Introduction

Oxygen isotopes are a well-studied tracer of water and thus the hydrological cycle1,2,3. Preservation of O isotopes within paleoenvironmental archives provides an opportunity to study past hydroclimatic variability4 as well as climate dynamics with external forcing different to the present5,6. Speleothems are excellent paleoclimate archives as they can provide continuous, high resolution δ18O records with well-constrained chronologies and they occur over most climatic zones where limestone karst exists (e.g., see refs. 7,8). These properties have motivated the collation of speleothem δ18O records into global databases9,10,11 that facilitate regional synthesis of these data to identify past climate patterns;12 and promote data-model comparisons to evaluate the performance of climate models across different past climate states13.

Measurement of speleothem δ18O is routine, and these values reflect the isotopic composition of source water (meteoric precipitation) and cave temperature14. However, speleothem δ18O may not always be an ideal proxy for hydroclimate owing to variable karst flowpaths between water falling as meteoric precipitation and emerging as dripwater within a cave15. Additional processes can also influence the fractionation of 18O/16O between dripwater and calcite14. In the quest to reach quantitative reconstruction of climate variability from speleothem δ18O, increasing attention has been focused on constraining the latter16,17,18,19 while the impact of flowpaths (karst store volume, infiltration thresholds, matrix versus fracture flow type) is less widely acknowledged. Some studies have utilised karst hydrology models to simulate the potential for the physical characteristics of flowpaths to impact dripwater δ18O20,21; but validation of the impact of these processes on the speleothem record is limited by the relatively few studies where speleothem δ18O has been accompanied by cave monitoring22,23,24,25,26,27.

The recognised complexities of speleothem δ18O means that replication of speleothem records from the same cave or karst region is considered the gold standard in assessing their robustness as paleo-environmental archives12,28. Yet coeval records from the same cave frequently do not replicate in detail—often displaying differences in mean, variability and trends (e.g., see refs. 29,30). Studies using coeval records commonly create merged datasets, termed master or composite records, by splicing techniques that scale records according to mean values31,32 or apply a filter through merged datasets33,34. The application of largely arbitrary data corrections may result in loss of information, including the statistical mean δ18O value that is a critical target for model performance (e.g., see ref. 35), as well as the loss of opportunity for further quantification of hydroclimatic information if a more mechanistic understanding of flowpaths was applied36.

Here, we quantify the within-cave differences in mean δ18O values using global compilations of speleothem and dripwater data. For speleothems, we used the SISALv2 database11 to identify caves with multiple coeval speleothem δ18O records, and for dripwater we enlarge the global dataset of ref. 37 from 39 to 50 caves using expanded criteria (see “Methods” section). We then improve our understanding of the processes giving rise to different mean values for dripwater δ18O between flowpaths through a case study of coeval speleothem records from Golgotha Cave (southwest Australia; Fig. 1). Uniquely, within the Golgotha Cave system, dripwater hydrochemistry is well-constrained by long-term monitoring38 and individual flowpaths have been characterised by a spatially dense array of 34 automated drip loggers and lidar mapping39,40,41. This setting allows us to, for the first-time, robustly assess the role that karst hydrology plays in determining the δ18O variability between coeval speleothem paleoclimate records.

Fig. 1: Locations of caves and mean differences used in global meta-analysis of dripwater and speleothem datasets.
figure 1

The range of mean dripwater δ18O values (purple) and the difference between mean values of coeval speleothem records (Δδ18Omeans) (green) are indicated by symbol size for each cave. For caves with more than one set of coeval speleothem records the filled circle is the average value and the open circle is the maximum value of Δδ18Omeans. Location of Golgotha Cave and other sites from the SISALv2 database are also shown. Darker grey shading indicates karst regions70.

