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3D numerical deformation model of the intrusive event forerunning the 2001 Etna eruption
Gilda Currenti, Ciro del Negro, Gaetana Ganci, Danila Scandura
To cite this version:
Gilda Currenti, Ciro del Negro, Gaetana Ganci, Danila Scandura. 3D numerical deformation model of the intrusive event forerunning the 2001 Etna eruption. Physics of the Earth and Planetary Interiors, Elsevier, 2008, 168 (1-2), pp.88. �10.1016/j.pepi.2008.05.004�. �hal-00532148�
Accepted Manuscript
Title: 3D numerical deformation model of the intrusive event forerunning the 2001 Etna eruption
Authors: Gilda Currenti, Ciro Del Negro, Gaetana Ganci, Danila Scandura
PII: S0031-9201(08)00089-7
DOI: doi:10.1016/j.pepi.2008.05.004
Reference: PEPI 4940
To appear in:
Physics of the Earth and Planetary InteriorsReceived date: 3-8-2007
Revised date: 5-5-2008 Accepted date: 7-5-2008
Please cite this article as: Currenti, G., Del Negro, C., Ganci, G., Scandura, D., 3D numerical deformation model of the intrusive event forerunning the 2001 Etna eruption,
Physics of the Earth and Planetary Interiors (2007), doi:10.1016/j.pepi.2008.05.004This is a PDF file of an unedited manuscript that has been accepted for publication.
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Accepted Manuscript
3D NUMERICAL DEFORMATION MODEL OF THE INTRUSIVE EVENT 1
FORERUNNING THE 2001 ETNA ERUPTION 2
3
Gilda Currenti1, Ciro Del Negro1, Gaetana Ganci1,2, Danila Scandura1,3 4
5
1Istituto Nazionale di Geofisica e Vulcanologia, Sezione di Catania, Italy 6
2Dipartimento di Ingegneria Elettrica Elettronica e dei Sistemi, Università di Catania, Italy 7
3Dipartimento di Matematica e Informatica, Università di Catania, Italy 8
9
Abstract 10
3D finite elements models were carried out in order to evaluate the ground deformation produced 11
by the dike intrusion occurred at Etna volcano in the 2001. The Finite Element Method (FEM) 12
allows for considering the medium heterogeneity and the real topography of the volcano. Firstly, 13
we validated the method in a homogeneous elastic half-space and compared the results with those 14
obtained from analytical dislocation models. We performed a convergence analysis to quantify the 15
discretization errors, which are sensitive to the size and quality of the mesh elements and can 16
cause inaccurate numerical solutions. Secondly, several numerical models were conducted to 17
appreciate how the complex distribution of elastic medium parameters and the topography make 18
the numerical results differ from the simple analytical solutions. The numerical model, which 19
account for the real topography of Etna volcano and medium heterogeneity, well match the ground 20
deformation observed at the GPS stations between 11 and 16 July 2001. It appears that 21
topography and heterogeneities provide more details about the ground deformation near the 22
summit crater area that are missed when homogeneous half-space models are used. However, 23
only few discrepancies between the analytical and the numerical models are observed at the GPS 24
stations, which coarsely sample the volcanic edifice far away from the summit craters.
25 26
Key words: finite-element method, ground deformation, medium heterogeneity, Etna volcano 27
28
Introduction 29
Geodetic observations play an important role for the monitoring of the volcanic activity and for the 30
quantitative evaluation of the geophysical processes preceding and accompanying volcanic unrest 31
(Bonaccorso and Davis, 2004). Fundamental insight about volume changes in the magma 32
reservoir and the dynamics of dike intrusion processes is generally obtained using ground 33
deformation (Voight et al.1998; Battaglia et al. 2003; Murase et al. 2006). However, an accurate 34
interpretation of deformation signals is necessary for improving the monitoring of active volcanoes 35
as well as developing a better understanding of the pre-eruptive mechanisms that produce them.
