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, FEBRUARY 2011, 62, 1, 55—63 doi: 10.2478/v10096-011-0005-z
Gravity instabilities in the Dohrn Canyon (Bay of Naples,
Southern Tyrrhenian Sea): potential wave and run-up
(tsunami) reconstruction from a fossil submarine landslide
VINCENZO DI FIORE, GEMMA AIELLO
*
and BRUNO D’ARGENIO
Institute for Marine Coastal Environment (IAMC), National Research Council of Italy (CNR), Calata Porta di Massa, Porto di Napoli,
80133 Napoli, Italy; *gemma.aiello@iamc.cnr.it
(Manuscript received June 30, 2010; accepted in revised form December 6, 2010)
Abstract: We discuss a mathematical model for wave and run-up generated submarine landslides in the canyons of the Bay
of Naples (Magnaghi-Dohrn canyon system). The morpho-bathymetry and submarine gravity instabilities of such incisions
have been investigated through the interpretation of a high resolution DEM. The canyons are located in a sector of the bay
where there is a variable interaction of volcanic activity (Phlegrean Fields and Ischia and Procida Islands) with sedimentary
processes due to the Sarno-Sebeto rivers. At present the Naples canyon-system is inactive, as is shown by the Holocene
sedimentary drapes deposited during the present sea-level highstand, but gravity instabilities occurred in the recent past at the
canyons’ heads. In particular the Dohrn Canyon is characterized by a double regressive head, while the Magnaghi Canyon
shows a trilobate head, formed by the junction of three main tributary channels and coincident with the retreat of the shelf
break around the 140 m isobath. The results of a simulation of failures in the above source areas show that the amplitude of
wave run-up, expressed in terms of the sea floor depth percentage, may range up to 2.5 % of the water depth at the sea bottom.
Key words: Bay of Naples, tsunamigenic potential, run-up landslide, numerical modelling.
Introduction
The aim of this paper is to study potential wave and run-up
events caused by submarine landslides located in the can-
yons of the Bay of Naples.
Tsunami waves, often caused by gravitative failures, may
be generated by earthquakes and less frequently by volcanic
eruptions. In the Bay of Naples all the above trigger factors
are present. As a consequence, the continental slope off the
bay represents an appropriate natural laboratory to study
geological events potentially leading to submarine slides
with their tsunamigenic potential.
The geological setting of the bay has been studied in detail
in the framework of research programmes for submarine geo-
logical cartography (Aiello et al. 2001; Bruno et al. 2003;
D’Argenio et al. 2004). In this gulf the continental slope and
the outer shelf are deeply incised by two submarine canyons of
kilometric extent, namely the Dohrn and Magnaghi Canyons,
representing the drainage system of this active volcanic area
during the Late Quaternary. Detailed mapping of the outer
shelf and slope morphology contributed to the understanding
of erosional and depositional processes related to continental
slope settings and allowed their geological interpretation to be
proposed (Aiello et al. 2001; D’Argenio et al. 2004).
Several studies about tsunamis have recently been carried
out in the Bay of Naples. Landslide-generated tsunamis in the
offshore of Ischia Island have been featured by Zaniboni et al.
(2007) in the framework of a project on the volcanic hazard
and risk assessment of the island of Ischia, by the National
Institute for Geophysics and Volcanology and the Italian
Department for Civil Protection. The above authors focussed
on the study of tsunamis generated by landslides from Ischia’s
slopes. The catastrophic collapse that formed the large scar in
the southern flank of Ischia (the Ischia Debris Avalanche of
Chiocci & de Alteriis 2006) may be considered as the upper
limit for tsunamigenic failures in the slopes of Ischia, even
though the duplication of such an event does not appear prob-
able at the moment. In this study we selected an area of the
Dohrn Canyon showing evidence of paleo-landslides and we
applied a model to evaluate the wave run-up generated by an
estimated flow, using a recent theoretical model (Lynett & Liu
2002; Di Fiore et al. 2008).
General setting of the area
The eastern margin of the Tyrrhenian Sea is characterized by
a number of basins formed during the latest Neogene-Quater-
nary across the structural boundary between the Apennine fold
and thrust belt and the Tyrrhenian back-arc extensional area
(Fig. 1). These basins, including the Bay of Naples and the
Bay of Salerno (Fig. 1) evolved as a consequence of the large-
scale orogen-parallel extension and related transtensional tec-
tonics that accompanied the anti-clockwise rotation of the
Apennine belt and lithospheric stretching in the central
Tyrrhenian Basin (Sacchi et al. 1994; Ferranti et al. 1996;
D’Argenio et al. 2004).