Results and discussion

Global speleothem and drip δ18O assessment

A collation of dripwater and speleothem mean δ18O values was prepared for 50 caves with 229 drip monitoring sites, and 64 caves with 146 pairs of coeval speleothem records (Fig. 1; and Supplementary Table 1, Supplementary Data 1, 2 and 3; see “Methods” section). For speleothems we calculate the difference in mean δ18O values (Δδ18Omeans) between paired coeval records and for dripwater we calculate the range in dripwater mean δ18O values. We find that within-cave range of dripwater mean δ18O values is greater than >0.3‰ for 52% of caves; and 45% of coeval speleothem pairs had a difference in mean δ18O values (Δδ18Omeans) >0.3‰. Analytical uncertainty is set at 0.3‰ based on inter-laboratory comparisons42,43; as each coeval dataset will likely come from an individual laboratory where routine reproducibility can be several times better (e.g., typically 0.05‰—see “Methods” section), our threshold for analytical uncertainty is very conservative and implies that our calculations represent the minimum percentage of caves demonstrating within-cave differences in mean δ18O values.

Our findings demonstrate that within-cave variability in mean δ18O values is common worldwide for both dripwater and speleothem data. The global average for the within-cave range in dripwater mean δ18O values is 0.51‰VSMOW and the global average speleothem Δδ18Omeans is 0.37‰VPDB (Fig. 2). This implies that the majority of the within-cave differences in mean δ18O values between coeval speleothem records may be inherited from the dripwater δ18O and thus attributed to differences in karst flowpath physical properties.

Fig. 2: Box and whisker plot comparing within-cave variability in dripwater and speleothem mean δ18O values.
figure 2

The analysis demonstrates that within-cave variability in speleothem mean δ18O values are comparable to the within-cave variability of dripwater mean δ18O values, inferring a flowpath control. Category 1 (purple circles) are the range of dripwater mean δ18O values for each cave and category 2 (green circles) are speleothem Δδ18Omeans for each pair of coeval records. Speleothem Δδ18Omeans are divided into Holocene (category 3, green crosses) and Pleistocene epochs (category 4; green diamonds). Orange squares indicate the mean value, boxes indicate the inter-quartile range and whiskers the 5th and 95th percentiles. Data from the global meta-analysis of dripwater and speleothem datasets.

Our analysis of the SISALv2 data utilised coeval speleothem records from all timescales including shorter, more finely resolved (annual to sub-decadal) records of the Holocene as well as longer records that span glacial–interglacial transitions. Dividing the data into two subsets representing speleothem records from the Holocene versus the Pleistocene epochs (Fig. 2), we show that the global average for either subset was not significantly different from the full dataset: p-value 0.29 (Holocene), p-value 0.20 (Pleistocene); one-tail distribution. The global average value of Δδ18Omeans was 0.34‰ for the Holocene (95 coeval speleothem pairs; 41% were >0.3‰) and 0.41‰ for the Pleistocene (51 pairs; 51% were >0.3‰) (Fig. 2). This demonstrates that within-cave differences in mean δ18O values of coeval speleothems is common and similar in magnitude for both time periods, regardless of whether they are characterised by climate stability or instability.

The meta-data available with these global datasets allows us to further demonstrate that within-cave variability in mean δ18O values in dripwater or coeval speleothems is not controlled by alternative factors such as site climate, cave depth or host rock geology. Cross-plots of within-cave variability in mean δ18O values versus precipitation, temperature, aridity index, seasonality, latitude and elevation show weak to no relationships supported by negligible to low Kendall’s tau values (Fig. 3). Multiple linear regression (MLR) models were calculated and indicate that these factors explain only 14% or less of the within-cave variability in mean δ18O values, whether dripwater or speleothem datasets were considered (Supplementary Table 2). Mann–Whitney U-tests using lithology as a factor showed no significant differences in mean values for different host rock types for either the dripwater or speleothem datasets (p-value = 0.05; Supplementary Fig. 1). We further investigate the possibility that within-cave differences in speleothem mean δ18O values arises from isotopic fractionation processes during calcite precipitation driven by cave microclimate instability, by assessing the distance from the cave entrance to the speleothem locations (Fig. 3) but a low Kendall’s tau value (−0.17) shows no clear relationship. Thus our global meta-analysis demonstrates that climate, geography, lithology or cave microclimate instability do not account for the ubiquitous within-cave variability in mean speleothem δ18O. Our meta-analysis further supports that flowpaths are responsible for the within-cave difference in coeval speleothem mean δ18O values.

