Slow dynamics of the Northern Hemisphere glaciation
Abstract
[1] Unraveling the dynamics of the Northern Hemisphere glaciation (NHG) in the Pliocene is a key step toward a quantitative theory of the climate transition from a greenhouse to an icehouse world. Extracting the ice volume signal from marine oxygen isotope (δ18O) records corrupted with “temperature noise” can be accomplished using statistical time series analysis. We use 45 δ18O records from benthic and planktonic foraminifera and globally distributed sites to reconstruct the dynamics of NHG initiation. We compare δ18O amplitudes with those of temperature proxy records and estimate a global ice volume–related increase of 0.4‰, equivalent to an overall sea level lowering of 43 m. We find the NHG started significantly earlier than previously assumed, as early as 3.6 Ma, and ended at 2.4 Ma. This long-term increase points to slow, tectonic forcing such as closing of ocean gateways or mountain building as the root cause of the NHG.
1. Introduction
[2] The Northern Hemisphere glaciation in the Pliocene was a climatic change from a greenhouse world [Crowley, 1991] to a world with periodically waxing and waning ice sheets [Berger et al., 1984]. Marine sedimentary records of ice-rafted debris (IRD) and oxygen isotopic composition reveal major glacial expansions at 2.5 Ma [Shackleton et al., 1984] and 2.7 Ma [Haug et al., 1999] ago. (All dates given in this paper refer to the absolutely dated Pliocene timescale in Table 1.) There appear to be two major obstacles to achieving a quantitative and causal understanding of the NHG. First, regarding the size of the glaciation, the δ18O values record not only changes in ice volume but also changes in regional water temperature [Shackleton, 1967]. Second, regarding the timing of the glaciation, the initiation of NHG has not yet been accurately estimated [Raymo, 1994]. There were certainly northern glacial episodes in the early Pliocene and Miocene, as documented by IRD events in the Norwegian Sea [Jansen et al., 1990], the Greenland Sea [Larsen et al., 1994], Baffin Bay [Thiébault et al., 1989], and the Fram Strait and Yermak Plateau [Wolf-Welling et al., 1996]. However, a significant increase in global ice volume in the Northern Hemisphere occurred only in the late Pliocene.
Event Number | Eventa | Typeb | Absolute Datec | Astronomical Tuning,d kyr B.P. | |
---|---|---|---|---|---|
Kiloyears, B.P. | Referencee | ||||
1 | Olduvai top | M | 1776 ± 30 | R1 | 1775 |
2 | Olduvai base | M | 1980 | R2 | 1945 |
3 | LAD D. brouweri | B | 1995 | ||
4 | Reunion | M | 2140 ± 30 | R1 | |
5 | FAD acme D. triradiatus | B | 2170 | ||
6 | LAD D. pentaradiatus | B | 2515 | ||
7 | LAD D. surculus | B | 2561 | ||
8 | Matuyama/Gauss | M | 2585 ± 50 | R3 | 2600 |
9 | LAD D. tamalis | B | 2869 | ||
10 | LAD G. altispira | B | 3020 | ||
11 | Kaena top | M | 3044 ± 30 | interpolation | 3046 |
12 | Kaena base | M | 3102 ± 51 | interpolation | 3131 |
13 | LAD S. seminulina | B | 3160 | ||
14 | Mammoth top | M | 3210 ± 10 | R4 | 3233 |
15 | Mammoth base | M | 3300 ± 20 | R4 | 3331 |
16 | Gauss/Gilbert | M | 3562 ± 28 | interpolation | 3594 |
17 | LAD Sphenolithus spp. | B | 3600 | ||
18 | LAD R. pseudoumbilicus | B | 3827 | ||
19 | S/O Pulleniatina | B | 3941 | ||
20 | NN14 base | B | 4141 | ||
21 | Cochiti top | M | 4190 ± 20 | R5 | 4185 |
22 | LAD G. nephentes | B | 4200 | ||
23 | Cochiti base | M | 4260 ± 20 | R5 | 4316 |
24 | Nunivak top | M | 4481 ± 14 | R5, R6 | 4479 |
25 | Nunivak base | M | 4620 ± 20 | R3, R5, R7 | 4623 |
- a Abbreviations are FAD, first appearance date; LAD, last appearance date; NN14, nannoplankton zone 14; S/O, sinistral/dextral coiling change.
- b Type M is magnetostratigraphic; type B is biostratigraphic.
- c Errors of absolute ages are 1-σ standard deviations calculated from individual measurement errors. Errors owing to varying age standards or decay constants are neglected. Errors of astronomically tuned ages depend on assumptions made and are not reported.
