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Sedimentary deposits left by the 2004 Indian Ocean tsunami on the inner continental shelf offshore of Khao Lak, Andaman Sea (Thailand)
Earth, Planets and Space volume 64, Article number: 11 (2012)
Tsunami waves leave sedimentary signatures both onshore and offshore, although the latter are hardly known. The objective of the present study is to provide new evidence for the 2004 Indian Ocean tsunami deposits left on the inner continental shelf of the Andaman Sea (Thailand) and to identify diagnostic sedimentological and geochemical properties of these deposits. Based on extensive seafloor mapping, three sediment cores were selected for study and were analysed for their sedimentary structures, grain size composition, chemical elemental composition, physical properties and 210Pb activity. Sediment cores retrieved from shallow water (9–15 m) within 7.5 km off the shore revealed distinct event layers, which were interpreted as being tsunami deposits. These 20–25 cm thick deposits were already covered with post-tsunami marine sediments. They were composed of several units, marine sand layers alternating with poorly sorted mud with terrigenous and anthropogenic components, representing different hydrodynamic conditions (probably during run-up and backwash phase). These sedimentological observations were supported by geochemical and physical data and were confirmed using 210Pb dating. A sediment core taken from a depth of 57 m at a distance of 25 km offshore did not reveal clear event deposits. Comparisons with available data from offshore tsunami deposits showed that there is no single set of signatures that could be applied to identify this kind of deposits.
Tsunamis are relatively frequent phenomena that occur worldwide (Scheffers and Kelletat, 2003). Recent examples of tsunamis include the 2004 Indian Ocean tsunami, tsunamis in Java in 2006 and Samoa in 2009, the Chilean tsunami in 2010 and the 2011 Tohoku tsunami in Japan. These events can have potentially large impacts on both the coastal zone and the continental shelf. As tsunami waves propagate into shallower water, they can erode, transport and deposit large amounts of sediments both onshore and offshore (e.g., Paris et al., 2010; Goto et al., 2011). Due to the number of processes involved (Shanmugam, 2011), tsunami deposits are very complex in terms of a number of characteristics, including grain size, sedimentary structures and sediment components (e.g., Luque et al., 2001; van den Bergh et al., 2003; Fujiwara and Kamataki, 2007; Kortekaas and Dawson, 2007; Noda et al., 2007; Paris et al., 2010; Chagué-Goff et al., 2011). Geological and environmental impacts of onshore tsunami deposits have been intensively studied in recent years (see Bourgeois, 2009 for a review), whereas the offshore behaviour and effects of tsunami waves during run-up and backwash are still poorly understood.
A basic problem in studying tsunamis is that our knowledge of the sedimentological features of offshore tsunami deposits is limited to a small number of case studies (e.g., van den Bergh et al., 2003; Noda et al., 2007; Paris et al., 2010). Tsunami impacts (erosion) on the seafloor have primarily been examined indirectly through studies of onshore deposits containing marine microfossils such as foraminifera (e.g., Hawkes et al., 2007; Uchida et al., 2010) or diatoms (e.g., Dawson, 2007; Sawai et al., 2009). The studies of shallow marine tsunami deposits that have been conducted to date have indicated that there is a large variability in the characteristics of these deposits. For instance, a distinct sandy layer was deposited by a tsunami generated during the Krakatau eruption in an embayment next to Java Island (van der Bergh et al., 2003). Around Banda Aceh, which was the most severely devastated region during the 26 December 2004 tsunami, this event left large fields of boulders on land and offshore (Paris et al., 2010). Displaced boulders were also previously reported by Goto et al. (2007) and Feldens et al. (2009) from the Andaman Sea coast and shelf, respectively. Sugawara et al. (2009) reported nearshore impacts of the 2004 tsunami in the Andaman Sea in water depths of 6 to 30 m based on the distribution of foraminifera in surface sediments. In several other studies (e.g., Abrantes et al., 2008; Goodman-Tchernov et al., 2009; Smedile et al., 2011), offshore tsunami deposits were interpreted from event layers composed of sediments that were coarser than the ambient marine sediments, contained indicators of a terrigenous provenance and specific microfossil assemblages. However, there have been no unique criteria for identifying offshore tsunami deposits. Recently, Goto et al. (2011) used repeated bathymetrical surveys and modelling and found that the amount of sediments mobilised by tsunamis is much more substantial offshore than on land.
Shallow water tsunami deposits from uplifted marine sedimentary strata were investigated by Fujiwara and Kamataki (2007) in Japan, and by Cantalamessa and Celma (2005) and Le Roux and Vargas (2005) in Chile. However, these older deposits can be reinterpreted, as in the case of backwash deposits in a shallow marine Miocene setting on the Mejillones Peninsula in northern Chile (Cantalamessa and Celma, 2005), which were recently found to be debris flow deposits with no evidence permitting an interpretation as tsunami deposits of any kind (Bahlburg et al., 2010).