Fig. 3: Cross-plots of within-cave variability in dripwater and speleothem mean δ18O values with climate and cave data.
figure 3

Cross-plots show low to no relationships between within-cave differences in dripwater (purple) or speleothem (green) mean δ18O values with variables: latitude, elevation, annual precipitation, aridity index, seasonality indices for precipitation and temperature, mean annual temperature, mean depth, and minimum distance from entrance for each cave. The lack of relationship with these variables, demonstrated also by the output from the multiple linear regression models in Supplementary Table 2, supports that karst hydrological heterogeneity is important over all climate types, cave depths and host rock types. Kendall’s tau values for each variable ranked against coeval dripwater and speleothem data are also shown, with p-values indicated in brackets. The p-values indicate that none of the relationships in are significant with the exception of elevation (SISAL; 95%) and mean depth (SISAL; 90%) although the Kendall’s tau values are low. Aridity and seasonality indices are dimensionless.

The global mean value for the within-cave difference in mean δ18O values of coeval speleothems, Δδ18Omeans, of 0.37‰VPDB for speleothems is large and is exceeded for 51 caves in our analysis. Seven caves have coeval speleothem records with a difference in mean δ18O values exceeding 1‰ (Supplementary Data 3), equivalent to one-third of glacial–interglacial cycles reproduced in stalagmites from the Asian monsoon region7. Thus, there is a need to further explore the role of flowpaths as the underlying mechanism for driving within-cave variability in mean speleothem δ18O values. Just four caves in our global analysis have both dripwater and speleothem datasets29,44,45,46,47,48,49,50 and only one cave (NW Scotland45,46; Fig. 1) has differences in mean δ18O values for both drip and speleothem datasets. This highlights the need for more coeval speleothem datasets from monitored caves in order to objectively quantify the karst hydrological control on speleothem δ18O variability.

Golgotha Cave case study

To address the above, we present a case study of four new stalagmite records that grew during the last eight centuries from Golgotha Cave, southwest Australia (Figs. 1 and  4a; see Supplementary Fig. 2 and ref. 38 for site description). Dripwater monitoring commenced after each stalagmite was removed and varies in length from 5 to 14 years duration (Figs. 4b and  5). Golgotha Cave represents a long and extensively characterised monitoring dataset38,39,40,41,51,52 to interrogate the influence of within-cave differences in karst flowpaths on speleothem δ18O records. Cave temperature can be expected to have remained relatively constant over the period investigated eliminating the need to consider this variable.

Fig. 4: Golgotha Cave speleothem δ18O records.
figure 4

a Speleothem records GL-S1 (red), GL-S2 (green), GL-S3 (navy blue) and GL-S4 (purple) for the last 800 years. b Comparison between speleothem (solid line), dripwater (dashed line) and farmed calcite (squares) for the last four decades. Dashed box in a indicates region re-plotted in b. Dripwaters were converted to calcite equivalent values using an empirical bulk fractionation factor derived from calcites farmed at the drip sites (Supplementary Note 1 and Table 1). Dripwater (calcite equivalent δ18O values) are used to extend the speleothem time series. The agreement (allowing for the rising trend) also supports the empirical fractionation factor calculated from Golgotha farmed calcites and dripwaters.

Fig. 5: Golgotha Cave monitoring data.
figure 5

a Smoothed monthly meteoric precipitation (P) anomalies (cerulean blue). b Monitored drip rates for speleothem sites GL-S1 (red), GL-S2 (green), GL-S3 (navy blue) and GL-S4 (purple). c Smoothed precipitation-weighted monthly rainfall δ18O (grey dash) and smoothed dripwater δ18O for drip sites where speleothems were collected (colours as for drip rates); mean δ18O values of matrix (orange squares) and fracture flow sites (blue diamonds) in the drip logger array sampled during five field campaigns. Error bars represent ±1σ of measurements from multiple sites. Monthly precipitation anomalies were calculated using the monthly climatological means from 1950 to 2020. An exponentially-weighted moving average (EWMA) was applied to monthly P anomalies with a half-life parameter of 36.6 months; similarly an EWMA was applied to monthly rainfall δ18O using a 25 month half-life, as well as a lag of 19 months supported by our field studies in refs. 40,51. Dripwater δ18O were smoothed with a loess 2nd order filter (span 0.3). Drip rates exhibit a threshold response to higher infiltration indicating the relative influence of fractures on each flowpath40. For example, the drip for GL-S4 rapidly increases in response to higher precipitation anomalies during 2013 compared to the much smaller rise in the drip rate for GL-S1, indicating that a larger fracture component is feeding GL-S4. Over the same period, mean drip rate of the logger array increased from 0.16 ± 0.02 to 0.20 ± 0.40 for matrix flow sites and from 2.21 ± 0.40 to 8.32 ± 3.43 for fracture flow sites. The relative contribution of fracture flow to each drip site is inversely related to drip δ18O values with activation of fractures occurring during periods of higher infiltration associated with lower rainfall δ18O values.

