# Record of the Climatic Variability and the Sedimentary Dynamics during the Last Two Millennia at Sebkha Dkhila, Eastern Tunisia

Authors: Elhoucine Essefi; Jamel Touir; Mohamed Ali Tagorti; Chokri Yaich
Journal: ISRN Geology
 (2013)

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## Abstract

This paper aimed to study the record of the climatic variability during the last two millennia within the sebkha of Dkhila. Six climatic stages were recognized along the 104 cm core: the Warming Present (WP), the Late Little Ice Age (Late LIA), the Early Little Ice Age (ELIA), the Medieval Climatic Anomaly (MCA), the Dark Age (DA), and the Roman Warm Period (RWP). The WP stretches along the uppermost 1 cm with a high grey scale as sign of a dry climate. The Late LIA is located between 1 cm and 6 cm. The ELIA is located between 6 cm and 40 cm. The MCA spanning from 40 cm to 72 cm is marked by a sharp increase of the GS revealing a wet period. The DA appears along the part between 72 cm and 84 cm; a shift from light to dark sediments is recorded. The RWP appears between 84 cm and 104 cm. Based on the grain size distribution, two low frequency cycles were identified indicating radical global changes of climatic conditions, the differential tectonics, and the groundwater fluctuations. On the other hand, high frequency cycles indicate local modifications of the climatic conditions.


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## Body

## 1. Introduction

It was previously proven [1–4] that the sebkha Dkhila (as part of the sebkha Sidi El Hani) is dominated by a hydrogeological basin feeding this depression by salty water. Consequently, the hydrogeological context remains stable regardless of the climatic change. In such a case, the playa would not record the climatic variability because the high salinity imposed by coming up of saline water does not radically change with respect to climatic changes. At the level of the watershed surrounding the depression, previous investigations [5] showed the outcrop of wet aeolian sediments mainly dominated by groundwater involvement rather than the climatic variability. Subsequently, it is not evident to find an obvious record of climate changes within the watershed. The aim in this paper is to overcome these handicaps and to infer the climatic variability during the last two millennia based on the visual description of cores, the magnetic properties, and the grain-size distribution.


## 2. Study Area

The sebkha of Dkhila is part of the sebkha of Sidi El Hani, which is in turn part of the system Mechertate-Chrita-Sidi El Hani. Though it has always been treated as a single unit, the sebkha of Sidi El Hani as such is actually made up of three communicated playas; from north to the south, one finds the playas of Sidi El Hani (sensu stricto), of Souassi Sou, and of Dkhila (Figure 1). The sebkha of Mhabeul is located in the southeast of Tunisia (Figure 1). It is an inland saline environment located in southeast Tunisia (Figure 1). Based on a 65 cm core, it was used by Marquer et al. [6] to infer the climatic variability during the last two millennia. Since it is the only known sebkha of which we have the record of the climatic variability during the last millennia, this sebkha serves as reference to find out the major climatic events in the sebkha Dkhila.Figure 1
Geographical location of sebkhas Dkhila and Mhabeul.