The above examples indicate the limitations of our understanding of the processes of erosion and deposition in shallow marine settings during tsunami events and the difficulties of identifying offshore tsunami deposits. Significant progress in the search for diagnostic criteria may be accomplished only through an increased number of well-documented case studies of modern tsunami deposits. The objective of this study is to provide evidence that the impact of the 2004 Indian Ocean tsunami can be identified in shallow water deposits offshore Khao Lak by using sedi-mentological methods and geochemical proxies.
2. Study Area
The study area is located on the continental shelf of the Andaman Sea offshore Khao Lak (Phang Nga province, Thailand) and extends to a distance of about 25 km offshore (Fig. 1). The coast is composed of embayed areas with sandy beaches separated by rocky headlands. The shelf is relatively flat and sloping offshore, reaching water depths of 50 m at a distance of 25 km from the coastline. The sea bottom is mainly composed of sand, sandy mud, muddy sand and bedrock outcrops (Usiriprisan et al., 1987; Di Geronimo et al., 2009; Feldens et al., 2009, 2012). In some regions, the seabed was subjected to offshore tin mining (Usiriprisan et al., 1987). The climate of this region is dominated by monsoons, with the southwest monsoon remaining active from May to September and generating heavy rainfall during this period. The northeast monsoon lasts from December to February and results in a calm, dry season (Khokiattiwong et al., 1991). The study area is located next to the area in Thailand which was most damaged during the 2004 Indian Ocean tsunami (Bell et al., 2005; Szczuciński et al., 2006). Moreover, strong storms are rare in this area, increasing the preservation potential of tsunami deposits on the seafloor (Jankaew et al., 2008; Kumar et al., 2008). Previous post-tsunami seafloor mapping surveys (Di Geronimo et al., 2009; Feldens et al., 2009) reported discontinuous muddy sediment patches and a channel-like system next to an ancient reef platform located in shallow water (5 to 15 m). Consolidated mud deposits containing grass, wood and shell fragments, likely transported by the backwash flow in the 2004 tsunami, were observed in grab samples and short cores (Feldens et al., 2009). Based on these data and further hydroacoustic surveys (Feldens et al., 2012), new target areas for sediment coring were selected (Figs. 1 and 2) to examine modern offshore tsunami deposits.
High resolution hydroacoustic mapping (Feldens et al., 2009, 2012) was performed during three research cruises (Nov.–Dec. 2007, Nov.–Dec. 2008 and Feb.–Mar. 2010). Data from these surveys form the basis for the selection of sediment coring sites. Sixty sediment cores were collected using a 2 m long Ruhmor type gravity corer in water depths of 5 to 70 m. Three cores were selected for the present study (Figs. 1 and 2, Table 1), two of which were obtained in water depths of 9.6 and 14.4 m, located 3.1 and 7.2 km offshore, respectively, while the third core was collected further offshore at a water depth of 57 m, 25.5 km offshore. Moreover, three samples from sites located within various onshore environments that had been subjected to tsunami erosion (pre-tsunami soils, mangrove soils, coastal plain sands) were obtained to provide data on terrigenous geochemical end-members (Fig. 1).
The cores were first analysed using non-destructive techniques; a Multi-sensor core logger (MSCL) and an X-ray fluorescence (XRF) core scanner. The following basic physical and acoustical sediment properties were measured: bulk density, gamma-ray attenuation, magnetic susceptibility and p-wave velocity. These physical properties are commonly used to find distinct layers such as debris flows and turbidites within sediment cores (Weber et al., 1997; Best and Gunn, 1999; Hofmann et al., 2005). An XRF core scanner was used to semi-quantitatively assess sediment composition; this method can serve as a tool for differentiating terrigenous materials from marine sediments (Lamy et al., 2001; Bahr et al., 2005; Ohta and Arai, 2007). The measurements were taken every centimetre directly at the surface of a split core. The instrument was set to a count time of 30 s with a voltage of 10 kV. At this setting, the measurement range covered thirteen elements (Al, Si, P, S, Cl, K, Ca, Ti, V, Cr, Mn, Fe and Rh). Data were provided as relative element intensities in counts per second (cps). These intensities depend mainly on element concentration, matrix effects and physical properties, as well as sample geometry (Jansen et al., 1998; Weltji and Tjallingii, 2008).
