Tectonophysics,
153
90 (1982) 153-166
Elsevier Scientific
Publishing
Company,
LATERAL AND VERTICAL STRUCTURE IN A SMALL
ROBERT
S. WHITE
Department
Amsterdam
- Printed
in The Netherlands
VARIABILITY IN CRUSTAL VELOCITY AREA OF THE NORTH ATLANTIC
and G.M. PURDY
*
of Earth Sciences, Bullard Laboratories,
Unioersity of Cambridge,
Cambridge EC3 OEZ (Great
Britain) * Woo& Hole Oceanographic (Final
version
received
Institution,
Woods Hole, Mass. 02543 (U.S.A.)
January
23, 1982)
G.M.,
1982. Lateral
ABSTRACT
White,
R.S. and Purdy,
area of the North
Atlantic.
sphere in Europe The detailed Atlantic
and the North
velocity
and vertical
In: E.S. Husebye
structure
Atlantic.
Tectonophysics,
using 358 explosive
fired into an array of eight ocean bottom,hydrophones. the upper crust increasing probably
anisotropic
a normal
oceanic
mantle.
Delay
associated
with a minor
similar
to that
median
valley extends
fracture
of the top, indicating
with a much flatter
down
charges Inversion
mapping
variability
with a small region of high delay times in the northwest probably
of the first arrival overlying
16.4-l airgun refracted
a typical oceanic
using two datasets is generally
corner caused
the normal
faulting
which
at least into layer 3. Our observations
Moho which constrains
in a small
Ma old crust on the flank of the mid and several hundred
shots
travel times
possible
models of crustal
containing
in
layer 3 and a arrivals
from
low over most of the survey
area,
by the presence
crust
zone. We find that the topography
that
structure
90: 153- 166.
at the seafloor
time function
show that lateral
velocity
of the Lithosphere-Astheno-
section about 5 km thick with a steep velocity gradient
from about 3.5 km/set
layer 3 and from the mantle
in crustal
The Structure
of a 70 by 35 km area of 6-10
Ridge at 24ON was studied
shows that the crust comprises
variability
(Editor),
of abnormal
of the base of layer 2 is
occurs
along
from mantle formation
the margins
arrivals
of the
are consistent
at the spreading
centre.
INTRODUCTION
Marine the general
seismic refraction features
profiles
of the crustal
throughout
the world’s oceans have shown that
seismic velocity
structure
are everywhere
remark-
ably uniform. Uniform layer solutions suggest that normal oceanic crust can be characterised by three layers; at the top are sediments of variable thickness and velocity overlying layer 2 (the “volcanic” layer) with a mean velocity of 5.07 * 0.63 km/set, beneath which is layer 3 (the “oceanic” layer) of velocity 6.73 * 0.19 km/set. Beneath the base of the crust, marked by the Mohorovocic discontinuity, is the mantle with a mean velocity of 8.15 -C 0.13 km/set (Raitt, 1963; Christensen and 0040-1951/82/ooOO-0000/%02.75
0 1982 Elsevier Scientific
Publishing
Company
(a)
3500-3800
between
location
of OBH’s.
numbers
b. Detailed
spreading
immediately
m.
Areas
of seafloor
deeper
Bottom lineations
array
within
are indicated area. Heavy
shaded
“H”
EXP; shading,
this area is shown
and areas shallower
than 3500 m lightly
shaded,
f-8
of refraction “H” EXP on Fig. la. Numbers
line shows position
in Fig.
and
over depths
stars are identification
by Detrick
with no shading
against
line discussed
is
lb. circles.
rift valley in numbered
Ridge
enlarged
N
offset in the mid-Atlantic
identifications
of the Mid-Atlantic with anomaly
The location
“H” EXP survey area and the right lateral
by fainter broken
boxed area marked
survey
than 3800 m are heavily
shot positions
of the detailed
in box labelled than 4000 m shaded.