## 3. Methods and Materials

Coring technique proves efficient to study the sedimentary dynamics and the record of the climatic variability [1, 7]. In the laboratory, cores underwent nondestructive and destructive analyses.The sediment darkness is a result of a high ratio of the organic matter content, which reflects high degree of confinement. As it was used by Marquer et al. [6], an arbitrary method was used in this study to evaluate this darkness on the basis of the grey scale (GS). Minimum grey-scale values are associated with high magnitude flood. This could characterize periods with high frequency of intense precipitation events, most probably during the wet seasons. Maximum grey-scale values are associated with more stable climatic conditions, marked by flood events of lower magnitude or lower-frequency scale. The evaluation of darkness needed software of image treatment because minor grey-scale variability could be detected only by such a sophistication (e.g., [6]). But, in the case of the Dkhila core, only visual method was used; consequently, it was more convenient to speak about the major grey-scale variability. Since we have been paving the way for comparison between the sebkha Dkhila core and the sebkha Mhabeul one, the minor grey scale detected by software in sebkha Mhabeul core had to be converted to the major grey scale detected by the naked eye.Wet process analyses were carried out by the FRITSCH laser grain-size analyzer. Then, the descriptive grain-size distribution was carried out based on the ternary diagram sand/silt/clay of Shepard [8]. The core was also investigated in terms of genetic grain-size distribution. This investigation distinguished between the aeolian, the geochemical, and the hydraulic sedimentations based on modes of the grain-size distribution [1, 9–12]. Sun et al. [9] considered the fraction centered around 6 μm as fine aeolian component and the fraction centered around 60 μm as coarse aeolian component, whereas the coarse hydraulic component is centered around 380 μm and the fine hydraulic fraction is centered around 1 μm. Based on their cumulative curves, Cailleux and Tricart [13] distinguished between 23 types of sedimentation: six estuary and deltaic, seven marine, two glacial, three aeolian, and five fluvial types. Added to the traditional sand/silt/clay subdivision used in the literature, Manté et al. [11] coined the term colloids as the fraction between 0.063 μm and 1 μm. This fraction is of a geochemical origin. Grain-size components of aeolian deposits depend on the nature of winds (i.e., high- and low-altitude air flows and near-ground winds) and transport distances (long or short distance) [9, 14, 15]. Based on the method of features of Allen and Haslett [10], the descriptive classification of Flemming [16] and the three reference cumulative curves of aeolian types (their transformation toward frequency curves) discussed by Cailleux and Tricart [13] and Essefi [1] distinguished between three types of aeolian sediments. First, the aeolian sand could be transported by strong wind. Its most important features are the mode at 500 μm and the two shoulders at 250 μm and 1600 μm. Consequently, this aeolian sediment is classified according to sand/silt/clay diagram of Flemming [16] as sand. Second, the slightly silty aeolian sand [16] could be transported by a moderate wind. The most important features are the mode at 315 μm and the two shoulders at 200 μm and 800 μm. Third, the silty aeolian sand [16] could be transported by calm wind. The most apparent features are the mode at 160 μm and the two shoulders at 250 μm and 1000 μm. To conclude, the fractions centered around 6, 60  [9], 160, 315, and 500 μm [1] mark the aeolian component. The hydraulic component is marked by the fractions 1 μm and 380 μm [9]. The geochemical fraction is marked by colloids, which are smaller than 1 μm [11].The magnetic susceptibility was measured by the Bartington MS2B probe in the laboratory of Sedimentary Dynamics and Environment, National engineering School of Sfax, at a frequency of 0.47 kHz. The use of the magnetic susceptibility is twofold. On the one hand, it allows the detection of high magnetic signature probably related to tephra layers, which may serve in dating the core. The use of magnetic susceptibility in tephrostratigraphy was recently discussed by Essefi et al. [17]. On the other hand, it may have a climatic or sedimentary significance.


## 4. Results

### 4.1. Correlation between Sebkhas Mhabeul and Dkhila

The correlation between core (104 cm) from sebkha Dkhila and a core from sebkha Mhabeul (65 cm) (Figure2) shows that the climatic variability recorded during the last two millennia in 65 cm is recorded in core of sebkha Dkhila in 104 cm. The rate of sedimentation is higher in this location of sebkha Dkhila than in sebkha Mhabeul. By following the major grey-scale variability and the three reference bands along both cores, the six climatic stages recognized in sebkha Mhabeul were also found out along the core of sebkha Dkhila. First, the Warming Present (WP) stretches along the uppermost 1 cm with its high grey scale as sign of a dry climate. Second, the Late Little Ice Age (Late LIA) is located between 1 cm and 6 cm. As in sebkha Mhabeul core, this period is limited at the bottom by the first reference sandy band. Third, Early Little Ice Age (ELIA) is located between 6 cm and 40 cm. Climatologically, the intermediate values of GS having a tendency toward increasing indicate that this stage may be classified as moderate with a tendency toward aridity. Fourth, the Medieval Climatic Anomaly (MCA) spanning from 40 cm to 72 cm is marked by a sharp increase of the GS revealing a wet period. Fifth, Dark Age (DA) appears along the part between 72 cm and 84 cm; a shift from light to dark sediments is recorded. As for the grain-size distribution, the second reference sandy band is detected in the top of the DA. Sixth, the Roman Warm Period (RWP) appears between 84 cm and 104 cm. According the major grey scale, this period may be divided into substages. The first (from 84 cm to 94 cm in sebkha Dkhila core) is marked by high GS values associated with dark sediments suggesting stable climatic conditions. The second (from 94 cm to 104 cm in the sebkha Dkhila core) is marked by a third sandy reference band and low GS values as signs of wet climate.Figure 2
Correlation between sebkhas Mhabeul and Dkhila based on the gray-scale variability and three sandy reference bands.


