Hydro-climatic variability in the southwestern Indian Ocean between 6000 and 3000 years ago
- 1Institute of Global Environmental Change, Xi'an Jiaotong University, Xi'an, China
- 2Department of Earth Sciences, University of Minnesota, Minneapolis, USA
- 3Department of Earth Science, California State University Dominguez Hills, Carson, USA
- 4Institute of Geology, University of Innsbruck, Innsbruck, Austria
- 5Francois Leguat Giant Tortoise and Cave Reserve, Anse Quitor, Rodrigues Island, Mauritius
- 6National Cave Research and Protection Organization, Raipur, India
Correspondence: Hai Cheng (email@example.com)
The “4.2 ka event” is frequently described as a major global climate anomaly between 4.2 and 3.9 ka, which defines the beginning of the current Meghalayan age in the Holocene epoch. The “event” has been disproportionately reported from proxy records from the Northern Hemisphere, but its climatic manifestation remains much less clear in the Southern Hemisphere. Here, we present highly resolved and chronologically well-constrained speleothem oxygen and carbon isotopes records between ∼6 and 3 ka from Rodrigues Island in the southwestern subtropical Indian Ocean, located ∼600 km east of Mauritius. Our records show that the 4.2 ka event did not manifest itself as a period of major climate change at Rodrigues Island in the context of our record's length. Instead, we find evidence for a multi-centennial drought that occurred near-continuously between 3.9 and 3.5 ka and temporally coincided with climate change throughout the Southern Hemisphere.
The “4.2 ka event” is considered to be a widespread climate event between 4.2 and 3.9 ka (thousand years before present, where the present is 1950 CE) (e.g. Weiss et al., 1993, 2016). Many paleoclimate records from the Northern Hemisphere (NH) have characterised the event as a multi-decadal to multi-centennial period of arid and cooler conditions across the Mediterranean, Middle East, South Asia and North Africa (e.g. Finné et al., 2011; Marchant and Hooghiemstra, 2004; Migowski et al., 2006; Mayewski et al., 2004; Staubwasser et al., 2003; Arz et al., 2006; Zielhofer et al., 2017; Stanley et al., 2003; Kathayat et al., 2017). The structure of the 4.2 ka event from many proxy records, such as peat cellulose records from the eastern Tibetan Plateau (Hong et al., 2003, 2018), speleothem from northeastern India (Berkelhammer et al., 2012) and southern Italy (Drysdale et al., 2006), marine sediments from the Gulf of Oman (Cullen et al., 2000) and the northern Red Sea (Arz et al., 2006), and the dust record in the Kilimanjaro ice core (Thompson et al., 2002), typically characterised it as a single pulse-like signal in the long-term context of these records. In contrast, the structure of the 4.2 ka event in the Southern Hemisphere (SH) remains unclear. Some proxy records from the tropical and subtropical regions of Africa and Australia show a shift towards drier conditions around 4 ka (e.g. Russell et al., 2003; Marchant and Hooghiemstra, 2004; Griffiths et al., 2009; Denniston et al., 2013; Berke et al., 2012; De Boer et al., 2013, 2014, 2015; Schefuß et al., 2011; Rijsdijk et al., 2009, 2011). Other records show virtually unchanged hydrological conditions (e.g. Tierney et al., 2008, 2011; Konecky et al., 2011) or two-pulsed multi-decadal length wet events (Railsback et al., 2018) during the period contemporaneous with the 4.2 ka event.
The goal of this study is to investigate a time period that spans the 4.2 ka event in a key region of the SH via highly resolved and precisely dated proxy records. Here, we present speleothem oxygen (δ18O) and carbon (δ13C) isotope records from La Vierge (LAVI-4) and Patate (PATA-1) caves from the Rodrigues Island (Fig. 1) in the southern subtropical Indian Ocean. The LAVI-4 and PATA-1 records span from ∼6 to 3 ka and from ∼6.1 to 3.3 ka, with an average resolution of ∼4 and 14 years, respectively. LAVI-4, which constitutes our primary record, has a precise age control and a sub-decadal resolution, which, together with the PATA-1 record, allows us to reliably characterise the multi-decadal to centennial hydro-climate variations in the southwestern Indian Ocean during the period from 6 to 3 ka.