The relative concentrations of eight elements, Al, Si, S, K, Ca, Ti, Mn and Fe from onshore samples (101207-89, 101207-91 and 101207-93) and samples from core 050310-C6, were analysed using principal component analysis (PCA) to evaluate the sediment provenance (Marques et al., 2008; Heise et al., 2010). Four elements were not used, due to either very low concentrations in some samples (at detection limits: P, V, Cr, Rh) or possible changes due to sample preparation (Cl). PCA is a data reduction technique used to convert a large number of geochemical variables into a small set of new variables called principal components or factors (PC) and to group samples based on their geochemistry (Ohta and Arai, 2007; Reid and Spencer, 2009).
Digital X-radiography images were obtained from 1 cm thick slabs taken from the surface of split sediment cores. This technique is used to detect any internal sedimentary structures or unconformities not visible to the naked eye. The images (Figs. 3–5) show the relative change in sediment bulk density. High bulk density sediment, such as pebbles, shell fragments or sand, reduce X-ray penetration and are displayed in light grey, whereas low bulk density sediment, as observed for fine-grained sediments, is represented by dark grey or black (Bouma, 1964).
To determine the grain size distribution, core materials were sampled in 1 cm intervals. The materials were digested with HCl and H2O2 to remove carbonates and organic matter prior to analysis with a Coulter LS-13320 laser-based particle sizer device with a measuring range of 0.04 to 2000 µm. From core 050310-C6, samples composed mainly of grains in excess of sand size (27–38, 40– 41, 72–73 and 87–88 cm) were not analysed. Statistical parameters of the grain size distribution (Figs. 3–5) were calculated using the logarithmic method of moments in GRADISTAT software (Blott and Pye, 2001).
210Pb dating has been widely used for the assessment of sediment accumulation rates over the last 100 years. Total 210Pb activity in the recent sediments comes primarily from two sources: supported (autochthonous) 210Pb is produced by the radioactive decay of uranium radioactive chain isotopes in sediments and excess (allochthonous) 210Pb is produced by the decay of 222Rn, mostly in the atmosphere, and is then deposited with the sediments. The excess 210Pb activity profile in the sediments is commonly characterised by the maximum activity at the surface and by the exponential decay, and is used for the assessment of sediment accumulation rates under several assumptions, depending on the applied model (Robbins and Edgington, 1975; Nittrouer et al., 1979; Carpenter et al., 1982). However, the shape of the 210Pb profile may also reveal information on changes in sediment accumulation rates, the presence of major erosional events and the presence of event layers (e.g., Nittrouer et al., 1979; Jaeger et al., 1998; Sommerfield and Nittrouer, 1999; Crockett et al., 2008; Szczuciński et al., 2009). An event layer can usually be observed in the portion of the 210Pb activity profile that shows no change downcore (usually due to rapid deposition during the event). However, more frequently, 210Pb depletion is observed due to dilution processes in larger sediment masses and/or the admixture of sediments containing low 210Pb activity due to a coarser grain size fraction.
210Pb activity was measured for samples from core 050310-C6 using gamma spectrometry at the Leibniz-Laboratory for Radiometric Dating and Isotope Research (Kiel, Germany). The 210Pb supported activities in the present study were assessed from minimum activities (40 Bq kg–1) found in the sediment core, which are similar to the supported activities reported for similar sediments in the region (Szczuciński, 2010). However, supported activities are typically ascertained by averaging the nearly uniform, low-level 210Pb activities below the region of radioactive decay or through independent measurements of 226Ra (often through 214Pb and 214Bi; e.g., Zaborska et al., 2007; Szczuciński et al., 2009). Because the uniform activities in the lowermost part of the core were not reached and the 226Ra was not measured, a precise estimation of 210Pb supported activities could not be obtained. Supported 210Pb activity values in the order of 10 to 26 Bq kg−1 were also reported by Kennedy et al. (2008) from the nearshore sediments on the Andaman Sea coast and are considered in the discussion of the calculated accumulation rates. The linear sediment accumulation rate (SAR) was determined from the decline in the excess 210Pb activities using the following equation (Robbins and Edgington, 1975; McKee et al., 1983):
where λ is the decay constant (= 0.0311 year−1);
z is the depth in the core (cm)
A0 is the specific activity of excess 210Pb at a particular reference horizon (Bq kg−1)
A z is the specific activity of excess 210Pb at depth z below the reference horizon (Bq kg−1).
Along with 210Pb, 137Cs activity was measured using gamma spectrometry.
In water depths of 5 to 20 m, several regions covered with mud or revealing a channel-like morphology (Di Geronimo et al., 2009; Feldens et al., 2009, 2010, 2012), were found to host tsunami deposits. Representative sediment cores from these regions were selected for the present study (core 050310-C6 from a mud patch and core 051207-32 from the channel).