### 4.2. Occurrence of Sedimentary Facies during the Climatic Stages

The descriptive grain-size distribution (Figure3) shows the evolution of the sedimentary dynamics within the sebkha of Dkhila. The top (H1), the middle (H8), and the bottom (H62) of the core are basically a mixture facies (F1) with dominance of the sandy fraction. The second facies (F2) is basically clayey represented by the samples H58, H59, H60, and H61. The third facies (F3) is basically a mixture of silt and clay represented by the samples H2, H4, and H10. The fourth facies is basically silty represented by the samples H3, H5, H6, H7, and H9.Figure 3
Samples of the core from sebkha Dkhila within the ternary diagram of Shepard [8].


### 4.3. Evolution of the Genetic Grain-Size Distribution during the Climatic Stages

Based on the mean of the grain-size distribution and the magnetic susceptibility, the core of sebkha Dkhila may be subdivided into different sedimentary facies (Figure4). These facies are the record of climatic change, groundwater fluctuations, and differential tectonics.Figure 4
Mean of the grain size distribution, magnetic susceptibility, and cyclostratigraphy along the core of sebkha Dkhila.The same sedimentary or transportation processes usually give birth to unimodal frequency curves of grain-size distribution. When involving more than one sedimentary or transportation process and sediments with a polymodal distribution, a polymodal distribution is the sum of all kinds of sedimentary components [9, 18–23]. The aeolian deposits possess clear grain-size distribution features different from other sediments (e.g., [18, 23–27]). Most modal peaks of grain-size frequency curves of aeolian deposits in lacustrine sediments are between 10 and 100 μm [19, 21, 22, 28–31]. Hence, we regard the primary modal peaks (between 10 and 100 μm, mode at about 40 μm) of ISL1A core samples as the aeolian component within lacustrine sediments. In arid regions, rivers with low discharge are normally not able to transport coarse particles (e.g., >60 μm) to the central part of a lake [30, 32]. Liu et al. [21] interprets the coarse-grained materials with mode at about 35–40 μm as aeolian component within lacustrine sediments in other arid and closed lakes on the QTP.


#### 4.3.1. Warming Present (WP) and the Late Little Ice Age (Late LIA)

The first facies is located at the first 5 cm; it is sandy silt. The WP period and Little Ice Age (Late LIA) [33] expand to 400 yrBP; that is, 320 years are dominated by a sandy sedimentation. The top of the cycle (Figure 5) shows an obvious coarsening; it is characterized by a primary mode (M: ca. 10 μm) as an indication of the fine aeolian sedimentation. This component coincides with the silty fraction of the sample. The secondary mode (m: less than 140 μm) is an indication of the coarse aeolian sedimentation. This component coincides with the silty fraction of the sample.Figure 5
Grain-size distribution of the WP and the Late LIA along the core from sebkha Dkhila.


#### 4.3.2. Early Little Ice Age

The clayey samples H2 and H4 (Figures6(a) and 6(c)) belong to the facies F3; they are expressed by a fine sedimentation (M: ca. 2.5 μm), which coincides with the minimum of accommodation. This decrease of accommodation is due to stable climatic conditions and/or water table rise. Genetically, this component is probably of hydraulic origin. However fine, H3 and H6 show a tendency towards coarsening (Figures 6(b) and 6(e)); genetically speaking, these silt facies F4 are characterized by the dominance of the fine aeolian fraction (M: ca. 6 μm) and the appearance of the coarse aeolian sedimentation (m: ca. 160 μm). It is worth noting however that, belonging to the same facies F4, H5 and H7 are genetically distinguished from H3 and H6. The coarse aeolian sedimentation (m: ca. 160 μm) is absent. This is one of the pitfalls of the descriptive grain-size distribution. As a matter of fact, Flemming [16] critically studied the credibility of ternary diagrams sand/silt/clay in the interpretation of sedimentary dynamics and depositional environments.Grain-size distribution of the Early Little Ice Agealong the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)
(f)


#### 4.3.3. Medieval Climatic Anomaly (MCA)

The MCA is marked by an increase of the mean of the grain-size distribution (Figure7). The obvious coarsening with a primary mode (M: ca. 160 μm) is an indication of the coarse aeolian sedimentation and a secondary mode (m: ca. 2.5 μm) is an indication of the fine hydraulic sedimentation and an absent (A: ca. 10–100 μm). This mixture of sand/silt/clay shows a tendency toward the coarse fraction.Figure 7
Grain-size distribution of the Medieval Climatic Anomalyalong the core from sebkha Dkhila.


