Timing and intensity of humid interglacial and interstadial periods from the Eemian in the southwestern Mediterranean region: new chronological and stable isotope data from Aït Said ou Idder (Middle Atlas) and comparison with other regional tufa deposits (Morocco and southern Spain)
- 1Laboratoire de Géographie Physique: environnements quaternaires et actuels (UMR 8591), CNRS – Université Paris 1 Panthéon-Sorbonne – Université Paris-Est Créteil, Meudon, France
- 2Trajectoires (UMR 8215), CNRS – Université Paris 1 Panthéon-Sorbonne, Paris, France
- 3Histoire Naturelle de l'Homme Préhistorique (UMR 7194), CNRS – MNHN, Paris, France
- 4Archéozoologie – Archéobotanique. Sociétés, pratiques et environnements (UMR 7209), CNRS – MNHN, Paris, France
- 5Département de Géologie, Université Mohammed V de Rabat, Rabat, Morocco
- 6Environnement, Ville, Société (UMR 5600, IRG), CNRS – Université de Lyon, Lyon, France
Correspondence: Julie Dabkowski (firstname.lastname@example.org)
Dabkowski, J., Wackenheim, Q., Falguères, C., Fiorillo, D., Tombret, O., Limondin-Lozouet, N., Boudad, L., and Berger, J.-F.: Timing and intensity of humid interglacial and interstadial periods from the Eemian in the southwestern Mediterranean region: new chronological and stable isotope data from Aït Said ou Idder (Middle Atlas) and comparison with other regional tufa deposits (Morocco and southern Spain), E&G Quaternary Sci. J., 71, 45–58, https://doi.org/10.5194/egqsj-71-45-2022, 2022.
In the last few decades, multidisciplinary research on calcareous tufas as palaeoenvironmental and palaeoclimatic records has intensively grown, which has provided an increasing number of well-documented sites. Consequently, inter-site comparisons and regional- to continental-scale reviews have developed, discussing the link between tufa distribution and climate or providing diachronic comparisons of climatic and environmental conditions prevailing during Quaternary interglacials (and interstadials). This paper proposes such a review for the southeastern Mediterranean area, including new dating and isotopic data from Aït Said ou Idder (northern Morocco) to be compared with available regional data, in order to discuss the intensity of some humid periods of the last 125 kyr.
According to several radiocarbon and U–Th dates, three chronological phases are indeed identified at Aït Said ou Idder: the Holocene, the Dansgaard–Oeschger (D–O) interstadial 8 and the Marine Isotopic Stage (MIS) 5e. Similarly, other tufa deposits from both Morocco and southern Spain (mostly Andalusia) appear to have preferentially developed during interglacial or interstadial periods, marked by maximal developments of the Mediterranean forest as reported in the palynological records from regional marine cores. Furthermore, isotopic data (δ18O and δ13C) from Aït Said ou Idder (and from other southeastern Mediterranean tufa deposits where available) suggest no significant difference in terms of temperature or air mass circulation between the Holocene, D–O 8 and MIS 5e. In terms of humidity conditions, no evidence of strong aridity is recorded even if D–O 8 appears drier than both interglacials. Conditions seems slightly wetter during the Holocene than during MIS 5e, but δ13C values at Aït Said ou Idder could also reflect strong differences in the seasonality of these interglacials. We demonstrate that calcareous tufa deposits have promising potential for discussing, in both space and time, the climate variability in the southeastern Mediterranean area, but new investigations, including dating and stable isotopes, are required to accurately feed such discussions.
In den letzten Jahrzehnten ist die multidisziplinäre Forschung zur Rolle von Kalktuffen (Tufa) als Paläoumwelt- und Paläoklima-Archiv intensiv ausgebaut worden, wodurch nun eine weiterhin wachsende Zahl gut dokumentierter Standorte vorliegt. Infolgedessen war es im Rahmen von Vergleichen zwischen verschiedenen Standorten und auf der Grundlage vergleichender Bewertungen auf regionalem bis hin zu kontinentalem Maßstab einerseits möglich, den Zusammenhang zwischen der Verteilung von Kalktuffen und Klima zu diskutieren, sowie andererseits diachrone Vergleiche von klimatischen Bedingungen und Umweltbedingungen während der Interglaziale (und Interstadiale) im Quartär durchzuführen. Diese Studie stellt eine solche vergleichende Bewertung für den südöstlichen Mittelmeerraum bereit und präsentiert darüber hinaus neue Datierungen und Isotopen-Daten aus Aït Said ou Idder (nördliches Marokko), die mit vorliegenden regionalen Daten verglichen werden, um somit eine Einschätzung der Intensität ausgewählter humider Abschnitte der letzten 125 kyr vornehmen zu können.
