Introduction
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Ben-Avraham et al (2012) |
Fig. 17.1
Tectonic setting of the Dead Sea fault — a transform plate boundary that connects the opening of the Red Sea with the collision in Turkey. Boxes indicate basins along the fault valley discussed in the text.
Ben-Avraham et al (2012) |
Fig. 17.1 - DST Tectonics |
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Ben-Avraham et al (2012) |
Profiles and location map from the Gulf of Elat.
Ben-Avraham et al (2012) |
Fig. 17.2 - Gulf of Elat |
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Ben-Avraham et al (2012) |
Profiles from the Zofar basin in the Arava valley.
Ben-Avraham et al (2012) |
Fig. 17.3 - Arava |
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Ben-Avraham et al (2012) |
Profiles from the Dead Sea basin.
Ben-Avraham et al (2012) |
Fig. 17.4 - Dead Sea Basin |
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Ben-Avraham et al (2012) |
Profiles from the Dead Sea basin.
Ben-Avraham et al (2012) |
Fig. 17.4 - Dead Sea Basin |
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Ben-Avraham et al (2012) |
Profiles from the Dead Sea basin.
Ben-Avraham et al (2012) |
Fig. 17.4 - Dead Sea Basin |
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Ben-Avraham et al (2012) |
Fig. 17.5
Profiles from the Sea of Galilee. A Location map showing main tectonic elements in the Sea of Galilee area. Bold lines indicated major faults, while dotted lines show the position of seismic profiles. Grey area shows the extent of the Yehudiyya transtensional one (after Shulman et al., 2004). Ben-Avraham et al (2012) |
Fig. 17.5A - Sea of Galilee |
Ben-Avraham et al (2012) |
Fig. 17.5 B and C
Profiles from the Sea of Galilee. B Profile from south of the lake showing both compressional and asymmetrical features (Zurieli, 2002). C Profile from north of the lake showing the Yehudiyya transtensional zone. Within the zone lies a compressional feature, the Qazrin structure, which is bordered on the west by the main fault zone (Shulman et al., 2004). Ben-Avraham et al (2012) |
Fig. 17.5 B and C - Sea of Galilee |
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Ben-Avraham et al (2012) |
Fig. 17.6
(after Zilberman et al., 2000). Ben-Avraham et al (2012) |
Fig. 17.6 - Hula Basin |
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Ben-Avraham et al (2012) |
Fig. 17.7
Ben-Avraham et al (2012) |
Fig. 17.7 - Ghab Basin |
Motion along the Dead Sea fault is not pure strike-slip and the direction of the plate boundary changes several times
resulting in areas of transtension and transpression. This is evident by the variable morphology and structure,
which is characterized by extensional, compressional and asymmetrical features. These features vary in size, from the
large-scale, which define the general structure of the valley, to the small-scale, which define the internal structure.
The Dead Sea fault valley itself is a large-scale transtensional feature, which formed as a result of oblique strike-slip
motion along the fault. The extensional component of motion is largely responsible for the formation of pull-apart basins
that occupy its length. Compression is caused by a step to the right of the left lateral strike-slip master fault and
results in structural saddles, which separate the main basins along the valley. Smaller compressional uplifts divide
several of the major pull-aparts into sub-basins and also occur along the fault valley. However, it is often hard to
determine whether these intra-basinal features are salt-related. Asymmetry is evident in the structure and topography
of the highlands, which border the valley and in the basins that lie within. The large-scale asymmetry across the Dead
Sea fault can perhaps be explained by the combined effect of normal faulting and isostatic uplift on existing pre-rift
topography (Wdowinski and Zilberman, 1996).
Numerous examples of basin asymmetry and compression features have been presented from locations worldwide, indicating that
these are not local phenom¬ena limited to the Dead Sea fault valley. The Cariaco basin in Venezuela, which crosses the
El Pilar fault, shows many similarities to the Dead Sea basin, displaying a clear asymmetry towards the main fault
(Ben-Avraham and Zoback, 1992). Additional examples exist along other continental transform faults and rift valleys,
such as the Motagua fault system in Guatemala, Lake Baikal, Lake Tanganyika in the East African rift system and the
north Anatolian fault in Turkey. Transform-normal extension may help explain the small-scale asymmetries observed
within the basins themselves. This seemingly contradicts the basic assumption that pull-aparts are formed as a result
of overlapping strike-slip faults. However, it is the extensional component that arises from such fault arrangements
that may well be responsible for resolving this 'conflict' ('leaky transform', Garfunkel, 1981). It is interesting to
note that very little or no mantle uplift exists under the Dead Sea fault in the Arava valley. This may explain the
large negative gravity anomalies associated with the fault that reflect primarily the thick sedimentary sequences
including salt layers, which are abundant along the length of the valley.
Source | Image | Description |
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Ben-Avraham et al (2012) |
Fig. 17.1
Tectonic setting of the Dead Sea fault — a transform plate boundary that connects the opening of the Red Sea with the collision in Turkey. Boxes indicate basins along the fault valley discussed in the text.
Ben-Avraham et al (2012) |
Fig. 17.1 - DST Tectonics |
Ben-Avraham et al (2012) |
Profiles and location map from the Gulf of Elat.
Ben-Avraham et al (2012) |
Fig. 17.2 - Gulf of Elat |
Ben-Avraham et al (2012) |
Profiles from the Zofar basin in the Arava valley.
Ben-Avraham et al (2012) |
Fig. 17.3 - Arava |
Ben-Avraham et al (2012) |
Profiles from the Dead Sea basin.
Ben-Avraham et al (2012) |
Fig. 17.4 - Dead Sea Basin |
Ben-Avraham et al (2012) |
Fig. 17.5
Profiles from the Sea of Galilee. A Location map showing main tectonic elements in the Sea of Galilee area. Bold lines indicated major faults, while dotted lines show the position of seismic profiles. Grey area shows the extent of the Yehudiyya transtensional one (after Shulman et al., 2004). Ben-Avraham et al (2012) |
Fig. 17.5A - Sea of Galilee |
Ben-Avraham et al (2012) |
Fig. 17.5 B and C
Profiles from the Sea of Galilee. B Profile from south of the lake showing both compressional and asymmetrical features (Zurieli, 2002). C Profile from north of the lake showing the Yehudiyya transtensional zone. Within the zone lies a compressional feature, the Qazrin structure, which is bordered on the west by the main fault zone (Shulman et al., 2004). Ben-Avraham et al (2012) |
Fig. 17.5 B and C - Sea of Galilee |
Ben-Avraham et al (2012) |
Fig. 17.6
(after Zilberman et al., 2000). Ben-Avraham et al (2012) |
Fig. 17.6 - Hula Basin |
Ben-Avraham et al (2012) |
Fig. 17.7
Ben-Avraham et al (2012) |
Fig. 17.7 - Ghab Basin |
Introduction
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Ben-Avraham et al (2008) |
Seismic profiles and location map from the Gulf of Elat
Ben-Avraham et al (2008) |
Fig. 2 - Gulf of Elat |
Source | Image | Description |
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Ben-Avraham et al (2008) |
Seismic profiles and location map from the Gulf of Elat
Ben-Avraham et al (2008) |
Fig. 2 - Gulf of Elat |
Source | Image | Description |
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Ben-Avraham et al (2008) |
Fig. 3
Moment release along the central subbasin.
Ben-Avraham et al (2008) |
Fig. 3 - Gulf of Elat |
To the north of the gulf's head lies the Arava Valley (Supplemental Figure 2), a 160-km-long morphotectonic
depression connecting the Gulf of Elat and the Dead Sea (Bentor et al. 1965, Ben-Avraham et al. 1979).
The southern part of the Arava Valley is marked by a structural saddle, resulting from mild compression
(Garfunkel 1981, Garfunkel et al. 1981, Garfunkel & Ben-Avraham 2001, Basson et al. 2002). This
compression can clearly be seen in upwarping Neogene and younger sediments. According to Ginat & Avni (1994)
the saddle, located 50-70 km north of the Gulf of Elat, was high and wide enough to allow a major drainage line
to flow westward across the Dead Sea Fault into the Negev during the Pliocene. In the southern section of the Arava,
just north of the Gulf of Elat, compressional features developed in the sedimentary fill (Basson et al. 2002).
These structures are young and formed as a result of recent changes in the geometry of the longitudinal master faults.
The Arava Valley is characterized by a series of elongated, en-echelon (left-stepping), tectonic subbasins filled with
clastic sediments, the Evrona, Ya'alon, and Zofar basins, and the Shizaf Basin north of the Zofar Basin (Supplemental Figure 2a)
(Bartov et al. 1998, Frieslander 2000). These basins are bound by subparallel high-angle strike-slip longitudinal faults
with normal displacement and range in depths from several hundred meters to a few kilometers and are filled with elastic
sediments. The southern ends of the Yaalon and Zofar basins seem to be aligned with the inter¬section of E-W Themed and
Paran dextral faults in the central Sinai-Negev and the Dead Sea Fault. These E-W faults predate left-lateral motion
along the Dead Sea Fault, as they themselves are displaced laterally. As such, they may have influenced the younger
structure along the Arava.
To the north, the Zofar and Shezaf basins are delimited by two NW-SE striking listric faults with large displacements.
In this area, the main strike-slip fault, the Arava Fault, is located on the eastern side of the valley (Garfunkel et al. 1981,
Garfunkel 1981, Atallah 1992). Predominance of strike-slip motion along the eastern boundary fault may explain the
asymmetry in the sedimentary fill of these subbasins. The Zofar Basin is bounded on the west and east by the Zofar
and Arava faults, respectively. Whereas motion along the Arava Fault is left-lateral strike-slip, the young motion
along the Zofar Fault is predominantly normal (Bartov et al. 1998, Frieslander 2000).
Seismic data indicates that the shallow Zofar Basin dips toward the north (Frieslander 2000). In addition,
a unique reversal in asymmetry occurs (Supplemental Figure 2b,c), where horizons within the southern part
of the basin dip toward the west, whereas in the northern section, horizons dip to the east. This is the
only known example along the Arava Valley where reversal in asymmetry occurs within a subbasin (instead of
between subbasins), and may indicate that the Zofar Basin can be structurally subdivided.