Calcites farmed during our monitoring study permit an assessment of the reliability of Golgotha Cave speleothems to record changes in dripwater δ18O. In addition to the well-known potential complications of disequilibrium and/or kinetic effects53, a recent study (ref. 19) hypothesised that in specific circumstances, speleothem δ18O may be impacted by a process known as prior-calcite precipitation (PCP), a term commonly used for the calcite lost from solution along the flowpath prior to reaching the stalagmite54. Ref. 19 utilised laboratory and modelling studies to interpret the δ18O of calcite which was precipitated by solution flowing on an inclined slope at a flow rate such that oxygen isotope disequilibrium between HCO3 and H2O occurred. For Golgotha Cave, empirical fractionation factors are calculated from in situ farmed calcites and dripwater to objectively constrain whether disequilibrium and/or kinetic effects, including PCP, are impacting the Golgotha Cave stalagmite δ18O records (Table 1). The fractionation factors are consistent across the four speleothem sites in Golgotha Cave (αcalcite-water = 1.03185 ± 0.00013, n = 9; Table 1). If other effects, including PCP, dominated at the time of calcite precipitation, this would manifest as different αcalcite-water values between drip sites. The range of 1000lnαcalcite-water values is 0.3‰ which may be an indication of the magnitude of disequilibrium/kinetic/PCP effects, or measurement uncertainty. Regardless, a value of 0.3‰ is much smaller than the isotopic range in recent speleothem δ18O values (0.8‰VPDB) between sites (Fig. 4b; see Supplementary Notes 13 for further information on the robustness of these records).

Table 1 Farmed calcite and dripwater δ18O data.

Annual dripwater δ18O mean values differ by up to 1‰VSMOW between monitoring sites within Golgotha Cave37 (Fig. 4b). Conversion of dripwater δ18O to calcite equivalent values, using our farmed calcites, demonstrates that dripwater δ18O gives a viable extension of the individual speleothem records associated with each drip (Fig. 4b). The difference in δ18O values between flowpaths in the monitoring data are consistent with the isotopic offsets between speleothem records further confirming that the speleothem δ18O records are primarily driven by differences in dripwater δ18O values. The isotopic differences between the four speleothems persist throughout the 800 years of coeval data (Fig. 4a), but with differences in temporal evolutions of individual records that in the absence of consideration of karst processes could otherwise be misinterpreted to represent very different hydroclimate histories.

Variability in mean dripwater δ18O associated with recharge thresholds and karst store behaviour can account for the differences observed in the δ18O values of coeval speleothems within Golgotha Cave. We demonstrate this by drawing on our longitudinal monitoring data, updated with new data since ref. 38 and with dripwater sampling from new sites in our large drip logger array (Fig. 5). The majority of water movement to the ceiling of Golgotha Cave is via flow through the matrix of the host-rock41 and is characterised by low drip rates with low variability38,40. A second flow type, fracture flow, displays a threshold increase in drip rate in response to activation of flow along a fracture40, while a third flow type termed combination flow has flow through an interconnected network of fractures and fissures/conduits41. Drips feeding the stalagmites in this study represent this range of flow types: predominately matrix (GL-S1, GL-S2), matrix plus fracture (GL-S4) and combination flow (GL-S3; Fig. 5b).