#### 4.3.4. Dark Age (DA)

The samples H9 and H10 are silty belonging to the facies F4 and F3, respectively. The top of this period H9 is coarser (Mean: 6.58μm); it is expressed by a coarse aeolian fraction (Figure 8(b)). The bottom of this period becomes finer (Mean: 6.58 μm); it is characterized by a primary mode (M: ca. 2.90 μm) as indication of the fine hydraulic sedimentation.Grain-size distribution of the Dark Agealong the core from sebkha Dkhila.
(a)
(b)


#### 4.3.5. Roman Warm Period

This period shows an obvious fining (F2: H58, H59, H60, and H61) of the mean of the grain-size distribution. The clayey facies F2 is dominated by the geochemical (less than 1μm) and hydraulic (centered around ca. 1.8 μm) fractions (Figures 9(a), 9(b), 9(c), and 9(d)). The stable climatic conditions are in favor of the sedimentation of the fine fraction.Grain-size distribution of the Roman Warm Period along the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)


## 4.1. Correlation between Sebkhas Mhabeul and Dkhila

The correlation between core (104 cm) from sebkha Dkhila and a core from sebkha Mhabeul (65 cm) (Figure2) shows that the climatic variability recorded during the last two millennia in 65 cm is recorded in core of sebkha Dkhila in 104 cm. The rate of sedimentation is higher in this location of sebkha Dkhila than in sebkha Mhabeul. By following the major grey-scale variability and the three reference bands along both cores, the six climatic stages recognized in sebkha Mhabeul were also found out along the core of sebkha Dkhila. First, the Warming Present (WP) stretches along the uppermost 1 cm with its high grey scale as sign of a dry climate. Second, the Late Little Ice Age (Late LIA) is located between 1 cm and 6 cm. As in sebkha Mhabeul core, this period is limited at the bottom by the first reference sandy band. Third, Early Little Ice Age (ELIA) is located between 6 cm and 40 cm. Climatologically, the intermediate values of GS having a tendency toward increasing indicate that this stage may be classified as moderate with a tendency toward aridity. Fourth, the Medieval Climatic Anomaly (MCA) spanning from 40 cm to 72 cm is marked by a sharp increase of the GS revealing a wet period. Fifth, Dark Age (DA) appears along the part between 72 cm and 84 cm; a shift from light to dark sediments is recorded. As for the grain-size distribution, the second reference sandy band is detected in the top of the DA. Sixth, the Roman Warm Period (RWP) appears between 84 cm and 104 cm. According the major grey scale, this period may be divided into substages. The first (from 84 cm to 94 cm in sebkha Dkhila core) is marked by high GS values associated with dark sediments suggesting stable climatic conditions. The second (from 94 cm to 104 cm in the sebkha Dkhila core) is marked by a third sandy reference band and low GS values as signs of wet climate.Figure 2
Correlation between sebkhas Mhabeul and Dkhila based on the gray-scale variability and three sandy reference bands.


## 4.2. Occurrence of Sedimentary Facies during the Climatic Stages

The descriptive grain-size distribution (Figure3) shows the evolution of the sedimentary dynamics within the sebkha of Dkhila. The top (H1), the middle (H8), and the bottom (H62) of the core are basically a mixture facies (F1) with dominance of the sandy fraction. The second facies (F2) is basically clayey represented by the samples H58, H59, H60, and H61. The third facies (F3) is basically a mixture of silt and clay represented by the samples H2, H4, and H10. The fourth facies is basically silty represented by the samples H3, H5, H6, H7, and H9.Figure 3
Samples of the core from sebkha Dkhila within the ternary diagram of Shepard [8].