Zone to the south of the detailed
anomaly
greater
Hydrophone
of 500 m and depths
of Ocean
magnetic
to the north
map of OBH and explosive
Ridge which commences
Purdy ( 1980).
position
offset at the Kane Fracture
lines. Seafloor
Note the 160 km left-lateral
by diagonal
indicated
map showing
et al. (1978). with an interval
location
from Purdy
Contours
Fig. 1. a. General
45” 10’ (b)
24”OO’
24’ 10’
24” 20’
156
Salisbury,
1975; Kozminskaya
the velocity predicted
structure
by synthetic
by a discontinuous
and Kapustyan,
by matching seismogram
(White,
studies
velocity gradient
or more in layer 2, and rather 1979; Spudich
1975). Refinement
observed
waveforms
and
small gradients
typically
better
of 0.7 see-’
’ in layer 3
of the order of 0.1 set-
1981). Superimposed
of
to those
suggest that the crust is described
with the highest gradients,
and Orcutt,
of the details
amplitudes
on ‘this general
velocity
structure are variations which we can attribute to the formation of anomalous crust in fracture zones (Detrick and Purdy, 1980; White and Matthews, 1980), to systematic changes with age (Christensen and Salisbury, 1975), to azimuthal variations in propagation velocity caused by crack or by crystal alignment (Raitt et al., 1969; Keen and Tramontini, 1970; Christensen and Salisbury, 1975; Bibee and Shor, 1976), or to lateral the bathymetric
inhomogeneity
expression
70 by 35 km area of 6-10 old that
most
portion
of the experiment
of normal
either correlated
Ma old crust in the North
of the systematic
occurred. The objective
in structure
of the crust. The survey reported
crust unaffected
velocity
changes
Atlantic,
caused
with or unrelated which is sufficiently
by ageing
have already
was to map the degree of lateral variability by fracture
zones,
to
in this paper is over a
though
large localised
in a delay
time residuals found in the northwest corner of the survey may be related to the presence of anomalous crust associated with an offset in the spreading centre. A full report containing an analysis of the stability of the delay time inversion is in preparation (White and Purdy, in press); for the present we will confine ourselves to reporting
the major results and their imp~cations
EXPERIMENTAL
east-west
of oceanic
crust.
(OBH; Koelsch and Purdy, Zone in the North Atlantic
1979), in an
METHOD
An array of eight ocean bottom hydrophones was deployed to the north of the Kane Fracture extended structure
for the formation
“H” configuration (Fig. la). In order to control the upper crustal velocity a 16.4-l (lOOO-inch3), airgun was fired once every 100m along two long lines crossing longer
all the OBH but the central
ranges
were generated
using
one. Deeper penetrating
arrivals
from
varying
in size from 3.6 to 116 kg (8 to 256 lbs.), fired along lines joining
358 explosive
charges
crustal of TNT the edges
and diagonals of the OBH array (Fig. lb). Ranges from each shot to the receivers were calculated from the direct water wave travel time using a velocity versus depth profile
within
the water
column
derived
from
nearby
temperature
and
salinity
profiles. The analogue tapes from the continuously recording OBH’s were digitised at a 4 msec sampling intervai, record sections plotted and first arrival travel times picked to give a total of 1613 different range-travel time pairs. Prior to using the set of travel time data to determine the crustal structure, corrections were made for the varying water depths at the seafloor ray entry points near each shot. We use a modified water delay correction (White and Purdy, in
157
press), which corrects shots had been
the travel times to those that would have been measured
detonated
mean
water
about
the configuration
a delay entry
depth
different
arising
azimuth
height,
interfaces,
Uncertainty
partly
6 above
the seafloor,
area. This correction
of sub-seafloor
time inversion.
point,
a uniform
over the survey
requires
many
to the track followed
of 24 * 20 msec in the topographic
so leaves us free to use the data in
of the shot to receiver
by the shooting correction.