Source | Image | Description |
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Ben-Avraham et al (2008) |
Fig. 4a
The Dead Sea Basin. A Digital Terrain Map (DTM) image showing the main tectonic elements of the Dead Sea Basin. Faults are marked as heavy lines (dashed where inferred) (after Ben-Avraham 1997). The Dead Sea Basin is divided into two subbasins, which are separated by the Lisan Peninsula, which is a large buried salt diapir. The two basins are thought to be divided by a large oblique normal fault, the Boqeq Fault. The two main strands of the Dead Sea Fault in this area are the Jericho Fault, which borders the northern subbasin on the west, and the Arava Fault, which borders the southern subbasin on the east. Geological profiles shown in b and c are indicated by red lines. Ben-Avraham et al (2008) |
Fig. 4a - DTM Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4b
The Dead Sea Basin. E-W geological cross section showing the deep subbasin located in the northern section of the southern Dead Sea Basin. The section is based on seismic reflection, seismic refraction, and drill hole data. Numbers are densities in kg m−3. Gravity models are shown on top (SD 1, Sedom Deep-1 borehole). The deep subbasin is bordered by deep vertical faults; the Sedom Fault in the west and the Ghor Safi Fault, which does not extend to the surface, in the east (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4b - Geologic X-section Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4c
The Dead Sea Basin. N-S geological cross section based on prestack depth migration seismic reflection profiles, as well as on the seismic refraction, gravity, and drill hole data. The section shows that the area of the deep subbasin is the deepest part of the Dead Sea Basin. It is bordered by deep vertical faults, the Boqeq Fault in the north, and the Amazyahu Fault in the south. Numbers are densities in kg m−3. Gravity models are shown on top (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4c - Geologic X-section Dead Sea Basin |
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Ben-Avraham et al (2008) |
Fig. 4a
The Dead Sea Basin. A Digital Terrain Map (DTM) image showing the main tectonic elements of the Dead Sea Basin. Faults are marked as heavy lines (dashed where inferred) (after Ben-Avraham 1997). The Dead Sea Basin is divided into two subbasins, which are separated by the Lisan Peninsula, which is a large buried salt diapir. The two basins are thought to be divided by a large oblique normal fault, the Boqeq Fault. The two main strands of the Dead Sea Fault in this area are the Jericho Fault, which borders the northern subbasin on the west, and the Arava Fault, which borders the southern subbasin on the east. Geological profiles shown in b and c are indicated by red lines. Ben-Avraham et al (2008) |
Fig. 4a - DTM Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4b
The Dead Sea Basin. E-W geological cross section showing the deep subbasin located in the northern section of the southern Dead Sea Basin. The section is based on seismic reflection, seismic refraction, and drill hole data. Numbers are densities in kg m−3. Gravity models are shown on top (SD 1, Sedom Deep-1 borehole). The deep subbasin is bordered by deep vertical faults; the Sedom Fault in the west and the Ghor Safi Fault, which does not extend to the surface, in the east (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4b - Geologic X-section Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4c
The Dead Sea Basin. N-S geological cross section based on prestack depth migration seismic reflection profiles, as well as on the seismic refraction, gravity, and drill hole data. The section shows that the area of the deep subbasin is the deepest part of the Dead Sea Basin. It is bordered by deep vertical faults, the Boqeq Fault in the north, and the Amazyahu Fault in the south. Numbers are densities in kg m−3. Gravity models are shown on top (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4c - Geologic X-section Dead Sea Basin |
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Ben-Avraham et al (2008) |
Fig. 4a
The Dead Sea Basin. A Digital Terrain Map (DTM) image showing the main tectonic elements of the Dead Sea Basin. Faults are marked as heavy lines (dashed where inferred) (after Ben-Avraham 1997). The Dead Sea Basin is divided into two subbasins, which are separated by the Lisan Peninsula, which is a large buried salt diapir. The two basins are thought to be divided by a large oblique normal fault, the Boqeq Fault. The two main strands of the Dead Sea Fault in this area are the Jericho Fault, which borders the northern subbasin on the west, and the Arava Fault, which borders the southern subbasin on the east. Geological profiles shown in b and c are indicated by red lines. Ben-Avraham et al (2008) |
Fig. 4a - DTM Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4b
The Dead Sea Basin. E-W geological cross section showing the deep subbasin located in the northern section of the southern Dead Sea Basin. The section is based on seismic reflection, seismic refraction, and drill hole data. Numbers are densities in kg m−3. Gravity models are shown on top (SD 1, Sedom Deep-1 borehole). The deep subbasin is bordered by deep vertical faults; the Sedom Fault in the west and the Ghor Safi Fault, which does not extend to the surface, in the east (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4b - Geologic X-section Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4c
The Dead Sea Basin. N-S geological cross section based on prestack depth migration seismic reflection profiles, as well as on the seismic refraction, gravity, and drill hole data. The section shows that the area of the deep subbasin is the deepest part of the Dead Sea Basin. It is bordered by deep vertical faults, the Boqeq Fault in the north, and the Amazyahu Fault in the south. Numbers are densities in kg m−3. Gravity models are shown on top (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4c - Geologic X-section Dead Sea Basin |
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Ben-Avraham et al (2008) |
Comparison of
The location of gravity lows coincides with the subbasins. The transition zone between the Kalia and Jericho basins corresponds to a structural saddle on the Bouguer gravity map and marks the termination of the joint lake-land subbasin. The subbasins marked in this figure indicate the extent of sediment fill close to the surface and not at depth. The moment tensor solution is for the Main shock of the Mb. 5.1 earthquake on February 11, 2004 (after EMSC 2004). Aftershocks are also plotted (data from the Geophysical Institute of Israel). Strands of the main strike-slip fault (dashed lines) are after Garfunkel (1997). Ben-Avraham et al (2008) |
Fig. 5 - Dead Sea Basin sub-basins and Gravity Map |
Source | Image | Description |
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Ben-Avraham et al (2008) |
Fig. 4a
The Dead Sea Basin. A Digital Terrain Map (DTM) image showing the main tectonic elements of the Dead Sea Basin. Faults are marked as heavy lines (dashed where inferred) (after Ben-Avraham 1997). The Dead Sea Basin is divided into two subbasins, which are separated by the Lisan Peninsula, which is a large buried salt diapir. The two basins are thought to be divided by a large oblique normal fault, the Boqeq Fault. The two main strands of the Dead Sea Fault in this area are the Jericho Fault, which borders the northern subbasin on the west, and the Arava Fault, which borders the southern subbasin on the east. Geological profiles shown in b and c are indicated by red lines. Ben-Avraham et al (2008) |
Fig. 4a - DTM Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4b
The Dead Sea Basin. E-W geological cross section showing the deep subbasin located in the northern section of the southern Dead Sea Basin. The section is based on seismic reflection, seismic refraction, and drill hole data. Numbers are densities in kg m−3. Gravity models are shown on top (SD 1, Sedom Deep-1 borehole). The deep subbasin is bordered by deep vertical faults; the Sedom Fault in the west and the Ghor Safi Fault, which does not extend to the surface, in the east (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4b - Geologic X-section Dead Sea Basin |
Ben-Avraham et al (2008) |
Fig. 4c
The Dead Sea Basin. N-S geological cross section based on prestack depth migration seismic reflection profiles, as well as on the seismic refraction, gravity, and drill hole data. The section shows that the area of the deep subbasin is the deepest part of the Dead Sea Basin. It is bordered by deep vertical faults, the Boqeq Fault in the north, and the Amazyahu Fault in the south. Numbers are densities in kg m−3. Gravity models are shown on top (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4c - Geologic X-section Dead Sea Basin |
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Ben-Avraham et al (2008) |
Ben-Avraham et al (2008) |
Fig. 6 - Tectonic Map Sea of Galilee and Golan Heights |
Source | Image | Description |
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Ben-Avraham et al (2008) |
Ben-Avraham et al (2008) |
Fig. 6 - Tectonic Map Sea of Galilee and Golan Heights |
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Ben-Avraham et al (2008) |
Ben-Avraham et al (2008) |
Fig. 6 - Tectonic Map Sea of Galilee and Golan Heights |
While the dominant motion along the Dead Sea Fault is left-lateral slip, transtensional and transpressional
features are often present. Thus the motion is not purely strike-slip. In detail, the structure probably
changed as a result of reorganization of plate boundary. Therefore, the structure is characterized by extensional,
compressional, and asymmetrical structures varying in size from large scale (defining the general structure of the
Dead Sea Fault Valley) to small scale (defining the internal structure).
Oblique strike-slip motion is largely responsible for the formation of the physiographic valley and of the
pull-apart basins along the southern part of the Dead Sea Fault. This oblique plate separation resulted in
the creation of collapsed structures and features evident in the many lows, i.e., pull apart basins, along
the valley floor. Compressional features are caused by a step to the right of the main left-lateral strike-slip
fault strands resulting in the formation of transverse structural saddles that separate the different basins.
Within the pull-aparts, smaller compressional uplifts and saddles divide them into distinct subbasins.
Another characteristic feature of the Dead Sea Fault Valley is asymmetry, both in the large scale, as exhibited
in the differing topography of the eastern and western-flanking cliffs, and the small scale, i.e., within the basins
and subbasins. Large-scale asymmetry could have been influenced by the combined effect of nor-mal faulting and
isostatic uplift on existing topography (Wdowinski & Zilberman 1996).
On the smaller scale, asymmetry within the pull-apart basins can be explained by transform-normal extension.
Overlapping strike-slip faults, which are respon¬sible for the formation of these basins, together with
rearrangement of plate motions, can result in the formation of an extensional component [the "leaky transform,"
termed by Garfunkel (1981)]. This asymmetry is not a local phenomenon, with other pull-apart basins along continental
rift zones clearly showing asymmetry toward the main fault. Examples may be found in the Cariaco Basin in Venezuela
(Ben-Avraham & Zoback 1992), the Motagua fault system in Guatemala, Lake Baikal, Lake Tanganyika in the East African
rift system, and the North Anatolian Fault in Turkey.
Although it seems that motion along the Dead Sea Fault was initiated some 18 Ma ago (Garfunkel 1981, Garfunkel et al. 1981),
the basins started to evolve later owing to changes in the fault pattern, sometimes probably related to slight shifts
in the pole of rotation between the Arabian plate and the Sinai subplate. This introduced a component of oblique motion
(Joffe & Garfunkel 1987), which led to the formation of the pull-aparts. An interesting question is the spatial
evolution of the basins along the Dead Sea Fault, i.e., did the southern basins evolve before the northern ones,
or did they all develop more or less simultaneously? Also, how did each basin evolve? For example, did the
Dead Sea Basin develop from south to north as some researchers have suggested (e.g., ten-Brink & Ben-Avraham 1989),
or from the center first and then to the north and south (Ben-Avraham & Schubert 2006), or simultaneously through the
entire length (Lazar et al. 2006)?
One of the characteristics of the Dead Sea Fault is the deep seismicity. As demon¬strated by Aldersons et al. (2003,
most microearthquakes nucleate at rather deep depths — some 20-30 km below the surface. In this respect, the
Dead Sea Fault is quite different from the San Andreas Fault, where most earthquakes occur within the top 15
km of the subsurface, although some anomalously deep crustal earthquakes have been recorded at depths between
20-30 km (Bryant & Jones 1992). This may have to do with the differences in slip-rates between the two fault systems;
the slip along the Dead Sea Fault is only approximately one tenth [4 mm year (Wdowinski et al. 2004)]
the overall slip along the San Andreas Fault [-50 mm year-1 (van der Woerd et al. 2006)].
Another interesting characteristic is the low values of heat flow exhibited along the Dead Sea Fault, except for the
Sea of Galilee, which is located within a large field of Tertiary volcanism and has a relatively high heat flow,
and the southern Gulf of Elat, close to the Red Sea. The Dead Sea Basin exhibits the lowest heat flow values along
the fault, 38 mW m-2 (Ben-Avraham et al. 1978). Recently, Forster et al. (2007) reported higher vales in southern
Jordan. The deep seismically found by Aldersons et al. (2003) suggests that this may not represent the regional
heat flux, but this issue requires further study.
The deep seismicity and low heat flow values suggest that the deformation might be brittle in the lower crust.
This also supports recent claims (Ginzburg et al. 2007) that some of the transverse faults within the Dead Sea
Basin are deep normal faults extending to the basement and no listric faults as previously assumed.
Source | Image | Description |
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Ben-Avraham et al (2008) |
Fig. 1
Map of the Dead Sea Fault showing general relative plate motion from the opening of the Red Sea in the south to the collision in the Taurus/Zagros Mountains in the north. Strike-slip motion occurs between the Arabian plate and the Sinai subplate. Owing to this oblique slip, a series of pull-apart basins developed along its length. Ben-Avraham et al (2008) |
Fig. 1 - |
Ben-Avraham et al (2008) |
Seismic profiles and location map from the Gulf of Elat
Ben-Avraham et al (2008) |
Fig. 2 - |
Ben-Avraham et al (2008) |
Fig. 3
Moment release along the central subbasin.
Ben-Avraham et al (2008) |
Fig. 3 - |
Ben-Avraham et al (2008) |
Fig. 4a
The Dead Sea Basin. A Digital Terrain Map (DTM) image showing the main tectonic elements of the Dead Sea Basin. Faults are marked as heavy lines (dashed where inferred) (after Ben-Avraham 1997). The Dead Sea Basin is divided into two subbasins, which are separated by the Lisan Peninsula, which is a large buried salt diapir. The two basins are thought to be divided by a large oblique normal fault, the Boqeq Fault. The two main strands of the Dead Sea Fault in this area are the Jericho Fault, which borders the northern subbasin on the west, and the Arava Fault, which borders the southern subbasin on the east. Geological profiles shown in b and c are indicated by red lines. Ben-Avraham et al (2008) |
Fig. 4a - |
Ben-Avraham et al (2008) |
Fig. 4b
The Dead Sea Basin. E-W geological cross section showing the deep subbasin located in the northern section of the southern Dead Sea Basin. The section is based on seismic reflection, seismic refraction, and drill hole data. Numbers are densities in kg m−3. Gravity models are shown on top (SD 1, Sedom Deep-1 borehole). The deep subbasin is bordered by deep vertical faults; the Sedom Fault in the west and the Ghor Safi Fault, which does not extend to the surface, in the east (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4b - |
Ben-Avraham et al (2008) |
Fig. 4c
The Dead Sea Basin. N-S geological cross section based on prestack depth migration seismic reflection profiles, as well as on the seismic refraction, gravity, and drill hole data. The section shows that the area of the deep subbasin is the deepest part of the Dead Sea Basin. It is bordered by deep vertical faults, the Boqeq Fault in the north, and the Amazyahu Fault in the south. Numbers are densities in kg m−3. Gravity models are shown on top (after Ben-Avraham & Schubert 2006). Ben-Avraham et al (2008) |
Fig. 4c - |
Ben-Avraham et al (2008) |
Comparison of
The location of gravity lows coincides with the subbasins. The transition zone between the Kalia and Jericho basins corresponds to a structural saddle on the Bouguer gravity map and marks the termination of the joint lake-land subbasin. The subbasins marked in this figure indicate the extent of sediment fill close to the surface and not at depth. The moment tensor solution is for the Main shock of the Mb. 5.1 earthquake on February 11, 2004 (after EMSC 2004). Aftershocks are also plotted (data from the Geophysical Institute of Israel). Strands of the main strike-slip fault (dashed lines) are after Garfunkel (1997). Ben-Avraham et al (2008) |
Fig. 5 - |
Ben-Avraham et al (2008) |
Ben-Avraham et al (2008) |
Fig. 6 - |
The Levant continental margin is divided into two units. From south to north these are Negev, Judea-Samaria, major segments by the Carmel structure, which and Galilee-Lebanon (Figure 2b). Ben-Gai and Ben-Avraham extends from the Dead Sea fault into the eastern [1995] divided the Levant continental margin into two crustal Mediterranean.
...
On the basis of seismicrefraction [Ginzburg and Ben-Avraham, 1992; Ben-Avrahamet al., 2002], gravity [e.g., Ben-Avraham and Ginzburg,1990] and magnetics [Ben-Avraham and Ginzburg, 1986], the area onland was divided into several distinct crustal units. From south to north these are Negev, Judea-Samaria, and Galilee-Lebanon (Figure 2b). Ben-Gai and Ben-Avraham [1995] divided the Levant continental margin into two crustal segments north and south of the Cannel structure, which correspond to the division onland between Judea-Samaria and Galilee-Lebanon. This is clearly seen in the pattern of the magnetic field [Folkman, 1980; Ben-Avraham and Ginzburg, 1986; Rybakov et al., 2000] and suggests that these segments were probably formed through different breakup processes [Ginzburg et al., 1975; Neev and Ben-Avraham, 1977; Ben-Avraham and Hall, 1977; Ginzburg and Ben-Avraham, 1992]. Offshore, Ben-Avraham and Ginzburg [1990] distinguished between the crustal structure of the Levant Basin and the Eratosthenes seamount. The Levant Basin crustal unit is underlined by oceanic crust, covered by a 10-14 km thick sedimentary sequence [Ben-Avraham et al., 2002]. In this area only the upper 3 km of the subsurface are known in detail, offshore the southern seg¬ment of the Levant margin [Garfunkel, 1998]. However, little is known about the subsurface of the basin offshore the northern segment.