4.1 Sedimentary structure and grain size
Unit 1 (0–22 cm), was composed of brown, poorly sorted laminated silt that contained up to 10.8% clay and up to 8.4% sand. Only a few bioturbation traces were preserved. This unit was divided into three sub-units. The upper part (subunit 1a, 0–15 cm) was very finely laminated. It contained both horizontal and cross laminations, as well as erosional surfaces. Grey-scale changes of the x-ray image suggested slight upward fining within the laminae. The second subunit (1b, 15–20 cm) was composed mostly of silt. In comparison to the units located above and below this sub-unit, it was slightly depleted in sand and enriched in clay. It contained very gently marked horizontal laminations. The upper contact was transitional while the lower contact was sharp. The lower subunit (1c, 20– 22 cm) was composed of slightly coarser silt than the subunit above. The sediment was fining upward and conformably overlaid the sediments of unit 2.
Unit 2 (22–40 cm) was composed of sand, gravel, clay clasts, pieces of laterites, rocks and shells. The arrangement of these particles was subhorizontal, with the largest clasts being up to 3 cm in diameter. Based on a detailed analysis, this unit was divided into two subunits. The upper subunit 2a (22–38 cm) was composed of sediments ranging from normal grading gravels to fine sand. The lower contact with subunit 2b was erosional. Subunit 2b (38–40 cm) was composed of laminated medium to coarse sand.
Unit 3 (40–69 cm) was represented by laminated silt and clayey silt that was slightly finer than the sediment forming unit 1. Its upper contact was erosional and the basal contact was sharp. Within this unit, at least three fining-upward sequences were differentiated (3a: 40–50 cm, 3b: 50–61 cm, and 3c: 61–69 cm). These sequences began with thin sandy silt laminae and became finer with decreasing depth, eventually becoming clayey silt. Moreover, in subunit 3b, an erosional surface was preserved in the middle of the subunit. The lamination in the unit was slightly inclined, and few small vertical burrows were preserved. A 2 cm-diameter gravel was found at the bottom of this unit.
Unit 4 (69–99 cm) was composed of laminated muddy sand, which was partly intercalated with consolidated mud that was almost white. The layering and laminations were partly disturbed. In the upper 10 cm of this unit, white consolidated mud did not extend continuously in the horizontal plane, while the lowermost 5 cm of the sediment in the core was composed entirely of this type of sediment. Some small gravel components were found at a depth of 92–94 cm.
Core 051207-32 was retrieved from a water depth of 14.4 m and was 30 cm in length (Figs. 1 and 2, Table 1). This core also revealed several different sediment types, and was therefore divided into four units (Fig. 4):
Unit 1 (0–5 cm) was composed of a yellowish medium to coarse sand with shell fragments. This unit had a massive structure and conformably overlaid the upper surface of unit 2.
Unit 2 (5–20 cm) had a relatively complex composition. It was composed of consolidated sandy mud, muddy sand and sand. It was variable in colour, ranging from yellow or light green to olive or black. It was partly laminated, but also contained muddy clasts, pieces of wood, laterites and red brick fragments (artefacts). Sand appeared in the form of intercalations. Moreover, gravel and small pebbles were scattered throughout the entire unit. The grain size in this unit did not show normal grading, except for the upper part. The lower contact was sharp and uneven.
Unit 3 (20–25 cm) was a massive layer of coarse sand and gravels.
Unit 4 (25–30 cm) was composed of muddy sand. The upper part contained admixtures of coarse sand from unit 3.
Core 031207-23 was retrieved from a water depth of 55.4 m and was 70 cm long (Figs. 1 and 5, Table 1). It was composed of poorly sorted sandy silt and silty sand, with only 5.2% of clay. Shells were abundant in this core, and it was possible to distinguish two units.
Unit 1 (comprising the upper approx. 51 cm) was composed mostly of silty sand with intercalations of sandy silt. Laminations were poorly preserved and shells were less abundant than in the lower unit. No distinct boundary was observed between the units, and the lower boundary was selected in conjunction with changes in geochemistry. The upper part of the unit contains sandy intercalations of several cm-thick. The lowest sand content was found at a depth of 20–30 cm.
Unit 2 (approx. 51–70 cm) was also composed of silty sand intercalated with sandy silt. The intercalations appeared in the form of poorly preserved layers. This unit contained more shell fragments than unit 1.
4.2 Geochemical and physical properties
Log-ratios of Titanium (Ti) and Calcium (Ca), which represent the relative variations of terrigenous versus marine constituents, are shown in Figs. 3–5. Ti is enriched in tropical soils in the form of laterites and bauxites and is relatively inert against diagenetic processes (Calvert and Pedersen, 2007), whereas Ca reflects the occurrence of CaCO3, which is mainly produced under marine conditions (Hofmann et al., 2005; Weltji and Tjallingii, 2008). In all of the studied cores, changes in the Ti/Ca log-ratio roughly reflected the sedimentary units described above. In core 050310-C6 (Fig. 3), the ratio was stable in units 1 and 3, variable in unit 2 and generally elevated in unit 4. In core 051207-32 (Fig. 4), this ratio was slightly lower in the sandy, shell-rich units (units 1 and 3). This ratio was mostly uniform in core 031207-23 (Fig. 5), where only a slight downward increase was observed in unit 2.