As a consequence, the Campania segment of the peri-
Tyrrhenian structural belt displays the characteristics of a pas-
sive continental margin, where Quaternary orogen-parallel
extension caused the formation of half-graben systems (Gulf
of Gaeta, Bay of Naples, Bay of Salerno and intervening
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structural highs (e.g. Sorrento Peninsula, Mt Massico),
trending perpendicularly to the main axis of the Apennine
thrust belt (Mariani & Prato 1988; Sacchi et al. 1994; Milia
& Torrente 1999; Aiello et al. 2000).
Off the Campania coasts the peri-Tyrrhenian basins often
form the seaward extension of the coastal plains, whose for-
mation was controlled by extensional tectonics during the
Plio-Quaternary (Mariani & Prato 1988; Brancaccio et al.
1991). Their tectono-sedimentary evolution is connected
with the Neogene evolution of the Apenninic chain (Royden
et al. 1987; Patacca & Scandone 1989). In particular, the de-
formational history of the peri-Tyrrhenian basins is charac-
terized by alternating compressional and extensional tectonic
phases during Plio-Quaternary times (Bartole 1984; Argnani
& Trincardi 1990; Agate et al. 1993; Sacchi et al. 1994).
The Neogene evolution of the south-eastern peri-Tyrrhe-
nian basins was controlled by large-scale extensional tecton-
ics, responsible for the thinning of the western sectors of the
southern Apenninic chain and dating back to the Late Mio-
cene. Thinning due to extension was not homogeneously
distributed along the overthrust belt, but rather localized in
discrete hyper-extension domains (Ferranti et al. 1996),
where the thrust pile was locally reduced to about one half of
its original thickness.
Modes of extension along the peri-Tyrrhenian basins are
often characterized by listric normal faults and associated
antithetic faults, which generated SW-NE trending half-gra-
ben systems along the Tyrrhenian Basin-southern Apennines
system. Most of them extend landward to the E-NE. This
causes a typical coastal landscape made of alternating trans-
versal mountain ridges and intervening coastal plains.
In the Campania Region Quaternary basin fillings overlie
submerged “internal” (western) tectonic structures of the Apen-
ninic chain, resulting from the seawards extension of the tecton-
ic units cropping out in the coastal belt of the southern
Apennines (D’Argenio et al. 1973: fig. 1). These units form the
acoustic basement of the coastal basins and are composed either
of terrigenous-shaly basinal sequences or of thick platform and
basinal Mesozoic-Cenozoic carbonates (Fig. 1). Extensional
tectonics accompanying the uplift of the southern Apennines
begin in the Early Pliocene and continue up to the Middle—Late
Pleistocene, playing a major role in controlling the present-day
physiography of the Campania Region. Indeed, Quaternary ma-
rine and continental sediments of the Campania coastal plains
reach a thickness of up to 3000 m in the Volturno Plain and of
1500 m in the Sele Plain (Ortolani & Torre 1981).
NW-SE, NE-SW and E trending post-orogenic structures
(mainly extensional faults) have been previously recognized
under the sea near the Campania Region (Bartole et al. 1983).
While the Apenninic (NW-SE) trending structures character-
ize the continental slope areas between the Pontine Islands and
the Cilento Promontory, the Anti-Apenninic (NE-SW) ones
often occur under the sea near the Bay of Salerno and the
structural high of the Sorrento Peninsula.
In turn, the Quaternary extension along the Campania seg-
ment of the Southern Apennine—Eastern Tyrrhenian hinge
zone caused the onset of intense volcanism. It was responsi-
ble for the creation of both single large volcanoes (Roc-
camonfina and Somma-Vesuvius – Principe et al. 1987:
fig. 1) and volcanic complexes (Ischia, Procida and Phlegrean
Fields – Rosi & Sbrana 1987: fig. 1). In the Phlegrean area
a thermo-metamorphic basement about 1500 m deep has been
inferred (Rosi & Sbrana 1987), whereas in the Volturno Plain
the “Villa-Literno” 1 and “Parete” 1 wells drilled into thick
basaltic and andesitic lavas (Ortolani & Aprile 1978).