Basierend auf mehreren Radiokohlenstoff- und U–Th-Datierungen können in Aït Said ou Idder drei chronologische Phasen ausgewiesen werden: das Holozän, das Dansgaard/Oeschger Interstadial 8 und das MIS 5e. In ähnlicher Weise scheinen sich andere Kalktuffablagerungen sowohl aus Marokko als auch aus Südspanien (hauptsächlich Andalusien) bevorzugt während solcher Interglazial- oder Interstadialperioden entwickelt zu haben, die basierend auf der palynologischen Auswertung regionaler mariner Bohrkernarchive durch eine maximale Entwicklung mediterraner Wälder gekennzeichnet sind. Darüber hinaus deuten Isotopendaten (δ18O and δ13C) aus Aït Said ou Idder (und aus anderen Kalktuffen des südöstlichen Mittelmeerraumes, sofern verfügbar) darauf hin, dass es keine signifikanten Unterschiede in Bezug auf Temperatur oder Luftmassenzirkulation zwischen dem Holozän, dem D/O 8 und dem MIS 5e gab. Im Hinblick auf die Feuchtigkeitsbedingungen finden sich keine Hinweise starker Aridität, auch wenn das D/O 8 relativ trockener erscheint als beide Interglaziale. Die Bedingungen scheinen während des Holozäns etwas feuchter gewesen zu sein als während des MIS 5e, aber die δ13C-Werte in Aït Said ou Idder könnten auch starke Unterschiede in der Saisonalität dieser Interglaziale widerspiegeln. Unsere Studie zeigt, dass Kalktuffablagerungen ein vielversprechendes Potenzial haben, um die Klimavariabilität im südöstlichen Mittelmeerraum sowohl räumlich als auch zeitlich zu diskutieren, aber neue Untersuchungen, einschließlich Datierungen und Untersuchungen an stabilen Isotopen, sind erforderlich, um diese Diskussion sorgfältig und genau zu untermauern. (Abstract was translated by Christopher Luethgens.)
In the last few decades, multidisciplinary research on calcareous tufas has intensively grown regarding their potential for palaeoenvironmental and palaeoclimatic studies: they are one of the few continental archives to simultaneously provide records of past environments (including fauna and flora) and independent proxies for climatic variations (from calcite stable isotopes) which can also be precisely and objectively dated (Andrews, 2006; Capezzuoli et al., 2014; Dabkowski, 2014). In parallel, as the number of well-documented sites has increased, inter-site comparisons and regional- to continental-scale reviews have developed, either discussing the link between tufa chronological distribution and climate and/or anthropogenisation (e.g. Dabkowski, 2020; Goudie et al., 1993; Ollivier et al., 2006; Pentecost, 1995; Vaudour, 1994; Weisrock, 1986) or providing diachronic comparisons of climatic and environmental conditions prevailing during Quaternary interglacials (Limondin-Lozouet, 2011; Limondin-Lozouet and Preece, 2014; Dabkowski and Limondin-Lozouet, 2021). However, investigations have mostly focused on European tufas so far. In Morocco, reviews on the ages of tufa deposits have been initiated on the basis of U–Th dating (Falguères et al., 2016; Rousseau et al., 2017; Weisrock et al., 2008), but they concerned indurated, well-crystallised deposits (so-called “travertines”), from which palaeoenvironmental and palaeoclimatic data are more difficult to retrieve (Capezzuoli et al., 2014; Dabkowski, 2014). The tufa sequence of Aït Said ou Idder in the Middle Atlas is the first to have recently provided palaeoenvironmental reconstructions based on malacological data (Wackenheim et al., 2020).
This paper proposes to review the climatic significance of tufa deposits in the southeastern Mediterranean area based on their chronological distribution and isotopic signal. It will first present new U–Th dating and isotopic data from Aït Said ou Idder to be compared with available regional data from Morocco and Andalusia in order to discuss the intensity of some humid periods of the last 125 kyr.