The PCA revealed that two principal components of onshore samples and sediment samples from core 050310-C6 (PC1 and PC2) explained 80.5% of the cumulative variance. PC1 (accounting for 69.7% of the variance) had highly negative factor scores for terrestrial elements, such as Al, Si, S, K, Ti, Mn and Fe. PC2 (accounting for 10.8% of the variance) had highly positive factor scores for Ca and Si. This finding indicates that PC2 was characterised by a marine component, and Si was most likely associated with marine sands. Plotting these two main factors together (Fig. 6) indicates the grouping of sediment samples (circled on the graph). Samples from unit 2 of core 050310-C6 and onshore sediments had positive values for PC1, which indicated a stronger terrestrial influence than units 1 and 3. For PC2, most of units 1, 2 and 3 of core 050310-C6 had positive values, whereas onshore samples had negative values. This finding suggests that unit 2 of core 050310-C6 also had marine components. Therefore, sediments from unit 2 of core 050310-C6 were a mixture of terrestrial and marine components.
The bulk density of the studied cores was generally uniform, with the exception of slight variations in units 2 and 4 of core 050310-C6. The other measured physical properties did not reveal significant changes.
4.3 210Pb data and interpretation
The total 210Pb activity profile of core 050310-C6 (Fig. 7) revealed a general decline of activities with depth, interrupted by one major and several minor anomalies that were interpreted as being event layers or periods of accelerated sediment accumulation. These event layers reflect a non-steady sedimentation regime.
Using data on sedimentary structures as supporting information, the total 210Pb profile was divided into three major parts, referred to as sedimentary units 1, 2 and 3 (Fig. 3).
The upper portion of unit 1 was composed of three sediment segments (approximately 0–15 cm, 15–20 cm and 20–22 cm), which were most likely deposited during events or periods of accelerated accumulation, as indicated by step-like activity profiles. The uppermost segment could also be interpreted as a surface mixed layer; however, the well-preserved laminations suggest that sediment mixing due to bioturbation was not significant. Precise calculations of sediment accumulation rates were not possible since the accumulation was not steady and the background activities were only assumed. Depending on the 210Pb supported activities used and considering the analytical accuracy, the calculated sediment accumulation rates were in the range of 1.3 to 5.7 cm y−1. In general, the lower the supported activities applied, the higher the accumulation rate that we obtain. Since the assumptions for this method were not fully met (the accumulation was not steady), the results should be regarded as an approximation; we can infer from these results that the accumulation rate occurring is in the order of a few cm per year. This finding suggests that the unit had to be deposited over a period of several to a dozen years. Considering that the core was sampled in 2010, it is possible that the sediments in unit 1 were deposited after 2004.
Unit 2 (around 22 to 40 cm) was partly composed of coarse sediments, which do not contain excess 210Pb, as indicated by a sample taken from a depth of 38 cm which showed only the activity of supported 210Pb. The activities in the upper part of the unit and below are similar. Therefore, this unit was assumed to be an event layer. Moreover, similar 210Pb activities in the lowermost part of unit 1 and in the uppermost part of unit 3 also suggested that the event that created unit 2 was effectively depositional and caused little or no erosion of the older sediments.
Unit 3 (below 40 cm) revealed a general decline of 210Pb activity with depth; however, there were three segments with slightly reversed trends. Those segments were found at approximately the following depths: 40–50, 50–61 and 61–69 cm. These segments roughly corresponded to the fining-upward subunits 3a, 3b and 3c and most likely represented sedimentary events or periods of accelerated deposition. Calculations of sediment accumulation rates in this unit, under the conditions specified above, indicated rates of approximately 0.7 to 2.4 cm y−1.
The 137Cs values indicated very low activities, often close or below minimum detection activity levels (Fig. 7). However, the presence of 137Cs throughout the core supports a 210Pb-based interpretation of a high accumulation rate since 137Cs has been present in the environment since the early 1950s (Robbins et al., 1978). The very low activities observed were due in part to high accumulation rates and the dilution effect of the radioisotope in the large mass of sediment, and in part to generally low 137Cs fallout at this latitude (see discussion in Szczuciński et al., 2009).