where & is the no assumptions
of 30 ‘-t 25 m in the seafloor
because
if the
depth
at the ray
ray paths
lay at a
ship, lead to possible
When
these
errors
errors
are added
to
uncertainties in the time of the first arrival of typically 10 msec, together with the possibility of small errors in the ranges and seafloor dips, the overall average uncertainty of corrected travel times is about 45 msec. VELOCITY
STRUCTURE
Normal
oceanic
crust
about
5 km thick was found
from conventional
reversed
refraction interpretations of arrivals from the explosive sources. The higher resolution of the velocity structure afforded by the denser coverage of airgun shots suggests
that
the compressional
velocity
in the
lf
to 2 km
“volcanic” layer), increases from approximately 3.5 km/set km/set at the base. This steep velocity gradient is typical presence
of open voids and cracks
increase in velocity deposited minerals, density
of cracks and fractures
deeper
material
associated
with a small fracture
variability
in the upper crustal
velocity
2 (the
with a downwards by secondarily and to a lower
than an abnormal
corner
profiles
layer
lf km
of the survey probably
record
only minor
lateral
structure,
lies beneath
km/set. Horizontal anisotropy is frequently observed beneath the spreading direction (Raitt
in the crust. Other
in the northwest
zone, the airgun
layer 3 (the ‘“oceanic”
of 6.7 km/set
at the top of the basement
due to a combination of partial crack infilling to crack closure under the increasing pressure
thick layer of 3.6 km/set
A normal
thick
near the seafloor to 6 of that caused by the
layer),
almost
layer 2. Mantle
3 km thick with a mean refractions
seismic
yield a velocity
of 8.0
in the velocity of the upper mantle of typically I-390 oceanic crust, with the maximum velocity parallel to et al., 1969; Keen and Tramontini, 1970; Keen and
Barrett, 1971; Christensen and Salisbury, 1975; Bibee and Shor, 1976). The azimuths of the mantle arrivals are similar to the spreading direction and simulations with artificial data having the same ~imuthal distribution show that the velocity we determine is close to the maximum velocity if the mantle is anisotropic (White and Purdy, in press). On a nearby north-south refraction line, which is perpendicular to the spreading direction, Detrick and Purdy (1980) found well-controlled mantle velocities of 7.62 kmj’sec over 17 Ma crust to the north, and 7.70 km/set over 7 Ma crust to the south of the Kane Fracture Zone (see Fig. la for Iocation). Since the north-south elsewhere, anisotropy
lines will sample the minimum the mantle is anisotropic, with of the order of 0.3 to 0.4 km/set.
velocity this suggests that a peak to peak horizontal
here, as velocity
158
DELAY
TIME FUNCTION
METHOD
The set of 1613 range-travel time pairs inverted using an iterative delay time function lateral
variability
basement
depth.
and the possibility
attempt inclusion
assumes
area on which
to explain
and Hanson,
of correlation
The delay time function
Raitt et al., 1969) the survey
that there is a uniform
the delay time and the 1969; Morris et al., 1969;
velocity-depth
perturbations
listed below,
free parameters velocity.
between (Morris,
travel times by making
1974) to the variables
(a) Mean refraction
method
are superimposed
the observed
of additional
from the array of eight OBH’s was technique to investigate the degree of
significantly
A fundamental
structure
in the delay least squares
testing
within
times.
at each stage whether
improves
assumption
We
fits (Lawson the
the fit.
of the delay time method
is that refractions travel in uniform velocity layers, so we do not use arrivals from layer 2, which is a region of high velocity gradients. We only illustrate results from subsets comprising layer 3 or mantle arrivals which have been returned from layers with small velocity gradients. (b) Mean delay time to refractor. (c) Two dimensional polynomial fit to order n of deviations in delay time to refractor as a function of geographic position. The delay time has been considered as represented at a position offset from the ray entry point through the seafloor near the source and the receiver by a constant distance along the azimuth of the raypath. The displacement is chosen such that the geographic location of the associated delay time lies above the region in the crust where we consider that most of the lateral inhomogeneity is present. Provided that lateral changes in the delay times occur over distances
that are large compared
offset is not critical (d) Systematic
and different
variations
to the offset, solutions
as they do, the magnitude
of the
give stable results.
in delay times as a function
of seafloor depth (and hence
basement depth since the sediment cover is negligible). This simple linear relationship is included to test whether there are systematic seismic velocity or thickness variations whether
beneath
bathymetric
highs
and
lows.
In particular,
the base of layer 2 and the base of the crust exhibit
the top of layer 2 (the seafloor)
or whether
deep crustal
we wish
to find
the same topography
interfaces
are flatter,
as since
this helps constrain possible models of processes at the spreading centre. There is a danger with delay time function mapping that artefacts will be introduced into the solution by, for example, the presence of refractor anisotropy or refractor topography (Whitcombe and Rogers, 1981) or by the poor distribution of sources and receivers. We have tested extensively the stability of the delay time inversions using sets of artificially generated arrival times from known velocity sructures, but with a random component added to each travel time to represent the errors to which each is subject. Results of these tests are discussed in detail by White and Purdy (in press) but, briefly, it suffices to say that we are satisfied that our inversions for the mean velocity, and the geographic delay time distribution, ((a)
159
through
(c) above),
is our survey
correctly
represent
area. The apparent
needs more care in interpretation, POLYNOMIAL
DELAY
TIME
We find that a fourth represent
the delay
of velocity
time-seafloor
depth
structure (A~/A~)
as it exists relationship
as we discuss later.