The Aït Said ou Idder (ASI) tufa is located in the Middle Atlas, northeast Morocco, about 40 km south of Fez in the vicinity of the Dayet Aoua (33∘38′49.50′′ N, 4∘59′38.33′′ E; Fig. 1). The studied profile, ca. 45 m long and 3 to 4 m high, was previously described in detail by Wackenheim et al. (2020). Two main phases of tufa deposition have been observed on the field (Fig. 2). The lower stratigraphical units 10 to 7 are sub-horizontal and characterised by fluvio-paludal facies (Pedley, 1990; Pedley et al., 2003) including large oncoliths and indurated phytoherms (units 10 and 9), silty to sandy stratified levels (unit 8), and a fine mudstone-like whitish unit at the top (unit 7; Fig. 2). No major discontinuity is clearly observed within these lower units in the eastern part of the profile where they are better exposed. However, in the central part, a stepped-shape incision at the top of unit 8 is locally observed, which may correspond to a hiatus between units 8 and 7 (Fig. 2, red line).
The upper part of the unit 7 is then clearly affected by erosive processes, and indurated angular fragments of it are preserved within the base of the overlying unit 6. The following units 6 to 1 show an east-to-west inclination and facies that are typical of slope tufa (Pedley, 1990), namely silty to granular tufa comprising fragments of encrusted vegetation alternating with silty to sandy tufa (Fig. 2). The lowermost unit 6 especially provides burned tufa fragments and millimetric charcoals evidencing a local fire event. These charcoals were large enough to be dated with confidence (see below). The whole ASI sequence, except unit 9 which was too indurated, was sampled for malacology and geochemistry (Fig. 2). The malacological investigations provide detailed palaeoenvironmental reconstructions and allow selecting shells of suitable species to be dated (Wackenheim et al., 2020). The resulting chronological data are summarised in the following section.
3.1 Former radiocarbon dating
All the previous dates obtained at ASI were through radiocarbon dating and are summarised in Table 1. Dated material includes three millimetric individual charcoals from unit 6, a bunch of microcharcoals from unit 5, and five bunches of mollusc shells from units 1, 3, 4 and 7 (Table 1 and Fig. 2; Wackenheim et al., 2020). While charcoals from unit 6 were handpicked on the field, the bunch of microcharcoal from unit 5 was subsampled within sedimentological samples under a binocular microscope. Dated shells were carefully selected within the malacological assemblages according to their abundance to have enough material to be dated from a single sample. In order to avoid the reservoir effect by old carbonate ingestion, the selection of tiny humidity-demanding species (Vertigo antivertigo, Pupilla muscorum, Cochlicopa lubrica) has been favoured (Table 1) (Pigati et al., 2013; Forman et al., 2021; Granai and Wackenheim, 2022). Radiocarbon date of the xerothermic Cochlicella barbara shell is consistent with the chronological framework (Wackenheim et al., 2020).
Radiocarbon dates assigned the upper part of the ASI tufa to the Middle Holocene (from ca. 6800 and 4800 cal BP) while unit 7 from the lower part is dated from the Upper Pleistocene by two coherent dates on land shells (around 37–40 ka cal BP; Table 1 and Fig. 3). To strengthen this chronological framework, we sought an additional date at the base of the tufa deposit. While no suitable organic material or shell was found in units 9 or 10, well-crystallised calcite deposits such as the strongly indurated phytoherms from unit 9 are suitable material for U–Th series analyses (Fig. 2).
3.2 Additional U–Th dating
The U–Th dating method requires well-crystallised calcite samples that are not easily retrieved from tufa deposits dominated by crumbly silty to sandy facies such as those at ASI (Fig. 2); only phytoherms from unit 9 are suitable here for such analyses. One sample selected from unit 9 (Fig. 2) was thus analysed by U series using ICP-Q-MS at the Muséum national d'Histoire naturelle (France). This method relies on the difference in solubility between uranium and thorium. The amount of radiogenic 230Th formed in ratio to its parent 234U yields the age of formation of the calcite (Bourdon et al., 2003; Ivanovich and Harmon, 1992).