5.1 Evidence of the 2004 Indian Ocean tsunami event layer
Sediment cores were collected within three to six years after the 2004 Indian Ocean tsunami. In the period between the tsunami and the time of collection, neither big storms nor intense anthropogenic offshore activities affected the region. Several tropical cyclones were recorded during the 20th century and passed near the study area; the last major cyclone in this region was Cyclone Gay in 1989 (Kumar et al., 2008; Brand, 2009). However, despite the fact that these events were recorded in middle continental shelf deposits (Szczuciński, 2010), they have not been found to cause significant sedimentological change in the eastern coastal region of the Andaman Sea due to their westward-oriented tracks (Brand, 2009). Consequently, the documented sedimentary event layers found in the inner shelf cores are considered to represent potential effects of the 2004 tsunami. For this event, maximum water velocities over the inner shelf have been modelled and show values in the order of several m s−1 (Suppasri et al., 2011).
In core 050310-C6, the most likely result of deposition by the 2004 tsunami was sediment unit 2, which was composed of poorly sorted sand and gravel between fine-grained deposits. This event layer contains compounds of terrestrial and marine origin: clay clasts, pieces of laterites, rocks and shells. The mixed provenance of the sediments was supported by the PCA, evaluating their chemical composition. These sediments were similar to samples taken from potential onshore sources, as well as marine sands (Fig. 6). Unit 2 is also marked by similar 210Pb activities above and below this unit and by anomalously low 210Pb activity in some samples taken from this unit, which supports its event origin. The deposits above and below (units 1 and 3) represent rapidly accumulating sediments (>1 cm y−1) with episodes of erosion and sedimentation indicated by sedimentary structures seen in X-radiographs (Fig. 3) and reflecting the dynamic nature of shallow water environments (water depths of approximately 10 m). The 210Pb-based assessment of accumulation rates confirmed, within error ranges, that unit 2 was several years old and could have been generated by the 2004 Indian Ocean tsunami.
Core 051207-32 was sampled within three years of the tsunami. The sand layer forming the uppermost portion of this core was very similar to sediments covering most of the continental shelf at water depths of 15 to 22 m (e.g., Feldens et al., 2009, 2010, 2012). This layer conformably covers units 2, 3 and 4 (>25 cm in thickness), which revealed many features of event deposits, such as poorly sorted sediments ranging from mud to gravel, muddy clasts, pieces of wood, laterites and pieces of red brick. The latter suggests that the sediments had material of terrigenous origin included. The changing character of the deposits (mud/sand/mud) may reflect changing flow velocities and directions, while minor changes in the Ti/Ca log-ratio may reflect changes in sediment sources. Based on this evidence and the assumptions presented above, units 2–4 are interpreted as having been deposited during the passage of the tsunami wave train.
The potential tsunami deposits in the two cores differed from one another in terms of the number of units with event deposits, their sedimentary characteristics and the relative input of terrestrial material. These characteristics may have been related to the various water depths (9.6 and 14.4 m), the distance offshore (3.1 and 7.2 km), and variations in the hydrodynamics of tsunami waves. Video records of the 2004 tsunami, which show the situation offshore Khao Lak revealed a high variability in flow patterns, including the formation of giant gyres (e.g., Di Geronimo et al., 2009).
Although there is a supporting age control for one core (in core 051207-32, it was not possible to evaluate those data due to the lack of suitable sediments above and below the event layer) and there was no evidence of recent heavy storms in the area, one may consider that the event deposits were formed by storms or cyclones. Storm deposits (tem-pestites) in shallow environments may reveal many various features depending on local conditions. There are no studies of storm deposits on the inner shelf in the Andaman Sea. However, in general, shallow water storm deposits may be sandy or muddy and often have basal erosional contact, normal gradation, plane lamination, wave ripples, thicknesses ranging from a few to more than 30 cm and hummocky cross stratification (e.g., Einsele et al., 1991; Weidong et al., 1997; Allison et al., 2005). Storm deposits may contain only one or many of these features. Moreover, as indicated by modern examples (e.g., Allison et al., 2005), changing flow conditions are also observed during a hurricane, and near-bottom velocities can reach more than 1 m s−1. Thus, many characteristics of storms and tsunamis over the continental shelf that affect sedimentation may be similar. The major features observed in the documented event layers, which are less likely, or unlikely, in storm deposits are: the frequent presence of terrestrial components, poor sorting and a massive character of some layers. Terrestrial components may be found in storm deposits if there is a big river nearby and can also occur due to coastal erosion. However, storms primarily tend to erode the coastline (beach, dune), while tsunamis may also deliver terrestrial material further inland such as human artefacts and plants. The poor sorting and massive character of sediments may indicate a kind of sediment gravity mass flow (expected during backwash). Gravity mass flows are also known to be generated by storms, for instance in form of wave-induced fluid mud flows (e.g., Nittrouer et al., 2007). However, the fluid mud flow deposits are usually better sorted, do not include oversized clasts and contain less terrestrial material when compared with tsunami deposits.