36
Volcanic processes are complex geophysical systems and it is difficult to derive analytical 37
deformation models, unless important simplifications and approximations are taken into account 38
(McTigue, 1986; Carbone et al., 2007). The simplest way to model the inflation or deflation of a 39
Accepted Manuscript
magma chamber at depth is a point dilatation source embedded in a homogeneous elastic half- 1
space (Mogi, 1958), which is quite appropriate to approximate spherical over-pressured source 2
when the radius is far smaller than its depth. Finite extended sources have been also analyzed and 3
spherical and ellipsoidal models have been devised to better model pressurized magma chamber 4
(McTigue, 1986; Davis, 1986; Battaglia & Segall, 2004; Yang and Davis, 1986). Instead, dike 5
intrusions and eruptive fissures are usually represented by an opening crack. Tensile dislocation 6
theory has been successfully applied to model rectangular shaped intrusion (Okada, 1992).
7
All these analytical elastic models are quite attractive because of their computational feasibility 8
(Currenti et al., 2007a). However, investigations on the effect of a non-uniform elastic medium are 9
indispensable for describing more realistic models (Currenti et al., 2007b). For the static elastic 10
deformation in a multilayered half-space, there exist a number of semi-analytical solutions 11
(Bonafede et al., 2002; Wang et al., 2003). Moreover, volcanic areas are usually characterized by 12
consistent topographic relief that is responsible for significant effects (Williams & Wadge, 1998).
13
Several studies have been carried out by means of numerical methods to assess the effect of 14
topography on ground deformation generated by magmatic pressurized sources in volcanic areas 15
(Cayol & Cornet, 1998; Williams & Wadge, 2000).
16
In the present work, we applied the 3D FEM (Finite Element Method) to asses the role that medium 17
heterogeneity and topography effects may play in modelling intrusive events at Etna volcano. We 18
focused our attention on modelling the intrusive events forerunning the 2001 eruption. Firstly, the 19
numerical results were compared to the analytical ones computed using the dislocation theory 20
(e.g., Okada, 1992). We assumed a homogenous, isotropic and half-space medium, in order to 21
validate the results of the numerical model with respect to the mesh resolution that strongly affects 22
the solution accuracy. Secondly, a 3D analysis was performed, by introducing the real topography 23
of Mt Etna, in order to examine the effect of the topography on the deformation field. In addition to 24
the topography, the effects of the elastic medium heterogeneities were included considering a 3D 25
complex distribution of medium properties in terms of Young modulus and Poisson ratio inferred 26
from seismic tomography investigations.
27 28
Numerical Model 29
The definition of a FEM problem requires to set up boundary conditions, optimal size of domain, 30
meshing, and the type of the elements that are not known a priori. Therefore, a robust preliminary 31
set-up is needed to obtain realistic results. We carried out the computations with the FE software 32
COMSOL (COMSOL 2004). In order to validate the size of domain and the mesh resolution in the 33
FEM model, we performed several computations and compared the numerical deformation fields 34
with the analytical solution from Okada’s dislocation theory (1992).
35
We considered a 3D FEM model reproducing a rectangular dislocation source in a homogeneous 36
and isotropic half-space. The geometry of the intrusion source is reported in Table I. We assumed 37
Accepted Manuscript
stress-free boundary condition at the upper surface, and zero displacement values at bottom and 1
lateral boundaries. The dislocation source is modelled as a rectangular discontinuity surface by 2
means of “pair elements”. The elements are added in pairs along the surface rupture, where in one 3
element the dislocation +U and in the other −U is assigned. A non null homogeneous dislocation 4
over the rupture area is imposed and an “identity pair” condition along the remaining surface is 5
enforced to assure the continuity of deformation fields on the volume surrounding the dislocation 6
source. The medium is assumed to be elastic with Lame’s coefficients λ=µ, namely Poisson 7
ratio ν =0.25, and Young modulus of 30 GPa. A computational domain of 50x50x35 km is 8
meshed with tetrahedral elements.
