the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
Towards quantitative reconstruction of past monsoon precipitation based on tetraether membrane lipids in Chinese loess
Martin Ziegler
Louise Fuchs
Youbin Sun
Francien Peterse
Variations in the oxygen isotope composition (δ18O) of cave speleothems and numerous proxy records from loess–paleosol sequences have revealed past variations in East Asian monsoon (EAM) intensity. However, challenges persist in reconstructing precipitation changes quantitatively. Here, we use the positive relationship between the degree of cyclization (DC) of branched glycerol dialkyl glycerol tetraethers (brGDGTs) in modern surface soils from the Chinese Loess Plateau (CLP) and mean annual precipitation (MAP) to quantify past monsoon precipitation changes on the CLP. We present a new ∼ 130 000-year-long DC-based MAP record for the Yuanbao section on the western edge of the CLP, which closely tracks the orbital- and millennial-scale variations in available records of both speleothem δ18O and the hydrogen isotope composition of plant waxes (δ2Hwax) from the same section. Combing our new data with existing brGDGT records from other CLP sites reveals a spatial gradient in MAP that is most pronounced during glacials, when the western CLP experiences more arid conditions and receives up to ∼ 250 mm less precipitation than in the southeast, whereas MAP is ∼ 850 mm across the CLP during the Holocene optimum. Furthermore, the DC records show that precipitation amount on the CLP varies at both the precession scale and the obliquity scale, as opposed to the primarily precession-scale variations in speleothem δ18O and δ2Hwax at Yuanbao and the 100 kyr cycle in other loess proxies, such as magnetic susceptibility, which rather indicates the relative intensity of the EAM. At the precession scale, the DC record is in phase with δ2Hwax from the same section and the speleothem δ18O record, which supports the hypothesis that monsoon precipitation is driven by Northern Hemisphere summer insolation.
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The East Asian monsoon (EAM) is one of the strongest monsoon systems on Earth and is driven by land–sea temperature contrasts. It consists of a warm and wet summer monsoon (East Asian summer monsoon; EASM) transporting moisture from low-latitude oceans to the eastern Asian continent and a cold and dry winter monsoon (East Asian winter monsoon; EAWM) that transfers high-latitude cold and dry air to eastern Asia (Liu and Ding, 1998). Ongoing global warming will likely affect the strength of the EAM and therefore the amount of moisture delivered to the continent by the EASM, where it regulates the water supply to over 20 % of the world's population (An et al., 2015). Past variations in EAM climate have been inferred based on the oxygen isotope composition (δ18O) of cave speleothems from low to mid-latitudes, which show a dominant precession signal (23 000 years, 23 kyr cycle) (Wang et al., 2008; Cheng et al., 2016; Wang et al., 2001) and support the hypothesis that monsoons are primarily driven by Northern Hemisphere summer insolation (NHSI) (Kutzbach, 1981). However, not only the presence of cyclicity but also the phasing with respect to the orbital parameters in a proxy record points to the forcing mechanism. For example, the 6–8 kyr lag of a stacked summer monsoon record from the Arabian Sea to NHSI led to the suggestion that monsoon variations are driven by changes in latent heat flux from Southern Hemisphere and global ice volume (Clemens and Prell, 2003). The observation that speleothem δ18O lags precession minima and thus NHSI maxima was suggested to be related to the occurrence of precession-paced North Atlantic cold events, which systematically delayed the onset of strong boreal summer monsoon intensity (Ziegler et al., 2010). The dominant eccentricity (100 kyr) and obliquity (41 kyr) cycles that appear in a δ18O record of planktonic foraminifera offshore the Yangtze River Valley reflecting EAM runoff after removing confounding factors on δ18O, such as temperature, were further presented as evidence that monsoon precipitation is more sensitive to ice volume and greenhouse gases instead of directly reacting to NHSI (Clemens et al., 2018). In addition, the 100 kyr cycles are dominant in records derived from loess–paleosol sequences from the Chinese Loess Plateau (CLP) in northern central China (Liu and Ding, 1998), where proxies such as magnetic susceptibility (MagSus) (Maher and Thompson, 1991; An et al., 1991), grain size (GS) (Xiao et al., 1995), and carbonate content (Sun et al., 2010) have recorded past variations in EAM climate (Sun et al., 2015). In short, glacials are characterized by a strong EAWM, creating overall cool and dry conditions with loess deposition, reflected by coarser GS and lower MagSus values, whereas interglacials are characterized by a more intense EASM with a warm and wet climate resulting in intensified soil formation, finer GS, and a higher MagSus value (Liu and Ding, 1998). Despite the presence of this strong glacial–interglacial cyclicity across the CLP, several newer proxies indicate that the precession signal is also recorded in the loess, pointing at NHSI as an important driver of the EASM after all (e.g. Beck et al., 2018; Guo et al., 2022a; Fuchs et al., 2023; Li et al., 2024). Regardless of this so-called “Chinese 100 kyr problem”, these reconstructions provided mostly qualitative changes in the strength of summer and winter monsoons, and they often represent a mixed signal of both temperature and precipitation (Cheng et al., 2022).