- d Tuning is orbital. Magnetostratigraphic dates are averages from dates in ODP Sites 677 [Shackleton et al., 1990], 659 [Tiedemann et al., 1994], and 846 [Shackleton et al., 1995b]. Biostratigraphic dates are averages from dates in ODP Sites 659 [Tiedemann et al., 1994] and 846 [Shipboard Scientific Party, 1992], and dates in the compilation by Berggren et al. [1995]. Errors of astronomically tuned dates of biostratigraphic events are likely larger than age errors of absolutely dated magnetostratigraphic events.
- e Sources are R1, Baksi et al. [1992]; R2, Walter et al. [1991]; R3, Wilson [1993]; R4, Renne et al. [1993]; R5, Clement et al. [1997]; R6, Hall and Farrell [1995]; and R7, Baksi et al. [1993]. Interpolation was carried out between bracketing magnetostratigraphic dates in Table 1, with the interpolation ratio following the compilation by Berggren et al. [1995].
[3] In an attempt to quantify the dynamics of the NHG, we employed a simple parametric model of a climate change. Our approach rests on (1) the construction of a large database of δ18O and temperature records for the interval from 2 to 4 Ma spanning the NHG and (2) the application of statistical time series analysis techniques for signal extraction. By analyzing many records with a quantitative method, we reduce the noise and filter out the ice volume signal. By subtracting the ice volume signal and using calibration formulas, we draw regional maps of temperature changes associated with the NHG. Other dynamical properties of this climate change, such as variability and persistence, are derived. The estimated start and end of the NHG interval help to reduce the set of feasible causal explanations, some of which are discussed here.
2. Data
[4] The database consists of marine proxy records for ice volume and temperature (δ18O, Mg/Ca, faunal assemblages). Because the period of NHG reflects the long-term trend in mean ice volume, coarsely resolved time series can also be utilized.
2.1. Timescale
[5] A new, absolutely dated magnetobiostratigraphic timescale (Table 1) was developed to redate older time series (published before 1994) and erect an accurate time frame for the 2–4 Myr interval. The magnetostratigraphic dates exhibit an excellent agreement with astronomically tuned dates, the average error is ∼25,000 years (kyr) [Mudelsee, 2005]. Biostratigraphic dates are likely less accurate because of stratigraphic uncertainties and site-specific dependences of the habitats.
2.2. Ice Volume and Temperature Proxy Records
[6] The NHG database (Table 2) includes recently published marine δ18O time series [Lisiecki and Raymo, 2005]. Twenty-five moderate to high-resolution isotope records (spacing less than 11 kyr or one half precession cycle) and twenty lower-resolution records (≥11 kyr, or with hiatuses) provide excellent global coverage. Records from benthic foraminifera (29, thereof 18 high-resolution) document changes in global ice volume and bottom water temperature (BWT); planktonic δ18O data (16, thereof 7 high-resolution) record ice volume and sea surface temperature (SST). Only four temperature proxy time series (from faunal assemblages and Mg/Ca techniques) are available for the 2–4 Myr interval (Table 2).
Record Site | Location | Water Depth m | Description (Foraminifera, Proxy Technique, Temperature Variablea) | sb, cm kyr−1 | dc, kyr | Referencesd | ||
---|---|---|---|---|---|---|---|---|