9
In the finite element analysis a critical step is the meshing of the computational domain. The 10
number of elements of the mesh largely influences the accuracy of the solution. Starting from a 11
coarse mesh, we incrementally refined the meshed domain increasing the number of nodes. We 12
examined the accuracy of the solution in terms of discretization error due to the meshing procedure 13
to test how the mesh resolution can affect the numerical solution. A convergence analysis was 14
performed to quantify the discretization errors caused by the mesh resolution. Eight different 15
meshes were constructed by refining the domain. The number of nodes was increased to improve 16
the mesh resolution and the solution accuracy (Table II). Besides the number of nodes, also the 17
mesh quality should be taken into account to assure an accurate solution. The mesh not only must 18
properly describe the geometrical boundaries, but it must not have degenerated elements that 19
make the numerical solution instable. Therefore, we defined a factor to track the mesh-quality 20
among the several meshes. For tetrahedral elements, more the element approaches an equilateral 21
tetrahedron, more the numerical solution is stable and accurate (Field, 2000; Edelsbrunner, 2001).
22
For each element in the mesh we evaluated its quality with respect to the equilateral tetrahedron 23
as:
24
3 2
)
(A B C D
f V
q= + + + 25 (1)
where V denotes the volume of the tetrahedron, A, B , C, and D are the areas of its faces and 26
3
=216
f is a normalizing coefficient ensuring that the quality of an equilateral tetrahedron is 27
equal to 1. The quality of the worst elements for each mesh is reported in Tab. II. In all the 28
computations the minimum mesh quality was higher than 0.2.
29
To quantify the accuracy of the numerical solutions, a mean misfit function with respect the 30
analytical solution is defined as:
31
∑
=
−
=
∆ N
i
AN i FE
i U N
U U
1
/ )
( (2)
32
Accepted Manuscript
where UiFE is the computed deformation at the i-th node for the numerical model, UiAN is the 1
corresponding result for the analytical model, and N is the total number of nodes in the meshed 2
domain. To provide a reference for the quality of the fit, we have normalized each mean misfit 3
value by the average magnitude of the deformation field:
4
N U U
M
N
i AN
i /
)
(
∑
=
=
1
5 (3)
The misfit function δm =∆
(
U) /
M(
U),
m=x,
y,
z, computed for each deformation component, 6decreases quickly as the mesh quality is improved (Fig. 1). The displacements due to strike-slip, 7
tensile, and thrust faulting in a homogeneous medium are compared to Okada’s dislocation 8
models. The results from the FEM models are generally consistent with those from the dislocation 9
model in a homogeneous half-space as the mesh reaches a number of about 15000 elements. The 10
ratio ∆(U)/M(U) is less than 0.1 for all the displacement components and no significant 11
improvements are obtained when using finer meshes. Therefore, the numerical results are found to 12
be in nearly perfect agreement with the analytical solutions.
13
The domain was proved to be big enough to avoid numerical artefacts in the solution due to the 14
finite boundary condition. The external boundaries of the domain depend on the extent of the 15
displacement components, which is especially related to the depth of the source. We performed 16
several tests for a tensile source, whose geometric parameters as the same as before (Tab. I), and 17
the depth is varied from 1 to 4 km. As the depth of the tensile source increases the deformation 18
components show a greater spatial extent. The deformation field decays to 10% of the maximum 19
value within 10 km from the source when the source is at 1 km depth, within 33 km when the 20
tensile source is at 4 km. The source depth controls the shape and the extent of the deformation 21
field, and so regulates also the computational domain size. As a rule of thumb, the domain size 22
must be at least twice the deformation field extent, or in other words about 40 times the depth of 23
the source to obtain an accurate numerical solution.