Fracture flow dripwaters have lower δ18O values compared with matrix flow dripwaters and the isotopic value of fracture flowpaths is lower as the degree of fracture flow increases (Fig. 5c). Dripwater sampling from the additional sites in the drip logger array confirms that there is an isotopic distinction between matrix flow (−4.0 ± 0.1‰, 1σ; n = 58) versus fracture flow (−4.7 ± 0.1‰, n = 22) classified drips40 (Fig. 5c and Supplementary Data 4). Importantly, matrix flow is similar in value to precipitation-weighted monthly rainfall δ18O (−3.9‰; Fig. 5c), indicating that matrix flow integrates the majority of rainfall events, whereas the lower δ18O values of fracture flow drips (Fig. 5c) indicate that supply to fractures is biased towards larger rainfall events, which have relatively lower δ18O values owing to the amount effect in this region52,55. This recharge bias indicates that a threshold in rainfall intensity is required for flow along fractures to occur56, consistent with studies elsewhere37.

A fracture activation episode is evident in our dripwater monitoring data as an abrupt 115% increase in drip rate during November 2013 (GL-S4 drip; Fig. 5a, b). This occurred in response to a wetter than usual rainfall season (annual total above the 90th percentile) and is consistent with rapid, deep delivery of infiltrating rainwater along a fracture40,56. The increase in flow was accompanied by a 0.5‰VSMOW decrease in GL-S4 dripwater sustained for several years (Fig. 5c). The drip monitoring suggests that the relative volume of water contributed by large rainfall events to karst reservoirs is amplified by fractures and is related to the size and/or number of contributing fractures. The drip rate response for the combination flowpath (GL-S3) similarly rises in 2013 (Fig. 5b), only here the larger network of permeable features40 smooths the response to infiltration. Dripwater δ18O values for this site are the lowest of the four monitored sites, are 1‰VSMOW lower than precipitation-weighted rainfall δ18O and display low variability (Fig. 5c), consistent with the karst store for GL-S3 being sustained largely by infiltration via fractures.

The monitoring and characterisation of the Golgotha Cave system allows us to interpret the differences between the mean values of Golgotha Cave δ18O speleothem records as well as the drivers of the variability through time. Records GL-S1 and GL-S4 have similar isotopic trends on multi-decadal to multi-centennial scales over the last eight centuries; however, the mean δ18O value for GL-S4 is 0.5‰ lower (Fig. 4a). This is consistent with our identification of GL-S4 as receiving a larger component of fracture flow whilst GL-S1 is supplied predominately by matrix flow. Oxygen isotopic values for stalagmite GL-S1 do not fall below −4.6‰VPDB, whereas they are typically below this value for GL-S4 (Fig. 4b). This indicates that selective recharge due to fracture activation during periods of higher rainfall was a persistent process impacting the flow pathway, hence the δ18O record, of GL-S4. Further support for this process-based understanding is the typical widening of the isotopic offset between the two records that is observed during periods of relatively lower δ18O values, e.g., 1250–1400 CE and 1580–1700 CE (Fig. 4a), indicative of enhanced fracture activation feeding GL-S4 in response to more intense rainfall events.

Additionally, from 1970 CE onwards, all records and their extended dripwater time series display rising δ18O trends coinciding with the sustained rainfall decrease in this region57. We quantify the associated change in rainfall δ18O to be 0.17‰VSMOW by applying the empirically-derived relationship between rainfall δ18O and amount for southwest Australia of ref. 52. The much larger >1‰ shift in the cave data demonstrates an additional mechanism is amplifying the isotopic response to climatic forcing and is consistent with a reduction in fracture flow, i.e., conditions were insufficient to overcome recharge threshold(s) for regular fracture activation56 resulting in a isotopic shift towards the matrix-flow end-member. This clearly demonstrates how flowpath characteristics (threshold for activation and fracture contribution) amplify the response of dripwater δ18O values to hydroclimate forcing.

Stalagmite GL-S2 δ18O values are initially similar to GL-S4 from 1330 to 1440 CE, intermittent between GL-S1 and GL-S4 until 1560 CE, then at or above GL-S1 for the remainder of the speleothem and dripwater record (Fig. 4a, b). Temporal flow-switching was documented previously for GL-S2’s drip site38 and is consistent with its location in the cave characterised by our lidar-based study as having high-spatial heterogeneity in flow regime40. In contrast, stalagmites GL-S1 and GL-S4 come from a section of the cave with low spatial variability in flow-paths attributed to their connectedness to the common hydrological domain of the matrix39,40.