Morpho-bathymetry and sea bottom instability of
the Naples bay canyons
An extensive, high resolution bathymetric survey of the
continental shelf/slope system of Campania, Southern Italy
Fig. 1. Tectonic sketch map of western
Campania Apennines (modified after
D’Argenio et al. 2004). 1 – Shallow-
water carbonate and deep basinal units
(Mesozoic); 2 – Piggy-back siliciclastic
units (Tertiary); 3 – Pyroclastic depos-
its and lavas (Quaternary); 4 – Conti-
nental and marine deposits (Quaternary);
5 – Normal fault; 6 – Detachment
faults (barbs indicate downthrown side).
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has recently been carried out. The relative bathymetric data
were acquired during the years 1997 and 2002, using Multi-
beam systems with an average vertical resolution of 0.25 %
water depth and a position accuracy of
10 m. The survey
data were successively merged with a Digital Terrain Model
(DTM) created from topographic maps of the Bay of Naples
onshore coastal area and islands, to produce a Digital Eleva-
tion Model (DEM) based on a homogeneous grid with cell-
spacing of 20 m (D’Argenio et al. 2004: fig. 2).
The shaded relief map has provided new, detailed infor-
mation on the morphology of the Campania coasts. This seg-
ment of the Italian continental margin displays evidence of
the latest Neogene-Quaternary interplay between tectonics
and volcanism, as well as of the depositional processes
largely developing as a consequence of frequent and large
volcano-sedimentary supply. The major morphological fea-
tures revealed by the 3D digital maps are: i) the system of
marine canyons (Dohrn and Magnaghi) that cut the continen-
tal slope at a depth between 250 m and 1100 m; ii) the conti-
nental slope system of the Ischia volcanic structure (Chiocci &
de Alteriis 2006; Aiello et al. 2009a); iii) the onshore and off-
shore volcanoes of the Campi Flegrei; iv) the rugged seafloor
area of the outer shelf of the city of Naples (Banco della Mon-
tagna – Sacchi et al. 2000; D’Argenio et al. 2004); v) the de-
bris flow/avalanche deposits on the inner continental shelf off
Mt Vesuvius (Milia et al. 1998, 2008), laterally grading into
the “Torre del Greco” volcanic structure (Aiello et al. 2010).
The DEM of the Bay of Naples, representing the base of
the geological and morpho-bathymetric interpretation, has a
20 20 m cell and has been based on the integration of dif-
ferent grids. This cell has resulted adequate in detecting the
most prominent topographic and bathymetric features of the
coastal zone larger than a few tens of meters.
Despite the great number of geological and volcanological
studies on the Gulf of Naples, among which Latmiral et al.
(1971), Finetti & Morelli (1973), Cinque et al. (1997),
Pescatore et al. (1984), Fusi et al. (1991), Milia (1996), Milia
et al. (1998, 2008), Aiello et al. (2001, 2004, 2005, 2009a,b,
2010), Bruno et al. (2003), the morpho-bathymetry and the
submarine gravity instabilities of the Dohrn and Magnaghi
Canyons have not been investigated in detail, nor have the
areas of incipient submarine sliding in the surrounding of the
canyons even been accurately defined.
The Dohrn Canyon formation was triggered off by the tec-
tonic uplift of both the outer shelf and the fluvial valley
mouths, during periods of eustatic fall of sea level (Milia
2000). During the Late Quaternary the Bay of Naples continen-
tal slope was characterized by slumping and canyon formation
and therefore it may be considered to represent an erosional
slope-system (Ross et al. 1994; Galloway 1998). The geologi-
cal conditions for the formation of the Dohrn Canyon appear
to be incompatible with models based on oversteepening, high
sediment supply, sea-level rise and retrogressive slumping.
The Dohrn Canyon developed along a central slope showing
low gradients and the landward rotation of the platform block
resulted in a substantial decrease of the slope. Moreover, the
canyon wall cuts the main body of the slumps, whereas the
most prominent scars show no correlation with the canyon
walls. So the Dohrn Canyon formation was controlled by a
sea-level eustatic fall, inducing a seaward migration of the riv-
er systems of the Late Pleistocene and the formation of the
valleys, coupled with a fault block rotation, responsible for the
outer shelf uplift (Milia 2000).
