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Holocene Forcing of the Indian Monsoon Recorded in a Stalagmite from Southern Oman

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Science  13 Jun 2003:
Vol. 300, Issue 5626, pp. 1737-1739
DOI: 10.1126/science.1083130

Abstract

A high-resolution oxygen-isotope record from a thorium-uranium–dated stalagmite from southern Oman reflects variations in the amount of monsoon precipitation for the periods from 10.3 to 2.7 and 1.4to 0.4thousand years before the present (ky B.P.). Between 10.3 and 8 ky B.P., decadal to centennial variations in monsoon precipitation are in phase with temperature fluctuations recorded in Greenland ice cores, indicating that early Holocene monsoon intensity is largely controlled by glacial boundary conditions. After ∼8 ky B.P., monsoon precipitation decreases gradually in response to changing Northern Hemisphere summer solar insolation, with decadal to multidecadal variations in monsoon precipitation being linked to solar activity.

Although lake [e.g. (13)] and marine [e.g. (4, 5)] records uniformly indicate that a major intensification in Indian Ocean monsoon (IOM) occurred at ∼10 ky B.P., discrepancies exist about the timing and nature of changes in IOM intensity later in the Holocene. Because the IOM plays an important role in the global hydrological and energy cycles, a key question is whether the IOM weakened gradually or abruptly during the middle to late Holocene. Furthermore, because of low temporal resolution and age uncertainties of almost all continental paleomonsoon records, there is little consensus about the timing and causes of centennial- and decadal-scale fluctuations in monsoon precipitation. Previous studies on stalagmites from Oman have shown that oxygen-isotope profiles can provide more detailed information about the timing and causes of IOM variability (6, 7), but these records cover relatively short time intervals and not the entire Holocene. Here, we present a δ18O monsoon record from a stalagmite from Southern Oman, which continuously covers the time interval from 10.3 to 2.7 ky B.P. and 1.4 to 0.4 ky B.P. with an average time resolution of between 4 and 5 years. The temporal range and resolution allow a precise reconstruction of changes in IOM precipitation and intensity on subdecadal to millennial time scales.

Stalagmite Q5 was collected from Qunf Cave (17°10 N, 54°18 E; 650 m above sea level) in Southern Oman (fig. S1A). The area is suitable to study the IOM for two reasons. First, Qunf Cave sits at the present northern limit of the summer migration of the intertropical convergence zone (ITCZ) and the associated IOM rainfall belt. Second, more than 90% of total annual precipitation (400 to 500 mm at the cave site) falls during the monsoon months (July to September), when dense clouds and mists cover the region. Presently, the cloud cover does not rise higher than 1500 m because of a temperature inversion created by the convergence between northwesterly winds and the low-level southwest monsoon winds (fig. S1A). As a result, monsoon precipitation occurs as fine drizzle, seldom exceeding more than 5 mm per day (unlike the heavy rains normally associated with strong convectional monsoonal rainfall) (8).

The time scale of the Q5 record is based on a total of 18 Th-U ages measured with thermal ionization mass spectrometry (TIMS) and multicollector inductively coupled plasma mass spectrometry (MC-ICPMS) (9) (tables S1 and S2; fig. S2). Stalagmite Q5 was deposited in two phases from 10.3 to 2.7 ky B.P. (the data are presented on the 14C absolute age scale where “present” is defined as 1950 A.D.) and from 1.4 to 0.4 ky B.P. (Fig. 1). The high-resolution δ18O profile is based on 1405 isotope measurements, sampled every ∼0.7 mm along the center of the growth axis (10) (Fig. 1). Other stalagmite-based δ18O profiles from the same and from a neighboring cave confirm the Q5 record and indicate that sample- and site-specific noise is almost negligible (fig. S3, A and B).

Fig. 1.

Q5 δ18O record from southern Oman. Black dots with horizontal error bars are TIMS and MC-ICPMS Th-U ages (see tables S1 and S2). Black dot with vertical error bars and gray shaded area show the δ18O range of modern stalagmites (101 stable-isotope measurements during the past 50 years). Heavy gray line shows the long-term trend as defined by RAMPFIT (34) for the early Holocene and a sinusoidal in the late part.

Study of modern cave drip waters and stalagmites from Qunf Cave demonstrates that Q5 was deposited in or very close to isotopic equilibrium (11). Furthermore, our previous work on speleothems in Oman shows that speleothem δ18O values accurately reflect δ18O values of regional precipitation, and that changes in calcite δ18O over time primarily reflect changes in the amount of monsoonal precipitation (6, 12). As mentioned before, in Southern Oman strong convective cloud development is presently prevented by a temperature inversion (13), whereas the height of this temperature inversion is dynamically linked to the mean latitudinal summer position of the ITCZ and to the southwest monsoon wind pattern over southern Arabia (fig. S2A). A more northerly position of the ITCZ lifts the height of the temperature inversion, leading to stronger convective cloud development and higher monsoon precipitation over southern Oman (fig. S2B). Owing to the amount effect, δ18O values become more negative as rainfall increases. Hence, the Q5 δ18O record can be regarded as a record of the amount of IOM precipitation, where the mean latitudinal summer position of the ITCZ over the Arabian Peninsula plays an important role.

