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1 GeoSisLab
Dipartimento di Scienze
della Terra
Università degli Studi "G.
D'Annunzio"
Via dei Vestini, 30
66013 Chieti Scalo (CH)
Italy
b.pace{at}unich.it
g.lavecchia{at}unich.it
p.boncio{at}unich.it
(B.P.,
G.L., P.B.)
2 Istituto Nazionale di Oceanografia e
di Geofisica Sperimentale (OGS)
Borgo Grotta Gigante 42/c
34010 Sgonico
(TS)
Italy
lperuzza{at}inogs.it
(L.P.)
| Abstract |
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5.5). We defined them as seismogenic boxes by using geological information
in terms of plan projection of active faults; the seismicity rates associated
with an individual source are based on the geometry and kinematics of the fault;
the recurrence model is controlled by the earthquake-source association, and,
when possible, we defined the occurrence time of the last major event, using it
in a time-dependent approach. Another layer is given by the instrumental
seismicity analysis of the past two decades, which allows us to evaluate the
background seismicity (M
<5.5); using a sliding-window
selection of events, we defined a model of regular adjacent cells of variable
a and b values of the Gutenberg-Richter relation. The last
layer utilizes all the instrumental earthquakes and the historical events not
correlated to known structures (4.5 < M
<6),
by separating them into seismotectonic provinces shaped on a
geological-structural basis. The seismic-hazard computations first use this
layered model in a traditional probabilistic scheme. The results indicate a
narrow belt of peak ground acceleration (PGA) higher than
0.30g (with standard deviation in attenuation functions) in the axial
part of the Apennine chain, with a maximum spot of PGA
>0.40g southeast of the area damaged by the 19971998
Umbria-Marche sequence (PGA expected not to be exceeded in 50 years
at 90% probability level). The background seismicity gives a nonnegligible
contribution to the hazard, at least for first damage levels. Then, a simplified
time-dependent hypothesis has been introduced for the individual sources alone,
computing the conditional probability of occurrence of characteristic
earthquakes for each source by Brownian passage time distributions. Adopting
equivalent fictitious seismicity rates, we obtained maps referring to the next
50 years by using traditional codes. These results show that the contribution of
the recently active sources vanishes, and the most hazardous sites are now
located south of L'Aquila and in the Sulmona area. We consider that the
methodology and results obtained are useful for seismic risk reduction
strategies. | Introduction |
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Long recurrence times for the largest events and diffuse deformation are common in Italy. Some seismogenic sources have slip rates lower than 1 mm/yr and recurrence times for surface-faulting events comparable to or longer than the completeness interval of the historical information (e.g., 8001000 years in the central Apennines according to Stucchi and Albini, 2000); seismotectonic and paleoseismological studies (e.g., Galadini and Galli, 2000; Morewood and Roberts, 2000; Valensise and Pantosti, 2001; Boncio et al., 2004a) have confirmed that some sources have been silent in the historical catalog time window, but active in the Late Quaternary. In recent years, these studies have changed the common thinking that the Italian earthquake catalogs are long enough and complete enough to estimate all the seismicity levels. In Italy, the PSH analyses developed for seismic zonation purposes use basically an earthquake statistics linked to seismotectonic zoning and historical catalogs (see Slejko et al., 1998; Meletti et al., 2000; Scandone and Stucchi, 2000; Gruppo di Lavoro, 1999, 2004; Romeo et al., 2000; Albarello et al., 2000; Lucantoni et al., 2001); only some authors have introduced cautious statistical criteria concerning the maximum magnitudes (e.g., Slejko et al., 1998; Gruppo di Lavoro, 2004), but no one has explored the computation geometries and/or seismicity rates derived directly from geological and paleoseismological observations. Nevertheless, the occurrence in 19971998 of the Umbria- Marche earthquake sequence signaled a turning point in the development of new models and methods for Italian PSH studies. Models aiming to define individual sources (seismogenic structures) responsible for major earthquakes, which can be supported by detailed geological evidence, give an independent constraint to the characterization of the seismicity (Barchi et al., 2000; Galadini and Galli, 2000; Galadini et al., 2000; Valensise and Pantosti, 2001; Boncio et al., 2004a). By addressing individual sources, the methods could enhance the introduction of time-dependent issues and some attempts to apply these approaches have already been published (e.g., Peruzza et al., 1997; Faenza et al., 2003; Marzocchi et al., 2003; Romeo, 2005).
The central Apennines are the best known area in Italy where such analyses can be performed. Following some preliminary studies (Peruzza, 1999; Peruzza and Pace, 2002; Pace et al., 2002b; Boncio et al., 2004a) that exclusively use individual sources to define the expected seismicity and introduce time-dependent assumptions, in this article we propose a new, more complex and complete seismogenic source model for central Italy. It is based on three combined layers of information to compute the relative seismic-hazard maps under Poisson and non-Poisson hypotheses.
| Seismotectonic Context |
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5.5). We consider active the
faults that show clear geological evidence of repeated displacement episodes
during Late Quaternary (i.e., the last 125 kyr) and/or clear association with
paleoearthquakes (recognized in trenches), historical earthquakes (reported in
earthquake catalogs), and recent seismic sequences (recorded
instrumentally).
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In Figure 1, we plotted some main tectonic elements and selected focal mechanisms. Note that all the recognized individual active faults are located along the Apennine chain (Boncio et al., 2004a).
The Seismotectonic Provinces
The nature and distribution of the seismicity and of the active structures
indicate that the active deformation field of central Italy is mainly
characterized by extension in the axial zone of the Apennines and by contraction
in the frontal part of the belt, close to the Adriatic sea border (Lavecchia
et al., 1994,
2002,
2003;
Frepoli and Amato, 1997; Montone et al., 1999).
From the Tyrrhenian coast to the Adriatic coast, we identify four SPs
parallel to the Apennines
(Fig. 2): A, the Tuscan-Latium
SP; B, the Apennine SP; C, the foothill SP; and
D, the coastal-Adriatic SP. To define the boundaries between the
provinces, we mainly take into account the 3D geometry of major active
structural elements, together with seismological data such as earthquake focal
mechanisms, rheologic and geodetic data. Our description, in geological terms,
of the provinces follows.
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SP A.