Fracture dominated flowpaths

Speleothems from drips that are dominated by combination or complex fracture flowpaths in Golgotha Cave show greater isotopic variability and less reliable growth consistent with their drip supplied by flow along fractures rather than through the matrix. Speleothem GL-S3 experienced discontinuous growth over the last 800 years (Fig. 4a), with rejuvenation of growth commencing with low δ18O values (e.g., 1180–1300 and again in the 1950s CE; Fig. 4a). This is consistent with flow to this speleothem dominated by fracture flowpaths40 with a higher recharge threshold requiring relatively high infiltration from larger rainfall events to activate56. For example, a relatively wet interval during the 13th century is supported by falling δ18O values supplied by the matrix to GL-S1 plus fracture activation initiating growth to stalagmites GL-S2 and GL-S4. The higher recharge threshold for GL-S3’s flowpath is evidenced by the δ18O values that are up to 1 ‰VPDB lower than the other records at 1200-1300 CE.

An enhanced non-linear response to recharge is also evident in GL-S3 shown by the rising trend that is initially similar in value to GL-S4 at 1300 CE after which, GL-S3 δ18O values rise steeply by 1.5 ‰ in less than three decades, exceeding the matrix-flow record (GL-S1; Fig. 4a). The continuity of all the other records at the time when GL-S3 ceases growing (approx. 1380 CE) indicates that infiltration to the cave system is still occurring but not to the fractures supplying GL-S3, i.e., a stranded reservoir. The fact that both GL-S2 and GL-S4 δ18O values are falling together (below matrix flow values) indicates that fractures are still supplying water elsewhere in the cave. The lack of supply to GL-S3 indicates flow-switching in a large complex fracture network with insufficient supplementation of flow from the matrix. The isotopic maximum prior to termination of the first growth phase in GL-S3: −2.5‰ (Fig. 4a) is similar to observed dripwater maxima (δ18O, calcite-equivalent; Fig. 4b), thus demonstrating that it could have been inherited from the dripwater, although additional processes may have also contributed as the amount of water feeding GL-S3 became increasingly diminished, including enhanced isotopic disequilibrium effects as the drip interval lengthens58.

Speleothems associated with large, complex fractures are more likely to show non-linear responses to hydroclimate forcing and more caution should be taken with interpreting paleoclimate information from them. In contrast, speleothems dominated by matrix flowpaths and simple fracture structures are likely to be more suitable. These can be identified where drip monitoring exists or using approaches similar to ref. 41 to identify fractures by way of stalactite distribution on the cave ceiling. Where duplicated records from the same karst/climate region exist, a comparison of these records could result in a more complete reconstruction of the hydroclimate drivers, rather than excluding records that don’t agree.

Implications for quantified hydroclimate reconstructions

The Golgotha Cave case study demonstrates that the differences between coeval speleothem δ18O records from the same cave can be controlled by the influence of the karst architecture (recharge thresholds, physical flowpaths) that results in dripwater δ18O that departs from rainfall δ18O that is in turn inherited by the speleothem. The global meta-analysis reveals that such within cave isotopic variability is common worldwide and is present in both dripwater and in replicated speleothem records across all timescales and is independent of hydroclimate, host rock geology, cave depth or cave microclimate instability. A previous global meta-analysis of monitored cave datasets showed that dripwater δ18O values were typically lower than precipitation-weighted mean annual rainfall δ18O at warmer locations37. Our expanded global study demonstrates that the additional impacts of flowpaths on within-cave isotopic variability are important over all climate types and karst characteristics.

Within-cave isotopic variability attributable to physical flowpath properties has been identified previously in cave monitoring studies59,60,61 and proxy system models15,62 have been used to simulate how flowpath variability can impact dripwater and speleothem δ18O. However, the outcome of these studies could be viewed as specific to a particular site or time domain. The novelty of our study is that we have utilised large global databases to demonstrate that within-cave variability in speleothem mean δ18O values is ubiquitous. While we have not investigated isotopic fractionation during calcite precipitation in the SISALv2 data beyond demonstrating that there is no relationship between speleothem replication and distance from the cave entrance (an indication of cave microclimate instability), the results of our study supports that within-cave variability in speleothem mean δ18O values may be accounted for by to within-cave variability in dripwater. Examination of other factors in the global meta-data analysis confirms the most parsimonious mechanism is the impact of flowpath characteristics—recharge threshold and fracture contribution of individual flowpaths—and we have captured this process in our case study.