## 4.3. Evolution of the Genetic Grain-Size Distribution during the Climatic Stages

Based on the mean of the grain-size distribution and the magnetic susceptibility, the core of sebkha Dkhila may be subdivided into different sedimentary facies (Figure4). These facies are the record of climatic change, groundwater fluctuations, and differential tectonics.Figure 4
Mean of the grain size distribution, magnetic susceptibility, and cyclostratigraphy along the core of sebkha Dkhila.The same sedimentary or transportation processes usually give birth to unimodal frequency curves of grain-size distribution. When involving more than one sedimentary or transportation process and sediments with a polymodal distribution, a polymodal distribution is the sum of all kinds of sedimentary components [9, 18–23]. The aeolian deposits possess clear grain-size distribution features different from other sediments (e.g., [18, 23–27]). Most modal peaks of grain-size frequency curves of aeolian deposits in lacustrine sediments are between 10 and 100 μm [19, 21, 22, 28–31]. Hence, we regard the primary modal peaks (between 10 and 100 μm, mode at about 40 μm) of ISL1A core samples as the aeolian component within lacustrine sediments. In arid regions, rivers with low discharge are normally not able to transport coarse particles (e.g., >60 μm) to the central part of a lake [30, 32]. Liu et al. [21] interprets the coarse-grained materials with mode at about 35–40 μm as aeolian component within lacustrine sediments in other arid and closed lakes on the QTP.


### 4.3.1. Warming Present (WP) and the Late Little Ice Age (Late LIA)

The first facies is located at the first 5 cm; it is sandy silt. The WP period and Little Ice Age (Late LIA) [33] expand to 400 yrBP; that is, 320 years are dominated by a sandy sedimentation. The top of the cycle (Figure 5) shows an obvious coarsening; it is characterized by a primary mode (M: ca. 10 μm) as an indication of the fine aeolian sedimentation. This component coincides with the silty fraction of the sample. The secondary mode (m: less than 140 μm) is an indication of the coarse aeolian sedimentation. This component coincides with the silty fraction of the sample.Figure 5
Grain-size distribution of the WP and the Late LIA along the core from sebkha Dkhila.


### 4.3.2. Early Little Ice Age

The clayey samples H2 and H4 (Figures6(a) and 6(c)) belong to the facies F3; they are expressed by a fine sedimentation (M: ca. 2.5 μm), which coincides with the minimum of accommodation. This decrease of accommodation is due to stable climatic conditions and/or water table rise. Genetically, this component is probably of hydraulic origin. However fine, H3 and H6 show a tendency towards coarsening (Figures 6(b) and 6(e)); genetically speaking, these silt facies F4 are characterized by the dominance of the fine aeolian fraction (M: ca. 6 μm) and the appearance of the coarse aeolian sedimentation (m: ca. 160 μm). It is worth noting however that, belonging to the same facies F4, H5 and H7 are genetically distinguished from H3 and H6. The coarse aeolian sedimentation (m: ca. 160 μm) is absent. This is one of the pitfalls of the descriptive grain-size distribution. As a matter of fact, Flemming [16] critically studied the credibility of ternary diagrams sand/silt/clay in the interpretation of sedimentary dynamics and depositional environments.Grain-size distribution of the Early Little Ice Agealong the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)
(f)


### 4.3.3. Medieval Climatic Anomaly (MCA)

The MCA is marked by an increase of the mean of the grain-size distribution (Figure7). The obvious coarsening with a primary mode (M: ca. 160 μm) is an indication of the coarse aeolian sedimentation and a secondary mode (m: ca. 2.5 μm) is an indication of the fine hydraulic sedimentation and an absent (A: ca. 10–100 μm). This mixture of sand/silt/clay shows a tendency toward the coarse fraction.Figure 7
Grain-size distribution of the Medieval Climatic Anomalyalong the core from sebkha Dkhila.


### 4.3.4. Dark Age (DA)

The samples H9 and H10 are silty belonging to the facies F4 and F3, respectively. The top of this period H9 is coarser (Mean: 6.58μm); it is expressed by a coarse aeolian fraction (Figure 8(b)). The bottom of this period becomes finer (Mean: 6.58 μm); it is characterized by a primary mode (M: ca. 2.90 μm) as indication of the fine hydraulic sedimentation.Grain-size distribution of the Dark Agealong the core from sebkha Dkhila.
(a)
(b)


### 4.3.5. Roman Warm Period

This period shows an obvious fining (F2: H58, H59, H60, and H61) of the mean of the grain-size distribution. The clayey facies F2 is dominated by the geochemical (less than 1μm) and hydraulic (centered around ca. 1.8 μm) fractions (Figures 9(a), 9(b), 9(c), and 9(d)). The stable climatic conditions are in favor of the sedimentation of the fine fraction.Grain-size distribution of the Roman Warm Period along the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)