Based on the interpretation of Multibeam bathymetry we
have outlined a schematic geomorphological map of the
Dohrn Canyon and of the surrounding continental slope,
which shows, in particular, the slide scars and the submarine
gravity instability areas (Fig. 2).
The main morpho-structures of the canyon system consist
of volcanic structural highs, relic morphologies of the Middle-
Late Pleistocene continental shelf, turbiditic slope fans and
Mesozoic carbonate structural highs. Some morphological lin-
eaments, such as the canyon’s walls, the shelf break, the slope
of the “Ammontatura” paleo-canyon, the slide scars and the
canyon’s axis have also been represented (Fig. 2).
The Dohrn Canyon’s width ranges from a few hundred
meters to more than 1 km, its depth from 250 m at the shelf
edge to some 1300 m at the merging with the bathyal plain;
the dip of its walls attains some 35° in the steepest sectors.
This canyon starts with two major curved branches. The
western branch merges into the shelf through a 1.5 km wide
and 20—40 m deep channel (“Ammontatura” channel), char-
acterized by a flat bottom and asymmetrical levees, located
along the —200 m isobath and by a sinuous shape in plan
view. The Dohrn eastern branch shows a meandering trend
and starts from the shelf break of the Sorrento Peninsula, lo-
cated along the —120 m isobath. The Dohrn western branch
is broader than the eastern one and more deeply incised; the
two branches form a typical Y-structure.
The abrupt termination of the “Ammontatura” shallow
channel against the Nisida volcanic bank, whose growth was
older or contemporaneous with the eruption of the volcanic
deposits of the NYT (Neapolitan Yellow Tuff – Scarpati et
al. 1993) suggests that the Dohrn canyon system is older than
the volcanic deposits of the NYT, which forms the main basis
of the city of Naples. This implies that most part of the canyon
system activity was probably older than 11—12 ka B.P., age of
the NYT deposits in the city of Naples (Di Girolamo et al.
1984; Rosi & Sbrana 1987).
The Magnaghi Canyon shows a triple incised head and is
pervasively affected by small-scale slope instabilities. It runs
parallel to the southern flanks of the Procida and Ischia Is-
lands and then is buried below the Ischia Debris Avalanche
(Chiocci & de Alteriis 2006; Aiello et al. 2009a). Three main
tributary channels join basinwards into the main axis. Ero-
sion and transport of volcanoclastics in the western sector of
the gulf, near the Ischia and Procida Islands, developed
along the Magnaghi Canyon axis and it appears unrelated to
the present fluvial drainage system on land.
As already noted, the Bay of Naples canyons start from the
shelf break near the Phlegrean Fields volcanic district, located
along the —140 m isobath. Their trends are controlled by the
main morpho-structures of the bay: the “Banco di Fuori”
structural high, bounding southwards the whole canyon sys-
tem and the Capri Island structural high, bounding eastwards
the Dohrn Canyon, near its confluence with the bathyal plain.
Both the Magnaghi Canyon and the Dohrn western branch
show morphological evidence of retreat of the canyon’s head.
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Based on the interpretation of the Multibeam bathymetry the
main features that we interpret as slide scars are located (Fig. 2):
a) on the head of the Dohrn western branch, showing a
double retrogressive head, controlled by extensive subma-
rine erosion;
b) on the western slope of the Dohrn western branch (Fig. 3),
at its boundary with the eastern flank of the Banco di Fuori
morpho-structural high (here a set of coalescent, large slide-
scars, not related to the canyon’s thalweg, may be observed);
c) on the continental slope, north of the Capri structural
high, where large scars are suggested by the trending of the
isobaths next to the Dohrn Canyon thalweg.
Here the canyon system is characterized by several terrac-
es and three rectilinear gullies converge into the canyon from
the northern slope of the Capri Island. An acoustic basement,
probably composed of Mesozoic-Cenozoic carbonate rocks
almost reach the sea bottom, under a thin drape of Holocene
sediments.
Fig. 2. Morpho-bathymetry of the Bay of Naples canyons and gravity instability map. Note that chief submarine instability areas are located
at the Dohrn Canyon’s head, on the slope surrounding the western Dohrn branch, on the slope southwards of the Magnaghi Canyon and on
the north-eastern slope of the Banco di Fuori structural high. Figures on the side refer to kilometric coordinates.