SURFACE
order double
times
the variation
delay
polynomial
satisfactorily,
delay time surface is sufficient
and that the significance
of adding
to
extra
ORDER 4
24” IO’ N
24”OO’
45” 10’ w
44” 30’
(a)
I
LAYER 3
%
At /Ah
I=
= -0.09
V = 6.7 km /set
G
d 5
5 & 2 n
-0.30
~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~ -1000 -500 0 500 1000
DEVIATION
FROM MEAN DEPTH (Ml
lb1 Fig. 2. a. Fourth
order double
areas show those regions constrained b. Deviation
polynomial
of the seafloor
delay time surface illuminated
by the data in these areas. Contour in delay time versus difference
the mean depth
for fourth
order solution
interval
between
from inversion
by the explosive
of layer 3 arrivals.
Unshaded
shots: the delay time surface
is only
is 0.05 sec.
seafloor
using layer 3 arrivals.
depth
at the ray entry and exit points
and
160
ORDER 4 24” 10’ N
24” 00’ 44” 30’
4i”lO’ w (a)
G i g F
0.30
--F-T
I ’ 7I ’ ’ 1’ I 1 , ’ ’ I 7 7 I
’I
7’ / ’ ’ ’ 7I ’
’
MOHO
‘.
0.15 -
yx _,_ .:
At/Ah
'.... ,,
=-0.15
G > iti
-0.30 ,,',.,",,""",'..~,'~~,,',,~~"~,,"~"L~,,"~~:',i 1000 -1000 -500 0 500
DEVIATION
FROM MEAN DEPTH (Ml
(b) Fig.3. a. Fourthorderdouble polynomial
delay time surface
interval 0.05 sec. b. Deviation in delay time versus difference the mean depth
for fourth
order solution
between
using mantle
seafloor
from inversion depth
of mantle
arrivals.
Contour
at the ray entry and exit points
and
arrivals.
terms to the polynomial series diminishes as higher orders are considered. In Figs. 2 and 3 we illustrate the fourth order polynomial surface, together with the corresponding correlation between delay time and seafloor depth, for inversions using the layer 3 and the mantle arrivals, respectively. The geographic delay time surface is normalised to the well-controlled delay time at OBH 7 in the centre .of the survey area, and the unshaded areas depict the Fresnel area beneath the shotpoints to
161
emphasise
how little of the upper
dense coverage
Delay
even with such a relatively
of shots and receivers.
The polynomial generally
crust is illuminated,
delay time surfaces
small variations
from both layer 3 and mantle
in delay times over the majority
times from layer 3 (Fig. 2) are the best constrained,
which they occur as first arrivals (8-25 receivers, ern corner
because
show
survey area.
the range over
km) is similar to the average spacing between
thus giving good ties between
layer 3 delay time deviations
arrivals
of the central
source and receiver
of a little over +O.l
of the survey, whilst elsewhere
delay times. Maximum
set are observed
the variations
in the northwest-
are typically
of the order of
0.05 sec. Since our average error in travel time is about 0.045 set, this represents only a small resolvable degree of lateral inhomogeneity over the majority of the survey area. Delay time variations from mantle arrivals (Fig. 3) show a similar pattern to those from layer 3 with a broad area of small deviations in the centre of the survey and a region of large delay times reaching over +0.25 set in the northwestern corner. The only significant difference in the pattern is that there is an area of high delay times along the southeastern edge. reaching over +0.20 sec. However, this is poorly controlled
because
predominance
it is on the edge of the survey
of arrivals
the northwestern
corner.