The sample was selected in the well-crystallised internal part of the phytoherm cylinder (Fig. 2), cleaned by removing clay and sand adhering on calcite, then cut using a mini rotary tool (Dremel™-like) with a diamond disc, and finally washed with distilled water in an ultrasonic bath. The carbonate (about 0.5 g) was dissolved in HNO3 acid, and a 233U–236U–229Th mixed spike was added. U and Th chemical extractions and purifications on UTEVA resins were performed according to the protocol detailed by Douville et al. (2010). Each fraction was then dried and dissolved in 2 % HNHO3 before dilution for isotopic analyses by ICP-Q-MS. The measurements were performed on a Thermo iCAP RQ ICP-Q-MS coupled with a Teledyne CETAC Aridus 3 desolvator device. Pre-screening analysis was first performed in order to optimise the final dilutions of each fraction. Then they were combined to be analysed together.
The interface was configured for high sensitivity, and the signal was optimised (tuning) for 238U and 235U on the desolvator and mass spectrometer. The signal intensities of the isotopes 229Th, 230Th, 233U, 234U, 235U and 236U were measured on an electron multiplier (SEM) in pulse-counting mode, and those of 232Th were measured in analogue mode. The helium mode (CCTS) of the collision/reaction cell was used to increase the signal by optimising the ions' focusing. The mass fractionation was corrected by comparing the measured spike ratio with its true known value. The ratio is obtained via the measurement according to the universal natural ratio (Hiess et al., 2012). An analytical standard (without chemistry) of uraninite (HU-1) with a spike, in secular radioactive equilibrium, was analysed along the sequence for machine deviation control. The calculated activity ratios obtained should correspond to the true ratios.
Ages were calculated using half-lives of 75.584 and 245.620 ka for 230Th and 234U, respectively (Cheng et al., 2013). The age uncertainty was estimated taking into account all sources of analytical uncertainty. The U content, isotopic ratios and U-series age of the ASI phytoherm sample are shown in Table 2. The U content is 57 ppb. The is high (more than 3.4) as usually observed in continental carbonates from Morocco (see Ghaleb et al., 2019). An age of 129±4 ka was obtained without correction, but the measured ratio of 14 indicates that correction of the age from detritic Th is mandatory. The corrected age, taking into account the average value of the atomic ratio of the Earth's crust (3.8±2; Ludwig and Paces, 2002), is 123±4 ka and demonstrates the contemporaneity of the bottom of the ASI sequence with Marine Isotopic Stage (MIS) 5e (Fig. 3).
The whole tufa sequence at ASI was sampled continuously every 5 cm (ca. 20 g of tufa was collected for each sample), with local adjustment to stratigraphy when required and excepting the lowermost units 9 and 10, which were too indurated. Each sample was ground when needed and then sifted to <200 µm to obtain 2 to 5 g of fine material. Stable isotope analyses were performed on CO2 derived from 40±10 µg of sifted sample, individually reacted with three drops of orthophosphoric acid (H3PO4) at 70 ∘C. Isotope ratios were measured at the Service de Spectrométrie de Masse Isotopique (SSMIM) of the Muséum national d'Histoire naturelle in Paris (France) on a Thermo DELTA V Advantage spectrometer interfaced to a Thermo KIEL IV Carbonate automatic preparation device.
A summary of ASI isotopic data is given in Table 3, and both δ18O and δ13C are shown in stratigraphic order in Fig. 3. Replicate analyses of the home-made laboratory standard (n=29) gave 2σ precision of 0.1 ‰ for δ18O and 0.08 ‰ for the δ13C. Maximal values, for both δ18O and δ13C, are recorded in samples G81 (−5.3 ‰ and −5.67 ‰, respectively) and G82 (−5.3 ‰ and −6.15 ‰) at the very top of unit 7, below the important sedimentary hiatus with unit 6. These singular values (Fig. 3) are likely to reflect strong diagenetic effects (due to surface alteration and the fire event) and were excluded from the following discussion.
For the remaining samples (n=103), the δ18O values range between −7.8 ‰ and −6.9 ‰ (mean value ‰), whereas δ13C values range between −9.74 ‰ and −7.56 ‰ (mean value ‰; Table 3). Correlation between δ18O and δ13C is not significant (; p=0.37; n=103).
At ASI, three phases can be defined, based on sharp variations in the δ13C at the units 8–7 and then units 7–6 boundaries (Fig. 3 and Table 3): the mean δ13C value is ‰ (n=11) in the lowermost unit 8, then increases to −7.78 in unit 7 (n=12), and finally decreases suddenly to −9.18 in the rest of the sequence (units 6 to 1; n=80). Boundaries between these three phases are correlated to main hiatuses observed in the stratigraphic sequence of ASI (Fig. 2). Conversely, the δ18O remains stable from part to part (−7.5 ‰, −7.4 ‰ and ‰, respectively; Table 3). Within each phase, variations in both δ13C and δ18O are low (standard variations equal or close to confidence intervals; Table 3). According to stratigraphy and dating, these phases correspond to three distinct periods of time separated by hiatuses: from bottom to top, units 9 and 8 are assigned to the early MIS 5e, unit 7 is dated to around 37–40 ka cal BP (during MIS 3), and units 6 to 1 record part of the Middle Holocene (Fig. 3).