Multiple studies have attempted to quantitatively reconstruct EAM precipitation on the CLP using various proxies. These include, for example, the Sr Ca ratio of microcodium, which is based on the principle that the elements incorporated into the structure of microcodium are impacted by the composition changes in soil solution between evolved soil solutes with a higher Sr Ca ratio and fresh water with a lower Sr Ca ratio (Li and Li, 2014). Additionally, phytolith assemblages reflect changes in vegetation under different moisture conditions (Lu et al., 2007), as does the carbon isotopic composition of total organic carbon (δ13CTOC), which reflects changes in C3 and C4 plants (Vidic and Montañez, 2004; Rao et al., 2013). Meteoric beryllium (10Be) stored in loess–paleosol sequences across the CLP provides another rainfall indicator, as it attaches to atmospheric dust particles that are mainly deposited during rainfall events (Beck et al., 2018; Zhou et al., 2023). However, the application of these proxies across the CLP does not generate consistent results. For example, precipitation estimates based on 10Be and phytolith assemblages for the southern CLP differ by up to 400 mm during glacials and 200 mm during interglacials (Lu et al., 2007; Beck et al., 2018). Similarly, comparing different proxy estimates of maximum precipitation during interglacials results in a spatial variation of > 800 mm across the CLP (e.g. ∼ 300 mm on the central CLP based on microcodium Sr / Ca (Li et al., 2017) vs. ∼ 1200 mm on the southern CLP based on 10Be (Beck et al., 2018) during Marine Isotope Stage 5 (MIS5)), far exceeding the modern gradient in mean annual precipitation (MAP) (∼ 500 mm) (Xu and Huang, 2023), whereas the inland reach of the EASM presumably exceeded the location of the CLP during these intervals. Together with the different orbital cyclicities represented in these proxy records, this suggests that these proxies all record a slightly different aspect of the EASM, still limiting a comprehensive understanding of the drivers and amount of past monsoon precipitation change.
Glycerol dialkyl glycerol tetraethers (GDGTs; Supplement Fig. S1) are a suite of membrane-spanning lipids of archaea and bacteria, and they have provided another means to reconstruct moisture availability on the CLP, for example, by comparing the abundance of archaeal isoprenoid GDGTs (isoGDGTs) to that of branched GDGTs (brGDGTs) produced by soil bacteria in loess–paleosol sequences, where values > 0.5 for this ratio (R indicate arid conditions (Xie et al., 2012; Yang et al., 2014). The threshold for this ratio is based on the assumption that ammonia oxidation is enhanced in alkaline (pH > 7.5) and arid soils, like loess, which promotes the growth of ammonia-oxidizing Nitrososphaerota (formerly Thaumarchaeota) that produce isoGDGTs (Xie et al., 2012). Similarly, the branched and isoprenoid tetraether (BIT) index, representing the relative abundance of brGDGTs to the isoGDGT crenarchaeol (Hopmans et al., 2004), i.e. basically an inverse of the , has been linked to soil moisture availability globally (Wang et al., 2013; Dirghangi et al., 2013). Application of the and the BIT index to the Weinan section on the southern CLP has revealed sharp peaks in proxy values during glacial terminations, which have been interpreted as the occurrence of megadroughts, likely caused by El Niño-like conditions in the tropical Pacific reducing the moisture transport to the Asian continent (Tang et al., 2017). Although of crucial value, these proxies also do not reflect quantitative changes in monsoon precipitation on the CLP.