originating
and
in the anomalously
The somewhat
greater variations
may be corrupted
by a
high delay time region
in
in delay times sampled
by
mantle arrivals compared to those from layer 3 may be evidence for some lateral inhomogeneity in the lower crust. Variation may be introduced into the lower crust subsequent
to its formation
by hydrothermal
and
metamorphic
activity
or by
off-axis intrusion in layer 3 over the first 30 Ma (Christensen and Salisbury, 1975). The small lateral variations in delay times of around 0.05 set over the majority of the survey area must originate in layer 2, since they are recorded by the layer 3 refractor. Lateral thickness changes in layer 2 of up to a few hundred metres will explain
the observed
the superimposed result, may km/set
for example, cause
delay time variations
effects
of lateral
velocity
et al., 1973). Interbedding
we cannot
changes.
from low grade metamorphism
the compressional
(Fox
although
velocity
to drop
distinguish
Lateral of basalt
from
of sediment
velocity
may
to zeolite facies, which
5.0-6.6 with
this from
changes
km/set
to 4.4-5.0
the extrusive
igneous
material, together with changes in the thicknesses of shallow basement layers and with variations in the amount of rubble and pillow lavas will also cause minor lateral heterogeneity. The high delay times in the northwest corner of the delay time surface are probably related to spreading centre jumps at this latitude. The survey area is positioned over a swathe of crust to the north of the Kane Fracture Zone exhibiting normal seafloor spreading magnetic anomaly lineations. However, near the north of our survey the lineations terminate and are offset some 60 km to the east (Fig. la). Unlike the offset across most fracture zones, which occurs over a narrow zone, this offset is spread
over a broad area (Rona
and Gray,
1980) which suggests that it may
162
be accommodated Fracture
zones
by a series commonly
1980; Sinha and Louden, in the shallow
steps
atypical
or jumps
crustal
in the spreading
structure
1981) often with thicker than normal
crust (Detrick
times in the northwest
of small
exhibit
and Purdy,
of our survey
(Schouten
centre.
and White,
low velocity
material
1980) and we suggest that the large delay
may lie over crust modified
by such a ridge
jump. DELAY
TIMES CORRELATED
Inversions
from
both
TO SEAFLOOR
layer
3 and
DEPTH
mantle
arrivals
show
a strong
correlation
between the delay time and the seafloor depth (which is equivalent to the depth to the top of the basement) at the ray entry and exit points. The magnitude of the ratio, At/Ah, increases as the order of the double polynomial delay time surface is increased up to the fourth order, thereafter tending to stabilise at about -0.10 set/km for layer 3 and -0.18 set/km for mantle arrivals (Fig. 4). A fourth order polynomial surface is required to describe adequately the geographical variations in delay times; At/Ah
values from lower order solutions
are corrupted
by the residual
delay times unaccounted for by the polynomial surface and so will be ignored. One of the major shortcomings with the delay time function method is that we represent
the delay time down to the specified
to one specific
-0.15
location,
whereas
in reality
refractor
the raypaths
as a vertical delay pertaining follow curved
paths
which
-
0
2
ORDER
4
6
8
OF POLYNOMIAL
Fig. 4. Plot of delay time-seafloor depth (Al/Ah)
ratio versus order of double polynomial delay time
surface from layer 3 and mantle arrivals for those cases up to order 8 where the inclusion of the depth-delay
time relationship significantly improves the fit to the observed dataset. We show results
using only those raypaths within 30° of the ship’s track (i.e. where the depth at the ray.entry point is reasonably we.11determined).
163
sample
an oblique
improve
section
of the crust.
the representation
of the geographical
delay time to apply at a location the depth
we cannot
we take
the seafloor
variable,
whereas
the point
some distance
of the lateral
a similar
depth
at which
and therefore
section,
delay time surface by considering
the majority
follow
because
in the previous
lying above the region where the raypath
at which we consider
Unfortunately,
As discussed
we the
intersects
inhomogeneity
to reside.
procedure
with
At/Ah
at the ray entry
point
as the independent
relationship,
the ray will meet the refractor
lie beneath
basement
at a different
will be offset
depth.
Raytracing
through models of the crust with the same velocity-depth structure throughout, and basement topography taken from our survey tracks shows that continuous refraction of the raypaths arrivals that
through
to exhibit
the At/Ah
artificially
a At/Ah ratios
generated
topography
the velocity
as the
gradient
ratio of typically
we measure
values, top.
indicate
The
degree
-0.10
in layer 2 causes
the layer 3
set/km.