Rodrigues (∼19∘42′ S, ∼63∘24′ E) is a small volcanic island (∼120 km2) situated in the southwestern Indian Ocean, ∼600 km east of Mauritius (Fig. 1). The island's maximum altitude is ∼400 m above sea level. Rodrigues' mean annual temperature is ∼24 ∘C and the mean annual rainfall is ∼1010 mm, of which nearly 70 % occurs during the wet season (November–April) with February being the wettest month. The seasonal distribution of rainfall is largely controlled by the seasonal migration of the ITCZ (Intertropical Convergence Zone) and the Mascarene High (Senapathi et al., 2010; Rijsdijk et al., 2011; Morioka et al., 2015) (Fig. 1). Given its location at the southern fringe of the ITCZ, the austral summer rainfall at Rodrigues is very sensitive to the mean position of the southern limit of the ITCZ. This is highlighted by backward (120 h) HYSPLIT (Draxler and Hess, 1998) trajectory composites of the low-level winds (850 hPa) during the years when the total January to March (JFM) precipitation was unusually low (dry) and high (wet) than the long-term mean (1951–2016) at Rodrigues (Fig. 1b). It is of note that there is a major increase in the fraction of air parcel trajectories arriving from the north of Rodrigues during the wetter years, indicating an enhanced contribution of northerly moisture resulting from a more southerly position of the ITCZ (Fig. 1b). This observation is further supported by analyses of the low-level wind trajectory cluster composites of February in those years when the southern boundary of the ITCZ was anomalously north or south (Lashkari et al., 2017; Freitas et al., 2017) of its long-term mean February position (Fig. S1a, b in the Supplement). In addition to the ITCZ, ENSO (El Niño–Southern Oscillation) also modulates austral summer precipitation at Rodrigues by modulating the Hadley and Walker circulations (Senapathi et al., 2010; De Boer et al., 2014; Griffiths et al., 2016; Zinke et al., 2016). Instrumental data and our trajectory composites for selected El Niño and La Niña years suggest that an increased (decreased) summer precipitation at Rodrigues is associated with the El Niño (La Niña) events (Fig. S1c, d).
2.2 Oxygen isotopes and climatology
Modern observations of δ18O of precipitation (δ18Op) in the study area are unavailable due to the lack of Global Network of Isotopes in Precipitation (GNIP) stations in Rodrigues. However, δ18Op data from the nearest GNIP station in Mauritius show a clear annual cycle in δ18Op with depleted values during the austral summer (Fig. S2a). Additionally, in the absence of GNIP data, we use simulated δ18Op data from the Experimental Climate Prediction Center's Isotope-incorporated Global Spectral Model (IsoGSM) (Yoshimura et al., 2008) to assess the large-scale dynamical processes that control δ18Op on interannual and decadal timescales. Our analyses show the presence of a strong negative correlation between the δ18Op and rainfall amount similar to the “amount effect” (e.g. Dansgaard, 1964) (Fig. S2b, c). We therefore interpret δ18Op variations in the cave catchment and, consequently, in speleothems from this region as primarily reflecting variations in rainfall amount in response to both local and large-scale atmospheric circulation changes. The relationship is such that more negative (positive) δ18Op values occur during times of either an anomalously southward (northward) position of the southern boundary of the ITCZ or El Niño (La Niña) conditions.
3.1 Speleothem samples
Two stalagmites, LAVI-4 and PATA-1, from La Vierge and Patate caves, respectively, were used in this study. La Vierge (19∘45′26 S, 63∘22′13 E; ∼32 m a.s.l.) and Patate (19∘45′30 S, 63∘23′11 E; ∼20 m a.s.l.) caves are located in Plaine Corail and Plaine Caverne, respectively, in southwestern Rodrigues (Middleton and David, 2013). The cave temperature and relative humidity at the time of sample collection (June 2015) were ∼25.5 ∘C and 95 % in La Vierge Cave and ∼22.5 ∘C and 95 % in Patate Cave. Samples LAVI-4 and PATA-1 were collected at a distance of ∼50 and 200 m from cave entrances, respectively. The diameters of LAVI-4 and PATA-1 are ∼75 and 95 mm, and their lengths are ∼400 and ∼334 mm, respectively. Both stalagmites were cut along their growth axes using a thin diamond blade and then polished.