Notably, the structural diversity of brGDGTs has been linked to environmental conditions. For example, brGDGTs can vary in the number of methyl branches attached to the alkyl backbone, which has been linked to growing season temperature (Weijers et al., 2007; Naafs et al., 2017b; Dearing Crampton-Flood et al., 2020; Raberg et al., 2024). This relationship has resulted in absolute temperature reconstructions for the EAM region (e.g. Peterse et al., 2011, 2014; Gao et al., 2012; Jia et al., 2013; Yang et al., 2014; Lu et al., 2019, 2022; Guo et al., 2024a) that currently go as far back in time as 3 Ma (Lu et al., 2022), indicating that brGDGTs are generally well preserved in loess. In addition, brGDGTs can also vary in the number of internal cyclization (degree of cyclization, DC; Sinninghe Damsté et al., 2009; Baxter et al., 2019) and the position of the methylation, which can vary between positions C-5, C-6, and C-7 (De Jonge et al., 2013; Ding et al., 2016). Both the DC and the relative abundance of 6-methyl brGDGT isomers, quantified in the isomer ratio (IR; De Jonge et al., 2014a), are positively related to pH in modern surface soils (De Jonge et al., 2014b; Naafs et al., 2017a). Given that soil pH is typically inversely related to precipitation as a result of increased leaching that lowers the soil pH with more precipitation (Slessarev et al., 2016), this relationship offers a basis for inferring past changes in precipitation using soil-pH-related proxies. An early study applied this concept to the Mangshan section in the southeast of the CLP, where brGDGT-based pH was inferred to reflect the precession-forced pacing of monsoon precipitation (Peterse et al., 2014). However, their reconstructed pH values are higher during the wetter interglacials than during the more arid glacials, which is opposite to what is generally expected and could thus not be quantitatively translated into realistic precipitation changes. In addition, this study predates the discovery of 5- and 6-methyl brGDGT isomers, which were not separated with the chromatography method used at the time but seem to have a different pH dependency in alkaline soils (e.g. Guo et al., 2022b).
Here, we examine the potential of the pH-sensitive ratios DC and IR as proxies for past monsoon precipitation in a ∼ 130 kyr long loess–paleosol sequence at Yuanbao, located on the western edge of the CLP. The proximity of Yuanbao to the main dust source has led to high deposition rates, allowing the generation of a high-resolution record (Chen et al., 1997; Sun et al., 2021). In addition, the absence of GDGTs in materials from loess source regions (Gao et al., 2012) or limited (Fietz et al., 2013) and neglectable amounts (Hopmans et al., 2004) in wind-transported dust suggest that GDGT-based proxies reflect in situ climate signals. The same holds for plant waxes in the same section, of which the hydrogen isotope composition (δ2Hwax) has demonstrated the sensitivity of Yuanbao section to orbital- and millennial-scale changes in EASM-associated precipitation dynamics (Fuchs et al., 2023), providing context for the assessment of the DC and IR as quantitative records of past monsoon precipitation on the CLP.