The high-resolution δ18O profile of stalagmite Q5 shows four distinct features (Fig. 1). First, a rapid increase in monsoon precipitation between 10.3 and 9.6 ky B.P. is indicated by a sharp decrease in δ18O from –0.8 to ∼–2‰. Second, an interval of generally high monsoon precipitation is observed between 9.6 and 5.5 ky B.P. with δ18O values averaging –2‰. Third, a long-term gradual decrease in monsoon precipitation starting at around 8 ky B.P. is indicated by a slow shift in δ18O from ∼–2.2‰ at 8 ky to ∼–0.9‰ (slightly more negative than δ18O values of modern stalagmites) at 2.7 ky B.P. (Fig. 1). Fourth, stalagmite deposition stopped at ∼2.7 ky B.P. and restarted from between 1.4 and ∼0.4 ky B.P. The δ18O values of the second growth phase lie within the range of modern stalagmites (Fig. 1). Superimposed on the long-term trend are distinct decadal and multidecadal second-order fluctuations in δ18O (Fig. 1).

In southern Oman the abrupt onset and rapid increase in monsoon precipitation between 10.3 and 9.6 ky B.P. indicate a rapid northward migration of the ITCZ and are in agreement with Arabian Sea upwelling records (4, 5) and regional lake level (3), ice core (14), and speleothem records (6, 12). Although some records (4, 5) indicate an initial increase in IOM strength between 13 and 12.5 ky B.P., there is no speleothem evidence in Oman for a monsoon intensification before ∼10.3 ky B.P. (6, 12). The comparison between the Q5 and GRIP δ18O records (15) clearly reveals that the abrupt increase in monsoon precipitation is in phase with increasing air temperature in the northern Atlantic region (Fig. 2). When age uncertainties of ±1 to 2% of the absolute age in both the Q5 and GRIP records are taken into account, decadal-scale intervals of reduced monsoon precipitation (more positive δ18O values) correlate with cooling events in Greenland and vice versa, as best expressed at 9.1 and 8.2 ky B.P. (15, 16) (Fig. 2). Although precise estimation of leads and lags is hampered by age uncertainties, the marked similarity between both records indicates that early Holocene IOM intensity was controlled on centennial and even on decadal time scales by glacial boundary forcing (e.g., Himalayan snow cover and North Atlantic sea surface temperatures). Such a strong teleconnection between low-latitude IOM variability and high-latitude temperature fluctuations during the late Pleistocene and last deglaciation is well known and was previously detected in marine cores from the Arabian Sea (4, 5, 1719), but not in such detail for an early Holocene monsoon record.

Fig. 2.

Comparison of the Q5 δ18O record with the smoothed (five-point running average) GRIP δ18O ice core record (15). Lower monsoon precipitation correlates with colder North Atlantic air temperatures (visualized by vertical tie-lines). The heavy black line shows “ramp” function trends (34). Change-point times are given with their statistical errors (1σ), which are estimated from bootstrap simulations. Taking dating uncertainties for both the Q5 and GRIP records into account (1 to 2%) shows that the changes occurred simultaneously.

After ∼8 ky B.P., the gradual long-term decrease in monsoon precipitation (as inferred by the shift toward modern δ18O values) indicates a continuous southward migration of the mean summer ITCZ and a gradual weakening of monsoon intensity in response to declining June to August summer insolation at 30°N(20, 21) (Fig. 3A). A decrease in summer insolation reduced the land/sea thermal contrast and, therefore, the northward pull on the ITCZ and the monsoonal rainfall belt into the Arabian Peninsula. Supporting evidence for a gradual middle to late Holocene weakening in IOM wind strength and intensity is indicated by a decrease in abundance of Globigerina bulloides in an upwelling record from the Arabian Sea (Fig. 3B) (19). Additional evidence for an insolation-controlled gradual southward migration of the ITCZ during the Holocene has also been found for tropical South America (22) (10°43 N; 65°10 W), where decreasing Ti content indicates a long-term decline in summer precipitation (Fig. 3C). Taken together, these lines of evidence suggest that postglacial to modern precipitation patterns in the northern tropics are controlled, probably on a global scale, by the gradual southward migration of the ITCZ and gradual weakening of the monsoons in response to orbitally induced decreasing summer insolation.

Fig. 3.