3.2 230Th dating
Subsamples (80–130 mg) for 230Th dating were drilled using a 0.9 mm carbide dental drill. 230Th dating was performed at Xi'an Jiaotong University, China, by using a Thermo-Finnigan Neptune Plus, which is a multi-collector inductively coupled plasma mass spectrometer (MC-ICP-MS). The method is described in Cheng et al. (2000, 2013). We used standard chemistry procedures (Edwards et al., 1987) to separate U and Th. A triple-spike () isotope dilution method was used to correct instrumental fractionation and to determine U ∕ Th isotopic ratios and concentrations (Cheng et al., 2000, 2013). U and Th isotopes were measured on a MasCom multiplier behind the retarding potential quadrupole in the peak-jumping mode using standard procedures (Cheng et al., 2000). Uncertainties in U and Th isotopic measurements were calculated offline at the 2σ level, including corrections for blanks, multiplier dark noise, abundance sensitivity and contents of the same nuclides in the spike solution. 234U and 230Th decay constants of Cheng et al. (2013) were used. Corrected 230Th ages assume an initial 230Th∕232Th atomic ratio of and those are the values for a material at secular equilibrium with the bulk earth 232Th∕238U value of 3.8. The correction for a few samples in LAVI-4 and PATA-1 is large because either U concentration is low (∼65 ppb) and/or the detrital 232Th concentration is elevated (>100 ppt) (Table S1, Fig. 2).
3.3 Stable isotope analysis
LAVI-4 and PATA-1 stable isotope (δ18O and δ13C) records were established by ∼962 and ∼190 data, respectively. The New Wave Micromill – digitally controlled tri-axial micro-mill equipment – was used to obtain subsamples. The subsamples (∼80 µg) were continuously micro-milled along the stalagmite growth axes of LAVI-4 and PATA-1 at increments of between 100 and 200 µm. The subsamples of LAVI-4 were measured using a Finnigan MAT-253 mass spectrometer coupled with an online carbonate preparation system (Kiel-IV) in the Isotope Laboratory, Xi'an Jiaotong University. The subsamples of PATA-1 were measured using an online carbonate preparation system (GasbenchII) connected to an isotope ratio mass spectrometer (DeltaplusXL) in the Isotope Laboratory, Innsbruck University. The latter technique is reported in Spötl (2011) and Spötl and Vennemann (2003). All results are reported in per mil (‰) relative to the Vienna PeeDee Belemnite (VPDB) standard. Duplicate measurements of standards show a long-term reproducibility of ∼0.1 ‰ (1σ) or better (Table S2, Fig. 2).
4.1 Age models
We obtained 26 and 7 230Th dates for samples LAVI-4 and PATA-1, respectively. The LAVI-4 and PATA-1 age models and associated uncertainties were constructed using the COPRA (Constructing Proxy Records from Age) (Breitenbach et al., 2012) and ISCAM (Intra-Site Correlation Age Modelling) (Fohlmeister, 2012) age modelling schemes (Fig. S3). Both schemes yielded virtually identical age models, and thus the conclusions of this study are not sensitive to the choice of the age model (Figs. 2 and S3).
The time interval from 6 to 3 ka in LAVI-4 speleothem corresponds to a sample depth of 274 to 81 mm below the top, respectively. A drip-water relocation occurred at a depth of 124 mm, which is associated with a Type L surface characterised by slow growth and narrow layers under progressively drier conditions (Railsback et al., 2013) (Figs. S3 and S4). It cannot be ruled out that there is also a hiatus at this depth (∼3.5 ka). If such a hiatus was indeed present, its duration would be about 100 years based on the age model (Fig. S4). The time interval from 6.1 to 3.3 ka in PATA-1 corresponds to a sample depth of 34 to 15 mm. The growth of PATA-1 ceased at ∼15 mm and then resumed about 630 years later, creating a hiatus (Fig. S3). The COPRA age models of PATA-1 and LAVI-4 (Figs. 2 and S3) are reported in Table S2 and used in the following discussion.