2.1 Study site and sampling
The Yuanbao section (35.63° N, 103.17° E; 2177 m above sea level) is situated near Linxia City on the western edge of the CLP (Fig. 1). Mean annual precipitation (MAP) is 500 mm, with 80 % occurring from May to September (China Meteorological Administration, http://www.cma.gov.cn, last access: 24 November 2023, Fig. S2). Samples (5 cm intervals) were collected from the Yuanbao section in August 2019 from a 6 m deep pit and a partly overlapping 38 m deep outcrop. Together, they cover the S0 (Holocene paleosol), L1 (Last Glacial loess), and S1 (Last Interglacial paleosol). The chronology of this section is established by Fuchs et al. (2023). In summary, the GS and MagSus records from Yuanbao were aligned to those from a nearby drilling core (Guo et al., 2021), which is in turn linked to the benthic δ18O record (LR04; Lisiecki and Raymo, 2005). Although this tuning approach may introduce the presence of a 100 kyr cycle in our records, the chronology is supported by optically stimulated luminescence (OSL) data from a nearby loess–paleosol section (Lai and Wintle, 2006; Lai et al., 2007). In addition, Heinrich stadials (HSs) in the GS records were tied to the absolute and independently uranium–thorium-dated speleothem δ18O record (Cheng et al., 2016). The chronology indicates that the loess–paleosol sequence of Yuanbao in this study covers the last ∼ 130 kyr, corresponding to a sedimentation rate of 17.8 cm ka−1 for S0, 39.3 cm ka−1 for L1, and 21.9 cm ka−1 for S1 on average.
2.2 GDGT extraction and analysis
To avoid anthropogenic perturbation, the upper 30 cm of both the pit and the outcrop were excluded from analysis. In total, 580 samples were analysed for GDGTs corresponding with an average resolution of our record of ∼ 220 years. For each depth, ∼ 30–60 g of freeze-dried and homogenized loess was extracted with dichloromethane (DCM) : methanol (MeOH) (9:1, ) using a Milestone ETHOS X (MEX) microwave extractor at 70 °C to obtain a total lipid extract (TLE). The TLEs were filtered using pre-extracted filter paper (Whatman Grade 42 ashless filter paper, 55 mm diameter) to remove remaining sediment and were dried under an N2 stream. Prior to analysis for GDGTs, a known amount of C46 glycerol trialkyl glycerol tetraether (GTGT) internal standard was added to the TLEs (Huguet et al., 2006). The TLEs were separated into apolar and polar fractions by passing them over an activated Al2O3 column using hexane : DCM (9:1, ) and DCM : MeOH (1:1, ), respectively. The polar fraction containing brGDGTs was evaporated to dryness under a gentle N2 stream. After this, the samples were re-dissolved in a hexane : isopropanol (99:1, ) mixture and passed over a 0.45 µm polytetrafluoroethylene (PTFE) filter. The GDGTs were injected on an Agilent 1260 Infinity ultra-high-performance liquid chromatography (UHPLC) system coupled to an Agilent 6130 single-quadrupole mass spectrometer (MS) with settings according to Hopmans et al. (2016). Target compounds were identified by scanning for the [M + H]+ ions in selected ion monitoring (SIM) mode for 1018.0, 1020.0, 1022.0, 1032.0, 1034.0, 1036.0, 1046.0, 1048.0, and 1050.0 (brGDGTs); 1292.3, 1296.3, 1298.3, 1300.3, and 1302.3 (isoGDGTs); and 743.8 (internal standard) with a mass window of 1.0. Quantitation was achieved by peak area integration in ChemStation B.04.03.
2.3 Proxy calculation
GDGT proxies were calculated according to the equations listed below, where the Roman numerals refer to the molecular structures shown in Fig. S1. Fractional abundances (FAs) of GDGTs are indicated by square brackets. The 6-methyl brGDGTs are denoted with a prime symbol (′).
The degree of cyclization (DC) and the isomer ratio (IR) were calculated according to Baxter et al. (2019) and De Jonge et al. (2014a), respectively:
2.4 Data analysis and visualization
Data visualization was performed in R version 4.2.2 (R Core Team, 2024). Scatter plots and line plots were generated with the package “ggplot2”. Spearman's correlation was used and considered significant at a level of p < 0.05. The DC–MAP calibration was established using Deming regression with the package “mcr” (method comparison regression) following the R script published by Naafs et al. (2017b), which accounts for error in both the proxy (i.e. DC) and the environmental parameter (i.e. MAP). To calculate the ratio of variances, the standard deviation of measured MAP of 120 mm and an assumed standard deviation of DC (0.05) were used. The calibration uncertainty is determined by the residuals of Deming regression. Bandpass filter and spectral analysis were conducted using Acycle (version 3.0) (Li et al., 2019). The records were interpolated to obtain constant time steps before spectral analysis using the periodogram function with default settings. The cross-spectral analysis is conducted between precession and the rest of the record, i.e. EAM proxies, ice volume and greenhouse gas, and was performed with the Blackman–Tukey approach using Arand-master and interpolation of the records at a constant time step of 1 ka. The following parameters were used to optimize variance properties of spectrum estimates: number of lags = 40 (∼ length of record) and samples per analysis = 120. The coherency spectra are compared at the 80 % non-zero coherency level.