(A) Smoothed (nine-point running average) Q5 δ18O record and insolation curve (heavy black line) at 30°N, averaged from June to August (20, 21). (B) Indian monsoon upwelling record based on abundances of G. bulloides (19). Higher abundances of G. bulloides reflect more intense upwelling due to increased IOM wind strength. (C) Smoothed Cariaco Basin metal record (nine-point running average) (22). High Ti concentrations reflect higher river discharge due to increased summer precipitation. (D) ODP 658 terrigenous dust record from West Africa (24). High terrigenous dust concentrations reflect greater aridity in West Africa.

Although in southern Oman monsoon precipitation continuously decreases from ∼8 ky B.P. to the present, lake records in the African and Indian monsoon domain (13, 23) and a marine dust record off West Africa (24) rather suggest that monsoon precipitation decreased abruptly between 6 and 5 ky B.P. (Fig. 3D). How can we explain this apparent mismatch? First, both fully coupled (ocean-atmospherevegetation) climate model simulations (25) and geological data (3, 24) suggest that this abrupt humid-arid transition in northern Africa can be best explained by a threshold response (negative vegetation-atmosphere feedback) of the African monsoon to orbitally induced summer insolation. Second, lake levels in Indian monsoon domain may show a nonlinear response to precipitation changes. A shorter monsoon season and/or high-amplitude fluctuations in monsoon precipitation can quickly induce a negative precipitation-minus-evaporation balance, leading to rapid desiccation of the lake and, thus, terminating the record. Furthermore, lakes dry out as soon as the summer monsoonal rainfall belt retreats south of their drainage basin. We suggest that the Q5 record is, by virtue of its nature and geographical position, more suitable to record the gradual middle to late Holocene decrease in IOM intensity and precipitation. The Q5 record reveals an almost linear response of the IOM to orbitally induced variations in summer insolation after ∼8 ky and, thus, confirms results of previously published climate model simulations (26).

Although during the early Holocene decadal to multidecadal changes in monsoon precipitation coincide with temperature fluctuations in the North Atlantic (Fig. 2), short-term fluctuations in IOM precipitation also occurred after 8 ky B.P. To examine the nature of these variations, we removed the long-term trend in the isotopic record by removing a sinusoidal fit to the later part (Fig. 1). We then compared the Q5 record to the tree-ring Δ14C record (27). The Q5 record was tuned—within the Th-U age uncertainties—to the Δ14C time scale [see (6) and fig. S4 for details]. The fine-tuned Q5 δ18O isotopic record shows a strong similarity to the detrended Δ14C residuals (14Cres) record (27), which largely reflects variations in solar activity (Fig. 4) (28, 29). In the fine-tuned Q5 record, intervals of weak (strong) solar activity correlate with periods of low (high) monsoon precipitation (Fig. 4). However, the visible correlation becomes less clear in the late Holocene when the Δ14Cres record shows only small amplitude variations in solar activity. Results of spectral analysis of both the detrended raw data and fine-tuned data further reinforce our interpretation that second-order variations in IOM precipitation were triggered by changes in solar activity, as indicated by statistically significant major solar cycles (within the 6-dB bandwidth) centered at ∼220, ∼140, ∼107, 11, and 10 years for the untuned and ∼240, ∼140, ∼90, ∼18, and ∼11 years for the fine-tuned δ18O paleoprecipitation record (figs. S5, A and B). Additionally, the cross-spectral analysis between both records confirms the correspondence of statistically significant solar cycles at 205 (de Vries cycle), 132, 105, 90 (Gleissberg cycle), 60, and 55 years (fig. S5C). Such a close Sun-monsoon connection was previously detected in a shorter stalagmite record from northern Oman (6) and is now confirmed and extended by the much longer Q5 record from southern Oman. Whether variations in solar output affect the IOM indirectly, by internal forcing mechanisms (6, 19), or more directly, by external forcing mechanisms (30), is not yet fully resolved. Although solar-induced variations in the record of North Atlantic drift ice (termed Bond events) (31) may have influenced the IOM indirectly by way of the monsoon-Eurasian snow cover link during the early Holocene (6, 19), Bond events are less evident in the middle to late Holocene Q5 and marine upwelling record offshore Oman (19). This weak correlation may indicate that after 8 ky B.P., when the Northern Hemisphere ice sheets were largely gone and North Atlantic thermohaline circulation was more stable, IOM circulation responded more directly to changes in solar output (external forcing) than to changes in North Atlantic northward heat transport and deep-water production (internal forcing).

Fig. 4.

Comparison between the detrended and smoothed (three-point running average) Q5 δ18O (black line) and detrended atmospheric Δ14Cres (red line) profiles. The correlation coefficient between both records is r = 0.48. Labeled triangles are Bond events in the North Atlantic (31).

Supporting Online Material

www.sciencemag.org/cgi/content/full/300/5626/1737/DC1

Tables S1 and S2

Figs. S1 to S5

References

References and Notes

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