5.1 ASI tufa chronology compared to other regional tufas and its climatic significance
In Morocco, Late Pleistocene tufa deposits are reported during both odd and even Marine Isotopic Stages (MISs) (Rousseau et al., 2017; Weisrock et al., 2008), i.e. during interglacial and glacial periods (Fig. 4). Over the last 130 kyr, at the northern border of the Moroccan Sahara, Weisrock et al. (2008) showed (based on U–Th dating) that most tufas were deposited during MIS 5, then between 50–30 and 24–11 ka (Figs. 1 and 4). In detail, at least two main phases of deposition occurred during MIS 5, at 120–130 ka (i.e. during MIS 5e) and 90–74 ka (Fig. 4; Boudad et al., 2003; Falguères et al., 2016; Weisrock et al., 2008). Few Holocene tufas have been reported in Morocco so far, except in the Ksabi basin (e.g. at Blirh and Aït Blal; Lefèvre, 1989; Limondin-Lozouet et al., 2013; Vaudour, 1986) and the Aïn Beni Mathar basin (Depreux et al., 2021; Wengler and Vernet, 1992), in the Moulouya catchment, where they are dated from the Early Holocene (Figs. 1 and 4). Later tufa deposits were recently dated from the last 5000 years at Imouzzer Kandar (Azennoud et al., 2022), only a few kilometres from ASI (Figs. 1 and 4).
On the other side of the Strait of Gibraltar, Spanish tufa deposits have been more extensively studied for decades and regional synthesis are available (see González Martín and González Amuchastegui, 2014). Many tufa or travertine deposits have thus been reported in Andalusia, mostly supporting geomorphological and sedimentological investigations (Durán, 1996; García-García et al., 2014; Martìn-Algarra et al., 2003; Pla-Pueyo et al., 2017; Prado-Pérez et al., 2013). From a climatic point of view, northeastern Morocco and Andalusia nowadays present strong similarities as they both experience Mediterranean conditions with hot summers and low-pressure westerlies bringing air masses from the Atlantic which result in mean annual precipitation in excess of 100 to 250 mm yr−1 during winters and springs (Larrasoaña et al., 2013; Lionello, 2012; New et al., 2000). It thus seems relevant in order to expand the corpus of comparison sites to include data from Andalusia where five phases of maximal tufa deposition have been identified since 130 ka (Delgado Castilla, 2007; Durán, 1996; Martìn-Algarra et al., 2003), including both MIS 1 and MIS 5 interglacials but also the MIS 2–MIS 1 transition and two phases during the Last Glacial Period at around 20–25 ka (MIS 2) and around 40 ka (MIS 3; Fig. 4).
Pleistocene deposits observed at ASI during the early MIS 5e, then around 37–40 ka cal BP, are thus contemporaneous with phases of maximal tufa deposition observed in both Spain and Morocco (Fig. 4). The youngest phase of maximal tufa deposition at ASI has only been faintly observed in Morocco, where only a few well-dated Holocene tufa deposits have been reported (in the Moulouya basin), but has been well identified in Spain (Fig. 4).
Under European mid-latitudes, tufa deposits are usually associated with interglacial conditions (Pentecost, 1993, 1995), but some examples show that they can rapidly develop as soon as climatic conditions improve and before the establishment of trees in the deglaciated landscape. Less is known about tufas in sub-tropical areas (Ford and Pedley, 1996), but they are usually considered records of humid (pluvial) phases (Butzer et al., 1978; Delgado Castilla, 2009; Hamdan and Brook, 2015; Nicod, 2000).
As recorded by maxima of the Mediterranean forest in marine cores from the SW Iberian margin and the Alboran Sea, the Mediterranean climate (characterised by warm and dry summers and especially humid winters) appears well expressed during interglacials (MIS 1 and MIS 5e); MIS 5 interstadials; and D–O interstadials 16–17, 8 and 7 (Combourieu-Nebout et al., 2002; Fletcher and Sánchez Goñi, 2008; Sánchez Goñi et al., 2008, 2000). Specifically, D–O event 8 corresponds to one of the longest and wettest interstadials recorded in the western Mediterranean during the glacial period (Combourieu-Nebout et al., 2002; Margari et al., 2010; Sánchez Goñi et al., 2008).