The concentration of brGDGTs and isoGDGTs varies between 0 and 32 ng g loess−1 and between 0 and 29 ng g loess−1, respectively (Fig. 2d). The concentration of GDGTs is consistently higher in paleosol layers than in loess layers, following the variations in MagSus (Fig. 2e). Downcore changes in the distribution of brGDGTs result in IR values varying between 0.2 and 0.8 over the past 130 kyr, where IR values are generally low during MIS5 but show a rapid increase from 0.2 to 0.6 within an ∼ 10 kyr interval over the transition from MIS5a into MIS4 (from ∼ 73 to 63 ka), after which the IR increases to a maximum of 0.8 during the Holocene (Fig. 2c). DC values vary between 0.2 and 0.7 over the past 130 kyr and are high (0.4–0.6) during interglacials (i.e. MIS1 and MIS5e) and low (0.2–0.4) during glacials (i.e. MIS2 and MIS4) (Fig. 2a). Notably, millennial-scale variations in the DC record match the variability recorded by GS and δ2Hwax in the same section, with prominent dry periods associated with the HS (Fig. 2a and e). Bandpass filters (Fig. 2b) and spectral analysis (Fig. 3) of the DC record indicate the presence of dominant 41 and 23 kyr cycles.
Both brGDGT-based proxy records show abrupt changes between ∼ 23 and 21 ka, corresponding to the transition from the outcrop to the pit (indicated in grey in Fig. 2a and c). Although this transition does not stand out in the conventional loess proxy records (MagSus and GS) derived from the same material (Fig. 2e) or the δ2Hwax record obtained from the same lipid extracts (Fig. 2a), this interval is not considered in our interpretation of the brGDGT proxy records.
4.1 Downcore changes in brGDGT-related records at Yuanbao
Although the 6-methyl brGDGTs respond to soil pH in the global surface soil dataset (De Jonge et al., 2014b; Raberg et al., 2022) and thus presumably also to precipitation amount, the IR record for Yuanbao does not exhibit the clear glacial–interglacial variations or precession cycles that are visible in other precipitation-related proxy records for this site, such as MagSus and δ2Hwax (Fig. 2a, c, and e). By contrast, the DC record shows a trend matching that of the δ2Hwax record (Fig. 2a), including a precession signal and millennial-scale climate variations, suggesting that the DC may in fact respond to precipitation changes. Indeed, a previous study has empirically linked the cyclization of brGDGTs in modern Chinese alkaline soils to soil pH and MAP (Wang et al., 2014). However, this study also predates the discovery of 6-methyl brGDGT isomers and thus comprises both the DC and the IR. The different trends in the IR and DC records for Yuanbao clearly indicate a distinct pH dependency of these indices in loess (Fig. 2a and c). Based on our current understanding of 5- and 6-methyl brGDGT distributions in modern soils, the 0.4 increase in IR within ∼ 10 kyr (from ∼ 73 to 63 ka) would correspond to a change in soil pH of ∼ 2 units (Raberg et al., 2022). Such a large shift in pH can only be explained by a major alteration in source material or hydrological conditions. Although the other proxy records for this site (increased GS and δ2Hwax values, decreased DC and MagSus values) indicate a hydrological transition towards more arid conditions, this event only lasts for ∼ 3 kyr, after which the records indicate sustained dry conditions until ∼ 60 ka (Fig. 2). The same event is also present in the speleothem δ18O record, where it is referred to as Chinese Stadial 20, representing the weakest EASM during the Last Glacial (Du et al., 2019; Zhang et al., 2017). Even though this shift to cold and dry conditions is shorter than the shift in IR, this hydroclimatic change may have triggered a microbial community response on the CLP.