Description | Image | Source |
---|---|---|
Fig. 1 - DTM Map E Med. |
Fig. 1
Digital terrain map (DTM) of the eastern Mediterranean basin showing the Levant continental margin, major tectonic elements [after Walley, 1998; Bartov et al., 2000; Shulman et al., 2004], location of disturbances (Gaza (G) and Palmahim (P)), and major submarine canyons (Achziv (A) and Damur (D)). Note the different appearance of the relief north and south of the Carmel (C) (which branches from the Dead Sea fault system, onland as well as offshore. Extension of the Carmel fault beyond the continental margin is marked after Garfunkel and Almagor [1985]. White frame indicates extent of the study area. Inset shows general tectonic framework. DST, Dead Sea transform. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 2 - Formation of Levant Basin |
Fig. 2
Levant continental margin
Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 3 - Seismic Survey Lines |
Fig. 3
Location map of the three seismic surveys used for this study. Dotted lines present previously unpublished single-channel seismic data from offshore Lebanon, while dashed and solid lines are multichannel and single-channel data from the southern Levant, respectively. Figures mentioned in the text are indicated. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 4 - Magnetic Intensity Anomaly Map |
Fig. 4
Total magnetic intensity anomaly with contour interval of 10 nT in red [after Ben-Avraham and Ginzburg, 1986]. Nature and trend of the magnetic anomalies are discussed in the text. This map is superimposed on the bathymetry (black contours). The prominent magnetic anomaly in the northeastern corner of the map is located directly above the steep and narrow continental slope of the Lebanese margin. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 5 - Bathymetry/Topography and Top and Base of Messinian Evaporitic Sequence |
Comparison between
Note the general similarity between the present-day bathymetry within the basin (Figure 5a) and the pre-Messinian surface (Figure 5c). Dashed white line on bathymetric map marks the overlapping area between the maps. White arrows on Figures 5b and 5c mark a sharp jump in the contours discussed in the text. Black arrow on Figure 5b points to the area where the average depth of the top Messinian increases. Dashed black line on Figure 5a indicates the location of box-shaped scar delimiting the head of the Damur canyons (DC). Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 6 - Offshore Lebanon Profile |
Single-channel seismic profile 6 (top) offshore Lebanon with (bottom) interpretation showing the main sedimentary and tectonic features (see inset for location) (modified after Ben-Avraham and Ginzburg [1986] with permission from Elsevier). The thinly spaced high-frequency reflectors comprising unit P represent Plio-Pleistocene sediments, which thicken eastward. Below the Messinian evaporitic unit appears between the M (top) and N (bottom) horizons as a sequence of diffused horizons. At the base of the continental slope, these two sedimentary units are highly deformed forming the deformation belt (DB), which is discussed in the text. A prominent strike-slip fault, the Damur fault (DF), is visible within this deformation belt (see also Figure 15). The bathymetry of the continental slope is cut by a marine canyon (C), where most of the Plio-Pleistocene sequence was removed. A dashed line on the interpretation schematically indicates the original slope. West of the DB, reflectors within the Messinian evaporitic sequence exhibit low-amplitude undulations. At the surface, two bathymetric steps are observed above shallow growth faults (black lines in the interpretation). The magnetic intensity anomaly values (in nT) obtained along the profile are shown in Figure 6 (top). Thick black vertical lines indicate growth faults mentioned in the text, with possible strike slip motion (sense of motion is T, toward, A, away). The fault that limits the deformation belt on the west is a N-S trending sinistral strike-slip fault, while the Damur fault is a WSW-ENE trending dextral fault. D indicates salt diapirs. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 7 - Profile 11 |
Fig. 7
Single-channel seismic profile 11 showing similar sedimentary and tectonic features observed in Figure 6. See inset for location. The submarine canyon (C) is not perpendicular to the continental slope but is angled, and therefore the Plio-Pleistocene sequence was preserved to the west of this feature and on the steep slope (P). A dashed line schematically indicates the original slope. Deformations of the PlioPleistocene section, within the DB, are more intense than the area north of this profile (e.g., Figure 6), and the sedimentary units are less defined laterally. CFZ marks the extent of the Carmel fault zone in this area. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 8 - Profile 1 |
Single-channel seismic profile 1 showing similar sedimentary and tectonic features observed in Figure 6. See inset for location. The Plio-Pleistocene sequence thickens dramatically toward the east above the highly deformed Messinian evaporites. Pronounced growth faults cut through the sedimentary sequence, at least from the Messinian evaporites to the seafloor (marked by black lines in the blowup in bottom panel). Asterisks mark slope-perpendicular hummocky ridges resulting from sedimentary deformations within the DB. These ridges can be clearly observed in the northern part of the DB but are less distinguishable in its south (Figure 12b). D indicates salt diapirs discussed in the text. Other annotations are the same as in Figure 6. The strike-slip fault delimits the deformation belt in the west (sense of motion is T, toward, A, away). Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 9 - Profile S of Carmel Structure |
Fig. 9
Single-channel seismic profile located south of the Carmel structure showing different behavior of the Messinian-Recent sedimentary sequence than that observed to the north. Profile and interpretation are after Tibor and Ben-Avraham [1992] (with permission from Elsevier). See inset for location. The sigmoidal progradation sequence is low-angled because of accumulation of Nile-derived sediments in a low-energy depositional environment. The volume of these sediments is lower to nonexistent offshore Lebanon. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 10 - Profile 4 |
Fig. 10
Single-channel seismic profile 4 showing similar sedimentary and tectonic features observed in Figure 6. See inset for location. A high-angle, sigmoidal prograding clinoforms sequence (SC) of the Plio-Pleistocene section developed on the steep continental slope. The angle of this feature is markedly steeper than similar features observed south of the Carmel structure (e.g., Figure 9). In contrast to Figures 6 and 7 the original continental slope was preserved in this area. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 11 - Profile S of Carmel Structure |
Fig. 11
Single-channel seismic profile located south of the Carmel structure. The continental slope is much gentler, and the appearance of the Plio-Pleistocene section, in the deformation belt, is not as well defined as north of the Carmel structure. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 12 - Map of Major Tectonic Elements |
(a) Map of major tectonic elements in the central Levant and offshore above the DTM of the region. Colored lines mark features interpreted in this study (see legend for explanation). Dashed red lines indicate the transition between the northern and southern deformation belts, which cannot be mapped owing to a gap in the seismic data. The faults onland are based on the work by Walley [1998], Bartov et al. [2000], and Shulman et al. [2004]; and the Carmel fault zone (CFZ) offshore is according to Schattner et al. [2006]. White box indicates the location of Figure 12b, which presents a detailed bathymetric map offshore Lebanon (SHALIMAR survey [Ifremer, 2005]).
These elements are discussed in the text. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 13 - Isopach depth map of Messinian evaporitic sequence |
Fig. 13
Isopach depth map of the Messinian evaporitic sequence with thickness ranging from ~1200 m in the Levant Basin to 0 at the continental slope. In the south, this sequence fills pre-Messinian features (Palmahim and Gaza disturbances). White arrow points to a sharp bend in contours evident offshore Damur and discussed in the text (Damur canyons). Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 14 - Shelf Marginal Wedge S Lebanon vs. Central Israel Depositional Model |
Comparison of
All the profiles are aligned with a vertical dashed line that represents the location of the shelf edge. The profiles (in Figures 14a and 14b) are presented in the same vertical and horizontal scale. The ancient shelf edge, marked by an arrow on Figure 14a, is now part of the continental slope of southern Lebanon.
Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 15 - Shore Perpindicular Seismic Profiles and one Shore Parallel Seismic Profile |
Fig. 15
Sections of three shore perpendicular seismic profiles (profiles 5, 6, and 7) and one shore-parallel (profile B) cutting across the Damur fault (see text for explanation). Black lines mark the location of the Damur fault. Strike-slip motion is inferred by different thicknesses of the Messinian evaporites on both sides of the fault in the shore parallel profile B. The solid lines on profile B indicate the N horizon. Sense of motion is T, toward, A, away. Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Fig. 16 - Seismic Profiles 3, 4, & 5 |
Fig. 16
Three consecutive seismic profiles, from north to south, profiles 3, 4, and 5, showing local narrowing of the deformation belt offshore Damur (black arrows). The narrowing occurs just north of the Damur fault (marked by a blue line on Figure 12). Ben-Avraham et al (2006) |
Ben-Avraham et al (2006) |
Elias et al (2007) and previous researchers (Morhange et al, 2006) examined uplifted benches on the Lebanese coast between Sarafand and Tripolis; some in the vicinity of Tabarja (~20 km. NE of Beirut). They radiocarbon dated fossil Vermetids on the tops of these benches in order to estimate when the bench top was last in the sub tidal zone (which approximates mean sea level). They identified four uplifts from
- Fig 2c Bench elevations from Elias et al (2007)
Figure 2C
Projected total station measurements of bench elevations relative to LMSL (living vermetid surface in swash zone). Note signifi cant scatter in elevation measurements on fossil levels, particularly B1 and B4, likely because of sub-levels with rounded edges and of irregularities due to deep pitting by microkarst.
Elias et al (2007)- Fig 1 Coastal uplift for the northern DST
from Elias et al (2007)Fig.1
- Location map of the Mediterranean (created using GMT) showing the Levant continental margin
- Dendropoma petraeum sampling sites are marked (red circles) on the regional DTM (courtesy — J.K. Hall). Circle size denotes the age of the sample in calibrated years before present. White lines denote major plate boundaries and tectonic faults mentioned in the text. The four segments appear as
Faults are marked after Westaway (2004) and Schattner et al. (2006). Abbreviations:
- GL=Galilee–Lebanon
- LM=Lebanon Mountains
- NL=Northern Lebanon
- WS=Western Syria
- CS= Carmel structure
- CF= Carmel fault
- CFZ= Carmel fault zone
- RF=Roum fault
- WLF, Western Lebanon flexure
- LRB=Lebanese restraining bend
- DSF= Dead Sea fault
- Elevation of K–D contacts above biological sea level plotted against latitude of sampling sites. A gray bar of ±10 cm marks the error of measurement around the present day sea level. Measured values are marked (red) denoting the sample age in calibrated years before present. Time weighted tectonic displacement calculations are marked (blue) with vertical error bars of ±20 cm
Sivan et al (2010)
3 or more [sizeable Mw = ~7.5] earthquakesin the past ca. 6-7 ka. They attributed the latest uplift (B1) to the 551 CE Beirut Quake while the earlier events (B2, B3, and B4) were no more precisely dated than between ~5000 BCE and 551 CE. Bench uplift on the earlier events (B2, B3, and B4) would likely have been due to uplift on the Mount Lebanon Thrust system - as was surmised for Event B1 and the 551 CE Beirut Quake.