The Tuscan-Latium thinned crust SP is a structural domain that
underwent Neogene extensional tectonics, with northwestsoutheast trending
extensional basins mainly of the Late Miocene-Pliocene
(Decandia et al., 1998). Regional uplift affected the area, mainly during the Late Pliocene and after 1
Ma hence (Argnani et al.,
1997,
2003). Presently, it is
characterized by a thin crust (average, 22 km), high heat- flow values, and
positive gravimetric anomalies. The active deformation field mainly consists of
subordinate vertical tectonics because of isostatic rebound processes and
localized zones of deformation corresponding to Quaternary volcanoes and/or
geothermal areas (e.g., Larderello-M. Amiata geothermal areas in Tuscany,
Volsini Mountains volcanic complex in northern Latium, and Colli Albani volcanic
complex southeast of Rome;
Fig. 1). On average, the
seismic activity is small (M <5.5) and located within the upper
crust, mostly at depths shallower than 7 km
(Amato et al., 1998;
Working Group Catalogo Parametrico dei Terremoti Italiani [CPTI], 2004;
Working Group Catalogo Strumentale dei Terremoti Italiani [CSTI], 2001).
The earthquake focal mechanisms and borehole breakout data indicate a prevailing
extensional regime (see Fig. 1)
(Frepoli and Amato, 1997; Montone et al., 1999).
SP B.
The Apennine extensional SP is a structural domain that has
undergone southwestnortheast extension since the Middle Pliocene. It is
presently characterized by active northeast- and southwest-dipping normal and
normal- oblique faults, mainly located along the axial belt of the Apennines,
with associated intramontane basins. The active extensional regime is
constrained by numerous earthquake focal mechanisms, Quaternary fault-slip data,
and related stress analysis (e.g.,
Frepoli and Amato, 1997;
Montone et al., 1999;
Boncio and Lavecchia, 2000a; Boncio et al., 2004a),
geodetic data
(Hunstad et al., 2003), and morphotectonic and paleoseismological data (e.g.,
Blumetti, 1995;
Michetti et al., 1996;
Pantosti et al., 1996;
Galadini and Galli, 2000;
D'Addezio et al., 2001).
Relatively frequent and moderate magnitude earthquakes (4.0 < M
6.0) recorded instrumentally over the past 20 years (see Figs.
1 and
2), as well as large historical
earthquakes (macroseismic intensity up to XI on the Mercalli Cancani Sieberg
(MCS) scale, M up to 7.0; see
Fig. 3) with long recurrence
intervals occur in this province. They are mainly concentrated in the upper
crust, at depths
15 km
(Boncio et al., 2004a).
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The eastern boundary of the SP B represents the eastern border of the crust, which is clearly undergoing extension, on the basis of all the available geological (surface and subsurface), seismological and geodetic data.
SP C.
The foothill SP corresponds to an area situated in an intermediate
position between the Apennines, undergoing extension, and the coastal-Adriatic
zone, undergoing contraction. Both shallow (<15 km) and relatively deep
(1525 km) small-magnitude earthquakes have been recorded recently
(Parolai et al., 2001;
Lavecchia et al., 2003).
Some of the historical earthquakes with MCS intensities up to IX X
(M up to 6.2; Fig. 3)
occurred in the province, especially in the western part. The few available
focal mechanisms are of mixed kinematics, with either normal, strike-slip, or
reverse-faulting mechanisms, suggesting that the tectonic regime is not uniform
within the province (Fig. 1)
(Gasparini et al., 1985;
Frepoli and Amato, 1997; Mednet
database at
http://mednet.ingv.it,
last accessed November 2004). Lavecchia et al.
(2003) proposed a seismotectonic
model with a change of the tectonic regime with depth: the lower crust is
considered under contraction and cut by a still active west- dipping crustal
thrust (the Adriatic Thrust) which would be seismogenic in the 1525 km
depth interval (upper part of the lower crust) according to the rheological
stratification of the crust; the upper crust (depths <15 km) would be mainly
under extension. The highly damaging historical earthquakes, with intensities
IXX MCS, such as Offida 1943, Camerino 1799, Fabriano 1741, and Cagli
1781, might be associated with relatively deep (1525 km) thrust
faulting.
SP D.
The coastal-Adriatic contractional SP is a structural domain
characterized by folds, thrusts, and strike-slip faults nucleated from Middle
Pliocene at the hanging-wall of the Adriatic Thrust
(Lavecchia et al., 2003).
The Adriatic Thrust emerges along the eastward convex Adriatic front and deepens
westward; its geometry at depth is constrained by the CROP 03 deep seismic
reflection profile
(Pialli et al., 1998). The province is characterized by upper crust seismicity (mostly <10 km) never
exceeding M 5.0 during the past 30 years; examples are the
events of Ancona 1972 (Ms 4.5;
Gasparini et al., 1985), Porto San Giorgio 1987 (Md 4.9;
Riguzzi et al., 1989),
and offshore Pesaro 2000 (M 4.1;
Santini, 2003), with prevailing
thrust and strike-slip focal solutions and P-axes trending from
southwestnortheast to eastwest
(Fig. 1). Historical
earthquakes, probably of shallow hypocentral source, have intensities up to IX
MCS (M up to 5.9) but mostly below IX. The eastern boundary of the
SP D coincides with the front of the Adriatic thrust. The western
boundary (between SP C and D of
Fig. 2) corresponds to the
surface projection of the intersection line between the Adriatic thrust and the
base of the brittle layer, which, in this area, is at
10 km depth,
according to rheological and seismicity data
(Lavecchia et al., 2003).
The Seismogenic Boxes
Most of the strong earthquakes of central Italy fall inside SP B,
within the Apennine chain. Moreover, only in this sector do the active faults
have unequivocal seismogenic characteristics at the surface. Compilations of
individual seismogenic sources have been proposed recently for this area
(Barchi et al., 2000;
Galadini and Galli, 2000; Galadini et al., 2000;
Valensise and Pantosti, 2001; Boncio et al., 2004a).
In this article, we use the model of 3D seismogenic sources proposed by Boncio
et al. (2004a), which
is based on an interdisciplinary analysis integrating structural- geological
(surface and subsurface), morphotectonic, paleoseismological, seismological, and
rheological data. It provides the geometry, kinematics, and first-order
segmentation pattern of the major active seismogenic faults, liable to undergo
large earthquakes (M
5.5).