4.2 Isotopic equilibrium tests
Conventional criteria to assess the isotopic equilibrium of stalagmites are provided by the Hendy Test (Hendy, 1971), which requires no correlation between δ18O and δ13C values measured along the growth axis as well as along the same growth lamina. The correlation between the δ18O and δ13C values in LAVI-4 and PATA-1 is 0.53 and 0.85, respectively, which suggests the possibility of isotopic disequilibrium during calcite precipitation. However, a number of studies (e.g. Dorale and Liu, 2009) pointed out that a correlation between δ18O and δ13C values does not automatically rule out isotopic equilibrium. Instead, the replication test (i.e. a high degree of coherence between δ18O profiles of individual speleothems from the same cave) is a more rigorous and reliable test of isotopic equilibrium. Particularly, the replication test is far more robust if the records used are from different caves with different kinetic/vadose-zone processes, as is the case for this study. Indeed, a high degree of visual similarity between the coeval portions of LAVI-4 and PATA-1 δ18O and δ13C records suggests that both stalagmites record primary climate signals, notwithstanding the offsets between the absolute values (Fig. 2a). The replication is further confirmed by statistically significant correlations between the LAVI-4 and PATA-1 δ18O (r=0.64 at 95 % confidence level) and δ13C (r=0.73 at 95 % confidence level) records calculated using the ISCAM algorithm (Fohlmeister, 2012) for their contemporary growth period between 3.4 and 6.0 ka (Fig. 2). ISCAM uses a Monte Carlo approach to find the best correlation between the proxy records by adjusting each record within its dating uncertainty. The significant levels are assessed against a red-noise background generated using artificially simulated first-order autoregressive time series (AR1). The offset in absolute δ18O values between LAVI-4 and PATA-1, however, remains unclear and possibly arises from processes related to the characteristics of the two karst systems, such as temperature differences as observed during our fieldwork in 2015. Therefore, in the following discussion we focus only on temporal variations of LAVI-4 δ18O and δ13C records due to their higher resolution and better-constrained chronology (Fig. 2).
5.1 Proxy interpretation
The temporal resolution of the LAVI-4 δ18O record between 6 and 3 ka varies from 1.2 to 16.4 years with an average resolution of ∼3.2 years. The δ18O temporal variability is large (∼3.5 ‰) and, as noted earlier, we interpret the δ18O variations to dominantly reflect changes in the precipitation amount. This line of reasoning is justified given the island's isolated setting far removed from large-sized landmasses and its low topographic relief, which minimises isotopic variability stemming from processes such as the continentality and altitude effects as well as the mixing of distant water vapour sources with significantly different isotopic compositions. This interpretation is additionally supported by moderate to strong covariance between the LAVI-4 δ18O and δ13C profiles. Although the process of stalagmite precipitation may be affected by evaporation and/or degassing (Treble et al., 2017; Cuthbert et al., 2014; Markowska et al., 2016; McDermott, 2004; Lachniet, 2009), the temporal variations in the latter can stem from changes in vegetation type and density, soil microbial productivity, prior calcite precipitation (PCP), and groundwater infiltration rates (e.g. Baker et al., 1997; Genty et al., 2003), all of which may drive δ18O and δ13C values in the same fashion (e.g. Brook et al., 1990; Dorale et al., 1992; Bar-Matthews et al., 1997). The significant covariance between the δ13C and δ18O records could therefore indicate that both proxies reflect a common response to changes in rainfall amount at Rodrigues or a rainfall limit on the extent of vegetation and other related processes in the epikarst as mentioned above.