within the range of error (±10 cm) at present day mean sea levelin the northern Israeli coast to up to +390 cm at the Orontes north site in Turkey. They noted the following
This positive gradient in vertical tectonic displacement could have been explained by elastic bending of the plate. However, studies from the last several decades show that the region is extensively faulted and folded (e.g., Freund and Tarling, 1979; Beydoun, 1981; Ron, 1987; Walley, 1998; Ben-Avraham et al., 2006; Schattner et al., 2006; Elias et al., 2007; Carton et al., 2009). Therefore the gradient suggests a northward increase in brittle failure of the Levantine coast during the Late Holocene.They divided the coast into structural segments which they described and interpreted tectonically in the table below:
Segment | Description | Interpretation |
---|---|---|
south of Galilee–Lebanon | south of the Carmel fault | The smallest vertical displacement values 1.5 cm (Habonim site, Table 1), calculated for northern Israel, correspond well with the zero displacement reported by Wdowinski et al. (2004) based on GPS measurements. Negligible vertical displacement was also reported based on archaeological evidence: the Galilee coast was stable for the last 3000– 4000 years (Sivan and Galili, 1999), while coastal sites in Caesarea indicate stability for the last 2000 years (Sivan et al., 2004). Since northern Israel was shown to be in isostatic equilibrium (Segev et al., 2006) the negligible vertical displacements suggest that it is tectonically stable (vertical displacements) during the last two millennia. Hence any measured change in relative sea level in this region stems conclusively from eustasy. |
Galilee–Lebanon | bounded by the Carmel and Roum faults (south and north) | Further north along the coast of southern Lebanon (Galilee– Lebanon structural segment) slightly larger values are calculated for the vertical tectonic displacement, between 50 and 150 cm (sites ZireSaida, Ras Qantara, Hotel Mounes and Ras Abou Zeid, Table 1; Marriner and Morhange, 2005; Morhange et al., 2006). Along this segment, which is bounded by the Roum fault in the north, the topography becomes progressively more prominent (∼1000 m) northwards (Schattner et al., 2006 and references therein). Internal deformations produced by the nearby DSF are manifested by second order southwest trending dextral faults (Ron, 1987; Walley, 1998) which extend to the Levantine coast. Our results show that differential vertical displacement occurs along the coast of the Galilee–Lebanon segment during the Holocene |
Lebanon Mountains | consists of the Western Lebanon Flexure (Walley, 1998) of the highly elevated part of the Lebanese restraining bend. This segment is bounded to the west by the marine “Beirut–Tripoli thrust” (after Daëron et al., 2001) | Much higher displacement values are calculated for the Lebanon Mountains segment north and east of the Roum fault. Both this segments and the Galilee–Lebanon are located along the Lebanese restraining bend, a right-step of the sinistral DSF along the NNE trending Yammunneh fault (Fig. 1). This slight divergence from the Nstriking axis of the DSF induces crustal overlap which is mainly absorbed by north-westward push of the Lebanon Mountains segment against the marine Beirut–Tripoli thrust (Schattner et al., 2006 and references therein). The highly elevated topography of this segment (∼3000 m) is not in isostatic equilibrium (Segev et al., 2006). It extends from the Lebanon and Anti-Lebanon mountains through the western Lebanon flexure to the coastline, where our results show high displacement values for the Holocene period, ranging between 60 and 340 cm (sites Phare, Palmier, Hannouch, Ras Koubba, Selaata, Ras Madfoun, Fidar sud, Nahr Ibrahim, North of Bouar, Safra, Tabarja, and South of Tabarja, Table 1; Sanlaville et al., 1997; Morhange et al., 2006). |
Northern Lebanon | a low laying topography juxtaposed from the south to the Cyprus arc convergent plate boundary | Only one Dendropoma site was measured along the coast of the northern Lebanese segment (site Tell Soukas, Table 1; Fig. 1; Sanlaville et al., 1997). In this low topography segment the calculated vertical displacement is 41 cm. The site is located closely south to the intersection of the Levantine coast with the Larnaka ridge (part of the Cyprus arc convergence plate margin). North of the Larnaka ridge, however, displacements show higher values, ranging between 40 and 130 cm (sites Ras Ibn Hani, Ras el Karm (Ibn Hani) and Maksar, Table 1; Sanlaville et al., 1997). This jump in displacement values reflects the active convergence across the easternmost Cyprus arc, where the latter sites are overthrusted. |
Western Syria | consists a part of the triple junction between the DSF, East Anatolian fault and the Cyprus arc. Two main ridges of the arc deform the coasts of this segment — Latakia and Larnaka ridges (e.g., Kempler, 1998; Robertson, 1998). | A similar change in the amount of vertical displacement is observed further north across the Latakia Ridge (part of the Cyprus arc convergence plate margin; Fig. 1). In Ras el Bassit site, south of the ridge, values range between 70 and 106 cm, while north of it vertical displacement extends between 142 and 360 cm — the highest values obtained along the entire margin (sites Orontes north, Table 1; Pirazzoli et al., 1991; Sanlaville et al., 1997). The northernmost sites (sites Guverdijne Kaya south, Table 1; Sanlaville et al., 1997) are also displaced and are located along the Kyrenia–Misis Ridge of the Cyprus arc. Here the values range between 85 and 230 cm, yet no comparable sites were sampled across the ridge |
Elias, A., et al. (2007). "Active thrusting offshore Mount Lebanon: Source of the tsunamigenic A.D. 551 Beirut-Tripoli earthquake." Geology 35(8): 755-758.
Morhange, C., et al. (2006). "Late Holocene relative sea-level changes in Lebanon, Eastern Mediterranean." Marine Geology 230(1): 99-114.
Sivan, D., Schattner, U., Morhange, C., Boaretto, E. (2010). "What can a sessile mollusk tell
about neotectonics?" Earth and Planetary Science Letters 296(3): 451-458.
Source | Image | Description |
---|---|---|
Aldersons and Ben-Avraham (2014) |
Fig. 3.1
Depth section of well-constrained seismicity (410 earthquakes, 1984–1997) along the Dead Sea transform (DST) from Aqaba-Elat to the Sea of Galilee. The square grid fill defines the Dead Sea Basin on the map. Conrad and Moho discontinuities from Ginzburg et al. (1981) (From Aldersons et al. 2003) Aldersons and Ben-Avraham (2014) |
Fig. 3.1 - Depth section of well-constrained seismicity |
Aldersons and Ben-Avraham (2014) |
Fig. 3.2
MW 5.3 earthquake of 11 February 2004, 08 h 15 m. Epicenters according to ISC, EMSC, JSO Bulletin, HOF: Hofstetter et al. (2008), EAT: Al-Tarazi et al. (2006), ELN: Abou Elenean et al. (2009), GII+JSO: this study (separate locations from GII seismograms alone and from JSO seismograms alone in dark grey, connected to final location by red lines). Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.2 - MW 5.3 earthquake of 11 February 2004 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.3
MW 5.3 earthquake of 11 February 2004, 08 h 15 m. Depths and uncertainties according to ELN: Abou Elenean et al. (2009), HOF: Hofstetter et al. (2008), EAT: Al-Tarazi et al. (2006), ALD: this study, JSO Bulletin, pP (ISC), ISC and EMSC. Upper-crustal depths in yellow, lowercrustal depths in dark blue Aldersons and Ben-Avraham (2014 |
Fig. 3.3 - MW 5.3 earthquake of 11 February 2004 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.4
Depth distribution for the 188 earthquakes (1986–2001) of the MPX dataset in the Dead Sea basin (0.3 ≤ ML ≤ 3.5), and depth of the MW 5.3 earthquake of 11 February 2004.
Aldersons and Ben-Avraham (2014) |
Fig. 3.4 - Depth distribution for the 188 earthquakes (1986–2001) |
Aldersons and Ben-Avraham (2014) |
Fig. 3.5
Focal depths of well-constrained seismicity in the Dead Sea basin (30°25′N ≤ Lat ≤ 32°12′N, 34°52′E ≤ Lon ≤ 35°40′E). Braeuer et al. (2012b) in the southern Dead Sea basin (31°00′N ≤ Lat ≤ 31°28′N, 35°18′E ≤ Lon ≤ 35°39′E).
Aldersons and Ben-Avraham (2014) |
Fig. 3.5 - Depth distribution for the 188 earthquakes (1986–2001) |
Aldersons and Ben-Avraham (2014) |
Fig. 3.6
MW 6.3 earthquake of 11 July 1927: instrumental epicenters and macroseismic epicentral regions.
Uncertainty ellipses in yellow. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.6 - MW 6.3 earthquake of 11 July 1927 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.7
Isoseismal map (MMI) of the earthquake of 11 July 1927 according to Vered and Striem (1977). ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from ISC-GEM (Storchak et al. 2013). The area in red (MMI=IX) defines the macroseismic epicentral region according to the authors. Israel Transverse Mercator (ITM) grid coordinates (km). (Redrawn from original publication) Aldersons and Ben-Avraham (2014) |
Fig. 3.7 - Isoseismal map (MMI) of the earthquake of 11 July 1927 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.8
Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Mean Intensities determined by Avni (1999), and published by Zohar and Marco (2012). ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from ISC-GEM (Storchak et al. 2013). The area in red defines the macroseismic epicentral region (drawn by hand) according to this dataset. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.8 - Isoseismal map (MSK) of the earthquake of 11 July 1927 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.9
Preferred epicenter, and tentative causative fault (Version 1) of the MW 6.3 earthquake of 11 July 1927. Epicenter at red concentric circles. Epicentral location uncertainty as dashed yellow ellipse. Subsurface causative fault trace as red dashed line (36 km long). Isoseismal intensity MSK=VIII curve produced by kriging of Mean Intensities determined by Avni (1999), and published by Zohar and Marco (2012). Mean Intensity (MSK) values determined by Avni (1999) in yellow. Macroseismic epicentral region, according to this dataset, drawn by hand in red. ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from Storchak et al. (2013). White asterisk on the northern shore of the Dead Sea: alledged location of photograph in Fig. 3.11. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.9 - Preferred epicenter, and tentative causative fault (Version 1) of the MW 6.3 earthquake of 11 July 1927 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.10
Preferred epicenter, and tentative causative fault (Version 2) of the MW 6.3 earthquake of 11 July 1927. Epicenter of the 1927 earthquake at red concentric circles. Epicentral location uncertainty as dashed yellow ellipse. Subsurface causative fault trace as red dashed line (25 km long). Epicenter of the MW 5.3 earthquake of 11 February 2004 at black concentric circles, and subsurface fault trace as black dashed line. 1927 Isoseismal intensity MSK=VIII curve produced by kriging of Mean Intensities determined by Avni (1999), and published by Zohar and Marco (2012). Mean Intensity (MSK) values determined by Avni (1999) in yellow. Macroseismic epicentral region, according to this dataset, drawn by hand in red. ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from Storchak et al. (2013). White asterisk on the northern shore of the Dead Sea: alledged location of photograph in Fig. 3.11. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.10 - Preferred epicenter, and tentative causative fault (Version 2) of the MW 6.3 earthquake of 11 July 1927 |
Aldersons and Ben-Avraham (2014) |
Fig. 3.11
Ground fissures caused by the 1927 earthquake. Possible location close to the Jordan River estuary at the Dead Sea. View probably from south to north, taken in the morning according to the direction of the shade (see Figs. 3.9 or 3.10 for possible location). Estimated intensity MSK=VIII (IX) (Photograph from American Colony, Jerusalem. Matson Photograph Collection) Aldersons and Ben-Avraham (2014) |
Fig. 3.11 - Ground fissures caused by the 1927 earthquake |
Aldersons and Ben-Avraham (2014) |
Fig. 3.12
Rheology of the Dead Sea Basin
Aldersons and Ben-Avraham (2014) |
Fig. 3.12 - Rheology of the Dead Sea Basin |
Aldersons and Ben-Avraham (2014) |
Fig. 3.13
Surface Heatow from the Red Sea axis to the Dead Sea basin
95 % confidence and prediction bands in red and blue respectively Aldersons and Ben-Avraham (2014) |
Fig. 3.13 - Rheology of the Dead Sea Basin |
Aldersons and Ben-Avraham (2014) |
Fig. 3.14
Temperature distribution along the Dead Sea Fault from the Sea of Galilee to the Gulf of Aqaba-Elat. Temperatures derived from the surface heat flow (top). Seismogenic zone (red dashed line) derived from the EMSC 2011 catalogue (Godey et al. 2006) for the entire profile, Aldersons et al. (2003) and Shamir (2006) for the Dead Sea area, and Navon (2011) for the Sea of Galilee area (From Shalev et al. 2012) Aldersons and Ben-Avraham (2014) |
Fig. 3.14 - Temperature distribution along the Dead Sea Fault from the Sea of Galilee to the Gulf of Aqaba-Elat |
Aldersons and Ben-Avraham (2014) |
Fig. 3.15
Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Mode Intensities determined by Avni (1999), and published by Zohar and Marco (2012). ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from ISC-GEM (Storchak et al. 2013). The area in red (MSK=IX) defines the macroseismic epicentral region (drawn by hand) according to this dataset. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.15 - Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Mode Intensities determined by Avni (1999) |
Aldersons and Ben-Avraham (2014) |
Fig. 3.16
Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Max Intensities determined by Avni (1999), and published by Zohar and Marco (2012). ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from ISC-GEM (Storchak et al. 2013). The area in red (MSK=IX) defines the macroseismic epicentral region (drawn by hand) according to this dataset. Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.16 - Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Max Intensities determined by Avni (1999) |
Aldersons and Ben-Avraham (2014) |
Fig. 3.17
Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Modal Intensities determined by Avni (1999) and Corrected for site attributes (± 1 unit MSK) by Zohar and Marco (2012). ISS (1927): instrumental epicenter from ISS. SHA (1993): instrumental epicenter from Shapira et al. (1993). ISC-GEM: instrumental epicenter from ISC-GEM (Storchak et al. 2013). The area in red (MSK=VIII) defines the macroseismic epicentral region (drawn by hand) according to this dataset. The region in green defines the macroseismic epicentral region according to the regressions of Zohar and Marco (2012). Israel Transverse Mercator (ITM) grid coordinates (km) Aldersons and Ben-Avraham (2014) |
Fig. 3.17 - Isoseismal map (MSK) of the earthquake of 11 July 1927 produced by kriging of Modal Intensities determined by Avni (1999) |