In contrast, an explanation for the relationship between the DC and precipitation in loess–paleosol sequences is more straightforward. Recent studies have indicated that the production of brGDGTs with cyclopentane moieties is promoted over that of non-cyclic brGDGTs by the availability of exchangeable calcium ions (Ca2+) (De Jonge et al., 2021; Halffman et al., 2022). Microbial ecological studies have shown that available Ca2+ plays a key role in shaping the soil microbial community (Allison et al., 2007; Neal and Glendining, 2019; Shepherd and Oliverio, 2024). It is, therefore, possible that an increase in Ca2+ specifically stimulates the bacteria that produce cyclic brGDGTs. Since loess is generally rich in CaCO3, it is likely that more Ca2+ will be available during periods with enhanced precipitation, which will facilitate the dissolution of CaCO3. Indeed, the DC in the Yuanbao section correlates well with variations in the Ca Ti record that reflect precipitation-induced weathering intensity in the nearby drill core (Guo et al., 2021). Assuming that brGDGTs respond to the Ca2+ availability at the time they are produced, periods with increased precipitation on the CLP will lead to an increase in the DC. Together with the trend in the DC record, this mechanism supports the potential of using DC as a precipitation proxy on the CLP.
4.2 Quantification of past monsoon precipitation amount
To assess the ability of the DC to record changes in precipitation amount, we determined the relationship of the DC with soil pH and MAP in the global surface soil dataset (Fig. 4). The DC shows different relationships with soil pH in more acidic and more alkaline soils. Specifically, the DC is (exponentially) positively related with pH in soils with pH < 7 (r= 0.55, p < 0.01; Fig. 4a), while it is negatively and only weakly related to the soil pH in alkaline soils with pH > 7 (r= −0.27, p < 0.01; Fig. 4a), as observed before in modern Chinese soils (Xie et al., 2012). A recent study comprising mid- and high-latitude soils demonstrated that the change in the direction of this relationship coincided with a shift in the soil bacterial community (De Jonge et al., 2021). This might indicate that brGDGTs in high- and low-pH soils have different producers that potentially respond to environmental changes differently. Notably, the IR based on the same dataset does not show this change in relationship with soil pH (Fig. 4b), suggesting that DC and IR record different environmental parameters, specifically in alkaline soils.
Although soil pH and MAP are related on a global scale, only the DC in soils with pH > 7 correlates with MAP (r= 0.57, p < 0.01; Fig. 4c). Notably, all modern soils from the CLP fall within this cluster, supporting the potential to establish the DC as quantitative proxy for monsoon precipitation in this area. Based on the relationship between the DC for modern soils from the CLP published by Wang et al. (2020) and MAP from meteorological stations, the following transfer function can be derived using Deming regression, which accounts for errors in both proxy and environmental variable data (Fig. 4e and f):
Even though we used Deming regression to avoid regression dilution that can appear in linear regressions, there is still a trend in the residuals, suggesting that other factors may influence the DC, in addition to MAP (Fig. 4f). Nevertheless, the strong correlation of the regression (r2= 0.77) indicates that MAP is the main control of DC on the CLP. Based on the range in the residuals, the uncertainty on MAP estimates is ±125 mm (Fig. 4f).
Using this function to translate the Yuanbao DC record into MAP results in values varying between 460 to 1000 mm over the past 130 kyr, where MAP was highest during MIS5e and lowest during MIS2 (Fig. 5a). Although anthropogenic disturbance of the upper part of the loess section does not allow us to directly compare DC-based MAP with modern precipitation data at Yuanbao, reconstructed MAP matches well with a previous reconstruction of summer precipitation for a nearby loess section based on δ13CTOC (Rao et al., 2013), assuming that summer (June, July, August) precipitation accounts for ∼ 50 % of the MAP, as is the case under modern climate conditions (Fig. S2). Nonetheless, the range of the DC in surface soils (0.06 to 0.50) does not cover the full range of the DC in the Yuanbao palaeorecord (0.19 to 0.68), which may introduce additional uncertainty to reconstructed MAP, especially for periods with a DC > 0.5 (e.g. MIS5e and the Holocene).