We therefore
3, which
are the same
as those
that the base of layer 2 has roughly
the same
from
layer
of scatter
topography on the base may be a somewhat surface (the seafloor), and still produce definitely
present
say that our data do not permit
in the
results
conclude
is such
that
the
subdued version of that of the basement acceptable At/Ah ratios, but we can an interpretation
with a flat base to layer
2. Measured At/Ah ratios from mantle arrivals are rather larger in magnitude than those from layer 3 (Fig.4). This is consistent with a model of the crust with a flat Moho, although the higher velocities of the lower crust mean that the resolution of the Moho topography is much poorer than that of the layer 2-layer 3 interface. Our conclusions are that the topography of the upper crustal layers is similar
to
that of the top of the volcanic basement, and that the observed At/Ah ratios are consistent with greatly subdued or flat relief on the Moho. The rugged seafloor relief in the Atlantic Ocean is created primarily by normal faulting at the margins of the median
valley
parallel
to the spreading
(Harrison
1977; Macdonald the Atlantic (Laughton constructional
and Stieltjes,
1977) the faults
centre (Laughton
and Rusby,
and Luyendyk,
Ocean,
and
and Searle, volcanic
form
1977):The within
1979) beyond relief
(Atwater, 1979), it is frequently around the volcanoes suggests
of up
2-4
forming
long linear
scarps
1975; Ballard and Van Andel,
faults are typically
2-2.5
km apart
km of the axis of the median
which little further
faulting
to 200 m is present
occurs.
in the
in
valley
Although
median
valley
blanketed by subsequent lava flows and faulting that the volcanoes sink into the crust after and
probably during their growth (Ballard and Van Andel, 1977). We are therefore left with the primary control on basement relief as the faulting in the crestal mountains. The presence of 7-8 km deep earthquakes on the Mid-Atlantic Ridge (Lilwall, 1980), is evidence for brittle faulting down to the Moho, and Lister (1974) and Williams et al. (1974) have postulated that fracturing with associated hydrothermal alteration may also penetrate as deep as the Moho. This then provides an explanation for the topography we infer on the layer 2-layer 3 interface; the upper crust,
164
already
formed by the time it is faulted into the crestai mountains,
into blocks and uplifted Although
by normal
the topography
faults extending
on the Moho is not so well constrained
that on the base of layer 2, we suggest
two main
much flatter
there is the geometric
than the basement.
at the margins crust.
This
tectonic
of the median
would
allow
tilts ranging
is simply chopped
down at least into layer 3.
Firstly,
of the crust
IO0 to 30” or 40
and
explain
in the fault
donald and Luyendyk, 1977; Atwater, 1979; Hall, 1979; Laughton Our second explanation is that the thermal structure of ridges temperature
isotherms
extend
at depth considerably
beyond
that the faults
out at the base of the
would
observed
by our results as for why it may be
reason
valley may be listric, flattening
extension
from
explanations
the outward blocks
(Mac-
and Searle, 1979). is such that high
the median
valley, and
that a normal Moho is not generally found at the spreading centre, but has developed by 10 or 20 km off axis (Fowler, 1976, 1978; Keen and Tramontini, 1970). There is also evidence of a growth in layer 3 over the first 30 Ma after formation (Christensen and Salisbury, 1975). Since the faulting occurs within 2-4 km of the axis, only f Ma after formation, the Moho structure will only be fixed subsequent to the faulting basement
after the deep crust has cooled and so will not reflect the shape of the in the way that the layer 2-layer
3 interface
does.
ACKNOWLEDGEMENTS
We thank the officers, crew and scientists aboard R/V “Atlantis” II during the cruise 96, leg 3, whose hard work and co-operation made this experiment possible. The ocean bottom hydrophones were built and maintained by D. Koelsch and C. Grant. C. Dean, R.S. Detrick, Dickson Ellison, L. Gove and M. Rosser assisted in various aspects of the data reduction and computer programming, for which we are most grateful. This research was sponsored by the Office of Naval Research under contract NO~l4-74 00262 NR083-004 to the Woods Hole Oceanographic Institution (WHOI). R.S. White acknowledges support from WHOI and Natural Environment Research Council
Postdoctoral
Cambridge bution
Fellowships.
contribution
number
number
Department
of Earth
Sciences,
194. Woods Hole Oceanographic
University
Institution
of
contri-
5025.
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Ocean:
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