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The geomorphological interpretation and the analysis of the
canyon morphometric parameters suggest that the submarine
instabilities of the canyon system are located (Fig. 2):
a) around the Dohrn western branch, from the canyon’s
head to the middle of the branch, north of the “Banco di Fuo-
ri” morpho-structural high;
b) on the continental slope, southwards of the Magnaghi
Canyon, where two large areas of instability, not connected
with the canyon’s thalweg, may be observed;
c) on the north-western slope of the “Banco di Fuori” mor-
pho-structural high, where the concave trending of the iso-
baths suggests the occurrence of an incipient and/or fossil
slide scar.
No slumped masses are preserved in the main thalweg,
suggesting a probable activity of low-density turbidity cur-
rents during the Late Quaternary evolution of the canyon.
Large isolated remnants, showing average dimensions of
300 400 m across are present on the canyon floor which, in
its upper part, is scoured by a minor meandering channel.
These rounded morphologies are interpreted as relic struc-
tures, probably due to a selective erosion acting along the
canyon’s valley. Moreover, terrace rims, located respectively
at —340 m and —300 m of water depth, suggest at least two
phases in the activity and retreat of the canyon head.
A relative abundance of the V-shaped erosional profiles
has been observed in both the branches of the Dohrn Can-
yon. The flat-bottomed valley depositional morphologies,
suggesting recent phases of canyon filling, occur mainly in
the wider, southernmost part of the Dohrn western branch
and at the confluence of the Dohrn northern and southern
branches.
The drainage system of the canyons is composed of a
dense network of tributary channels, controlling the over-
flow of sediments in the surrounding areas of the continental
slope. Two main tributary channels originate from the shelf
break off the Phlegrean submarine volcanic banks, located
along the 140 m isobath and run along the continental slope
between the Dohrn and the Magnaghi Canyons, giving rise
to channel-lobe systems (Fig. 2). A complex system of tribu-
tary channels, located at water depths ranging from —200 m
and —500 meters, fed the Dohrn southern branch, starting
from the shelf break off the Sorrento Peninsula and it ap-
pears partly fault-controlled. This interpretation is suggested
by the rectilinear shape in plan view of the southernmost
four channels. A system of lobes, genetically linked with
some of these channels, has been recognized on a morpho-
logical terrace located at water depths of 340 m. Moreover
fossil tributary channels hung over the main branches testify
stages of rapid re-incision, switching off the feeding from
lateral sources and forming suspended valleys.
In conclusion, several submarine slides and scars are evi-
dent on the canyon’s walls, especially along the western
flank of the Dohrn northern branch and on the continental
slope as well. The north-western branch of the Dohrn Can-
yon is affected by instability, with an incipient slump caus-
ing a broad depression, 200—300 m across and away from
the canyon’s edge, and a semi-circular scar on the canyon
walls, showing lateral coalescence and defining a large area
Fig. 3. Detailed bathymetric map of the canyons showing the location of modelled submarine landslide (arrow).
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where (see also nomenclature below):
µ is the frequency-dispersion parameter (h
0
/l
0
), i.e. when
the ratio of water depth to wavelength is small. In general the
guideline for dispersive properties is that the depth-integrat-
ed equations are valid for wavelengths greater than two wa-
ter depths;
ur
=
)
,
( v
u
is the horizontal velocity vector;
is the horizontal gradient vector;
p is the depth-dependent pressure;
is the nonlinearity parameter (a/h
0
), i.e. when a<<h
0
, the
nonlinearity is not important (the initial wave amplitude is rela-
tivity small compared to the wavelength and the water depth).
Fig. 5 shows the parameters used in the algorithm imple-
mentation.
In many cases, the seafloor displacement is small with respect
to the local water depth. Since the free-surface displacement is
directly proportional to the seafloor displacement, namely
D(
)=D( h).
The boundary conditions applied are:
On the free surface z=
x y, t), the usual kinematic and
dynamic boundary conditions, considering the depth integra-
tion interval between z=[—h,
], we set:
on (4.4)
p=0,
where p is water pressure.
Along the seafloor where z=—h, the kinematic boundary
condition requires
on z=—h (4.5)
Integrating from z=—h, to z=
, the depth-integrated
continuity equation, we obtained:
of instability, located westward of the north-western slope of
the “Banco di Fuori” morpho-structural high (Fig. 2).