Figure 3 shows the SBs identified in central Italy. The original model by Boncio et al. (2004a) has been implemented with the seismogenic sources of the northern part of SP B (SBs 26, 27, and 28), defined on the basis of an original seismotectonic analysis (Brozzetti et al., 2001). Table 1 summarizes the geometrical characteristics of each source, used later on as input parameters for seismic hazard analyses. The maximum rupture area (RA) has been calculated from the along-strike length (L) and the down-dip length (W), assuming a simplified rectangular shape of the source. L represents the length of the major structures (seismogenic master faults) that may be slightly discontinuous at the surface (small-scale segmentation), but it can be considered continuous at depth, as it is not interrupted by first-order (kilometer scale) structural-geometrical complexities. W has been evaluated from the average inclination of the faults and the thickness of the local seismogenic layer.
The SBs are characterized by a set of paleoseismological, historical, and/or instrumental earthquakes. The SB- earthquake associations are given in Table 2, whereas a more general description of the seismological databases is reported in the next section. Paleoevents, when available, are recorded in the table. Historical earthquakes have been associated to the SB by the analysis of the distribution of the highest intensity data points; instrumental earthquakes by seismological considerations, such as the distribution of the aftershock sequences.
In detail, the easternmost boxes (SB 13) are characterized by some prehistoric events defined by paleoseismological analyses in trenches, but none of the historical events of the area can be satisfactorily correlated to these structures, except for the 1639 earthquake (I = X, M 6.3) which ruptured the northern portion of SB 2 (M. Gorzano). The intermediate seismogenic boxes (SB 415 and 2628) are the most seismically active; they are characterized by some prehistoric earthquakes (SB 15), and several historical and instrumental earthquakes (for details see Table 2 and Boncio et al., 2004a). The westernmost seismogenic boxes (SB 16 25) are in some places less constrained from geological data, and their seismogenic importance is debated. This is the case of SB 16 and 17, SB 18 (Michetti et al., 1995), and SB 25. In the central-southernmost sector, several paleoseismological (SB 21 and 22), historical (September 1349, February 1904, January 1915, July 1654), and instrumental (May 1984) earthquakes occurred (see Table 2 for associations and references). In some cases (see the examples of SB 1, 8, and 9 or 2, 10, and 11) we have partial overlap of sources, motivated by the 3D fault geometry. The overlaps can have considerable influence on the seismic hazard results, but we currently do not have data to refute the complex 3D geometry.
Outside the SP B we actually have no comparable seismotectonic information. By using fault dimensions that derive from magnitude and constraining the geometrical pattern by intensity data points of historical earthquakes, some authors (e.g., Gasperini et al., 1999; Valensise and Pantosti, 2001) propose seismogenic boxes whose definition criteria are therefore different from ours; we do not use them for the sake of homogeneity, but let the seismogenic potential of earthquakes belong to the province.
| Seismological Databases |
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The CPTI Earthquake Catalog
The first version of CPTI catalog
(Working Group CPTI, 1999)
is a compilation obtained by merging the data sets (namely NT4.1 stays for
Camassi and Stucchi, 1997;
Catalogo dei Forti Terremoti Italiani (CFTI) for Boschi et
al., 1995;
1997) collected independently by
national institutions during the 1990s; in its principal section it describes
2480 earthquakes from the second century B.C. to 1992. In 2004, a new
version has been released: it reports earthquakes until 2002
(Working Group CPTI, 2004).
The compilations maintain the hazard-oriented choices done by the NT4.1
historical catalog, retaining only independent earthquakes over the damage
threshold (Io
V/VI MCS, or M
4.0); the
foreshock and aftershock removal is done with a "simple" 90- day and
30-km distance window. The first version reports out-of-criteria events in
separate appendices. Most of the events being historical ones, the parameters
are homogeneously derived from macroseismic data; location and epicentral
intensity is mainly derived from the distribution of the highest intensity
points. In the 1999 version four types of magnitude are given, computed from
macroseismic equivalence (Me, Mm),
obtained by instrumental data (Ms) or as "weighted
mean" (Ma): the dispersion of these estimates is, in
general, very limited and is always in the range of experimental uncertainties.
The 2004 version keeps only Ma and introduces some columns
of derived magnitude for hazard computation (see the catalogs for further
details). The central Apennines are probably the region where seismological data
collection is more reliable and complete. This consideration does not exclude
that events may be missing or mislocated and that completeness is not
homogeneous for all magnitudes. Data completeness is quite a complex issue,
which has serious consequences in terms of balance of seismic moment release.
This aspect, explored in previous analyses
(Peruzza, 1999;
Peruzza and Pace, 2002), is
outside the scope of this article and will only be mentioned here.
Several tests have been done for the study area (latitude from 41.5° to
44.5° N, longitude 11.5° to 14.5° E) by (1) plotting the cumulative
number of earthquakes versus time (Ncum plots), above given
magnitude thresholds; (2) plotting the seismic moment release in time and space
(computed on grid points using variable search distance and time and referring
the seismic moment release to unit time and unit area). The discontinuities in
the slope of Ncum plots indicate the data set complete from
1000 to 1200 A.D. onward for the highest magnitude (Ma
6.4 corresponding to IXX MCS), and from 1500 to 1600 onward for
Ma >5.5 (VIII MCS). Below this value, completeness is
limited to much shorter periods. In addition, the seismic moment release has
been quite homogeneous since the seventeenth century, but a similar slope is
also present around the fourteenth century.
Historical considerations prompt us, therefore, to approximate data
completeness to 1000 years, for Ma
6.4 and to 400 years
for Ma
5.6, the same criteria adopted in previous
studies using the NT4.1 catalog
(Peruzza, 1999;
Pace et al., 2002b): we
stress that in this area most of the records of the CPTI catalog
derive from the NT4.1, but the energetic content expressed by the
Ma value is slightly higher than those of
Mm reported in NT4.1. The CPTI catalog has been
used to associate events to the seismogenic boxes (see
Fig. 3 and
Table 2) and to parameterize
the seismicity models of the seismotectonic provinces.
The Instrumental Earthquake Databases
Two compilations of instrumental records on a national scale have been
analyzed in this study, plus some studies on the Umbria-Marche 19971998
seismic sequence.