24 25
2001 Etna Eruption 26
The numerical modelling procedure is applied to study the ground deformation observed during the 27
Etna 2001 eruption. Late night on 12 July 2001 an intense seismic swarm preceded and 28
accompanied the opening of a system of fractures at the base of the South East (SE) crater and 29
continued without any fall in energy release till the late night of July 16. Some 800 earthquakes 30
were recorded by the early morning of July 13, from a total of 2645 occurring between 12 and 18 31
July (Patanè et al., 2002). In concomitance with the seismic crisis, marked ground deformation (50 32
to 120 mm) were recorded at the GPS permanent stations. Tilt variations were very small in the 33
northern flank, of few µrad in the western flank, and much more marked at stations close to the 34
Accepted Manuscript
fracture field (Bonaccorso et al., 2002). The deformation was mainly cumulated during the late 1
night of July 12 and the following two days. Bonaccorso et al. (2002) modelled the ground 2
deformation changes recorded in the days before the eruption onset (between July 11 and 16) by 3
means of analytical solutions. The tilt and GPS data inversion indicated the response to a tensile 4
mechanism with an opening dislocation of ca. 3.5 m that evidenced an intrusion in the volcano 5
edifice along a ca. N-S direction (Bonaccorso et al., 2002). The location of the tensile source lies 6
within the zone of the seismic swarm that occurred during the magma ascent.
7
Although the analytical model provided an acceptable representation of the dyke intrusion occurred 8
on the south flank, it is not able to justify all the details. The simplified assumption of elastic half- 9
space medium disregards effects caused by the topographic relief and the presence of medium 10
heterogeneity, while they could play a role in the modelling procedure. To evaluate how the 11
topography and medium heterogeneity could affect the computed ground deformation, we carried 12
out numerical models including the real topography of the volcano edifice and the medium 13
heterogeneity inferred from seismic tomography study. In the numerical computations we used the 14
source geometry (Tab. III) obtained by the analytical inversion model from Bonaccorso et al.
15
(2002). We evaluate three numerical models in which we considered: (i) an homogeneous elastic 16
medium with a flat surface, (ii) an homogeneous elastic medium with the real topography of Mt 17
Etna, and (iii) an elastic heterogeneous medium with the real topography relief.
18 19
Flat Topography and Homogeneous Medium 20
We performed a 3D FEM model considering a rectangular tensile dislocation embedded in a 21
homogeneous, isotropic and elastic half-space. The medium is assumed to be elastic and 22
poissonian (λ =µ) with a Young modulus of 30 GPa. This numerical model is equivalent to the 23
Okada’s analytical model. Indeed, all the deformation components well match the analytical ones 24
within the computational error, assuring the validity of the domain size, mesh resolution and 25
boundary conditions used in the numerical computations (Fig. 2).
26 27
Real Topography and Homogeneous Medium 28
To examine the effects of topography on the deformation at Mt Etna, we included in the numerical 29
model the real 3D topography of the volcano using a digital elevation model from the 90 m Shuttle 30
Radar Topography Mission (SRTM) data. The domain was modelled using a total of 15585 31
elements and 3288 nodes. Numerical results highlighted the influence of topography on the 32
deformation field. Ground deformation components differ significantly in shape and amplitude from 33
those of the simple model based on the assumption of a homogeneous half-space medium (Fig.
34
3). The discrepancies between the numerical and analytical models are mainly restricted to the 35
volcano summit area where the topography of Mt Etna is most irregular. The symmetry of the 36
solution observed in the analytical solution is lost in the numerical results since the volcano edifice 37
Accepted Manuscript
is rather asymmetric having a strong mass deficit in the eastern sector with respect to the western 1
sector in correspondence of Valle del Bove. The amplitudes of the deformation components are a 2
little smaller because the effective distance between the source and the ground surface is 3
increased. To evaluate the effect of topography, we compare numerical and analytical solutions for 4
source at different depths. We find out that the topography strongly influences the ground 5
deformation especially when the source is quite shallow. . The residuals, the difference between 6
the analytical and the numerical models, gradually increase as the source became shallower (Fig.
7
4). This discrepancy depends also on the horizontal distance between the observation points and 8
the position of the source. We compute the residuals on different grid sizes centred on the tensile 9
dyke extending: (i) 5x5 km, (ii) 10x10 km, (iii) 20x20 km and (iv) 30x30 km. As the grid extends 10
farther from the dyke the numerical solution converges to the analytical one.