To provide more context for the reconstructed MAP at Yuanbao, and to assess the wider applicability of our transfer function, we use the DC to reconstruct MAP at two other sections located on the middle (Xifeng; Lu et al., 2019) and southern (Weinan; Tang et al., 2017) CLP for which brGDGT data are available for the same time interval (Fig. 5b and c). Both MAP records generally show a similar precipitation pattern to that at Yuanbao, albeit in a lower resolution. Hence, millennial-scale events that are reflected in the Yuanbao record are not recorded at Xifeng or Weinan. Still, reconstructed MAP faithfully reflects wetter conditions during interglacials and drier conditions during glacials at both locations, ranging from 470 to 900 mm at Xifeng and from 660 to 1030 mm at Weinan. These MAP estimates are in the same range as those based on 10Be from nearby sections (uncertainty of 1 standard deviation, 190 mm) (Zhou et al., 2023; Beck et al., 2018). Considering the uncertainty on the DC–MAP calibration of ±125 mm, the records indicate that all sites received approximately the same amount of EASM precipitation during interglacials, i.e. ∼ 850 mm during the Holocene optimum and ∼ 950 mm during MIS5e. By contrast, spatial differences in precipitation occurred during glacials, where the southern part of the CLP received up to ∼ 250 mm more precipitation than the middle and the western parts of the CLP, mimicking the modern spatial gradient with more precipitation in the southeast than the northwest of the CLP. These spatial and absolute trends in MAP are in agreement with the presumed reach of the EASM rain belt to the west of the CLP during interglacials and with gradual shifts during glacial–interglacial transitions (An et al., 2000; Li et al., 2018; Yang et al., 2015).
4.3 Implications for EASM precipitation reconstructions
The close resemblance of the DC and δ2Hwax records for Yuanbao on the precession band and in showing millennial-scale events suggests that the δ2Hwax signal largely represents precipitation amount. However, offsets between these two records occur during MIS5, the transition from MIS4 to MIS3, and the Last Glacial Maximum (Fig. 2a). Specifically, the DC record indicates wetter conditions during MIS5e than during MIS5c and MIS5a, while the δ2Hwax record shows increasingly depleted values from MIS5e to MIS5a, suggesting more intense EASM precipitation during MIS5a (Fig. 2a). This opposite trend can be explained by warm climate conditions during MIS5e, which would enhance evapotranspiration and local recycling and result in less negative δ2Hwax values (Gat, 1996; Sachse et al., 2012; Liu et al., 2019). Similarly, the DC record indicates dry conditions during the second half of MIS4 and the Last Glacial Maximum, while the δ2Hwax record shows more negative values, suggesting that δ2Hwax was likely impacted by a change in moisture source during this time, possibly derived from the westerlies that bring moisture relatively depleted in 2H (Fuchs et al., 2022).
Importantly, next to the precession signal that dominates the records of EASM precipitation based on precipitation isotopes (i.e. δ2Hwax, Fuchs et al., 2023; speleothem δ18O, Cheng et al., 2016), the DC record from Yuanbao additionally shows a clear obliquity signal (Figs. 3a, b, and e; S5). This could be introduced by the longer growing season of soil microbes that produce brGDGTs under generally warm and wet conditions compared to that of leaf wax synthesis incorporating precipitation 2H by plants. Similarly, reduced microbial activity in winter may also explain the absence of a clear glacial–interglacial cycle that appears in MagSus and GS record from the same section (Fig. 3a, c and d; Fuchs et al., 2023), although the manifestation of this cycle is likely also restricted by the length of our record (∼ 130 kyr). The obliquity signal in the DC record suggests that, while the moisture source and intensity of the EASM follow precession, the amount of precipitation at Yuanbao responds to the summer insolation at high-latitude regions, which contains a stronger obliquity signal than at lower latitudes. Reconstructed precipitation amounts based on microcodium Sr Ca ratios from the middle CLP similarly show an obliquity cycle over the last 1500 kyr (Li et al., 2017). However, the dominant orbital forcings driving EASM precipitation vary spatially across the CLP and also between different proxies. For example, precipitation amounts reconstructed for the middle (Xifeng; Zhou et al., 2023) and southern (Baoji; Beck et al., 2018) parts of the CLP based on 10Be show precession and glacial–interglacial cycles. Although spatial differences in loess deposition rates may influence the expression of obliquity and precession cycles in different proxy records (e.g. Ao et al., 2024), the offsets also suggest that these proxies are sensitive to different aspects of EASM precipitation, that they integrate a different part of the year, and/or that the amount of monsoon precipitation is increasingly influenced by high-latitude insolation towards the northwestern CLP.
