atlantic origin in its interior. These anticyclones are characterized by double diffusive instability and winter mixing phenomena driven by salty surface waters of Levantine origin. Conditions for the salt finger regime occur steadily and dominantly within the Eastern Mediterranean anticyclones. The winter mixing is usually observed in December–January, characterized by instability conditions in the water column, a gradual deepening of the mixed layer depth and the consequent downward doming of the isohalines. The mixing generally involves the first 200 m of the water column (but occasionally can affect also the intermediate layer) forming a water mass with well-defined thermohaline characteristics. Conditions for salt fingers also occur during mixing events in the layer below the mixed layer.
Article
Dense water (DW) formation commonly occurs in the shallow Northern Adriatic Sea during winter outbreaks, when there is a combination of the cooling of surface waters by the winds and high salinity as a result of reduced river inputs. These DWs subsequently propagate southwards over a period of weeks/months, eventually arriving in the Southern Adriatic Sea. The investigation is based on a new nonhydrostatic (NH) formulation of the 3D finite element model SHYFEM that is validated for a number of theoretical test cases. Subsequently this model is used to simulate, through high-resolution numerical simulations, an extreme DW event that occurred in the Adriatic Sea in 2012. We perform both hydrostatic (HY) and NH simulations in order to explicitly see the impact of NH processes on the DW dynamics. The modeled results are compared to observations collected in the field campaign of March–April 2012 in the Southern Adriatic Sea. The NH run correctly reproduces the across isobath bottom-trapped gravity current characterizing the canyon DW pathways. It also more accurately captures the frequency and intensity of dense water cascading pulsing events, as the inclusion of NH processes produces stronger currents with different DW mixing characteristics. Finally, the NH run simulates internal gravity waves (IGW), generated during the cascading at the edge of the canyon, which propagate downslope. This IGW activity is not captured in the HY case.
Article
The CEC/MAST-MTP PELAGOS Project, which was conducted in 1994 and 1995, found a new dynamic hydrological regime in the Cretan Sea–Cretan Straits region that is interacting with and affecting the whole basin of the Eastern Mediterranean. In the Cretan Sea, the upper thermocline general circulation shows no significant seasonal signal, but the circulation patterns observed were significantly different from those observed in 1986–87, suggesting that there is substantial interannual variability. There was a persistent outflow of Cretan Deep Water (CDW) with an annual mean flow of 0.6 Sv, which was making a substantial contribution to the formation of a new warmer, saltier and denser Deep Water of the Eastern Mediterranean, that was displacing upwards the Eastern Mediterranean Deep Water (EMDW) of Adriatic origin. Thus, the Cretan Sea is the unique source of a new type of the EMDW. There is an inflow of Transition Mediterranean Water (TMW) of low salinity, temperature and oxygen, but rich in nutrients into the South Aegean Sea (Cretan Sea) at intermediate depths (200–600 m) from the open sea areas of the Eastern Mediterranean, which is drastically changing the chemical conditions of the region. Biomass concentrations, primary production rates, the chemical constituents of the suspended particulate matter and the total mass fluxes of settling particles confirm that the South Aegean is one of the most oligotrophic regions of the world. Dissolved element concentrations are comparable to those reported for other straits of the Mediterranean. Particulate Fe and Mn occur in unusually high concentrations, probably originating from hydrothermal sources in the South Aegean Sea. It is expected that the nutrient enrichment of the intermediate layers in the Cretan Sea will influence the extremely oligotrophic character of the South Aegean and is having a direct effect on the biology of the region.