Golgotha Cave hydrology experiences matrix flow through the highly porous Pleistocene aeolinite host rock38. Globally, most karst is older and retains little or no primary porosity, hence water movement is likely to be more impacted by heterogeneities in flowpaths through fractures. In mature limestones, a high density of fissures, sediment-filled structures and paleokarst could similarly act as porous media; and drips with matrix flow properties have been identified in many monitored caves from mature limestones (e.g. refs. 27,60,61).

Fractures and their activation thresholds result in a bias of the contribution of rainfall events to different flowpaths giving rise to drip sites with different mean δ18O values. Speleothems with a larger fracture contribution to their flowpath will likely have a mean value that is further from precipitation-weighted mean annual rainfall δ18O. This has implications for using speleothems as isotopic targets for assessing the performance of climate models, e.g., ref. 13. Calibrated karst proxy system models62 would allow for the possibility of reconstructing mean precipitation δ18O, which is directly comparable to output from isotope-enabled general circulation models13. This highlights the importance of developing proxy system models that represent karst processes.

Our findings that the relative contribution of fracture versus matrix flow impacts dripwater and speleothem δ18O also has important implications for the interpretation of speleothem δ18O within an individual record. Larger contributions from fracture flow are activated during periods of higher rainfall. This amplifies the non-linear relationship between rainfall and speleothem δ18O as shown in our case study. A quantified reconstruction of past rainfall from Golgotha Cave speleothems requires a calibrated proxy system model able to reconcile the within-cave variability in δ18O arising from matrix versus fracture flow and is an objective for a forthcoming study. For other studies, we highlight that the implications of our findings suggest that variability within speleothem δ18O can be larger than what can be attributed to direct changes in rainfall δ18O and this should be considered whether applied to last millennia climate reconstructions or to assessing glacial–interglacial transitions in older speleothems.

Methods

Global meta-analysis

The dataset of ref. 37 was extended to include studies with at least quarterly dripwater sampling over 12 months and to include additional sites that had been rejected by ref. 37 on the basis of not having nearby rainfall δ18O data. Mean δ18O for each drip site over a 12 month period was calculated and the range of these mean values for each cave was determined (Supplementary Data 1). For speleothem data, we utilised the SISALv2 database10,11,13 to identify caves with coeval speleothem δ18O records satisfying the following criteria, coded in R package v1.0.7., mineralogy = calcite AND coeval interval exceeds 10% of the minimum age of overlap AND overlap interval exceeds twice the age uncertainty linearly extrapolated beyond the maximum age AND twice the age uncertainty linearly extrapolated less than the minimum age AND each section contain >10 δ18O measurements. We used the chronologies as they appear in SISALv2. The mean δ18O value for each speleothem record was calculated for the duration of replication and difference between the means calculated (Δδ18Omeans) for each pair of coeval records (Supplementary Data 2 and 3). If a hiatus was entered in SISALv2 within the period of coeval growth, data were omitted from the other record over this interval before calculating the mean of each speleothem record. For Δδ18Omeans > 0.5‰ a plot of the SISALv2 data (not shown) for each coeval pair and their mean values was generated to visually check if hiatuses were identified. In one case (entity ID 487) it was apparent that the mean value was impacted by a hiatus not identified in SISALv2 and this record was removed from our analysis. Additionally, where data from the same speleothem appears in SISALv2 as separate entities owing to revised records in different publications, the entity with the longer record (time span) was used. If the growth interval was the same, the entity with the higher resolution record was used. We assessed the robustness of our approach by examining the impact of varying the criteria (Supplementary Table 1). Cave meta-data were extracted from SISALv211 and climate variables from WorldClim V1;63 the latter use 1960–1990 as the period for climatology. Aridity index was calculated as precipitation divided by actual evapotranspiration, WorldClim V1 products, Bio4 and Bio15, were used as seasonality indices for temperature and precipitation, respectively. Cave depth and distance to entrance data were not available for all sites. In cases where elevation data were not provided, these were taken from ref. 64. Mean depth is the estimated mean thickness of host rock above site of dripwater monitoring or collected speleothem.