5.2 Hydro-climate variability between 6 and 3 ka at Rodrigues
The z-score-transformed profiles of LAVI-4 δ18O and δ13C records reveal several decadal to multi-decadal intervals of significantly drier and wetter conditions ( standard deviation) (Fig. 3) but no distinct long-term trends (Figs. 2 and 3). The interval corresponding to the 4.2 ka event in the LAVI-4 δ18O record, typically between 4.2 and 3.9 ka (e.g. Weiss et al., 2016), includes two dry (∼4200 to 4130 yr BP and ∼4020 to 3975 yr BP) and two wet (∼4130 to 4020 yr BP and ∼3975 to 3945 yr BP) periods (Fig. 3). During this time interval the LAVI-4 δ13C record shows two wet periods peaking at ∼4115 and 4015 yr BP, respectively, which correlate within age uncertainties with two wet pulses in proxy records from Mawmluh Cave (Kathayat et al., 2018), Tangga Cave (Wurtzel et al., 2018), Makassar Strait (Tierney et al., 2012), Liang Luar Cave (Griffiths et al., 2009), KNI-51 Cave (Denniston et al., 2013) and Dante Cave (Railsback et al., 2018) (Fig. 4).
Overall, the climate variations recorded at Rodrigues from 4.2 to 3.9 ka are characterised by high-frequency (decadal to multi-decadal) fluctuations, including the major arid/wet events mentioned above. Notably, however, the mean hydro-climatic state of this time interval inferred from both δ18O and δ13C data is indistinguishable from the average state between 6 and 4.2 ka (Fig. 3). In this regard, the climatic events or anomalies between 4.2 and 3.9 ka are not distinctly larger in amplitude nor longer in duration in comparison to similar anomalies between 6 and 4.2 ka (Figs. 3 and 4). Consistently, in the context of the long-term climate variance between 6 and 3 ka, there is no evidence for an unusual climate anomaly between 4.2 and 3.9 ka.
The most prominent feature of our record is a switch from an interval characterised by high-frequency δ18O variance (i.e. from 6 to 3.9 ka) to a multi-centennial excursion with progressively higher δ18O and δ13C values: a prolonged mega-drought at Rodrigues. Starting at ∼3.9 ka, this mega-drought became progressively more severe leading to a diminished growth rate or a ∼100 yr long hiatus around 3.5 ka in LAVI-4. Growth rate picked up subsequently, followed by abrupt (∼100 yr long) and large decreases in both δ18O (∼2 ‰) and δ13C (∼5 ‰) to their average values of the entire records between 6 and 3 ka. As such, the structure of the mega-drought event shows a saw-tooth pattern with a multi-centennial drying trend followed by a ∼100 yr long return to the mean state (Fig. 3). The multi-century mega-drought recorded by our stalagmites between 3.9 and 3.5 ka is also evident in Sahiya Cave, north India (Kathayat et al., 2017), and from Lake Edward (Russell et al., 2003), Lake Victoria (Berke et al., 2012), the Zambezi Delta (Schefuß et al., 2011) and the Tatos Basin (De Boer et al., 2014) (Fig. 5). In the eastern sector of the southern Indian Ocean, speleothem records from Tangga (Wurtzel et al., 2018), KNI-51 (Denniston et al., 2013) and Liang Luar (Griffiths et al., 2009) caves also show a shift to drier condition at approximately 4 ka (Fig. 4).
The LAVI-4 δ13C record shows a pattern broadly similar to the δ18O record and clearly delineates three major droughts between 6 and 3 ka, centred at 5.43, 4.62 and 3.54 ka, respectively. These three drought events share a distinct saw-tooth pattern characterised by a long-term gradual positive excursion (drying) followed by an abrupt return to the mean values (Fig. 3).
To sum up, our Rodrigues records show evidence of multi-decadal–decadal hydro-climate fluctuations around the mean state between 6 and 3 ka. After 3.9 ka, the hydro-climate was characterised by a multi-centennial trend toward much drier conditions, which ended with a return at ∼3.5 ka within ∼100 years to the mean hydro-climate state. This pattern is different from the “pulse-like” event between 4.2 and 3.9 ka as documented in many other proxy records mainly from the NH. Additionally, the mega-drought between 3.9 and 3.5 ka is clearly a later event unrelated to the 4.2 ka event.