The first one is the instrumental catalog released in 2001 by Working Group CSTI; it collects and uniformly describes the data recorded by the national and local networks from 1981 to 1996. The catalog has about 34,700 events with an associated magnitude (mainly computed from duration); earthquakes with M <2.0 are strongly affected by incompleteness, but the data set may be incomplete locally even for magnitudes as high as 2.52.8, as the quality of instrumental coverage has been constantly improving. The time span of the catalog covers some seismic crises that occurred in the region like that affecting the Gubbio area in April 1984 and the Val di Sangro area in May 1984, but with a resolution power of the network that has strongly varied in time.
The most recent instrumental earthquake catalog is the one compiled in the frame of a 4-year project funded by the National Civil Protection Department (Amato and Selvaggi, 2004) and it was published very recently (Castello et al., 2005). The Catalogo della Sismicità Italiana (CSI) catalog refers to a longer period (19812002) and therefore covers the 19971998 Umbria-Marche seismic sequence. The global number of located events is two times greater than CSTI catalog (99,780 compared with 46,701), but in the study area only about 60% of the locations have an associated magnitude estimate during the period covered by both the catalogs (11,706 events in CSTI; 6839 in CSI); the increased level of the seismic activity since 1997 and the temporary networks installed in the Colfiorito area account for the other 10,815 events with a magnitude estimate listed in CSI from 1997 until 2002. Magnitude distributions in the study area in both the catalogs exhibit a peak on M 1.71.8. We will see afterward how these additional 6 years of seismic monitoring influence the characterization of the low- level seismicity.
These databases contain foreshocks and aftershocks, and therefore they are
not suitable for use in traditional seismic-hazard analyses that consider
independent events only. We therefore processed the catalog for
fore- and aftershock removal. We discarded the "cold"
criteria used by the historical catalogs, and we abandoned also some well-known
filtering algorithms used in the literature
(Gardner and Knopoff, 1974;
Knopoff et al., 1982;
Slejko and Rebez, 2002, developed for northeastern Italy), because they turned out to be too rigid if
applied to low-magnitude data sets. We used, therefore, the original table
proposed by Knopoff (2000),
extended downward to magnitude M 3 by interpolating it in the
form of the following relationships:
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We found that the best filtering algorithm is the empirically based step function used by Knopoff (2000), because it is capable of preserving the main features of the instrumental seismicity in the central Apennines, often done by long-lasting swarms. In fact, these simple formulas, applied to both the instrumental catalogs, obtain a filtered data set of earthquakes very similar to that obtained by using the Reasenberg procedure (24,850 CSI events with M >2.0 became 18,852 or 18,789 using the Reasenberg or Knopoff methods, respectively; with CSTI, the M >2.0 original 17,365 events remain 15,475 and 15,364; Fig. 2), with significant consequences for the estimates of the seismicity levels in the area. When the filtering algorithms are used on a single seismic sequence (we tested the Umbria-Marche sequence of 19971998; data from Selvaggi et al., 2002), the aftershock removal proposed by equations (1) and (2) recognizes all the major shocks corresponding to distinct ruptures of fault segments as "main events," more effectively than the Reasenberg procedure, guaranteeing that the complex faulting pattern is represented by "independent" events.
| Seismic-Source Modeling |
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Seismogenic Boxes: Medium-to-Large Earthquakes Linked to Individual Structures
Source characterization of a fault consists in quantifying the magnitude
distribution of the segment and in defining their occurrence model. In this
section we will try to infer the long-term seismic potential of fault segments
using the seismogenic boxes defined in
Figure 3 and the geometric
parameters and observations gathered in Tables
1 and
2.
Various types of primary observations have been used in literature to estimate the magnitudes of earthquakes not detected by instruments and, therefore, to infer the maximum expected magnitude (Mmax) on a fault segment; the mean coseismic displacement on the fault trace and the size of the surface or subsurface fault are by far the most commonly used parameters. In Italy, and in particular, in the central Apennines, observations of coseismic displacement are rare; the full 3D geometry of the seismogenic fault is therefore the best way to get a Mmax estimate.
Using the approach tested in previous articles
(Pace et al., 2002b;
Peruzza and Pace, 2002), we
calculated for each seismogenic box the Mmax values with
empirical relationships calibrated on normal faulting
(Wells and Coppersmith, 1994)
by using the maximum subsurface fault length and area (respectively, L and
RA in Table 1). We
derived Mmax also from the relationships between fault
dimensions and scalar seismic moment (M0) expressed by:
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After having calibrated a regression relationship of L versus W on about 180 earthquakes around the world (see Peruzza and Pace, 2002, for details), we corrected the maximum possible along-strike rupture as a function of down- dip extension of the fault ("corrected length") and so the Mmax values of the more shallow sources (e.g., the Valle Umbra sources, SBs 16 and 17); we obtain more reasonable Mmax values, which are comparable to the observed historical and instrumental earthquakes.
Figure 4 shows the
Mmax values computed for each seismogenic box and compares
them with the associated earthquakes (see also
Table 2). For SBs 4,
8, 16, 17, 19, 26, and 27 we used the corrected lengths reported in parentheses
in Table 1. The dispersion of
the computed Mmax values is fairly small (a maximum scatter
of about 0.3) and is fully comparable with instrumental uncertainties. In 11 of
28 seismogenic boxes a maximum event of Mmax occurred during
historical times, following our proposed earthquake-box association. Only in the
case of the 1915 earthquake, in SB 22, did the observed magnitude
significantly exceed the calculated one. The instrumental magnitude
(Margottini et al., 1993,
referenced in the previous catalog NT4.1,
Camassi and Stucchi, 1997) is
derived from 22 recordings with an associated standard deviation of 0.74, and it
is classified as a Ms type: accepting the equivalence in the
definition of Ms and Mw in the range
67.5 (e.g.,
Ekström and Dziewonski, 1988), the difference (Mmax observed of 7.0 against 6.6 computed)
is inside the aleatoric uncertainty. Using geodetic observations,
Ward and Valensise (1989)
estimated a Mw close to 6.6, similar to that obtained by
Amoruso et al. (1998) using a nonlinear inversion approach that takes into account both near-field
surface deformations and far-field first- motion polarities; they identified a
fault length parameter of
24 km, a value close to the coseismic rupture
recognized by Oddone (1915) and
to the length assigned to SB 22 in this study
(Table 1).
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Then, to enhance the use of the geometric and kinematic parameters assigned
to the boxes and to have an independent constraint to the seismic
characterization, we calculated the mean recurrence time
(
) of the maximum
event in each source; we did it indirectly, because for most of the
SBs we do not have recurrence intervals or paleoseismological
observations providing reliable mean values.