Golgotha Cave dripwater and rainfall data

Data presented here are an extension of published38 drip and rainfall δ18O data plus new dripwater data collected at the site of speleothem GL-S4 (2012–2019) as well as additional samples collected over 2–5 days durations from the automated logger array during five separate field campaigns. Methods for drip and rainfall δ18O appear in ref. 38 with the exception of δ18O measurements being made using Picarro L2120-I Water Analyser at ANSTO (see ref. 65 for method) from 2012 onwards. Supplementary Table 3 contains identification codes for dripwater and speleothem pairing and summarises site data. To estimate the impact of the 1970s rainfall decrease on rainfall δ18O, the rainfall δ18O-amount relationship determined for Golgotha Cave (based on daily rainfall sampling between 2005–2018) of ref. 52 was applied to the daily rainfall data from the nearest Australian Bureau of Meteorology station (station ID 9547; record began 1926), <4 km from Golgotha Cave. Mean values were compared between 1926–1969 and 1970–2018.

Stalagmite stable isotopes

Stalagmites were collected under scientific license CE003472 issued by Western Australia’s Department of Biodiversity, Conservation and Attractions. Each speleothem was milled along the growth axis using a Taig micromill to produce homogenised powders representing increments of 0.1–0.2 mm, depending on the speleothem growth rate. Powders were weighed to 180–220 μg and analysed for δ18O and δ13C using a Finnigan MAT-251 isotope ratio mass spectrometer coupled to a Kiel I carbonate device, or a Thermo MAT-253 isotope ratio mass spectrometer coupled to a Kiel IV carbonate device (using 110–130 μg samples), at the Research School of Earth Sciences, ANU. Analyses were calibrated using NBS-19 standard (δ18Ov-PDB = −2.20‰ and δ13Cv-PDB = 1.95‰). A further linear correction for δ18O measurements was carried out using the NBS-18 standard (δ18Ov-PDB = −23.0‰). The original delta values for NBS-19 and NBS-18 are used to maintain consistency of results through time in the RSES Stable Isotope Facility. Analytical precision for the analyses reported here (NBS-19) are ±0.04‰ for δ18O and ±0.02‰ for δ13C (N = 236) for the MAT-251; and ±0.05‰ for δ18O and ±0.01‰ (N = 27) for the MAT-253 instrument (±1σ standard deviation).

Speleothem chronologies

Speleothem chronologies were determined by combining information from the date of collection, bomb pulse chronology66, laminae counting of annual Sr concentration and U-series disequilibrium (see Supplementary Table 4 for further information). U-Th age measurements followed the method of ref. 67. Briefly, calcite wafers weighing 100–200 mg were dissolved and equilibrated with a mixed 229Th–233U–236U tracer before U and Th are extracted in a single solution using Eichrom TRU resin before measurement on a Nu Plasma multicollector ICPMS where isotope ratios of both elements are measured simultaneously. A ratio of initial [230Th/232Th] = 0.33 ± 0.25 was applied and is defined by modelling the ratio required to bring ages into age-depth order for each stalagmite. This ratio is further supported by comparing the U/Th ADM to the laminae chronology for stalagmite GL-S4. Data for age measurements are given in Supplementary Data 5.

X-ray fluorescence microscopy (XFM) maps of Sr concentration were acquired on the speleothem polished slabs at 2 μm resolution (pixel size) at the XFM beamline at the Australian Synchrotron68 using a monochromatic incident energy of 18.5 keV focussed to spot size of 1.5 μm, and dwell per pixel from 1 to 4 ms. The XFM elemental maps were created and analysed using GeoPIXE software, quantified by using single element Mn, Fe and Pt foils (Micromatter, Canada) and corrected by using a Ca matrix factor. Laminae counting and error estimate was made by determining the position of the Sr peaks on two parallel areas of the Sr maps at three confidence levels (>95, 50–95 and <50% confidence) using ImageJ software package according to the method outlined in ref. 69.