11 12
Real Topography and Heterogeneous Medium 13
Finally, we evaluated the deformation pattern caused by a tensile dislocation embedded in a 14
heterogeneous medium. Instead of using a simple multi-layered crustal rigidity model (Currenti et 15
al., 2006), a complex distribution of elastic medium properties was considered. At each node of the 16
mesh different values of Young modulus and Poisson ratio are assigned on the basis of seismic 17
tomography investigations. In this way, smooth elastic medium heterogeneities, instead of sharp 18
boundary layers, may be included that are effectively most likely for many geological settings.
19
Moreover, this procedure allow to better represent the presence of a high rigidity body centered 20
below the SE sector, inferred from recent seismic tomography studies (Chiarabba et al., 2000). We 21
used P-wave and S-wave seismic velocities to derive the elastic medium parameters. Particularly, 22
the Young modulus was estimated by using the following equation (Kearey and Brooks, 1991):
23
( ν ) ρ +
= 2 V
s21
E
(4)24
where Vs is the seismic shear wave propagation velocity, and ρ the density of the medium which 25
was fixed to 2500 kg/m3. Instead, the values of Poisson ratio were obtained using the equation 26
(Kearey and Brooks, 1991) 27
] 2 ) / ( 2 /[
] 2 ) /
[( 2 − 2 −
= Vp Vs Vp Vs
ν (5)
28
where Vp is the seismic P-wave propagation velocity. On the basis of Eqs. 4 and 5, the Young 29
modulus varies from 11.5 GPa to 133 GPa, while the Poisson ratio is in the 0.12-0.32 range. We 30
considered three different media with: (a) homogeneous Young modulus and heterogeneous 31
Poisson ratio, (b) heterogeneous Young modulus and homogeneous Poisson ratio, and (c) 32
heterogeneous Young modulus and heterogeneous Poisson ratio. In the (a) case where only the 33
Accepted Manuscript
Poisson ratio is heterogeneous, the discrepancy with respect to the homogeneous model is 1
negligible. The models with heterogeneous Young modulus are those that engender higher 2
perturbations in the numerical models considering the inhomogeneity of medium properties.
3
Nevertheless, results compared to homogeneous medium model do not reveal significant 4
differences in pattern and intensity of the deformation field (Fig. 5). The influences of the medium 5
heterogeneity seem to affect mainly the horizontal components (Fig. 5 a-b) with respect to the 6
vertical uplift (Fig. 6 c). The discrepancies are on the order of few centimetres. To better appreciate 7
the discrepancies with respect to the analytical results, we compared the displacement field at the 8
locations of GPS continuously running stations. Figure 6 shows the horizontal component of GPS 9
data together with results achieved by the numerical models. The observed vectors are obtained 10
from the interval comparisons 11-16 July before the eruption onset. Discrepancies of at most a few 11
cm between the numerical and analytical models are observed at the GPS stations (Fig. 6). In fact, 12
almost all the GPS stations are located far enough from the summit area and are not significantly 13
affected by the topography. A more general agreement is achieved with respect to the deformation 14
computed from the analytical model at ERDV station. Nevertheless, a higher discrepancy with 15
respect to the observed deformation still remains at the EMFN station on the eastern flank of the 16
volcano and at EGDF on the northern flank. Both the topography and medium heterogeneity 17
included in the numerical model cannot account for the displacements observed by the EMFN and 18
EGDF geodetic stations.
19
Among the considered models, a good match is achieved by the model including only the 20
topography (cyan arrows in Fig, 6). The residuals, the difference between observed field and 21
numerical solutions, show a standard deviation: of 2.3 cm for the analytical model, of 1.7 cm for the 22
numerical model with topography, and of 2.0 cm for the numerical model including the topography 23
and the medium heterogeneity. When the tomography is included in the numerical model the 24
residual increases. The topography is known with higher resolution and accuracy, whereas the 25
medium heterogeneity is estimated from the 3D velocity model. Three factors can alter this 26
estimate: (i) the low spatial resolution of 3 km in the tomography model by Chiarabba et al. (2000), 27
(ii) the variation of 3D velocity model in the analyzed period, (iii) the difference between the static 28
elastic modulus and the dynamic elastic modulus deduced from the P-wave velocity. Recently, 29
Patanè et al. (2006) obtained new 3D velocity models at higher resolution on Mt Etna, detecting 30
significant variations in the elastic parameters during different volcanic cycles. Further comparisons 31
of different 3D velocity models could show up how the accuracy on medium heterogeneity can 32
affect the numerical solutions.