Aldersons and Ben-Avraham (2014) |
Table 3.1
Velocity model Dead Sea 2013 (in bold) and perturbations Aldersons and Ben-Avraham (2014) |
Table 3.1 - Velocity model Dead Sea 2013 |
Aldersons and Ben-Avraham (2014) |
Table 3.2
Selected parameters for the MW 5.3 earthquake of 11 February 2004, 08 h 15 m, according to various sources Aldersons and Ben-Avraham (2014) |
Table 3.2 - parameters for the MW 5.3 earthquake of 11 February 2004 |
Aldersons and Ben-Avraham (2014) |
Table 3.3
Time span of each dataset, Relative Frequency of the seismicity in the upper crust and lower crust, and Seismogenic Thickness TS according to two criteria Aldersons and Ben-Avraham (2014) |
Table 3.3 - Time span and Seismogenic Thickness |
Aldersons and Ben-Avraham (2014) |
Table 3.4
Earthquake of 11 July 1927: main parameters according to various sources of instrumental results Aldersons and Ben-Avraham (2014) |
Table 3.4 - Earthquake of 11 July 1927: main parameters |
Aldersons and Ben-Avraham (2014) |
Table 3.5
Earthquake of 11 July 1927. Source parameters from spectral amplitudes of surface waves (Ben-Menahem et al. 1976) Aldersons and Ben-Avraham (2014) |
Table 3.5 - Earthquake of 11 July 1927. Source parameters from spectral amplitudes |
Aldersons and Ben-Avraham (2014) |
Table 3.6
Depth estimates according to Medvedev’s methods and Shebalin’s method. MSK Intensities from Avni (1999): MD (Mode), MN (Mean), MX (Max); MSK Intensities corrected by Zohar and Marco (2012): MD-C1 (Mode Corrected 1); MMI Intensities from Vered and Striem (1977): VRD. I0: highest Intensity isoseismal. m-MED and m-SHB: Isoseismal Index number according to Medvedev and Shebalin respectively. MS: Surface Wave Magnitude according to Eq. 3.7 from Ambraseys (2006). h: source depth (km) according to Medvedev’s methods 1 (MED- 1) and 2 (MED-2), and Shebalin (SHB). Valid depths in bold. Cells with inconsistent values have been greyed out Aldersons and Ben-Avraham (2014) |
Table 3.5 - Earthquake of 11 July 1927. Source parameters from spectral amplitudes |
Description | Image | Source |
---|---|---|
Fig. 1 - Recorded Seismicity |
Fig. 1
Recorded seismicity of the study area from 1900 to 2002 (Geophysical Institute of Israel, available online at http://www.gii.co.il). Black lines are the active faults. Abbreviations are:
The locations of the two ML≥6.0 earthquakes from the 20th century are indicated by the year numbers. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 2 - Assumed Historical Quakes |
Fig. 2
Location and year date of the 14 historical earthquakes (MS≥6.0) along the Dead Sea Fault System (DSFS) of the last 1500 years (for details see Table 1). Dashed circles indicate the locations after shifting the epicentres onto the nearest major active fault. JW:1202 and 1759b should be swapped. 749 is too far south. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 3 - Assumed Historical Quake Breaks |
Fig. 3
Location and year date of the 14 historical earthquakes (MS≥6.0) along the Dead Sea Fault System (DSFS) of the last 1500 years (for details see Table 1). Dashed circles indicate the locations after shifting the epicentres onto the nearest major active fault. JW:1202 and 1759b should be swapped. 749 is too far south. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 4 - Fault Segments (3D) |
Fig. 4
3D model sketch of the study area. The numbers at the various fault segments give the applied tectonic loading rate (slip rate) in mm/yr below the locking depth w at 12.5 km. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 5a - ∆CFS since 551 CE South DSF |
Fig. 5a
Evolution of ΔCFS for five fault zones along the Dead Sea Fault System (DSFS) from 551 (ΔCFS= 0) to 2005. In order to suppress unrealistic edge effects at the endings of each rupture plane, the five last points are smoothed. Plotted segments are shown on the overview maps as thick black lines. Lines with increasing gray scale represent the stress state of the given year. Stars indicate the position of the earthquake. Dashed lines are the 0 ΔCFS level and the thin grey lines in panels a and b are the 4 MPa ΔCFS level. Note the increased ΔCFS values in year 2005 for a 30-km-long section of the eastern Dead Sea Fault (a) and a 90-km-long section for the Jordan Fault (b) which could according to Eq. (1) produce MS = 6.8 and MS = 7.4 earthquake, respectively. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 5b - ∆CFS since 551 CE North DSF |
Fig. 5b
Evolution of ΔCFS for five fault zones along the Dead Sea Fault System (DSFS) from 551 (ΔCFS= 0) to 2005. In order to suppress unrealistic edge effects at the endings of each rupture plane, the five last points are smoothed. Plotted segments are shown on the overview maps as thick black lines. Lines with increasing gray scale represent the stress state of the given year. Stars indicate the position of the earthquake. Dashed lines are the 0 ΔCFS level and the thin grey lines in panels a and b are the 4 MPa ΔCFS level. Note the increased ΔCFS values in year 2005 for a 30-km-long section of the eastern Dead Sea Fault (a) and a 90-km-long section for the Jordan Fault (b) which could according to Eq. (1) produce MS = 6.8 and MS = 7.4 earthquake, respectively. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 5c - ∆CFS since 551 CE Carmel Fault |
Fig. 5c
Evolution of ΔCFS for five fault zones along the Dead Sea Fault System (DSFS) from 551 (ΔCFS= 0) to 2005. In order to suppress unrealistic edge effects at the endings of each rupture plane, the five last points are smoothed. Plotted segments are shown on the overview maps as thick black lines. Lines with increasing gray scale represent the stress state of the given year. Stars indicate the position of the earthquake. Dashed lines are the 0 ΔCFS level and the thin grey lines in panels a and b are the 4 MPa ΔCFS level. Note the increased ΔCFS values in year 2005 for a 30-km-long section of the eastern Dead Sea Fault (a) and a 90-km-long section for the Jordan Fault (b) which could according to Eq. (1) produce MS = 6.8 and MS = 7.4 earthquake, respectively. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 5d - ∆CFS since 551 CE Roum Fault |
Fig. 5d
Evolution of ΔCFS for five fault zones along the Dead Sea Fault System (DSFS) from 551 (ΔCFS= 0) to 2005. In order to suppress unrealistic edge effects at the endings of each rupture plane, the five last points are smoothed. Plotted segments are shown on the overview maps as thick black lines. Lines with increasing gray scale represent the stress state of the given year. Stars indicate the position of the earthquake. Dashed lines are the 0 ΔCFS level and the thin grey lines in panels a and b are the 4 MPa ΔCFS level. Note the increased ΔCFS values in year 2005 for a 30-km-long section of the eastern Dead Sea Fault (a) and a 90-km-long section for the Jordan Fault (b) which could according to Eq. (1) produce MS = 6.8 and MS = 7.4 earthquake, respectively. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 5e - ∆CFS since 551 CE Yammouneh Fault |
Fig. 5e
Evolution of ΔCFS for five fault zones along the Dead Sea Fault System (DSFS) from 551 (ΔCFS= 0) to 2005. In order to suppress unrealistic edge effects at the endings of each rupture plane, the five last points are smoothed. Plotted segments are shown on the overview maps as thick black lines. Lines with increasing gray scale represent the stress state of the given year. Stars indicate the position of the earthquake. Dashed lines are the 0 ΔCFS level and the thin grey lines in panels a and b are the 4 MPa ΔCFS level. Note the increased ΔCFS values in year 2005 for a 30-km-long section of the eastern Dead Sea Fault (a) and a 90-km-long section for the Jordan Fault (b) which could according to Eq. (1) produce MS = 6.8 and MS = 7.4 earthquake, respectively. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Fig. 6 - Est. Fault Stress in 2005 |
Fig. 6
Present-day stress state of the Dead Sea Fault System. Displayed are the cumulative ΔCFS values calculated for the varying orientation of each fault in 1-km steps. The ΔCFS values include the coseismically induced stress changes superimposed by the stress effect from tectonic loading for the period from 551 to 2005. Note the large positive values along the Jordan Fault and the eastern segment of the Dead Sea Fault. Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Table 1 - Model parameters for historical earthquakes |
Table 1
Model parameters for the historical earthquakes Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Table 2 - Results of ΔCFS analysis |
Table 2
Results of ΔCFS analysis Heidbach and Ben-Avraham (2007) |
Heidbach and Ben-Avraham (2007) |
Crustal deformation and seismicity in the Levant region are mainly related to the plate-boundary Dead Sea Fault (DSF) and the intraplate Carmel-Gilboa-Faria Fault System (CGFS). The intersection between these two major fault systems is generally treated as an ~35-km-wide deformation belt stretched between the Faria and Gilboa Faults. Here, we present spatial and temporal analysis of faulting near this intersection. Our analysis is based on new geological mapping, new high-resolution airborne light detection and ranging (LiDAR) data, and seismic reflection profiles and indicates northward migration and localization of the intersection over time since the early Miocene. We discovered and mapped outcrops of Miocene, Pliocene, and Pleistocene rock units as well as faults and reconstructed the evolution of deformation. Three main tectonic phases were identified in this area covering the following periods: the early-middle Miocene, the late Mio¬cene-Pliocene, and the Quaternary. During the first phase, the DSF and the CGFS developed, and the CGFS faulted along a series of subparallel grabens and elongated NW-SE, between the southernmost Faria and the northernmost Gilboa faults, over a belt width of —35 km. During the second phase, deformation along the CGFS migrated northward and concentrated at an ~6-km-wide zone in the northern Faria Anticline. During the third stage, small-scale northward migration and localization of the deformation to a width zone of ~1-2 km at the southern boundary of the Beit She'an Valley occurred. Faults from the third phase reveal both sinistral and nor¬mal faulting. We propose that the currently active intersection between the DSF and the CGFS is located east of this localized deformation zone, near a right step of the DSF and the uplifted area of Tel Al-Qarn in the eastern Jordan Valley. We suggest that the northward migration and localization of this intersection are related to regional tectonic changes, spatial variations in the Sinai-Arabia Euler pole, and the localization of deformation along the DSF.
The CGFS, a major intraplate fault within the Sinai plate (Fig. 1), defines the boundary between two major tectonic blocks within the Sinai plate (e.g., Dembo et al., 2015; Gomez et al., 2020; Hamiel and Piatibratova, 2021). The CGFS is ~80 km long, branches from the DSF at the central part of the Jordan Valley segment, and continues in the ~NW direction to the northern tip of Mt. Carmel and farther northwestward into the Mediterranean continental shelf (e.g., Garfunkel and Almagor, 1984; Ben-Gai and Ben-Avraham, 1995; Hofstetter et al., 1996). The Carmel, Gilboa, and Faria Faults comprise the main fault segments of this system (Fig. 1B). The Carmel Fault, the northwesternmost fault segment of the CGFS, is an oblique, sinistral-normal fault (e.g., Ben-Gai and Ben-Avraham, 1995; Achmon and Ben-Avraham, 1997; Sadeh et al., 2012; Dembo et al., 2015). The Gilboa Fault in the north and the Faria Fault in the south are the two main easternmost segments of this system (Fig. 1). They are normal faults that dip in the NE direction (Hatzor and Reches, 1990; Shaliv eta., 1991). Recent geodetic studies (e.g., Sadeh et al., 2012; Hamiel et al., 2016, 2018; Gomez et al., 2020; Hamiel and Piatibratova, 2021) showed that the current strike-slip rate along the DSF decreases from ~5 mm/yr south of the intersection with the CGFS to ~4 mm/ yr north of it, which suggests that slip is transferred from the DSF to the CGFS and that an active triple junction is located at the intersec¬tion between them. These studies also calculated an oblique strike-slip motion of 0.5-1.6 mm/yr across main segments of the CGFS and proposed that the observed reduction in slip rate along the DSF is due to transfer of slip to the CGFS. Hamiel and Piatibratova (2021) demonstrated a relative motion of 0.8 ± 0.4 mm/yr, sub-parallel to the DSF, between the southern and central Sinai tectonic blocks, i.e., south and north of the CGFS. This result was found to be in a good agreement with the CGFS total slip rate vector and the observed reduction in slip rate along the DSF near the intersection with the CGFS.
The intersection between the DSF and the CGFS is generally treated as an ~35-km-wide deformation zone between the Faria and Gilboa Faults and the central Jordan Valley segment of the DSF (e.g., Shaliv et al., 1991; Segev et al., 2014; Dembo et al., 2015). The northern end of this intersection zone is defined by the Beit She'an Valley, which is located between the Gilboa Fault and the DSF (Fig. 1B). However, it is unclear whether the entire zone between the Gilboa and Faria Faults is active, and if not, where exactly this intersection occurs and how it evolved over time since its formation in the Miocene. In this study, we investigate the spatial and temporal variations in the deformational processes of this area and better locate the intersec¬tion of the DSF and CGFS. To accomplish these tasks, we performed an integrated geological and geophysical study of faulting in this region.
The study area extends from the Faria Fault in the south, through the Faria Anticline,
and to the southern part of the down-faulted basin of the Beit She'an Valley in the north
(Fig. 1C). This area developed as an interaction zone between the NW-trending CGFS and the
N-trending tectonic system of the DSF. The axis of the Faria Anticline is in the SSW—NNE direction.
The rock formations exposed in this region belong to several stratigraphic groups, ranging
from the Jurassic Arad Group to the Quaternary Dead Sea Group. While old rock formations, i.e.,
Jurassic and Lower Cretaceous rock formations, are exposed at the core of the Faria Anticline,
younger rocks of the Upper Cretaceous to Paleocene Mount Scopus and the Eocene Avedat Groups
are exposed along the eastern flank of the anticline, forming the western boundary of the Jordan
Valley (Mimran, 1984; Shaliv et al., 1991). The Faria Anticline is traversed by several NW-trending
faults that demonstrate vertical displacements ranging from 500 m to 800 m. The major faults
are the Faria Fault in the south and the southern boundary of the Beit She'an Valley in the north.
Between the Faria Fault and Beit She'an Valley, less prominent faults also oriented NW, such as the
Buqea and Tayasir Faults (Fig. 1), are observed (Shaliv et al., 1991; Mimran et al., 2016).