Despite the differences between proxies and sections across the CLP, the spectral analysis of proxy records for Yuanbao and speleothem δ18O show a consistent precession signal (Fig. 3). We subsequently performed cross-spectral analyses to compare the timing of EAM records with the precession extremes. The DC record, as an indicator of precipitation amount, lags the precession minimum (i.e, NHSI maximum) by ∼ 3 kyr. Similarly, the MagSus, δ2Hwax, and δ18O are coherent with precession and lag the precession minimum by ∼ 3, 1 and 3 kyr, respectively, indicating that they are relatively in phase (Fig. 6). Despite the arguments against interpreting speleothem δ18O as an EASM precipitation signal (e.g. Clemens et al., 2010), the independent δ2Hwax record for the Yuanbao section is also dominated by a precession cycle and is in phase with the cave records, suggesting that both sites have recorded the same moisture source (Fuchs et al., 2023). Although δ2Hwax may be influenced by the same confounding factors as the cave records, the DC-based MAP record is independent of precipitation isotope composition, yet it is in phase with speleothem δ18O and δ2Hwax at the precession cycle (Fig. 6). Thus, our record supports the hypothesis that NHSI exerts a stronger influence on EASM precipitation than ice volume and greenhouse gases.
The downcore distribution of brGDGTs at the Yuanbao section on the western CLP reveals that absolute changes in monsoon precipitation over the past ∼ 130 kyr are recorded by the degree of cyclization (DC) of the brGDGTs, based on their relationship with exchangeable Ca2+ that becomes available upon the dissolution of CaCO3 during periods with enhanced precipitation. The DC record aligns with the orbital- and millennial-scale variations in EASM precipitation recorded by speleothem δ18O and the δ2Hwax from the same section. Using the modern DC–MAP relationship to quantify past MAP across the CLP reveals that MAP consistently varies over glacial–interglacial timescales but that differences in precipitation amount are most pronounced during glacials, when the middle and western CLP experience relatively more arid conditions compared to the southern CLP. The in-phase relationship of the DC with δ2Hwax from the same section and with speleothem δ18O on the precession band suggests that the supposed response of monsoon precipitation to NHSI is not an artefact of confounding factors on proxies recording precipitation isotopes but that NHSI is a direct forcing of precipitation amount.
All data can be found online at PANGAEA (https://doi.org/10.1594/PANGAEA.971325, Guo et al., 2024b) and Open Science Frame (https://doi.org/10.17605/OSF.IO/ASG46, Guo et al., 2024c).
The supplement related to this article is available online at: https://doi.org/10.5194/cp-21-343-2025-supplement.
FP, MZ, and YS designed the study. FP and YS collected the sample material. JG and LF conducted the biomarker analysis. JG interpreted and visualized the data under the supervision of FP, MZ, and SY. JG wrote the paper with input from all co-authors.
The contact author has declared that none of the authors has any competing interests.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors.
Klaas Nierop and Desmond Eefting in the GeoLab at Utrecht University are acknowledged for technical support. We thank Hao Lu for providing the map, Shivam Mishra for helping with data generation, and Zhipeng Wu and Fei Guo for helping with wavelet and cross-spectral analysis. The editor Denis-Didier Rousseau, two anonymous reviewers, and David Naafs are appreciated for their feedback that has further improved this article.
This research has been supported by the Nederlandse Organisatie voor Wetenschappelijk Onderzoek (Vidi grant no. 192.074) and the National Natural Science Foundation of China (grant no. 42230514).
This paper was edited by Denis-Didier Rousseau and reviewed by David Naafs and two anonymous referees.
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