Phases of maximal tufa deposition observed in Morocco and southern Spain thus appear contemporaneous with these periods of maximal development of the Mediterranean forest, which confirms that their chronological distribution is mainly driven by climatic parameters (Delgado Castilla, 2007; Rousseau et al., 2006; Weisrock et al., 2008). At ASI, tufa deposits are reported during periods when Mediterranean climatic conditions, especially winter humidity, were particularly marked, i.e. during the Holocene, the Eemian, and D–O interglacial 8 (Sánchez Goñi et al., 2008; Shackleton et al., 2004; Zielhofer et al., 2017; Fig. 4).
5.2 Comparison of intensities of the Holocene and Eemian interglacials and D–O interstadial 8 at Aït Said ou Idder
Climatic parameters influencing stable isotopes in modern and Quaternary tufa deposits have been well identified (Andrews, 2006; Andrews et al., 1997; Dabkowski et al., 2011). Tufa calcite δ18O is directly linked to local air mass composition, which mainly depends on their source, rainout effects due to “continentality”, altitude or processes such as the amount effect, and changes in the atmospheric temperature. On the other hand, tufa calcite δ13C is influenced by biomass type and abundance and rainfall amount (i.e. moisture availability).
The three chronological phases identified at ASI are characterised by different isotopic signatures: regarding the δ13C, sedimentary hiatuses between those phases correspond to shifts in the carbon isotope composition of tufa, while the δ18O shows smaller variations (Fig. 3). This remarkable homogeneity of δ18O values (Table 3) suggests no significant difference in terms of temperature or air mass circulation between the Holocene, D–O interstadial 8 and MIS 5e. Regarding carbon isotopes, D–O 8 records values close to −8 ‰ (Table 3), significantly higher than during the interglacials, which reflect a lesser development of soil and vegetation under relatively “drier” conditions during this MIS 3 interstadials (Fig. 5). On the other hand, both interglacials present δ13C values typical of a strong influence from C3 plant-/soil-zone CO2 in δ13C (Andrews, 2006; Fig. 5), suggesting relatively wet conditions. The narrower range of carbon isotope variations recorded during MIS 5e at ASI may result from a lower number of samples for the period (n=11) compared to the Holocene (n=80; Table 3); however, considering means and standard deviations, MIS 5e seems to record higher δ13C values, suggesting slightly reduced moisture with regard to the Holocene (Table 3).
These observations are consistent with the environmental reconstructions provided by malacological investigations on the very same profile at ASI (Wackenheim et al., 2020): mollusc assemblages assigned to D–O 8 (i.e. from unit 7) suggest a more open environment under drier conditions than during the Holocene (from units 6 to 1). In the units assigned to MIS 5e, shells are fewer but may suggest wet conditions, similar to those observed during the Holocene.
Palaeoclimatic reconstructions obtained from a transfer function technique on fossil pollen assemblages from marine cores from west and east Iberia (MD95-2042 and ODP 976; Fig. 1) suggest that temperature conditions during MIS 3 interstadials were similar to present-day (Holocene) values (Sánchez Goñi et al., 2002) as also suggested by the ASI δ18O record. Estimated annual rainfall is less reliable due to methodological limits. Nevertheless, the transfer function reconstructs annual precipitation that is similar during D–O 8 and MIS 1 on both sides of Iberia (Sánchez Goñi et al., 2002). However, MIS 3 interstadials, including D–O 8, are millennial-scale events during which the development of temperate and Mediterranean forests remained reduced with respect to the MIS 1 and MIS 5e interglacials (Camuera et al., 2019; Combourieu-Nebout et al., 2002; Sánchez Goñi et al., 2000; Fig. 4). As the moisture signal recorded by tufa δ13C partly depends on the biomass abundance, the higher carbon isotopic values observed at ASI during D–O 8 could reflect the lesser development of the forest cover while the rainfall amount and other moisture factors are consistent with those from interglacial periods.