Sediments in core 031207-23 were taken from a water depth of 57 m. Distinct event layers were not recognised in this core, suggesting that the 2004 tsunami had no or very limited depositional effect in this region, which is supported by conclusion of Szczuciński (2010) based on 210Pb analyses of sediment cores from the mid continental shelf offshore Khao Lak.
5.2 Processes of offshore sedimentation by the tsunami
Assuming that the interpretation of the event layers as tsunami deposits in cores 050310-C6 (unit 2) and 051207-32 (units 2–4) is correct, these deposits may serve as a source of information about tsunami sedimentation processes.
In core 050310-C6 (water depth 9.6 m, 3.1 km offshore), unit 2 (interpreted as being a tsunami deposit) began with a subunit that is approximately 2 cm thick (2b). It is composed of horizontally laminated medium to coarse sand. This subunit showed no indication of terrigenous origin (the Ti/Ca ratio was similar to that in the sediments beneath it). There are several processes able of forming laminated sandy deposits, including flows in the upper and lower flow regimes, storms and turbidity currents (Reineck and Wunderlich, 1998). In the case presented in this study, it is likely that the sand was transported from water depths of 15-22 m, where medium and coarse sands are common (Feldens et al., 2012), toward the shoreline during the runup phase. To confirm this fact, a detailed analysis of micro-fossils is recommended in the future. The transport of sand could occur as a unidirectional flow in lower or upper plane bed conditions. Later on, an erosional surface was created, along with the deposition of unit 2a (approximately 16 cm thick). The subunit is likely to have been deposited as a result of decelerating flow conditions because it revealed a normal gradation. Considering the largest size of pebbles found in the lower part of the unit, the water velocity had to be at least in the order of several tens of cm s−1. This sub-unit contains many terrigenous components; moreover, its chemical composition is similar to the onshore sediments analysed (Fig. 6). Therefore, this unit probably was created during the backwash flow.
Units 2–4 in core 051207-32 (water depth 14.4 m, located 7.2 km offshore) could be interpreted as tsunami deposits. Because the retrieved sediment core does not reach below unit 4, it is unclear how the sequence of tsunami deposits begins. The lowermost unit is composed of massive consolidated mud with scattered gravel, pieces of wood, mud clasts and red brick fragments. Its chemical composition also suggests a terrigenous origin, and thus, this unit was most likely formed during backwash. This finding is supported by the presence of over-sized clasts “floating” in the finer sediment mass and by a relatively high sediment consolidation. This subunit was approximately 5 cm thick and was covered by coarse sand and gravel with a massive appearance. The Ti/Ca log-ratio in this thin layer was lower than that of the layer below, so these sediments may have no, or a lower, terrigenous contribution. The lack of clear lamination suggests that the deposition was rapid. The sand was covered by a complex, stiff mud with many over-sized compounds of sand and gravel (unit 2), which is very similar to the lowermost portion of unit 4. This finding is interpreted as being an effect of the backwash flow, although the terrestrial contribution is not clear in the sediment geochemistry. However, during the backwash from the second wave, the inundated land was already mostly covered with water (e.g., Choowong et al., 2008), so there was much less erosion on land than during the first wave backwash phase. The upper part of this unit was partly laminated and reflected an upward fining in grain size. It is possible that the sediment-gravity flow evolved, due to a decrease in flow density, into simple settling from suspension, or that the unit represents two (or more) events (or pulses).
5.3 Diagnostic features of offshore tsunami deposits
Onshore tsunami deposits are characterised by a complex set of diagnostic features that have been presented in many studies (e.g., Dawson and Shi, 2000; Goff et al., 2001; Shiki et al., 2008; Bourgeois, 2009; Mamo et al., 2009; Chagué-Goff, 2010; Goto et al., 2010; Chagué-Goff et al., 2011). However, such criteria have not yet been summarised for offshore tsunami deposits, and the published data are limited. In the literature, offshore tsunami deposits are frequently related not only to the direct effect of deposition from tsunami-induced water flow (run-up or backwash), but also to tsunami-induced secondary processes such as turbidity currents (Dawson and Stewart, 2007; Shiki et al., 2008) and formation processes of so-called “homogenites” (Cita et al., 1996). The present discussion is limited to the recent shallow water deposits most likely formed due to direct deposition from tsunamis.