33
It is worth to note that we adopted source parameters from analytical inversion of GPS data by 34
Bonaccorso et al. (2002). To enhance the match between the data and the numerical solution 35
including topography and medium heterogeneity, we performed an exploration through the 36
parameter space varying the width, the depth and the opening of the dyke. The range of variability 37
Accepted Manuscript
of these parameters was also chosen on the basis of the location of the seismic swarm 1
accompanying the dyke intrusion (Fig. 6 Musumeci et al., 2004). The earthquakes were quite 2
shallow from 1000 m asl to -2000 bsl. Starting from the parameter suggested by the analytical 3
inversion (Bonaccorso et al., 2003), we performed a grid search on the numerical model, which 4
includes both the topography and the medium heterogeneity, varying the width within 2000–3000 5
m, the opening within 2-4 m and the depth within 0-1400 m asl. The residuals show a variation 6
range of 2.5 centimeters with a minimum of 1.9 (Fig. 7). The “best” model, associated with the 7
minimum residual, has an opening of the dyke of 2.5 m, a width of 3000 m, and a depth of 1400 m, 8
that well matches the hypocenters of the seismic events occurred during its intrusion (Fig. 7).
9
However, the best solution does not differ too much with respect to the numerical solution obtained 10
using the dyke parameters inferred from the analytical inversion. Even if the parameters vary in a 11
wide range, the solutions for all the considered models computed at the GPS stations are quite 12
similar. The standard deviation affecting measurements in the horizontal components ranges 13
between 0.2 and 0.5 cm while, over measurements in the vertical component, between 1 and 2 cm 14
(Bonaccorso et al., 2003). Thus, a maximum uncertainty of ± 1 cm and ± 4 cm at the 95%
15
confidence interval can be assumed over the horizontal and vertical component, respectively.
16
Therefore, considering the measurement errors and the computed misfit values, all the numerical 17
models can be assumed as valuable solutions.
18
We also computed the sensitivity of fit to the “best” numerical model for the depth and width 19
parameters (Fig. 8). The sensitivities with respect to these parameters evaluated at the GPS 20
stations are continuous decreasing functions with residuals from 0.2 to 1.6 cm. The low residuals 21
and the sensitivity values point out that it is not possible to better constrain the depth and width 22
parameters of the dyke only on the basis of ground deformation at the available GPS stations. To 23
understand whether this uncertainty is due to the far location of the GPS stations or to the inherent 24
ambiguity of the used model, we recomputed the sensitivities functions over a grid of points 25
extending 10x10 km around the source (Fig. 9). In this case, the depth sensitivity increases, while 26
the width sensitivity is almost unchanged. Therefore, a better coverage of the summit area could 27
enhance the capability to constrain the source depth.