A bathymetric profile has been constructed in correspon-
dence to the scars involving the Dohrn western branch in or-
der to give quantitative constraints to the numerical
modelling. A detachment area, about 415 m across occurs at
water depths ranging between —250 m and —370 m. Also de-
bris accumulation develops in water depths ranging from
—380 m and —450 m, while the junction with the foot of the
thalweg occurs, at water depths of about —430 m (Fig. 4).
Methods of analysis and modelling
In this paragraph we discuss the problems of the possible
tsunami generation and characteristics, as we may infer from
the above analytical description of the Bay of Naples canyon
system. We apply here a mathematical model already pro-
posed by Lynett et al. (2002) in which the generation and
propagation of tsunamis is reconstructed from ancient sub-
marine landslides. In such a model we assume that there is a
weak frequency dispersion, which means that the ratio of
water depth to wavelength is small or <<1. In general, for
dispersive properties the depth-integrated equations are valid
only for wavelengths greater than two times the water depth,
whereas the depth-averaged model is valid for lengths great-
er than five times the water depth (e.g. Nwogu 1993). In
Lynett et al. (2002) the full nonlinear effect is included,
namely the ratio of wave amplitude and water depth is order
one, and therefore, this model is more general as compared to
other models (Liu & Earickson 1983) where the Boussinesq
approximation was used.
The motion can be described by Euler’s equations:
Fig. 4. (a) Model scheme referred to the parameters
utilized in this paper and evolution of submarine
slope surface shape during landslide movement.
The detachment area relative to the slide and the de-
bris accumulation area, covering a total distance of
620 m, have also been represented. (b) Detailed
bathymetric map of the area and slice location
(A—B) of the ancient marine landslide.
(4.3)
;
1
(4.2)
;
(4.1)
;
0
2
2
2
2
2
z
z
t
z
t
z
p
ww
w
u
w
p
u
w
u
u
u
w
u
r
r
r
r
r
r
⎟⎟
⎠
⎞
⎜⎜
⎝
⎛
y
x
,
u
w
t
r
2
,
z
0
2
2
t
h
h
u
w
r
;
0
1
⎥⎦
⎤
⎢⎣
⎡
∫
t
h
H
dz
ur
(4.1)
(4.2)
(4.3)
(4.6)
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where H =
h .
After integral resolution of the two-dimensional governing
equation, we applied the finite difference algorithm to solve
the general model equation (Lynett et al. 2002). In their pa-
per Lynett et al. (2002) developed an algorithm for the gen-
eral two-horizontal-dimension problem analogously to Wei
& Kirby (1995) and to Wei et al. (1995). The difference be-
tween the two models is that in Wei et al. (1995) terms due
to a time-dependent water depth and some nonlinear-disper-
sive terms have been added, while in this study we use an
impulsive bottom movement in a constant water depth.
The previous governing equation was approximated onto a
two-dimensional horizontal plane. Some assumptions are
listed below to resolve the approximate two-dimensional
governing equation (Lynett et al. 2002):
1. only one-horizontal-dimension is examined;
2. nonlinearity is assumed so is small;
3. frequency dispersion is weak so µ
2
is small;
4. all spatial derivatives are differenced to fourth-order in
numerical analysis.
Fig. 5. Schematic representation of the geometrical parameters used in
wave-run up computation. h
0
– characteristic water depth and vertical
length scale; l
0
– characteristic length of the submarine slide region
and horizontal length scale; l
0
/(gh
0
)
1/2
– time scale; a – char-
acteristic wave amplitude and scale of the wave motion.
Fig. 6. Water wave amplitude vs. time-series located in x/h = 0 (horizontal coordinates of the midpoint of the seafloor movement). The rapid
decadence of the amplitude after 8 s is evident. Note that the amplitude wave run-up expressed in terms of depth of sea floor percentage
ranges from 0 to 2.5 %. In absolute terms the wave height amplitude corresponds to 5—6 m.
Finally, the numerical analysis was applied resolving two-
dimensional equation so obtaining the relative run-up.
The bottom movement, consisting of a length l
0
= 620 m
(Fig. 5), pushed the water masses vertically upwards. The
change in depth for this experiment is about 0.1 ( h/h
0
), and
therefore nonlinear effects should play a small role near the
source region, and 20 times the water depth from the edge of
the source region. The landslide is located near the Dohrn
Canyon head (Fig. 3) and we assume that the landslide may
move rapidly.