Table 2 summarises major features of tsunami deposits on the inner shelf or within 15 km of land that were generated by the eruption of Santorini in ca. 1630–1550 BC (Goodman-Tchernov et al., 2009), the eruption of Krakatau in 1883 (van den Bergh et al., 2003), earthquakes on the Portuguese margin in 1755 and 1969 (Abrantes et al., 2008), several tsunamis in the Mediterranean (Smedile et al., 2011) and the 2004 Indian Ocean tsunami (Paris et al., 2010 and present study). Several sedimentological studies (e.g., Massari and D’Alessandro, 2000; Takashimizu and Masuda, 2000; Fujiwara and Kamataki, 2007) on potential shallow marine tsunami deposits from the geological past are not included in the discussion because they are not related to a specific tsunami event but are interpreted as being tsunami-generated based on sedimentological properties. The comparison proves how variable offshore tsunami deposits can be. The deposits may form an event layer several cm, several tens of cm or even over 1 m thick. The layers tend to have sharp lower contacts, which are often ero-sional. The upper contact may be blurred by bioturbations. They are composed of all grain size classes; often several classes are present in one layer resulting in poor sorting. Frequently, offshore tsunami deposits contain some typical terrigenous particles (wood, plants, etc.) and, if available, human-made pottery, brick, etc. This finding suggests the important role of tsunami backwash flows in the formation of these deposits. The fossil assemblage within the event layers may represent organisms from various environments. There was a high degree of variation in typical geochemi-cal indicators of marine (Ca) or terrestrial origin (Fe, Mn, Ti). The tsunami deposits may appear in the form of a single layer or several layers and may present the whole range of sedimentary structures: laminations, fining or coarsening upward, a massive structure, erosional surfaces, imbrications, lag deposits, etc. Finally, the key to the interpretation of these structures is accurate dating, with analyses such as 210Pb activity profiles being particularly helpful. For instance, in the case of 1969 tsunami deposits on the Portuguese shelf, there was no visible change in sediment properties apart from a slight change in the 210Pb profile (Abrantes et al., 2008).
The presented comparison of offshore tsunami deposit characteristics reveals that their interpretation may be even more difficult than in the case of onshore tsunami deposits. It appears that the identification will always have to be based on several characteristics and a broad knowledge of local conditions. Distinguishing offshore tsunami and storm deposits will be a considerable challenge for future studies.
The present study provided new evidence of probable 2004 Indian Ocean tsunami deposits left on the inner shelf of the Andaman Sea (Thailand) and identified the diagnostic sedimentological and geochemical properties of these deposits. The deposits were restricted to the shallow marine environment (water depths of 9–15 m) within 8 km of the shoreline. Deposition occurred during the run-up phase, causing landward redeposition of marine sand, and during backwash flow events, which also deposited terrigenous sediments. The transport and deposition of sediments were driven by several processes, including unidirectional flow in various flow regimes and high-density sediment-gravity flow.
Typical features of these event deposits included the following: a thickness in the order of 20–25 cm, a wide range of grain sizes and poor sorting, in contrast to underlying and overlying sediments, the presence of several layers, marine sand alternating with poorly sorted mud with terrigenous and anthropogenic components, representing different hy-drodynamic conditions (run-up and backwash phase).
Geochemical and geophysical analyses, and particularly 210Pb activity measurements, were helpful supplementary tools in the identification of event layers. However, the analysis of available data on offshore tsunami deposits showed that there is no single set of signatures that could be universally applied to identify these deposits. Future studies will need to include more proxies (microfossils and advanced geochemistry in particular) to establish an identification key for offshore tsunami deposits.
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We are grateful to Phuket Marine Biological Center (PMBC) for supporting us with ship time of RV Chakra-tong Tongyai and RV Boonlert Pasook as well as with other facilities during field campaigns. We further thank Dr. Warner Bruckmann and Dr. Dieter Garbe-Schonberg for supporting the MSCL and XRF scanner measurements. Gratitude is also expressed to Dr. Nils Anderson and Dr. Helmut Erlenkeuser for their helpful comments and 210Pb determination. We thank Dr. Bjorn Heise and Daniel Unverricht for their tremendous help and inspiring ideas. Acknowledgements are due to Dr. P. M. De Martini and Dr. C. Chagué-Goff for their very constructive and detailed reviews. This research was funded by Deutsche Forschungsgemeinschaft (DFG) grant SCHW 572/11, National Research Council of Thailand (NRCT) and DAAD (Deutscher Akademischer Austausch Dienst) fellowship provided to Ms. Daroonwan Sakuna for a Ph.D. study at Kiel University.
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Sakuna, D., Szczuciński, W., Feldens, P. et al. Sedimentary deposits left by the 2004 Indian Ocean tsunami on the inner continental shelf offshore of Khao Lak, Andaman Sea (Thailand). Earth Planet Sp 64, 11 (2012) doi:10.5047/eps.2011.08.010
- 2004 Indian Ocean tsunami
- offshore tsunami deposits
- Khao Lak