28 29
Conclusions 30
3D finite elements models were carried out in order to evaluate the ground deformation produced 31
by dip-slip, strike-slip and tensile dislocation sources. The numerical results were compared to 32
analytical solutions from Okada’s dislocation theory for validating their accuracy. The meshing 33
procedure was found to be a very delicate procedure in setting up the numerical models. However, 34
the refined mesh, which gives a good compromise between the computational cost and the 35
solution accuracy, is not so computational heavy to run. The FEM technique enabled to consider 36
both the topography and the medium heterogeneity in modeling the intrusive event occurred at Mt 37
Accepted Manuscript
Etna in July 2001. The topography significantly alters the general pattern of the ground deformation 1
especially near the volcano summit. On the contrary, the medium heterogeneity does not strongly 2
affect the expected deformation. Several computations were performed to better understand the 3
effects induced by the numerical model. Although we did not perform a new numerical inversion of 4
the deformation data, we explored the source parameter space with a grid search. In comparison 5
to the analytical solution, the numerical model associated with the minimum residual provides 6
tensile source with a reduced opening and a wider extension which well matches the hypocenters 7
of the seismic swarm occurred during the dyke intrusion. However, this numerical model does not 8
differ too much from the analytical one. The numerical and the analytical solutions are both 9
valuable solutions given the measurement errors and the location of GPS stations. A good match 10
between the observed and the computed deformation was achieved at most stations. An exception 11
is represented by the EMFN station located within the Valle del Bove in the eastern flank, and 12
EGDF station located near the North East Rift. The numerical model is not able to account for the 13
higher discrepancies at the EMFN station. Therefore, the heterogeneity and the topography cannot 14
give an explanation for the displacement observed on the eastern flank. Indeed, the response of 15
the eastern flank of the volcano to the intrusive event is more composite because of the presence 16
of intricate geological structures. The eastern sector is confined in the northern flank by the North- 17
East Rift zone and by the East-West trending left lateral-transtensive Pernicana fault (Fig. 6), while 18
the southern sector is delimited by the Mascalucia-Trecastagni fault system (Rasà et al., 1996).
19
The EGDF and EMFN stations are closer to these geological structures that are not taken into 20
account into the numerical model. A new model should be set up including these discontinuity 21
surfaces to better draw the complex interaction between the magmatic intrusions and the tectonic 22
processes responsible for the kinematics of the eastern flank.
23 24
Acknowledgements 25
This work is supported by the Etna project (DPC-INGV 2004-2006 contract) and the European 26
Commission, 6th Framework Project – ‘VOLUME', Contract No. 08471. This work was developed 27
in the frame of the TecnoLab, the Laboratory for the Technological Advance in Volcano 28
Geophysics organized by DIEES-UNICT and INGV-CT. We thank the editor Keke Zhang and two 29
anonymous reviewers for their useful comments on this paper.
30 31
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Accepted Manuscript
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Accepted Manuscript
Figure Captions 1
2
Figure 1. Misfit values between numerical and analytical solutions for all the displacement 3
components. Dip-slip (a), strike-slip (b) and tensile (c) dislocation sources are considered.
4
Figure 2. Deformation field due to a tensile dislocation in a homogeneous, isotropic and elastic 5
half-space: (a) eastern component, (b) northern component, (c) vertical uplift. Contour lines are at 6
0.05 m.
7
Figure 3. Deformation components caused by the 2001 intrusive dike in a homogeneous, isotropic 8
and elastic medium with the real topography of Mt Etna: (a) eastern component, (b) northern 9
component, (c) vertical uplift. Contour lines are at 0.05 m.
10
Figure 4. Comparisons between the analytical and numerical solutions including the Mt Etna 11
topography. The computations were performed for different depths of the source and varying the 12
extent of the grid point on which the misfit is evaluated.
13
Figure 5. Deformation fields of the tensile crack in a heterogeneous medium with the real 14
topography of Mt Etna: (a) eastern component, (b) northern component, (c) vertical uplift. Contour 15
lines are at 0.05 m.
16
Figure 6. Observed and expected horizontal displacements at the GPS stations between 11 and 17
16 July 2001. The vertical uplift, computed by the “best” numerical model using real topography 18
and medium heterogeneity, is shown. The black circles represent the epicentres of the seismic 19
event accompanying the dyke intrusion (after Musumeci at el., 2004).
20
Figure 7. Residuals between the observed ground deformation and numerical solutions. The circle 21
represent the numerical model with source parameters coming from the analytical inversion, while 22
the square is the “best” numerical model (with minimum residual).
23
Figure 8. Sensitivity of fit to depth and width parameters of the intrusive dyke. The residuals on the 24
x-component (circle), the y-component (square), and vertical uplift (triangle) are computed at the 25
locations of GPS stations.