We estimate the
using two different techniques. The first one obtains the values of
using the
criterion of the "segment seismic moment conservation," proposed by
Field et al. (1999):
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| (4) |
Figure 5 shows the
calculated for
each seismogenic box, using the two different methods and the three
Mmax values of
Figure 4. The recurrence time
estimates vary significantly, about 30% of the mean values (about 300 years over
1000, with some of the worst cases in SBs 2, 26, and 27).
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Magnitudes from seismic moment (M 3 in
Fig. 4) and their related
recurrence times, calculated using the "segment seismic moment
conservation" criterion (T6 in
Fig. 5), will be used in the
following text to parameterize the whole seismic activity of the seismogenic
boxes. By far, Mmax and
are the least
constrained parameters available, but the geological observations, coupled with
the seismological data, are the only way to constrain the model of long
recurrences of the maximum events, as is necessary in seismic- hazard
assessment.
With regard to the occurrence model, the literature includes two very diverse
approaches in dealing with the mechanical behavior of faults. Some models assume
that individual faults, or fault segments, essentially tend to generate the
same-size earthquakes or characteristic ones with a relatively narrow range of
magnitude at or near the Mmax (e.g., the characteristic
earthquake model of
Schwartz and Coppersmith, 1984).
These models are essentially driven by geological observations where, at a point
along a fault, the displacement during successive surface-faulting earthquakes
remained more or less constant. Some other models, essentially derived by
statistical studies of the seismicity distribution in a region, assume that the
number of earthquakes from a single source/fault is exponentially distributed
with earthquake magnitude. The general form of these recurrence models is the
well-known Gutenberg-Richter (G-R) relation
(Gutenberg and Richter, 1944):
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| (5) |
A priori, for each seismogenic box we decided to use one of these
two well-known earthquake recurrence models. For the sources that have a nearly
continuous spectrum of magnitudes documented by seismological observations, we
adopted the G-R model. The G-R distribution is anchored
and truncated on the different (Mmax,
) values of the
boxes and has a constant b = 1.0; this value was obtained by the
G-R interpolation of all the earthquakes occurring in the Apennine
extensional seismotectonic province (SP B, described in
Fig. 7), as single boxes are
insufficient for statistics. For the SBs in which single-value
magnitudes prevail, we use the "characteristic earthquake" model
(CH): the occurrences are calculated by a truncated Gaussian distribution,
peaked on Mmax and
, with a
value of 0.3, representing a simplified estimate of
Mmax uncertainties. A small tail of G-R
exponential distribution models the queue of low magnitude for these sources; it
is anchored to the rate of occurrence of moderate events and has a constant
b = 1.0, if magnitudes as low as 0.50.7 compared to
Mmax have been observed, but with an occurrence rate much
lower than that predicted with the simpler G-R model: we name this
behavior "Hybrid" according to the definition given by Wu et
al. (1995). If no
earthquakes with M >4.5 have been reported by historical and
instrumental catalogs, the tail is modeled only in terms of cells of variable
a and b values, as depicted by the contribution of the
background instrumental seismicity described later on; we classify these sources
as pure characteristic earthquake sources. The type of model used for the
seismogenic boxes is indicated in
Table 3.
|
Having chosen the occurrence model, and given a calibration point
(Mmax,
) to the model, we
can derive straightforwardly the seismicity rates of the seismogenic boxes by
imposing a seismic-moment budget. The assumption of seismic-moment conservation
is easy to comprehend if we consider the pure characteristic earthquake model,
where a spike of seismicity corresponds to the characteristic event. If, instead
of using a spike, we model the characteristic earthquake rates with a peaked
Gaussian distribution function, we have to impose the condition that the total
amount of seismic moment released by the fault system (e.g., some magnitude
classes around the Mchar value) does not exceed the seismic
moment released by the characteristic magnitude alone, whatever the
magnitude-sampling factor of the Gaussian function is (here the step chosen is
0.3). Similarly, when we use a G-R distribution, the sampling factor
controls the total amount of energy released. Therefore, it is necessary to
impose the condition that the total amount of seismic moment released in a given
period by the distribution (sampled magnitude) is equal to the moment released
by the maximum expected earthquake, at the same time. The seismic-moment
conservation is therefore done by (1) fixing the budget of seismic-moment
release in terms of the seismic-moment rate given by the maximum expected
earthquake (i.e., M0[Mmax] in
years) and (2)
scaling the occurrences of each magnitude class in such a way that the summation
of seismic-moment rates over all the classes equals the seismic-moment rate
obtained from the maximum expected earthquake. In the future, geodetic data
(e.g.,
Hunstad et al., 2003) will provide additional constraints in performing seismic-moment budgeting,
which has never been applied in Italy until now.
Figure 6 reports some
examples of seismicity rates, computed by using different occurrence models and
compared with instrumental rates (earthquakes located inside each seismogenic
box by Working Group CSTI
[2001] and by
Castello et al.
[2005]). Working on
such a detailed scale, we recognize that epicentral locations may sometimes be
affected by uncertainties because of the spacing of stations of the national
seismic network. This is the case, for example, of the mainshock
(Ms 5.8) of the 1984 Val di Sangro sequence, whose
location is quite uncertain and lies outside the SB 24 polygon; the
temporary stations installed in the area after the main event depicted the true
geometry of the source
(Pace et al., 2002a). The two instrumental catalogs (CSTI and CSI;
Fig. 6) give similar rates for
the sources not involved in the 19971998 seismic sequences; in the
epicentral region (SB 6) the G-R slope is quite
impressively constant (b
0.9), with an evident bulk at M
>5. We attribute these differences to the changes in the geometry of the
network and in the processing of the data.
|
The graphs suggest that careful selection of the recurrence models, constrained by the geometry and kinematics of the individual sources, may give reasonable seismicity rates; they can be extrapolated for low magnitudes too, giving rates that agree with those derived from short instrumental monitoring. The time-dependent seismicity rates (plusses in Fig. 6, reported for some sources) will be described later.
Seismotectonic Provinces: Diffuse Seismicity on Large Areas
The seismotectonic provinces previously described were used to model the
earthquake occurrences with M
5.5 that are not directly correlated
to individual seismogenic sources. In fact, no seismogenic boxes in
SPs A, C, and D are supported by independent geological and/or
paleoseismological information.