The Faria Anticline developed during the late Turonian—early Eocene as part of the Syrian arc structures
(Krenkel, 1924) and was reactivated during the Oligocene—early Miocene as part of a tectonic phase
that followed plate separation along the Red Sea (Mimran, 1984; Shaliv et al., 1991). Later, during
the Miocene, this region was faulted along the north-south-trending DSF and along the NW-trending CGFS
to form a major intersection area (Freund et al., 1970; Garfunkel, 1981; Mimran, 1984; Shaliv et al.,
1991; Rozenbaum et al., 2016). The simultaneous activity of faulting of the two systems is still ongoing
and divides the Sinai Plate into two tectonic domains south and north of the CGFS (Ben-Avraham and Ginzburg,
1990; Hofstetter et al., 1996; Sadeh et al., 2012; Dembo et al., 2015; Gomez et al., 2020; Hamiel and
Piatibra-tova, 2021). Early Miocene faulting was accompanied by extensive volcanic activity, which is
termed the Lower Basalt (e.g., Schulman, 1962). Near the Gilboa Fault (Fig. 1B), this volcanic phase
started at ca. 17.5 Ma (Shaliv et al., 1991). Normal faulting accompanying this phase probably
occurred under the same tensile regime that triggered volcanic eruptions during the Lower Basalt
period (e.g., Hatzor and Reches, 1990; Shaliv et al., 1991; Dembo et al., 2015). The deposition of
the Hordos conglomerate during the early—middle Miocene on the eastern flank of the Faria Anticline
marks the development of a deep tectonic basin along the Jordan Valley at that time. Most of the
clastic materials deposited within this basin were derived from the eastern flank of the Faria
Anticline and expose Late Cretaceous to Eocene rocks. Similar conglomerates were derived from the
high, faulted flanks of the Faria, Buqea, and Tayasir Grabens, which indicates the formation of
these grabens that dissected the axis of the Faria Anticline in the early Miocene (Bentor, 1961;
Schulman and Rosenthal, 1968; Shaliv et al., 1991).
During the late Miocene, a new phase of normal faulting occurred. These faults, striking to the NW-SE direction,
ruptured only the northern part of the Faria Anticline and enhanced the tectonic relief along pre-existing
faults that originally developed in the early Miocene (Shaliv et al., 1991). One of the larger tectonic
basins that developed at this stage is the Beit She'an basin, which accumulated a thick sequence of the
late Miocene Bira Formation (ca. 10-7 Ma; Rozenbaum et al., 2019) and was followed by the deposition of
the late Miocene to early Pliocene Gesher Formation (ca. 7-5 Ma; Rozenbaum et al., 2019).
During the late Miocene and the early Pliocene, regional extensional deformation occurred in northern Israel.
This is evidenced by the extensive volcanic activity that formed the Cover Basalt Formation in northern Israel
(Shaliv et al., 1991; Heimann et al., 1996). In the northeastern sector of our study area, near Manna Feiyad
(Figs. 2A and 2C), several volcanic bodies of this phase are exposed and dated to 5.65-5.90 Ma (Shaliv et al., 1991;
Dembo et al., 2015). A tectonic phase of faulting in the northern Faria Anticline occurred after the deposition
of the Cover Basalt. This tectonic phase triggered the incision of the drain-age system on which the early
Quaternary Wadi Malih Formation was deposited, especially at the outlet of the Wadi Malih drainage system
to the southeastern part of Beit She'an Valley (Fig. 2), forming an extensive fan (Mimran, 1984;
Shaliv et al., 1991; Mimran et al., 2016). Farther north, a similar fan was deposited at the outlet of
Nahal Bezeq draining the southern flank of the Gilboa Mountains into the Beit She' an Valley (Figs. 1-2;
Hatzor, 2000). The late Quaternary is characterized by tectonic faulting along the western margin of the
Jordan Valley, followed by deep erosion and later deposition of the late Pleistocene Lisan Formation (e.g.,
Begin et al., 1974). Recent tectonics are demonstrated by the deformation of Lisan and younger sediments.
Based on the studies mentioned above, Mimran et al. (2016) published an updated version of the geological map
of the northern part of the region. However, the southern part of our study area is only described by a
regional scale (1:200,000) geological map (Sneh et al., 1998), which in some places does not correlate
well with the map of Mimran et al. (2016). Furthermore, previous works (e.g., Schulman and Rosenthal,
1968; Mimran, 1984; Shaliv et al., 1991) and geological maps (Sneh et al., 1998; Mimran et al., 2016)
correlate the Neogene sequences exposed in the study area to the Neogene sequence exposed ~30-50 km
to the north, near the Sea of Galilee, which was described by Picard (1943) and Schulman (1962).
This long-distance correlation ignores the large variety of local facies changes observed within the
stratigraphic sequence studied and therefore may cause misleading correlations.
In the present work, we demonstrate that careful examination and revision of this correlation leads to
a better understanding of the geological sedimentary sequence and sheds new light on the Neogene-Quaternary
tectonic evolution of our study area and in particular on the DSF-CGFS intersection.
Our observations indicate dramatic changes in the tectonic setting of the intersection between the DSF and the CGFS since the late Mio
cene. This change is manifested in both the stratigraphy and the faulting architecture of this intersection area.
As described above and summarized here, there are several major differences between our new map and previous geological maps
of this area: (1) based on lithological characteristics, dating, and field relations, large outcrops along the northern
part of the Faria Anticline, which border the Beit She'an Valley and were previously mapped as undivided outcrops of the
Hordos and Umm Sabune Formation of early-late Miocene Age (Shaliv et al., 1991; Mimran et al., 2016), were found to belong to younger Neogene
2016), were found to belong to younger Neogene and late Miocene–early Pliocene Gesher Formations. (2) Some of these previously mapped
outcrops (Shaliv et al., 1991; Mimran et al., 2016) were found to be pseudo-conglomerates of pedogenic origin, locally known as
“Nari” of Pliocene to early Quaternary age, which formed due to weathering and pedogenesis on the exposed outcrops.
(3) New outcrops of the Quaternary Wadi Malih Formation were found and mapped. (4) Based on lithological characteristics
and field relations, lage outcrops along and near the Faria Graben, which were previously mapped as unclassified
Neogene–Quaternar units (Sneh et al., 1998), were found to belong to the early–middle Miocene Hordos Formation.
(5) New outcrops of the Hordos Formation com-posed of polymictic conglomerates cemented by carbonates were found
and mapped in the southern part of the Faria Anticline, along and between the Faria and Buqea Grabens.
(6) New faults that rupture Neogene and Quaternary units were found and mapped, especially in the northern sector
of the Faria Anticline. Most of them are normal faults, and two are oblique faults, which demonstrate a
combination of sinistral and normal faulting. (7) Faults that rupture Pliocene and Quaternary units were only
found along the northern part of the Faria Anticline and the south-ern part of the Beit She’an Valley.
We show that since the late Miocene, the fragmentation of the Sinai Plate along the CGFS has been
accompanied by northward migration and localization of deformaWe show that since the late Miocene, the fragmentation of the Sinai Plate along the CGFS has been accompanied by northward migration and localization of deformation to the southern boundary of the Beit She'an Valley. Figure 13 summarizes the spatial distribution of the main phases of tectonic evolution. During the early—middle Miocene, the CGFS was composed of an —35-km-wide deformation belt that stretched from the Faria to Beit She'an Valleys. This belt was dominated by normal faulting and created NW-trending grabens, such as Faria, Buqea, and Tayasir Grabens (Fig. 13). Then, during the late Miocene and the Pliocene, tectonic activ¬ity migrated northward to a deformation belt of —6 km in the northern Faria Anticline (Fig. 13). Since the late Pleistocene, the deformation has been localized to a zone of —1-2 km along the southern boundary of the Beit She'an Valley (Fig. 13). At this stage, both normal and sinistral faulting can be clearly identified (Figs. 6, 10, and 12). A major fault in this localized zone is the Wadi Malih Fault, which ruptured the late Pleistocene Lisan Formation (Figs. 3, 6, 8, and 13). It marks a clear lineament that crosses the Jordan Valley as it branches from the DSF (at the eastern side of the Jordan Valley), where a right-lateral step and a change in the strike of the DSF are observed near the uplifted (push-up) area of Tel Al-Qarn (e.g., Ferry et al., 2007; Figs. 2A and S1). This fault defines the current boundary between the Faria Anticline and Beit She' an Valtion to the southern boundary of the
Beit She’an Valley. Figure 13 summarizes the spatial distribution of the main phases of tectonic
evolution. During the early–middle Miocene, the CGFS was composed of an ~35-km-wide deformation belt that stretched
from the Faria to Beit She’an Valleys.
We show that since the late Miocene, the fragmentation of the Sinai Plate along the CGFS has been accompanied by northward
migration and localization of deformation to the southern boundary of the Beit She'an Valley. Figure 13 summarizes the
spatial distribution of the main phases of tectonic evolution. During the early—middle Miocene, the CGFS was composed
of an ~35-km-wide deformation belt that stretched from the Faria to Beit She'an Valleys. This belt was dominated by
normal faulting and created NW-trending grabens, such as Faria, Buqea, and Tayasir Grabens (Fig. 13). Then, during
the late Miocene and the Pliocene, tectonic activity migrated northward to a deformation belt of ~6 km in the northern
Faria Anticline (Fig. 13). Since the late Pleistocene, the deformation has been localized to a zone of ~1-2 km along
the southern boundary of the Beit She'an Valley (Fig. 13). At this stage, both normal and sinistral faulting can be
clearly identified (Figs. 6, 10, and 12). A major fault in this localized zone is the Wadi Malih Fault, which
ruptured the late Pleistocene Lisan Formation (Figs. 3, 6, 8, and 13). It marks a clear lineament that crosses the
Jordan Valley as it branches from the DSF (at the eastern side of the Jordan Valley), where a right-lateral step and
a change in the strike of the DSF are observed near the uplifted (push-up) area of Tel Al-Qarn (e.g., Ferry et al.,
2007; Figs. 2A and S1). This fault defines the current boundary between the Faria Anticline and Beit She'an Valley and
shows clear evidence of normal faulting in the subsurface data (Fig. 12B). Farther NW of our study area, the observed
post-late Miocene faults are connected to the Gilboa Fault (Fig. 1; Shaliv et al., 1991; Sneh et al., 1998; Dembo et al., 2015).
The localization of deformation near the Beit She'an Valley and the Gilboa Fault agrees with current GPS
observations (Hamiel and Piatibra-tova, 2021). The results of this study highlight the significant deformation
near the intersection of the DSF and the CGFS and suggest that most of the deformation in the eastern section
of the CGFS occurs along the southern boundary of the Beit She'an Valley (i.e., near the Wadi Malih Fault and the
Mehola Fault), and the current contribution to deformation of the Faria Fault is negligibly small.
The localization of deformation near the Beit She'an Valley and the Gilboa Fault is also in agreement
with paleomagnetic observations and mechanical models (Dembo et al., 2015). Dembo et al. (2015) showed
localization of deformation near the Cannel and Gilboa Faults at sites younger than ca. 8 Ma. Previous
studies suggest that dramatic changes in plate kinematics occurred in the Levant during the late Miocene—early
Pliocene (e.g., Garfunkel, 1981; Joffe and Garfunkel, 1987; Marco, 2007). Such studies divided the deformation
along the DSF and surrounding areas into two main phases: before and after —5 m.y. ago. At this transition stage,
a shift in the location of the Sinai-Arabia Euler pole took place, leading to changes in the style and rate of
deformation as well as the internal structure and localization of the DSF system (e.g., Garfunkel, 1981;
Joffe and Garfunkel, 1987; Marco, 2007). Farther north of our study area, along the DSF and within the Sea
of Galilee and Hula depressions, studies have shown that changes and reorganization of the main and marginal
faults occurred at ca. 4-5 Ma (e.g., Heimann and Ron, 1993; Hurwitz et al., 2002; Schattner and Weinberger, 2008;
Heimann et al., 2009; Matmon and Zilberman, 2017). Other studies suggest that major changes in the regional
plate tectonics and the structure of the DSF occurred at ca. 10 Ma. Around this time, the collision of Arabian
and Eurasian plates along the Bitlis suture initialized in SE Anatolia (e.g., McQuarrie and van Hinsbergen,
2013), the DSF was fully developed as a plate boundary (e.g., Gomez et al., 2020), and the tectonic
activity along the intraplate Sinai—Negev Shear Zone terminated (Weinberger et al., 2020). Similar
to these studies, in our study area, a major transition in tectonic deformation was found to have started at ca.
10 Ma, when deposition of the Bira Formation first began. Spatial analysis of the new geological map (Figs.
3, 8, and S2) shows the migration of post-late Miocene faulting from SW to NE, which deepened the Beit She'an
Valley toward the NE. The volcanic activity in the SE sector of our study area (Fig. 3), which is dated to
5.65-5.90 Ma (Shaliv et al., 1991; Dembo et al., 2015), is probably related to the same tectonic phase that
started during the late Miocene and continued until the Pliocene. The strike of most post-late Miocene faults
is in the NW direction, some are in the NNW direction, and a small minority of faults are in the NE direction.
Many of the NW faults are probably rejuvenated faults that initiated during the early—middle Miocene tectonic
phase or even before, as indicated by the early stages of faulting along the CGFS (e.g., Shaliv et al., 1991;
Segev et al., 2014). Finally, we propose that the northward migration and localization of the intersection
between the CGFS and the DSF that has occurred since the late Miocene is probably related to the above-mentioned
regional tectonic and stress field changes, the transition in the Sinai-Arabia Euler pole location, and the
localization of deformation along the DSF. We also propose that our observations, along with current GPS
measurements (e.g., Gomez et al., 2020; Hamiel and Piatibratova, 2021), suggest the fragmentation of
the Sinai plate since the late Miocene.