26
Figure 9. Sensitivity of fit to depth and width parameters of the intrusive dyke. The residuals on the 27
x-component (circle), the y-component (square), and vertical uplift (triangle) are computed over a 28
grid extending 10x10 km at the ground surface around the source.
29 30 31 32 33 34 35 36 37
Accepted Manuscript
Tables 1
2
Table I. Geometrical parameters of the dislocation source.
3 4
Length:
L [m]
Width:
W [m]
Inclination angle:
δ[degree]
Strike angle:
θ[degree]
Depth of top:
d [m]
Dislocation:
B r
[m]
1000 1000 90° 0° 1000 1
5 6 7 8
Table II. Statistics for the eight simulations in which the mesh parameters are changed.
9 10
Simulation # 1 # 2 # 3 # 4 # 5 # 6 # 7 # 8
Mesh vertices 2228 2513 2570 3195 3977 5101 8591 36196 Elements
(Tetrahedral) 9858 11236 11505 14663 18888 25141 45021 205700 Minimum
element quality 0.3544 0.3083 0.3441 0.3109 0.3417 0.2960 0.3050 0.2454 11
12
Table III. Parameters of the intrusive dike forerunning the 2001 eruption (Bonaccorso et al., 2002).
13 14
Tensile dislocation: B
r [m]
Length:
L [m]
Width:
W [m]
Depth of top:
d [m]
Inclination angle:
δ [degree]
Strike angle:
θ[degree]
3.5 2200 2300 1400 asl 90° 7°
15 16 17 18 19 20 21
Accepted Manuscript
1 2
Figure 1. Misfit values between numerical and analytical solutions for all the displacement 3
components. Dip-slip (a), tensile (b) and strike-slip (c) dislocation sources are considered.
4 5 6 7
Accepted Manuscript
1 2
Figure 2. Deformation field due to a tensile dislocation in a homogeneous, isotropic and elastic 3
half-space: (a) eastern component, (b) northern component, (c) vertical uplift. Contour lines are at 4
0.05 m. In red the position of the intrusive dyke.
5
Accepted Manuscript
1 2
Figure 3. Deformation components caused by the 2001 intrusive dike in a homogeneous, isotropic 3
and elastic medium with the real topography of Mt Etna: (a) eastern component, (b) northern 4
component, (c) vertical uplift. Contour lines are at 0.05 m. In red the position of the intrusive dyke.
5
Accepted Manuscript
1 2
Figure 4. Comparisons between the analytical and numerical solutions including the Mt Etna 3
topography. The computations were performed for different depths of the source and varying the 4
extent of the grid point on which the misfit is evaluated.
5 6 7
Accepted Manuscript
1 2
Figure 5. Deformation fields of the tensile crack in a heterogeneous medium with the real 3
topography of Mt Etna: (a) eastern component, (b) northern component, (c) vertical uplift. Contour 4
lines are at 0.05 m. In red the position of the intrusive dyke.
5
Accepted Manuscript
1 2 3
4 5
Figure 6. Observed and expected horizontal displacements at the GPS stations between 11 and 6
16 July 2001. The vertical uplift, computed by the “best” numerical model using real topography 7
and medium heterogeneity, is shown. The black circles represent the epicentres of the seismic 8
event accompanying the dyke intrusion (after Musumeci at el., 2004).
9
Accepted Manuscript
1 2
Figure 7. Residuals between the observed ground deformation and numerical solutions. The circle 3
represent the numerical model with source parameters coming from the analytical inversion, while 4
the square is the “best” numerical model (with minimum residual).
5 6 7 8 9
11 10
Figure 8. Sensitivity of fit to depth and width parameters of the intrusive dyke. The residuals on the 12
x-component (circle), the y-component (square), and vertical uplift (triangle) are computed at the 13
locations of GPS stations.
14 15 16
Accepted Manuscript
1 2
Figure 9. Sensitivity of fit to depth and width parameters of the intrusive dyke. The residuals on the 3
x-component (circle), the y-component (square), and vertical uplift (triangle) are computed over a 4
grid extending 10x10 km at the ground surface around the source.
5 6