As common practice in the requirements of PSH studies, we
extracted the earthquakes located inside the polygons, representing
seismotectonic provinces, to get statistics from them. All the seismological
databases were used, the two instrumental catalogs (namely CSTI and
CSI), declustered for aftershock removal, and the historical
CPTI catalog, in adequate time windows. As previously stated, data
completeness for the CPTI database is taken from the past 400 years
for M <6.4 and 1000 years for M
6.4; below
M 5.5 this data set can be not complete. The instrumental
catalogs are considered complete for the periods they refer to (16 years for
CSTI, 22 years for CSI); magnitudes lower than 2.0 and
events deeper than 50 km have been discarded from our completeness analysis. The
historical and instrumental databases overlap in time namely for M
>4.0.
The G-R relationships for each province have been obtained by interpolating the cumulative annual number of events with the least-squares (lsq) and the maximum likelihood (mlk) methods (Aki, 1965; Utsu, 1965, 1966; Weichert, 1980), obtaining the a (normalized to 1 year) and b coefficients. The distributions obtained from historical and instrumental databases (Fig. 7) are properly connected; it suggests that the periods selected for data completeness are adequate, and no discontinuities in the magnitude estimate between the historical and instrumental records are evident.
The seismic crisis that occurred in the Umbria-Marche region in 19971998 is not represented by the CSTI data, but the CSTI and CSI instrumental data sets are rather impressively similar in SP B and C, in the provinces where the crisis occurred, whereas in SP A and D, the rate of activity (a value in the G-R relation) is lower in the longest catalog (CSI) for normalization reasons. This analysis confirms the invariance of the G-R with respect to the Umbria-Marche sequence, the strongest that occurred in Italy after the 1980 (Ms 6.9) Irpinia earthquake, as already demonstrated by previous analyses of the data recorded by local and temporary networks (see Peruzza, 1999; Cattaneo et al., 2000). These considerations lead us to prefer the CSTI catalog, as less influenced by heterogeneity in the monitoring network; the G-R relationships obtained by CSTI (lsq coefficients reported in Fig. 7) can be considered representative of the seismicity of the province for magnitude below approximately 5.05.5. At higher magnitude, the seismicity rates of the provinces are better represented by the historical catalog CPTI. The G-R relationships obtained by the least-squares method on M >4.5 are reported in Figure 7 also.
Three provinces (C, D, and, in part, B) present a bulk departure from a G-R trend; it may be both the expression of "characteristic earthquake" behavior of individual sources inside the province, or the consequence of "clustering" in magnitude classes due to the use of macroseismic data. The identification of individual seismogenic boxes in SP C and D will probably help to solve this question in the future.
For the Apennine extensional SP B, in
Figure 7, we also reported the
sum of the rates calculated from the "geological" seismic-source
modeling of the seismogenic boxes. This graph demonstrates that individual
sources alone are capable of explaining all the observed seismicity and in some
magnitude classes even to overcome it; historical rates (clustered with the same
step used for the seismogenic boxes, white plusses in
Fig. 7b) are lower than the
"geological" rates for M
>5.5 and at
M 4.5 also. This scenario is compatible with the lack of
experimental data because of incompleteness (missing earthquakes in the past 400
years for low M and seismic sources not active in the last 1000 years
for the highest M). We stress again that the seismicity rates of the
seismogenic boxes and those of the provinces follow different assumptions. In
the first case, we keep the seismic- moment rate of each individual source
constant; while using earthquake statistics on wide-area sources, we conserve
the seismicity rates. The good agreement between experimental (historical rates)
and modeled data (
of the geological rates) in
Figure 7b makes us consider the
seismotectonic constraints adopted to quantify the seismicity in this sector of
the Apennine chain reliable. As already stated, additional studies are necessary
to increase our knowledge of the other provinces. To evaluate the probabilistic
seismic hazard of the seismotectonic provinces A, C, and D, we can now only use
the experimental data; the expected seismicity rates have been calculated for
M
5.5 by the G-R relationships derived from the
CPTI catalog. For reasons of caution, we truncated the distribution
to a maximum magnitude value corresponding to a mean recurrence time of
1000 years.
Grid Elementary Sources for Low-Level Background Seismicity
The third layer of seismic sources is related to medium- to-low seismicity,
an energetic level that usually receives less attention in Italian
PSH analyses, but it has a strong relevance for high-vulnerability
areas, such as most of the historical towns in central Italy. The medium-to-low
seismicity (2
M < 5.5, herein referred as
"background" seismicity) is modeled on the instrumental catalogs
available, following a philosophy similar to that adopted by "spatially
smoothed seismicity" techniques (e.g.,
Frankel, 1995). In fact, the
basic assumption of homogeneously distributed seismicity is a necessary but
simplistic approximation, bypassed by the increase of knowledge; small-magnitude
events do not usually leave a geological record, and macroseismic data may be
dominated by effects not related to the source; therefore, only the instrumental
seismological data can be representative of the spatial distribution of minor
seismicity to describe local variations (e.g., the limits of volcanic districts,
inside SP A). Using the declustered instrumental catalogs, we
extracted groups of seismic events within a given distance from a grid point to
compute a and b coefficients of the G-R
relationship. After a sensitivity analysis, we chose a grid node spacing of
0.1° both in longitude and in latitude (corresponding roughly to 711
km) and a search radius of 20 km. This value represents a compromise between the
requirements for statistics and the detail of lateral variation of the seismic
characters. The partial overlap of the circular search areas smoothes the
differences between adjacent nodes of the grid. Data interpolation to obtain the
G-R relationship coefficients has been done using the traditional
algorithms of least squares (lsq) and maximum likelihood (mlk)
(Aki, 1965; Utsu,
1965,
1966;
Weichert, 1980). The a
values have been normalized taking into account the time window of the catalogs
and the spatial extension of the search areas to represent the "activity
rate" of one year and an arbitrary 10 x 10 km unit area.