To analyse this model we have introduced the characteris-
tic water depth h
0
, as the vertical length-scale, the character-
istic length of the submarine slide region l
0,
as the horizontal
length-scale, l
0
/ (gh
0
)
1/2
as the time-scale, and the character-
istic wave amplitude a as the scale of wave motion.
Fig. 6 shows the results of the analysis in terms of ampli-
tude vs. time-series at x /h = 0. It is possible to notice that the
amplitude wave run-up expressed in terms of depth of seaf-
loor percentage, ranges from 0 to 2.5 %. In absolute terms
the wave height amplitude corresponds to 5—6 m.
Discussion and conclusion
Submarine landslides play a fundamental role in originat-
ing tsunamis, especially near the coast. Our experiment in
the Bay of Naples could be used as example in the areas
where there is a high probability for these events to occur
(Tinti et al. 2003). The idea is to produce an offshore hazard
map delimiting both the potential tsunamis areas (located
near the instability zone) and the influence zone of the water
wave.
The morphometric analysis of the Dohrn Canyon slope
provides insight into tsunami hazard, including the locations
of mass movements, the size of mass failures, their relative
importance for the structure of a given margin, and the po-
tential for landslide-generated tsunami hazard. We do not
have enough evidence to consider all these detachment areas
located on the Dohrn Canyon edges as generated by land-
slides with impulsive character, or if there has been an evo-
lution over time controlled by small detachments, not signif-
icant if compared to the potential needed to generate
anomalous waves. The nature of the materials that character-
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ize the area is both volcanic (Campanian Ignimbrite) and
sedimentary. Therefore we deal with a non-coherent material
that, together with the presence of the active volcanoes
(Somma-Vesuvius and Phlegrean Fields), need to be analy-
sed with regard to its ability to trigger landslides.
The tsunami predictions according to Booth et al. (1993)
have to be related not so much to the slope gradient alone,
but instead to sedimentation, erosion, local geology, fluid
overpressure and regional seismicity as complex causative
triggers. This whole complex is critical in determining land-
slide location and ultimately size of the derived tsunami,
considering that the continental shelf of the Gulf of Naples
is dipping in average 6° and has a width of 20—22 km, ex-
tending for 560 km
2
, while the continental slope dips up to
45°. Our study suggests that the tsunami hazard is higher on
the canyon margin: in fact, Fig. 2 shows several slide scars
and large submarine instability areas near to canyon borders.
In conclusion we observe that the morphological evolution
of the analysed area depends on complex systems where vol-
canism, sedimentation and tectonics affect the coast and the
marine bottoms, that show the potential to develop slope in-
stability, even though high urbanization has impacted signif-
icantly on the sedimentation, reducing the accumulation rate
of materials potentially prone to slide.
Due to the lack of more detailed morpho-bathymetric stud-
ies as well as of innovative methods for hazard evaluation in
coastal areas, the balance of these opposite trends is difficult
to assess. However we stress the importance of the analysis
of submarine gravity instability, mainly for its implications
in terms of geo-hazard related to landslides as the cause of
tsunamis. Much remains to be done to reach an accurate un-
derstanding of these problems.
Nomenclature
wave amplitude
displacement function
gravity
characteristic water depth or baseline water depth, function
of space
water depth profile, function of space and time
total water depth (
h)
characteristic horizontal length-scale of the submarine slide
depth-dependent pressure
time
depth-dependent components of velocity in (x, y, z)
horizontal velocity vector, (u, v)
Cartesian coordinates
characteristic, or maximum, charge in water depth due to
seafloor motion
nonlinearity parameter (a/ho)
frequency-dispersion parameter (ho/lo)
free-surface displacement
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wave amplitude
displacement function
gravity
characteristic water depth or baseline water depth,
function of space
water depth profile, function of space and time
total water depth (
h)
characteristic horizontal length-scale of the subma-
rine slide
depth-dependent pressure
time
depth-dependent components of velocity in (x, y, z)
horizontal velocity vector, (u, v)
Cartesian coordinates
characteristic, or maximum, charge in water depth
due to seafloor motion
nonlinearity parameter (a/ho)
frequency-dispersion parameter (ho/lo)
free surface displacement
a
D
g
h
0
h
H
l
0
p
t
u, v, w
u
x, y, z
h
µ
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