Comparing the Holocene and MIS 5e interglacials, a compilation of continental and marine palaeoenvironmental records from North Africa and the surrounding areas suggests that mean annual precipitation in Mediterranean Africa, including northern Morocco, was higher than in the present day at both 6–10 and 122–128 ka cal BP (up to 1000 mm yr−1, while present-day mean annual precipitation is ≤500 mm yr−1) (Larrasoaña et al., 2013). At the regional scale, the palynological data from a long core from the Padul wetland (Andalusia) suggest warmer and/or wetter conditions during the last interglacial compared to the Holocene (Camuera et al., 2019), as in other pollen records from the Mediterranean regions (e.g. Djamali et al., 2008; Litt et al., 2014; Tzedakis and Bennett, 1995). In detail, these different climates may result from strong differences in seasonality: explicitly more marked summer droughts but higher winter precipitation during the last interglacial (Camuera et al., 2019).
The growth of tufa deposits is by nature linked to water availability (Pentecost, 2005); tufa deposition is thus likely to be reduced during dry summers but favoured by autumn/winter rainfall. However, δ13C data from ASI are not consistent with those observations as they rather suggest no difference or even slightly drier conditions during MIS 5e compared to the Holocene. We notice that such strong MIS 5e seasonality may also affect the δ18O signal through the “amount effect” (concentration of precipitation during the wet/cool season) and the seasonal growth of tufa deposition, both of which would lead to the selective record of winter (cool) temperature conditions. In this case, the record of warmer (summer) MIS 5e conditions (as observed in the Padul record) in ASI δ18O would be dampened.
5.3 Comparison with Spanish data
Isotopic data are also available from some tufa deposits from southern Spain (Figs. 1 and 5). The Alcaraz tufa deposits in Castilla–La Mancha have been clearly assigned to the Middle Holocene based on pollen and mollusc data and on two radiocarbon dates (Andrews et al., 2000). At least part of the Alcaraz deposits is contemporaneous with those from ASI (Fig. 4).
Unfortunately, the chronological attribution of the isotopic data available in Andalusia is less precise: the authors provide a chronology based on U–Th dating of several phases of tufa development in the area (Fig. 4) but have not clearly discriminated the geochemical samples according to those phases (Durán, 1996; García-García et al., 2014); i.e. each sample cannot be specifically assigned to a period. Data from Andalusian tufas shown in Fig. 5 are dated from the Late and Middle Pleistocene (Table 4), mostly from MIS 5 except in the Tolox–Yunquera–Jorox area, where more than half of the samples are older than 300 ka (Table 4). Only two samples, at Jorox, are assigned to the Holocene (Durán, 1996). At Frailes, tufa developed during MIS 5 (around 100–110 ka) and then during the Early Holocene, but the specific chronological attribution of the seven samples analysed at this site is not given (García-García et al., 2014; Pla-Pueyo et al., 2017).
As at ASI, most δ13C values from southern Spain range between ca. −10 ‰ and −8 ‰, whatever their age, which demonstrates a strong influence from C3 plant-/soil-zone CO2 (Andrews, 2006; Fig. 5) and suggests relatively wet conditions. Carbon isotope values from Frailes are higher (up to −6.35 ‰; Pla-Pueyo et al., 2017) but remain close to those prevailing at ASI during D–O 8, never reaching values typical of unwooded areas (Fig. 5). On both sides of the western Mediterranean, there is thus no evidence of strong aridity that would have led to evaporation processes and less negative δ13C values in tufa (Andrews, 2006). This is strongly consistent with the prior assumption that, in pluvial and sub-tropical areas, tufa deposits are observed during humid (interglacial or interstadial) phases (Butzer et al., 1978; Delgado Castilla, 2009; Depreux et al., 2021; Hamdan and Brook, 2015; Nicod, 2000).
Regarding δ18O values, larger variations are observed. Alcaraz (Holocene) oxygen data are roughly similar to those from ASI (typically between −7.5 ‰ and −6.7 ‰; Andrews et al., 2000). At Frailes, δ18O values remain close to those from ASI (ranging from −6.70 ‰ to −5.67 ‰; Pla-Pueyo et al., 2017), but those from Pleistocene Andalusian tufa deposits studied by Durán (1996) are significantly higher, whatever their age (Fig. 5). In the Tolox–Yunquera–Jorox area, where a majority of analysed samples are older than 300 ka (Table 4), δ18O values are the highest and reach up to −4.2 ‰ (Fig. 5; Durán, 1996).