## 4.3.1. Warming Present (WP) and the Late Little Ice Age (Late LIA)

The first facies is located at the first 5 cm; it is sandy silt. The WP period and Little Ice Age (Late LIA) [33] expand to 400 yrBP; that is, 320 years are dominated by a sandy sedimentation. The top of the cycle (Figure 5) shows an obvious coarsening; it is characterized by a primary mode (M: ca. 10 μm) as an indication of the fine aeolian sedimentation. This component coincides with the silty fraction of the sample. The secondary mode (m: less than 140 μm) is an indication of the coarse aeolian sedimentation. This component coincides with the silty fraction of the sample.Figure 5
Grain-size distribution of the WP and the Late LIA along the core from sebkha Dkhila.


## 4.3.2. Early Little Ice Age

The clayey samples H2 and H4 (Figures6(a) and 6(c)) belong to the facies F3; they are expressed by a fine sedimentation (M: ca. 2.5 μm), which coincides with the minimum of accommodation. This decrease of accommodation is due to stable climatic conditions and/or water table rise. Genetically, this component is probably of hydraulic origin. However fine, H3 and H6 show a tendency towards coarsening (Figures 6(b) and 6(e)); genetically speaking, these silt facies F4 are characterized by the dominance of the fine aeolian fraction (M: ca. 6 μm) and the appearance of the coarse aeolian sedimentation (m: ca. 160 μm). It is worth noting however that, belonging to the same facies F4, H5 and H7 are genetically distinguished from H3 and H6. The coarse aeolian sedimentation (m: ca. 160 μm) is absent. This is one of the pitfalls of the descriptive grain-size distribution. As a matter of fact, Flemming [16] critically studied the credibility of ternary diagrams sand/silt/clay in the interpretation of sedimentary dynamics and depositional environments.Grain-size distribution of the Early Little Ice Agealong the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)
(f)


## 4.3.3. Medieval Climatic Anomaly (MCA)

The MCA is marked by an increase of the mean of the grain-size distribution (Figure7). The obvious coarsening with a primary mode (M: ca. 160 μm) is an indication of the coarse aeolian sedimentation and a secondary mode (m: ca. 2.5 μm) is an indication of the fine hydraulic sedimentation and an absent (A: ca. 10–100 μm). This mixture of sand/silt/clay shows a tendency toward the coarse fraction.Figure 7
Grain-size distribution of the Medieval Climatic Anomalyalong the core from sebkha Dkhila.


## 4.3.4. Dark Age (DA)

The samples H9 and H10 are silty belonging to the facies F4 and F3, respectively. The top of this period H9 is coarser (Mean: 6.58μm); it is expressed by a coarse aeolian fraction (Figure 8(b)). The bottom of this period becomes finer (Mean: 6.58 μm); it is characterized by a primary mode (M: ca. 2.90 μm) as indication of the fine hydraulic sedimentation.Grain-size distribution of the Dark Agealong the core from sebkha Dkhila.
(a)
(b)


## 4.3.5. Roman Warm Period

This period shows an obvious fining (F2: H58, H59, H60, and H61) of the mean of the grain-size distribution. The clayey facies F2 is dominated by the geochemical (less than 1μm) and hydraulic (centered around ca. 1.8 μm) fractions (Figures 9(a), 9(b), 9(c), and 9(d)). The stable climatic conditions are in favor of the sedimentation of the fine fraction.Grain-size distribution of the Roman Warm Period along the core from sebkha Dkhila.
(a)
(b)
(c)
(d)
(e)


## 5. Conclusion

The VCD was a useful tool for correlation between Dkhila cores and a core from sebkha Mhabeul in order to guess the climatic variability during the last two millennia in this clay pan. This method has permitted the guessing of the climatic variability in sebkha Dkhila during the last two millennia. The six climatic stages recognized in sebkha Mhabeul core were identified in the core of Dkhila clay pan. Furthermore, the studied core proves that sebkha Dkhila is more subsiding than sebkha Mhabeul. These climatic stages are combined with a radical change of the sedimentary dynamics detected based on the genetic study of the grain-size distribution.



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*Source: 936198-2013-07-15.xml*