Description | Image | Source |
---|---|---|
Fig. 1A - |
Fig. 1A
A map of the Levant region shows the tectonic plates and the location of the Dead Sea Fault (DSF) and Carmel–Gilboa–Faria Fault System (CGFS). The black rectangle shows the location of panel B. Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 1B - |
Fig. 1B
Location map of a broad area surrounding the intersection of the DSF and the CGFS shows the locations of major faults in the CGFS, i.e., the Carmel Fault (CF), Gilboa Fault (GF), and Faria (FF) Fault, locations of earthquakes since 1985 (from the catalogue of the Seismology Division of the Geological Survey of Israel; https://earth-quake.co .il), and the DSF sinistral slip rates (in mm/yr) based on GPS measurements (Hamiel and Piatibratova, 2021). The black rectangle shows the location of panel C. Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 1C - |
Fig. 1C
Location map of the study area shows the Faria Anticline and the Beit She’an (BSV) and Jordan Valleys. The dashed black lines denote the locations of the main faults and indicate the southern boundary of the Beit She’an Valley.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 2A - |
Topographic map shows the northern Faria Anticline as well as the Beit She’an and Jordan Valleys. The dashed black lines denote the locations of major morphological features and faults, and the dashed blue line denotes the trace of the current Wadi Malih channel. The red rectangles show the location of panels C and D. The inset shows the northern area in panel A. Note the NW–SE lineament that crosses the Jordan Valley and denotes by the Wadi Malih and the Wadi Al-Qarn. Blue arrows indicate the locations and fow directions of Wadi Malih and Wadi Al-Qarn, located east of the Jordan River. The black and green dots denote the locations of the Shadmot Mehola Fault shown in Figures 9 and 10A, respectively. The red dot denotes the location of the Mehola Fault shown in Figure 10B.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 2B - |
Topographic map of the southern Faria Anticline and the Jordan Valley. The dashed black lines denote the locations of major morphological features and faults, and the dashed blue line denotes the trace of the current Wadi Malih channel. The red rectangles show the location of panels C and D. The purple lines denote the locations of the seismic lines shown in Figure 12.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 2C - |
High-resolution slope maps on top of shaded topography were based on our new airborne light detection and ranging data. Maps shows the southernmost part of (C) the Beit She’an Valley. The data presented were downgraded to a pixel resolution of 3 × 3 m2. Morphological features that indicate variations in slope along lineaments are marked by dashed black lines. These lineaments were found to be major faults. The black and green dots denote the locations of the Shadmot Mehola Fault shown in Figures 9 and 10A, respectively. The red dot denotes the location of the Mehola Fault shown in Figure 10B. The purple lines denote the locations of the seismic lines shown in Figure 12.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 2D - |
High-resolution slope maps on top of shaded topography were based on our new airborne light detection and ranging data. Map shows the northern tip of the Faria Anticline. The data presented were downgraded to a pixel resolution of 3 × 3 m2. Morphological features that indicate variations in slope along lineaments are marked by dashed black lines. These lineaments were found to be major faults. The purple lines denote the locations of the seismic lines shown in Figure 12.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 3 - |
Fig. 3
The new geological map of the study area is shown. Note that while the early–middle Miocene Hordos Formation is exposed in the southern and central parts of the study area, along the NW-trending grabens and the eastern flank of the aria Anticline, the late Miocene Bira, late Miocene–early Pliocene Gesher, and early Pleistocene Wadi Malih Formations are exposed only in the northern part of the study area. The geological units east of the Jordan River (easternmost part of the map) were not mapped. Dashed blue lines denote the locations of profilesA and B presented in Figure 6. The purple dot denotes the location of sample SM1 (Fig. 4D), which is dated to the late Miocene Bira Formation age of the sample. Black dots denote the locations of faults presented in Figures 5A–5F and 10A–10B. Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 4 A-F - |
Fig. 4 A-F
Images of the mapped
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 4 G-H - |
Fig. 4 G-H
Images of the mapped
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 5 - |
Photos show faults that rupture Neogene and Quaternary units. The locations of these images are presented in Figure 3.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 6 - |
Schematic diagrams show
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 7 - |
Fig. 7
Seismic line L11 was acquired across the Faria Graben in the southern part of the study area. The location of the line is presented in Figure 2. Red dashed lines denote faults at the subsurface. The yellow line indicates the surface, and the green line indicates the bottom of the late Pleistocene Lisan Formation, which varies from ~140 m to ~30 m below the surface. Note that faults do not rupture this rock unit. For more details, see the Supplemental Material (see text footnote 1). Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 8 - |
Color-keyed evolution of the faulting map on top of the new geological map is shown (Fig. 3). Black lines denote faults that ruptured pre-late Miocene Bira Formation rocks. Light-green lines denote faults that ruptured the late Miocene Bira Formation rocks. Yellow lines denote faults that ruptured the late Miocene–early Pliocene Gesher Formation rocks. Orange lines denote faults that rup-tured the early Pleistocene Wadi Malih Formation rocks. Red lines denote faults that ruptured the late Pleistocene Lisan Formation rocks. Note the migration of faulting to the NE direction over time. The locations of the Shadmot Mehola Fault (SMF), Mehola Fault (MF), and Wadi Malih Fault (WMF) are also indicated. The northeasternmost faults are found near the eastern part of Wadi Malih and the southern Beit She’an Valley. All faults south of this map and within the study area were found to rupture only middle Miocene or older rock units (black lines). Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 9 - |
(A) Photo and (B) schematic cross section (vertical exaggeration of 1:2) show the Shadmot Mehola Fault exposed along an artificialslope cut. The location of this outcrop is marked by black dots in Figure 2. As observed, the ~250-m-wide fault zone consists of six major internal blocks that are reverse and normally displaced on major fault planes. Major and minor faults are marked by thick and thin solid vertical lines, respectively; stratigraphic contacts are marked by thin solid lines; bedding is marked by dashed lines.
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 10 - |
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 11 - |
Fig. 11
Shaded relief map is based on our new airborne light detection and ranging data for the northern study area and shows the interaction between the Wadi Malih stream and the Shadmot Mehola Fault (SMF), Mehola Fault (MF), and Wadi Malih Fault (WMF). The black arrow shows the location where the SMF intersects with Wadi Malih Valley. At this location, a left-lateral shift of ~150 m in the ridge location and Wadi Malih valley occurs (Fig. 9A). Blue arrows indicate changes in the fow direction of Wadi Malih where it crosses the MF (Fig. 9B). Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 12A - |
Fig. 12A
Seismic lines acquired across major faults in the northern part of the study area are shown. The locations of the lines are presented in Figure 2. For more details, see the Supplemental Material (see text footnote 1). Seismic line L12 within the southern Beit She’an Valley shows no evidence for faulting within the valley. Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 12B-D - |
Fig. 12B-D
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 12C-E - |
Fig. 12C-E
Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 13 A - |
The tectonic evolution at the intersection between the Dead Sea Fault (DSF) and Carmel-Gilboa-Faria Fault System (CGFS) is shown. Map of the study area shows the area that deformed during the three main tectonic stages: early-middle Miocene (yellow area), late Miocene-Pliocene (light orange area), and Quaternary (dark orange area). Green area denotes the defor-mation zone of the DSF, which has been tectonically active since the early Miocene. Hamiel et al. (2022) |
Hamiel et al. (2022) |
Fig. 13 B - |
The tectonic evolution at the intersection between the Dead Sea Fault (DSF) and Carmel-Gilboa-Faria Fault System (CGFS) is shown. A S—N schematic cross-section across the CGFS, west of the intersection with the DSF, shows the migration and localization of faulting during the main three tectonic stages that have occurred since the early Miocene. Note that normal faulting was the dominant component of deformation before the Pleistocene, and since then, a combination of sinistral and normal faulting has been observed. BSV-Beit She'an Valley. Hamiel et al. (2022) |
Hamiel et al. (2022) |
To address one of the central questions of plate tectonics — How do large transform systems
work and what are their typical features? — seismic investigations across the Dead Sea Transform (DST), the boundary between the African and Arabian plates in the Middle East, were
conducted for the first time. A major component of these investigations was a combined reflection/refraction survey across the territories of Palestine, Israel and Jordan. The main results of
this study are:
The DST is a system of left-lateral strike-slip faults that accommodate the relative motion between the African and Arabian plates.
Except for a mild compressional deformation starting about 80 Ma,
the larger Dead Sea region has remained a stable platform since the
early Mesozoic. Approximately 17 Ma, this tectonic stability was
interrupted by the formation of a transform, the DST, with a total left-lateral displacement of 105 km until today (Quennell 1958;
Freund et al. 1970; Garfunkel 1981).
The crystalline basement of the area represents the NW part of the
Arabo-Nubian Shield (ANS) and consists of mainly juvenile Late
Proterozoic rocks (Stoeser & Camp 1985; Stern 1994). Regarding
both isotopic and chemical data of xenoliths, the involvement of
older crustal material in the lower crust of the ANS seems improbable (Henjes-Kunst et al. 1990; Stern 1994; Ibrahim & McCourt
1995). There is a gradual transition from the continental crust of
the ANS with thicknesses of 35–40 km (El-Isa et al. 1987; Makris
et al. 1983; Al-Zoubi & Ben-Avraham 2002) to the crust of the eastern Mediterranean, that is assumed to be partly underlain by typical
oceanic crust with thicknesses smaller than 10 km (Ginzburg et
al. 1979a; Makris et al. 1983; Ben-Avraham et al. 2002), see also
Fig. 1(b).
The Precambrian basement is usually overlain by an Infracambrian to Early Cambrian volcano-sedimentary succession of variable thickness. Whereas coarse-grained clastics (Saramuj and Elat
conglomerates) are restricted to fault-bounded basins, fine-grained
clastics, mostly consisting of arkosic sandstones and associated volcanic rocks (Zenifim Formation, Haiyala Volcaniclastic Unit and
equivalent rock units) have been observed in large parts of the Israel and Jordan subsurface (Weissbrod & Sneh 2002). In boreholes
close to the WRR and NVR profiles (Fig. 1b) the Zenifim Formation
was determined to be several hundreds of metres thick (> 500 m in
Maktesh-Qatan, MQ, and >2000 m in Ramon-1, R1), although its
base has not been encountered in any of the Israeli boreholes.
The position of the study region at the NW edge of the ANS, i.e.
at a passive continental margin since early Paleozoic times, is reflected in facies changes and varying sedimentary thicknesses along
the seismic profiles (Fig. 2). The Phanerozoic along the northwestern part of the profile is dominated by Cretaceous and Tertiary rocks
underlain by Jurassic, Triassic and Permian sequences that thin out
towards the east. East of the DST, however, Permian to Triassic strata
are missing and Lower Cretaceous rocks unconformably overlie Ordovician and Cambrian sandstones. The crystalline basement rocks
(calc-alkaline granitoids and rhyolites) cropping out in the Jebel
Humrat Fiddan area east of the DST are thought to be equivalent to
the basement rocks of the Timna region in Israel, near Elat.
Previous crustal-scale wide-angle reflection/refraction experiments in the study area (Fig. 1b) include that in Israel in 1977 (Ginzburg et al. 1979a), the onshore-offshore experiment between the northwestern end of the WRR profile and Cyprus in 1978 (Makris et al. 1983; Ben-Avraham et al. 2002) and that in Jordan in 1984 (El-Isa et al. 1987). However, there was no profile, which crossed the DST to provide a complete image across this structure. Moreover, deep seismic reflection data only exist from the area between the Dead Sea and the Mediterranean (Yuval & Rotstein 1987; Rotstein et al. 1987), and high-resolution seismics (Frieslander 2000) are mostly limited to the western part of the Arava Valley. Further south within the Afro-Arabian rift system seismic profiles, which cross the rift structures, have proved to be very useful to understand the crustal structure as, for example, the E-W profiles crossing the Kenya rift (Maguire et al. 1994; Braile et al. 1994; Birt et al. 1997). Seismic crustal investigations of the Afro-Arabian Rift system are summarized by Mechie & Prodehl (1988) and Prodehl et al. (1997).
In deep crustal reflection data the Moho is commonly defined as
the break-off of lower crustal reflectivity (Fig. 11b). The increase in
Moho depth from ∼30 to 38 km, that is observed in the WRR data
beneath the NVR profile, is more or less in accordance with the NVR
data. A few small discrepancies between the reflection and refraction
seismic data (as for example at the western end of the NVR line)
are not unusual for coincident seismic reflection/refraction surveys
(see e.g. Mooney & Brocher 1987). Note also that reflections from
Moho depths typically have dominant frequencies of 12–13 Hz in
the NVR data, in contrast to 6–7 Hz in the WRR data. At the same
time the differences between the reflection and refraction Moho are
in the range of measurement uncertainties (see also WRR modelling,
Section 3.3).
In comparing the depths to the seismic basement with those obtained from previous experiments in the area, the depths obtained in
this study west of the Arava Valley (Figs 10a and 11a) are smaller
than those obtained by Ginzburg et al. (1979a). This may be due in
part to somewhat lower average velocities used by Ginzburg et al.
(1979a). On the other hand the depths to the seismic basement obtained here west of the Arava Valley are in good agreement with
those obtained by Perathoner (1979). The larger value for the depth
to the seismic basement beneath the coast obtained by Makris et al.
(1983) from the offshore-onshore experiment in 1978 probably indicates that the depth to the seismic basement increases towards the
coast to the NW of the region of ray coverage for the model obtained
here. Beneath the Arava Valley itself, the depth to the seismic basement obtained here is greater than those obtained by Ginzburg et al.
(1979a) and Perathoner (1979) from the N–S profile within the Arava Valley (Fig. 1b). This is probably due to the fact that although,
for the N–S profile, the shot was in the Dead Sea, the recording
stations were at the western side of the Arava Valley and sometimes
on the shoulders of the Arava Valley. To the east of the Arava Valley the depth to the seismic basement obtained here is within 1 km
of the depth obtained by El-Isa et al. (1987) from the N–S profile
on the eastern shoulder of the Arava Valley (Fig. 1b). The depths
to the boundary between the upper and lower crust obtained in this
study (Figs 10b and 11a) agree to within 1 km with the depths to
this boundary obtained from the previous experiments in this area
(Fig. 1b; Ginzburg et al. 1979a; El-Isa et al. 1987).