Using the Online Isotopes in Precipitation Calculator (OIPC; Bowen, 2022; Bowen and Revenaugh, 2003; IAEA/WMO, 2015), extrapolations of the mean annual δ18O for modern precipitation are ‰ at ASI, ‰ at Alcaraz and ‰ at Frailes, and they range between ca. −6 ‰ and −5.5 ‰ at other Andalusian sites. The rainfall water δ18O values are thus similar at ASI, Frailes and Alcaraz but are up to 3 ‰ higher at Andalusian sites studied by Durán (1996), the same amplitudes as observed in tufa δ18O (Fig. 5).
ASI, Frailes and Alcaraz are all at relatively high altitude (>975 m a.s.l.), while the other tufa deposits studied in Andalusia are below 500 m a.s.l. Tufa δ18O values decreasing with altitude have been similarly observed at Alpine sites; the combined effects of the progressive rainout of air mass and condensation of water at high altitude result in lower rainfall δ18O (Andrews et al., 1997). Consequently, the lower δ18O values observed at ASI, Frailes and Alcaraz are likely to reflect orogenic effects. Furthermore, with the lack of precise chronological attribution of δ18O data from Andalusia, whether or not Pleistocene interglacials were warmer compared to the Holocene in Spain cannot be solved, in contrast with Morocco where a remarkable consistency is recorded at ASI between MIS 5, D–O 8 and the Holocene.
Tufa chronological distribution in the southwestern Mediterranean area is mainly driven by climatic parameters: tufas are characteristic of humid (interglacial or interstadial) phases. At Aït Said ou Idder and more generally in both Morocco and southern Spain, phases of maximal tufa deposition appear indeed contemporaneously with periods of maximal development of the Mediterranean forest. Additionally, ASI δ13C values show no evidence of evaporation processes that may result from strong aridity, which is similarly observed in tufa deposits from Andalusia. However, we may notice that no tufa deposit is reported during D–O 16–17, neither in Morocco nor in southern Spain, while one of the strongest developments of the Mediterranean forest is recorded during this event (Fig. 4). This questions the relationship between tufa deposits and both the duration and the seasonality of humid periods: some humid events might be too short to allow the onset of tufa deposition, and/or contrasting seasons are not favourable to it.
No significant difference in terms of temperature or air mass circulation is observed in the Middle Atlas between the Holocene, D–O interstadial 8 and MIS 5e, according to ASI oxygen stable isotopes. Regarding moisture conditions, D–O 8 is marked by a lesser development of soil and vegetation as conditions were drier than during MIS 1 and MIS 5e. During both these interglacials, wet conditions are recorded according to ASI δ13C, but MIS 5e could be slightly less wet than the Holocene. However, comparisons with regional (marine and continental) climatic records suggest that this observation might actually reflect stronger seasonality during MIS 5e. Such diachronic comparison cannot be extended to Morocco and southern Spain yet, nor can comparison between both sides of the Strait of Gibraltar be made because of the lack of well-dated isotopic data from tufa deposits in the area.
Our preliminary investigations thus demonstrate that calcareous tufa deposits have strong potential to feed discussions on climate variability, at different scales of space and time, in the southeastern Mediterranean area where they appear to be well represented. However, new dates and new isotopic data are required from both already known sites and newly investigated sequences.
Full data are available on request to Julie Dabkowski (email@example.com).
Tufa samples are available on request to Julie Dabkowski (firstname.lastname@example.org).
JD, QW, NLL and LB conducted the fieldwork, with contributions from JFB. QW performed the malacological analyses under the supervision of NLL and provided selected material for radiocarbon dating on shells. CF and OT performed the U–Th series analyses on calcite. DF ran the isotopic analyses at the SSMIM (MNHN, Paris) and provided support to JD in terms of data discussion. The manuscript was written by JD with contributions from all the co-authors.
The contact author has declared that neither they nor their co-authors have any competing interests.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
The authors thank both reviewers for their kind and constructive comments on the manuscript.
Fieldwork and analyses at Aït Said ou Idder were mostly funded by the PALEOMEX (INSU–INEE) Transect Maghreb research programme (Jean-François Berger). Radiocarbon ages have been supported by the LMC14 (CEA, Gif-sur-Yvette) Artemis programme and by the Czech Science Foundation (grant no. P504/17-05696S).
This paper was edited by Becky Briant and reviewed by Jonathan Holmes and Philip Hopley.
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