Figure 8 summarizes the a and b values distribution in central Italy obtained by the CSTI catalog using the lsq method; nodes with less than five events were discarded. Large lateral fluctuations have been obtained for the G-R coefficients, despite the relative stability exhibited by the previous analysis concerning the provinces. These fluctuations may be ascribed both to the characteristics of the seismic activity and of the instrumental network. Using the CSTI catalog we believe we are less influenced by instrumental reasons, as the catalog does not include the 19971998 sequence, with the very closely spaced stations installed after the beginning of the seismic crisis (September 1997). We therefore assume that the threshold of earthquake detection of the national seismometric network (Rete Sismica Nazionale Centralizzata [RSNC], www.ingv.it, that integrates some local networks in central Italy) may be considered geometrically and temporally sufficiently homogeneous from 1981 until 1996, with the only exception of some areas close to the coasts. These considerations let us ascribe the lateral variations of the G-R coefficients to the spatial variations of the seismicity. Future efforts to define accurately the spatial and time variations of instrumental completeness will give additional constraints to such analyses.
|
|
Some examples of G-R fitting are shown in Figure 9 prompting also the choice of the fitting algorithm; they are taken from the northern part of SP C (point a in Fig. 8), the central part of SP B (b), the southern part of SP A (Colli Albani region, c), and in the Maiella region (d). We can clearly see in the graphs that the least-squares (lsq) algorithm fits the experimental data better than the maximum likelihood (mlk) algorithm in the magnitude range 2 < M < 4. Because it is reasonable to consider this magnitude interval complete, we will use it in our modeling; lower magnitudes can be considered incomplete for instrumental shortcomings, whereas higher magnitudes are incomplete because the temporal window of the catalog (16 years) does not permit us to see the complete seismic process.
The a and b values of Figure 8 were finally used to compute the seismicity rates of regular adjacent square (in degrees) cells, centered on the mapped nodes. The G-R relationships are extrapolated to the magnitude lower limit that is modeled by the other layers of sources (range 25.5 for the provinces A, C, and D; range 24.5 for the boxes in SP B). The use of cells of variable a and b values permits evaluation of the medium-to-low level of expected seismicity, without imposing additional geological evidence, which is difficult to define for some places. Examples are the seismicity correlated to the activity of the Latium active volcanic zones (Colli Albani area) or the seismicity localized in the Maiella region, an area that even today is not very decipherable from a seismotectonic point of view.
| PSH Analysis |
|---|
|
|
|---|
The Poisson Hazard Assessment
Poisson hazard assessments are those obtained through the use of the three
levels of seismic sources previously described, accepting the assumption of
stationarity of seismicity. The results are illustrated in Figures
10 and
11.
|
|
In Figure 10a we mapped the contribution to hazard of the layer defined as low-level background seismicity; in Figure 10b the source model refers to the layers of the seismotectonic provinces (SP A, C, and D) and of the seismogenic boxes (inside SP B). Figure 11 reports the global results deriving from all three layers of seismic-source modeling. PGA values include the uncertainties in attenuation.
The background seismicity
(Fig. 10a) is modeled using the
seismicity rates coming from G-R interpolation of instrumental recent
seismicity in the magnitude range 25.5; in the Apennine extensional
SP B area we considered only the interval 2
M < 4.5
to use the SBs model rates completely. Despite this choice, and
despite the fact that the 19971998 seismic crisis in the Umbria-Marche
region was not in the instrumental catalog we used, the hazard results give
considerable PGA values for the whole region. The expected
PGA values using background seismic-source models reflect the
distribution of the instrumental seismicity of the past two decades
(CSTI catalog,
Fig. 2), with some important
peculiarities. For example, the seismicity concentrated in the volcanic district
of Lake Bolsena (northwest of Viterbo) has a minimum impact on the hazard maps,
whereas a few events concentrated in the Lake Trasimeno (west of Perugia) zone
give relatively high hazard, which follows westward (on the boundary of our
maps) because of the contribution of the Tuscan seismicity (M. Amiata
seismicity). Finally, the area around the town of Chieti, affected, on the
whole, by only few events in the 19811996 period, gives a relative
maximum, with expected PGA values between 0.20g and
0.25g.
These PGA levels are significant in terms of seismic risk reduction, even if they derive from low-level seismicity, always neglected by Italian PSH studies in the past. Notably, the background hazard map has spatial variations, following the a and b coefficient fluctuations, a feature unlikely to happen when using extended areal sources (SPs).
Flat, low, and spatially homogeneous PGA values result despite the use of the seismotectonic provinces (G-R models of SPs A, C, and D in Fig. 7); by spreading the available seismicity over the whole area, the hazard is considerably reduced, with PGA values as high as 0.10g (Fig. 10b). Only the influence of the nearby individual SBs make them higher (0.100.20g). Inside SP B, in Figure 10b, the distribution of hazard is strictly correlated to the location and the geometry of the individual SBs. The partial overlap of sources, due to the 3D geometry, creates one spot of PGA values (>0.40g). Moreover, the choices on the energetic parameterization of the SBs made important differences to the expected PGA values; in fact, the SBs modeled with an exclusive "characteristic earthquake" model have less impact than those with a G-R behavior, both with pure G-R distribution (e.g., SBs 4, 7, 16, 17, and 24) or with a Hybrid model (e.g., SBs 8, 9, and 20). In addition, the expected PGA is larger when the source fault is relatively short (e.g., SBs 7 and 12), because the smaller maximum magnitude gets shorter recurrences to a given slip rate, producing high hazard. For longer faults (e.g., SBs 1, 2, 3, and 19), although the recurrence rates are low, they may dominate longer return-period ground motions because of the larger maximum magnitudes.
The final poissonian results (Fig. 11) were obtained using all the source models. On average, the PGA values are higher than those obtained with traditional models (e.g., Slejko et al., 1998; Gruppo di Lavoro, 1999; Romeo et al., 2000; Albarello et al., 2000; Lucantoni et al., 2001; Gruppo di Lavoro, 2004); the influence of the individual sources and the background seismicity model is clear. The most recent national seismic hazard map (Gruppo di Lavoro, 2004) gives maximum values of PGA between 0.25g and 0.275g, located on the southern part of the axial Apennine chain studied here. In the same area, our maps give values that can be 50% higher, with localized spikes with values at about 0.4g. Our maps are more variable, following the individual sources pattern and the fluctuations modeled by the background seismicity; we identify areas with relatively high hazard outside the axial SP B too, with PGA values >0.25g (e.g., P. San Giorgio area) despite the values between 0.175 and 0.2g of the national map. The volcanic areas (e.g., Colli Albani area, south of Rome), clearly visible in both the maps, again reach higher values in our maps (0.20.25g versus 0.150.175g); in our analysis they are not connected to the axial belt of maximum hazard but concentrated only in the volcanic districts. Their shapes follow the lateral variation of the seismicity only and are not forced by the zoning. Finally, our maps are little influenced by the geometry of the seismotectonic provinces, which can be considered equivalent in their meaning to the "seismogenic zones" used in the Gruppo di Lavoro (2004) model.