With respect to the depths to the Moho, west of the Arava Valley
there is agreement to within 3 km between the depths obtained
here (Fig. 10c) and those obtained by Ginzburg et al. (1979a) and
Makris et al. (1983). Beneath the Arava Valley itself the Moho depth
obtained here agrees with that obtained by Perathoner (1979) from
the N–S profile within the Arava Valley, but it is 5 km deeper than
the value obtained by Ginzburg et al. (1979a). To the east of the
Arava Valley the Moho depths obtained here are also about 5 km
deeper than those obtained by El-Isa et al. (1987) from the N–S
profiles on the eastern shoulder of the Arava Valley. In fact, the
Moho depths obtained by El-Isa et al. (1987) from the N–S profiles
on the eastern shoulder of the Arava Valley (Fig. 10c) are more in
agreement with the depth at which strong reflections are observed
in the NVR section (Fig. 11b). In order to find out where PmP
reflections would occur in the record sections assuming that the
Moho depths are as indicated by either the near-vertical incidence
reflection section or by El-Isa et al. (1987), a model was constructed
with Moho depths taken from the near-vertical incidence reflection
section and El-Isa et al. (1987) and an average lower crustal velocity
of 6.7 km s−1. Tracing rays through this model results in arrival times
for the PmP reflection which are 0.8–1.0 s earlier than those for the
preferred model shown here (Fig. 11a) in the record sections from
the densely spaced data from the Arava Valley from shots 9 and 10
(Figs 8b and 9b). In these data there are no strong reflections 0.8–
1.0 s earlier than the PmP reflections shown. For this reason and as
the data from the previous experiments in the area are sparser than
the data along the WRR profile, it is thought that the Moho depths
obtained here are more accurate than those obtained by El-Isa et al.
(1987). Alternatively, the discrepancy may be, at least in part, due
to strong 3-D variations of the Moho in the vicinity of the DESERT
profile. Such variations are evident in the receiver-function data (A.
Mohsend, personal communication, 2003).
A remarkable feature in Fig. 11(b) is a zone of high reflectivity at a depth of 28 km below the Jordan highlands between profile km 78 and 92. This is about the depth and position along the
profile from which the possible phase, Pi2P in the WRR data is
reflected, although the boundary associated with the Pi2P phase,
if present, would have to occur for at least about 90 km under the
profile (Fig. 10d) instead of just about 20 km as identified in the
NVR data. This zone of high reflectivity in the NVR data might
be due to a lithological contrast caused by underplating. In this case
higher velocities of about 7.0 km s−1 would be expected to occur
across the region of high reflectivity. If a 7.0 km s−1
layer of limited
thickness is, in fact, present at about 30 km depth, this would only
have a small effect on the estimated Moho depths, such that they
would still be within the error limits of ±3 km given above (Section
3.3). Strong magmatic activity that occurred in the region both in
Late Precambrian/Early Cambrian, Cretaceous and Neogene times
could possibly have caused such a proposed underplating, or sill-like
intrusions into the lower crust. Another possibility for the creation
of such a high reflectivity is a zone of localized strain close to the
base of the crust, which is in agreement with the conclusions of
Sobolev (unpublished data) (see also later discussion) which show a
zone of high shear deformation and possible lower crustal flow east
of the transform. It is expected that a gravity analysis currently being carried out along the profile might give some further constraints
for interpreting these reflectors. The high reflectivity at Moho depth
west of the AF is in accordance with the eastern part of a deep
seismic reflection line between the Mediterranean and the Dead Sea
(Yuval & Rotstein 1987; Rotstein et al. 1987) that shows a similar
reflectivity pattern of the crust as observed here.
Imaging near-vertical structures by near-vertical seismic reflection
techniques is difficult (e.g. Meissner 1996). It is, however, possible
to get indirect evidence of the depth continuation of steeply dipping
faults by the offset of crustal reflectors or an observed change in
crustal reflectivity.
However, although the DST/AF is clearly recognized on satellite
data as a rather straight line between the Red Sea and the Dead Sea
(DESERT Team 2000) it cannot unambiguously be delineated in the
Common Depth Point (CDP)section (Figs 11b and A5). There is no
pronounced difference in crustal structure west and east of the Arava
Fault and in the immediate vicinity of its surface trace sedimentary
reflections are missing. The absence of sedimentary reflectors might
be due to strong deformation of the rocks close to the fault, but could
also be caused by the absorption of high frequencies (Fig. A2) in an
area covered by sand dunes and alluvium.
Whereas a possible Moho offset has been proposed for the San
Andreas Fault in northern California from deep crustal seismic reflection and refraction studies (Henstock et al. 1997), and for the
DST north of the Dead Sea Basin from the analysis of gravity data
(Ten Brink et al. 1990), there is no evidence for such an offset at
the AF along the NVR profile. Nonetheless it is inferred that the AF
reaches down to the mantle, changing into a broader deformation
zone at mid-crustal level, because of the following reasons:
Some features in the near-surface structure of the Arava Valley, e.g. surface topographic expression, sedimentary fill and normal faults at the edge of the valley, resemble those of rift structures. However, the narrow, only ~10 km wide, shallow sedimentary basin mainly to the west of the AF (Fig. 2b), a seismic basement offset of 3 to 5 km on the eastern side of the Arava Valley and the small but visible, asymmetric Moho topography (~1.5 km) with a coupled upwarp-downwarp structure beneath the Arava Valley (Fig. 11), although possibly related to the slight extension across this part of the DST, are untypical for rift structures. For example, the southern portion of the Kenya rift, a classical continental rift, has been under extension since about 10 Ma, and the Moho there is uplifted 5–10 km causing considerable crustal thinning (Mechie et al. 1997). We therefore conclude that rifting–type deformation (fault perpendicular extension) did not play a dominant role in shaping the crustal structure of the DST. A thermo-mechanical model of the DST by Sobolev (unpublished data) confirms this by showing that the crustal structure of the DST results mainly from the geologically documented 105 km left-lateral displacement between the Arabian plate and the African plate (Figs 13a and b) placing lithospheric blocks with different crustal structures opposite each other. The modelling also supports the scenario that changes in surface and Moho topography and in crustal structure result from large, localized deformation accommodating the transform motion within a narrow zone crossing the entire crust. However, this process is combined with less than 4 km of fault-perpendicular extension (Garfunkel 1981; Sobolev et al. 2003 Fig. 13c). Thus the ‘rift component’ at the DST between the Dead Sea and the Gulf of Aqaba, defined as the ratio between fault perpendicular extension [4 km] and strike slip motion [105 km], is probably smaller than 4 per cent. This small extension nevertheless produces a large topography because the extension is localized within the narrow (20 km wide) upper mantle and lower crustal shear zones, where viscosity is reduced due to the high strain rate produced by the strike-slip motion (Sobolev et al. 2003), thus giving the Arava Valley the appearance of a rift valley.
A comparison with the San Andreas Fault (SAF), another end-member of transform structures (see e.g. Holbrook et al. 1996;
Bonner & Blackwell 1998), shows several differences, especially in
the shallow structure, and some similarities in the deeper structure.
Fault Zone Guided Waves from controlled source experiments in the
Arava Valley (Haberland et al. 2003) sample the top few hundred
meters of the Arava Fault and are best explained by a fault model
with a narrow, only 3–10 m wide low-velocity zone. This thickness is
much smaller than the typical width of 100 to 170 m of low-velocity
zones in the SAF system (Li et al. 1990), and is possibly due to
the smaller total slip on the DST (105 km) versus the slip of more
than 350 km at the SAF, or it could be a local feature controlled by
the young sediments in the area where the DESERT profile crosses
the AF. In contrast to the SAF the Arava Fault under the DESERT
profile acts as a localized fluid barrier separating a high- from a
low-velocity block in the uppermost crust. This contrast is visible in
the combined magnetotelluric sounding and high-resolution tomography of Ritter et al. (2003). Such a feature is remarkably different
from active segments of the SAF, which typically show a conductive
fault core acting as a fluid conduit (Unsworth et al. 2000).
If, however, deeper crustal and mantle structures are compared,
it becomes apparent that both transform systems show deep reaching deformation zones (Sobolev, unpublished data, Rumpker et al.
2003 for the DST and Holbrook et al. 1996; Henstock et al. 1997; Unsworth et al. 1997; Silver 1996 for the SAF) accompanied by a strong asymmetry in subhorizontal lower crustal reflectors
(lower crustal flow, sill-like intrusions?). We therefore suggest that
these features are common features of continental transform plate
boundaries.
Our study provides the first whole-crustal image across the Dead Sea Transform (DST), one of the Earth’s major transform faults. Under the Arava Fault (Fig. 11), the main fault of the southern DST system, the seismic basement is offset by several kilometres, but the Moho depth increases steadily from ~26 km at the Mediterranean to ~39 km under the Jordan highlands, except for a small but visible, asymmetric topography under the Arava Valley. The general trend of continuous Moho-depth increase is confirmed by the interpretation of potential field data (Al-Zoubi & Ben-Avraham 2002) and the results of a receiver functions study (A. Mohsen, personal communication, 2003). Based on the interpretation of the NVR data, we infer that the AF cuts through the crust, becoming a broad zone in the lower crust, and reaches down to the mantle. This agrees with the results of the thermo-mechanical modelling of Sobolev et al. (2003) and the SKS-splitting observations by Rumpker et al. (2003), which suggest that the DST cuts through the whole lithosphere, thus accommodating the motion between the African and the Arabian plates (Fig. 1). The lack of significant uplift of the Moho under the Arava Valley speaks strongly against a potential rift structure in this area. We therefore conclude that rift-type deformation (fault perpendicular extension) did not play a dominant role in the dynamics of the DST, a fact corroborated again by the results of Sobolev (unpublished data). Although the shallow structure at the DST differs significantly from the structure at the San Andreas Fault, the deep reaching deformation zones accompanied by a strong asymmetry in subhorizontal lower crustal reflectors appear to be similar for both fault zone systems. We therefore suggest that these deep features are common for large continental transform plate boundaries
Description | Image | Source |
---|---|---|
Fig. 1a - |
Fig. 1a
Seismic experiments in the Middle East. The 260 km long wide-angle reflection/refraction profile (WRR, dark blue dots) crosses Palestine, Israel and Jordan. The near-vertical seismic reflection profile (NVR, cyan) coincides with the inner 100 km of the WRR. A red line and two red arrows indicate the Dead Sea Transform (DST) between the Dead Sea and the Red Sea. The white arrows indicate the left-lateral motion of 105 km between the African and Arabian plates. Red stars mark large earthquakes. (Inset) Tectonic setting of the DST. Weber et al. (2004) |
Weber et al. (2004) |
Fig. 1b - |
Fig. 1b
Previous wide-angle reflection / refraction experiments in the study area (dashed black; Ginzburg et al. 1979a; Ginzburg et al. 1979b; Makris et al. 1983; El-Isa et al. 1987) together with the WRR profile of DESERT (blue) and the DST (red). The black circles are boreholes used in the interpretation
|
Weber et al. (2004) |
Fig. 2 - |
Fig. 2
|
Weber et al. (2004) |
Fig. 11 - |
|
Weber et al. (2004) |
Fig. 13 - |
Sketch of the DST dynamics along the DESERT profile, based on results shown in Fig. 11 and the results of Sobolev (unpublished data).
|
Weber et al. (2004) |
Description | Image | Source |
---|---|---|
Fig. 1a - |
Fig. 1a
Seismic experiments in the Middle East. The 260 km long wide-angle reflection/refraction profile (WRR, dark blue dots) crosses Palestine, Israel and Jordan. The near-vertical seismic reflection profile (NVR, cyan) coincides with the inner 100 km of the WRR. A red line and two red arrows indicate the Dead Sea Transform (DST) between the Dead Sea and the Red Sea. The white arrows indicate the left-lateral motion of 105 km between the African and Arabian plates. Red stars mark large earthquakes. (Inset) Tectonic setting of the DST. Weber et al. (2004) |
Weber et al. (2004) |
Fig. 1b - |
Fig. 1b
Previous wide-angle reflection / refraction experiments in the study area (dashed black; Ginzburg et al. 1979a; Ginzburg et al. 1979b; Makris et al. 1983; El-Isa et al. 1987) together with the WRR profile of DESERT (blue) and the DST (red). The black circles are boreholes used in the interpretation
|
Weber et al. (2004) |
Fig. 2 - |
Fig. 2
|
Weber et al. (2004) |
Fig. 11 - |
|
Weber et al. (2004) |
Fig. 13 - |
Sketch of the DST dynamics along the DESERT profile, based on results shown in Fig. 11 and the results of Sobolev (unpublished data).
|
Weber et al. (2004) |
Begin, Z. B., J. N. Louie, S. Marco, and Z. Ben-Avraham (2005).
Prehistoric seismic basin effects in the Dead Sea pull-apart. Geol. Survey of Israel, Jerusalem: 31.
Ben-Avraham, Z., et al. (2006). "Segmentation of the Levant continental margin, eastern Mediterranean." Tectonics 25(5).
Ben-Avraham, Z., et al. (2008). "Geology and Evolution of the Southern Dead Sea Fault with
Emphasis on Subsurface Structure." Annual Review of Earth and Planetary Sciences 36(1): 357-387.
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