5.3 Possible mechanisms
A close examination of our Rodrigues δ18O and δ13C records shows that a persistent multi-centennial drying trend began effectively at ∼4.1 ka and ended at ∼3.5 ka, suggesting a prolonged northward shift of the mean position of the ITCZ (Figs. 3 and S1a). This inference, if correct, is partially in contrast with the southward shift of the ITCZ, which is often invoked to explain the weakening of the Asian monsoon since ∼4.2 ka (e.g. Wang et al., 2005; Kathayat et al., 2017). Thus, the observed drying trends on both the northern and southern fringes of the ITCZ in both hemispheres argue against the model of a southward shift in the mean position of the ITCZ as a viable cause of the 4.2 ka event. A more likely explanation involves an overall contraction in the north–south range of the migrating ITCZ belt in the region (e.g. Yan et al., 2015; Denniston et al., 2016; Scroxton et al., 2017). This mechanism is broadly consistent with the spatial pattern of hydro-climate changes observed in both hemispheres around and after the 4.2 ka event. As mentioned above, the wet period between ∼4.1 and 4.0 ka recorded at the northern fringe of the ITCZ (Kathayat et al., 2017, 2018) coincided with a wet period on the southern limit of the ITCZ as recorded in Dante Cave (Railsback et al., 2018), the Zambezi Delta (Schefuß et al., 2011), Tatos Basin (De Boer et al., 2014), La Vierge Cave (this study) and KNI-51 Cave (Denniston et al., 2013) (Figs. 4 and 5). The subsequent arid period between ∼3.9 and 3.5 ka was also basin-wide and affected both the northern and southern limits of the ITCZ over the Indian Ocean and adjacent regions (Figs. 4 and 5).
In parallel with drier condition along the southern limit of the austral summer ITCZ, proxy records from Lake Edward (Russell et al., 2003), Lake Victoria (Berke et al., 2012) and Tangga Cave (Wurtzel et al., 2018), which are located near the northern limit of the contemporary austral summer ITCZ, also exhibit drier conditions. In contrast, records within the core location of the austral summer ITCZ, such as Lake Challa (Tierney et al., 2011), Lake Tanganyika (Tierney et al., 2008), Lake Malawi (Konecky et al., 2011) and Makassar Strait (Tierney et al., 2012), show either slightly wetter or virtually unchanged hydro-climatic conditions (Figs. 4 and 5). Based on the observed spatial patterns, we suggest that the contraction of the ITCZ both in terms of a north–south meridional shift as well as with respect to its overall width may have played an important role in modulating the hydro-climate in our study area during and after the 4.2 ka event.
All data needed to evaluate the conclusions in the paper are presented in the paper. Additional data related to this paper may be requested from the authors. The data will be archived at the National Climate Data Center (https://www.ncdc.noaa.gov/data-access/paleoclimatology-data, last access: 2 December 2018). Correspondence and requests for materials should be addressed to Hai Cheng (firstname.lastname@example.org).
The supplement related to this article is available online at: https://doi.org/10.5194/cp-14-1881-2018-supplement.
HC, AS and HYL designed the research and experiments; HC, AS, JB, YFN, AAA, AM and HYL completed the fieldwork; HYL, HC, YFN and CS performed stable isotope measurements and 230Th dating work. AS and HYL did the data analyses. HC, HYL and AS wrote the paper, with the help of all co-authors.
The authors declare that they have no conflict of interest.
This article is part of the special issue “The 4.2 ka BP climatic event”. It is a result of “The 4.2 ka BP Event: An International Workshop”, Pisa, Italy, 10–12 January 2018.
We thank Nick Scroxton and another anonymous reviewer for their contribution
to the peer review of this work. We very much appreciate editorial help from
Raymond Bradley. This work was supported by grants from the NSFC (41472140,
41731174 and 41561144003), US NSF grant 1702816 and a grant from the State Key
Laboratory of Loess and Quaternary Geology, Institute of Earth Environment,
Edited by: Raymond Bradley
Reviewed by: Nick Scroxton and one anonymous referee
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