The Time-dependent Hazard Assessment
The last goal of our article is to introduce time dependence into the
seismic-hazard analysis. We chose to produce maps in which the time elapsed
since the last maximum event, when known, entered into the computations. We
therefore adopted the simplest time-dependent process, namely the renewal one.
The time dependency has been associated with the seismogenic boxes only,
using the formulation of Brownian passage-time (BPT) distributions,
one of the most physically motivated models that has appeared in recent
literature
(Matthews et al., 2002).
The time- dependent model is only applicable to the individual sources, because
only for these sources do we know or we infer the date of the last maximum
earthquake (see Fig. 4 and
Table 2).
The time elapsed since the last event is used to determine the conditional
probability of having an event in the next 50 years. Input parameters for the
calculation of the probability of occurrence of an earthquake for an individual
source are: Tela, the time elapsed since the most recent
maximum earthquake; µ, the mean recurrence time; and
, a dimensionless measure of aperiodicity given by (see Matthews
et al. [2002]
for details):
|
| (6) |
|
| (7) |
|
| (8) |
Because we do not have experimental data of repeated earthquakes on the
individual structures we decided to use the statistics on the calculated
to derive
µ and
values
(Fig. 5 and
Table 3). For sources without a
dated major event (see Table 2,
source code underlined in
Fig. 12) we imposed 4000 years
of elapsed time, taking into consideration the completeness stated by historical
and archeological studies in central Italy (e.g.,
Guidoboni and Mariotti, 1997;
Stucchi and Albini, 2000; Galadini and Galli, 2001) for
the highest level of energy; however, these sources will be treated in the
following discussions under Poisson assumptions.
|
Figure 12 compares the mean
recurrence times with the time that elapsed since the last maximum event and
gives the BPT conditional probabilities for the next 50 years. From
the graph we recognize that less than 50% of the sources exhibit an appreciable
probability value in the next 50 years (20042053). Among them, some
sources like SBs 12, 13, 15, 21, and 28 have a
Tela
µ; sources 14, 19, 20, 23, and 24 have
an elapsed time two to three times longer than the mean recurrence time and an
value
1/4. These are, with SB 21, the sources
most prone to a maximum event in the future, according to these analyses.
Significant values of conditional probability are also associated with recently
activated sources, such as SBs 26 and 27, because of the high
value. Finally, when the Tela is greater
than 3 µ, usually, the conditional probability drops, due to the
regular seismic cycle modeled by small (<0.3)
values.
Then, using the simplification proposed by Wu et al.
(1995), equivalent fictitious
seismicity rates have been merged into the seismic-hazard code; the fictitious
recurrence time Teq for the Mmax is
computed by solving the equivalence of the probabilities given by
|
| (9) |
Uncertainties in terms of Mmax and
enter directly
into the distribution functions; the uncertainty on the characteristic event is
the standard deviation of the Gaussian magnitudes distribution; the aperiodicity
in BPT function represents the uncertainty in the
temporal behavior.
The results of the application of the time-dependent model, in terms of expected PGA values in the next 50 years, are illustrated in the seismic hazard map of Figure 13. The picture is quite different from the one obtained under Poisson assumptions. The contribution of the recently active sources, like SB 6 (Colfiorito) or SB 22 (Fucino) (activated during the 1997 and 1915 earthquakes, respectively; Table 2), vanishes in the overall seismic hazard. On the other hand, some sources, for the high BPT conditional probabilities (Fig. 12), become the most hazardous sites (SB 21, Campo Felice-Ovindoli, and SB 14, Sulmona), with PGA values >0.5g. The spot with expected PGa >0.4g in the Poissonian map (Fig. 11) are now only as high as 0.3g; L'Aquila becomes the most hazardous city in the study area as a consequence of the probable activity on the southernmost structure of Campo Felice-Ovindoli (SB 21) in the time- dependent model. The differences between stationary and nonstationary maps are illustrated in Figure 14; in the area where we have an increasing of hazard in the time-dependent map (area between Campo Felice-Ovindoli and Sulmona), the PGA values are about 50% higher (Fig. 14a) than the Poissonian ones, with a maximum increase up to 0.25g (Fig. 14b); on the contrary, in the areas where the nonstationary results decrease with respect to the stationary ones (e.g., the Umbria-Marche area and the Fucino area), the values are locally up to 20% lower (Fig. 14 a) with a maximum decrease of about 0.07g (Fig. 14 b).
|
|
| Final Remarks |
|---|
|
|
|---|
The elaborated model is a layered model, where the available
information enters at different levels into the seismic-hazard computation. The
individual structures liable to undergo major earthquakes (M
5.5)
are parameterized in terms of "seismogenic box," representing the
plan projection of active faults; the magnitude (M) and recurrence time
(T) distributions are calibrated independently on the geometric and
kinematic constraints and by the earthquake-structure association; they are also
adequate for use in a time- dependent approach. The background seismicity
(M approximately <5.5) is evaluated using the instrumental
seismicity registered in the past two decades. The remaining seismicity is
modeled with seismotectonic provinces that are defined using
geological-structural and seismotectonic information. The global seismogenic
source model proposed here represents seismic-moment release conditions
compatible with the long-lasting series of seismological observations and with
the few geodetic data available for the area.
The seismic-hazard computations use both Poisson and non-Poisson hypotheses. In addition to the common stationary assumptions, a time-dependent hypothesis has been introduced; by adopting equivalent fictitious seismicity rates, starting from conditional probabilities computed by BPT distributions, we obtain maps referring to the next 50 years (from 2004 onward) by using public traditional codes, with an accuracy that is acceptable for engineering purposes.
Some questions still remain, like the evaluation of the uncertainties introduced in the model, or the definition of new individual sources. Nevertheless, we believe that the PSH assessments presented here represent, in actual fact, the most complete regional evaluations in terms of complexity and use of all the available data. The reduction of the critical uncertainties (e.g., slip rates and recurrence times) needs additional studies aimed, in particular, at evaluating all the geological markers.
We consider the methodology and results obtained useful for the strategies of seismic risk reduction.
| Acknowledgments |
|---|
|
|
|---|
Manuscript received November 30, 2004
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