Latitude | Longitude | Datae | Timescalef | |||||
Benthic δ18O Records | ||||||||
V28–179 | 4°37′N | 139°36′W | 4509 | G. subglobosa | 0.45 | 32.2 | R1 | 2, 8, 11, 12, 14, 15, 16 |
DSDP 397 | 26°50′N | 15°10′W | 2900 | mainly U. peregrina | 7.5 | 35.2 | R2 | 2, 4, 8, 11, 12, 14, 15, 16, 21g |
DSDP 502 | 11°29′N | 79°23′W | 3051 | Cibicidoides spp. | 2.8 | 28.5 | R3, R4 | 11, 12, 14, 15, 16, 21, R4h |
DSDP 552 | 56°03′N | 23°14′W | 2311 | Cibicidoides spp. | 1.4 | 9.2 | R5, R6 | this worki |
DSDP 586 | 0°30′S | 158°30′E | 2218 | C. wuellerstorfi | 2.8 | 78.2 | R7 | 1, 8, 10, 16, 19 |
DSDP 586 | 0°30′S | 158°30′E | 2218 | O. umbonatus | 2.8 | 65.5 | R7 | 1, 8, 10, 16, 19 |
DSDP 590 | 26°07′S | 161°14′E | 1533 | C. kullenbergi | 2.8 | 66.2 | R8 | 2, 8, 11, 15, 16, 20j |
DSDP 606 | 37°20′N | 35°30′W | 3007 | G. subglobosa | 4.2 | 10.7 | R9 | 2, 4, 8, 11, 12, 14, 15, 16, 21k |
DSDP 606 | 37°20′N | 35°30′W | 3007 | P. wuellerstorfi | 4.2 | 10.7 | R9 | 2, 4, 8, 11, 12, 14, 15, 16, 21k |
DSDP 607 | 41°00′N | 32°58′W | 3427 | Cibicidoides spp. | 4.2 | 4.2 | R10, R11, R12 | Table 1l |
DSDP 610 | 53°13′N | 18°53′W | 2417 | Cibicidoides spp. | 3.4 | 5.6 | R13 | 4, 8, 11, 12, 14, 15, 16, 21 |
ODP 659 | 19°05′N | 21°02′W | 3070 | C. wuellerstorfi | 2.8 | 4.1 | R14 | see data |
ODP 662 | 1°23′S | 11°44′W | 3821 | Cibicidoides spp. | 4.3 | 3.5 | R12 | 3, 5, 6, 7, 9, 17m,n |
ODP 704 | 46°53′S | 7°25′E | 2532 | Cibicidoides spp. | 3.0 | 8.0 | R15 | 2, 4, 11, 12, 14, 15, 16, 21o |
ODP 722 | 16°37′N | 59°48 E | 2028 | Uvigerina spp | 2.7 | 7.7 | S. Clemens (unpublished data, 2004) | R16 |
ODP 758 | 5°23′N | 90°21′E | 2925 | C. wuellerstorfi | 1.3 | 7.4 | R17 | 2, 8, 11, 12, 14, 15, 16, 21k |
ODP 806 | 0°19′N | 159°22′E | 2520 | C. wuellerstorfi | 3.3 | 3.3 | T. Bickert (unpublished data, 2004) | see datal |
ODP 846 | 3°06′S | 90°49′W | 3296 | mainly C. wuellerstorfi, Uvigerina spp. | 4.1 | 2.4 | R18 | R19 |
ODP 849 | 0°11′S | 110°31′W | 3851 | C. wuellerstorfi, Uvigerina spp. | 2.7 | 4.0 | R20 | R19 |
ODP 925 | 4°12′N | 43°29′W | 3040 | Cibicidoides spp. | 3.1 | 4.3 | R21, R22, R23 | see data |
ODP 927 | 5°28′N | 44°28′W | 3326 | Cibicidoides spp. | 3.3 | 4.5 | R21, R22p | see data |
ODP 929 | 5°56′N | 43°44′W | 4361 | Cibicidoides spp. | 2.7 | 4.5 | R21, R22, R23 | see data |
ODP 982 | 57°31′N | 15°53′W | 1145 | C. wuellerstorfi | 2.7 | 3.2 | R12, R24 | Table 1l |
ODP 999 | 12°44′N | 78°44′W | 2828 | C. wuellerstorfi | 3.0 | 3.8 | R25 | see data |
ODP 1014 | 32°49′N | 119°58′W | 1177 | C. mckannai | 9.8 | 19.5 | R26 | R27m |
ODP 1018 | 36°59′N | 123°17′W | 2467 | C. wuellerstorfi | 9.8 | 19.7 | R26 | R27m |
ODP 1085 | 29°22′S | 13°59′E | 1725 | C. wuellerstorfi | 5.3 | 2.0 | R28, R29 | see data |
ODP 1143 | 9°22′N | 113°17′E | 2772 | C. wuellerstorfi, U. peregrina | 3.5 | 3.0 | R30 | see data |
ODP 1148 | 18°50′N | 116°34′E | 3294 | Cibicidoides spp., Oridorsalis spp., Uvigerina spp. | 2.5 | 7.5 | R31 | see data |
Planktonic δ18O Records | ||||||||
DSDP 572 | 1°26′N | 113°51′W | 3893 | G. sacculifer | 1.4 | 7.7 | R32 | see dataq |
DSDP 586 | 0°30′S | 158°30′E | 2218 | G. sacculifer | 2.8 | 56.5 | R7 | 1, 8, 10, 16, 19 |
DSDP 586 | 0°30′S | 158°30′E | 2218 | Pulleniatina spp. | 2.8 | 56.5 | R7 | 1, 8, 10, 16, 19 |
DSDP 590 | 26°07′S | 161°14′E | 1533 | G. sacculifer | 5.3 | 55.7 | R8 | 2, 8, 11, 15, 16, 20j |
DSDP 606 | 37°20′N | 35°30′W | 3007 | G. bulloides | 4.2 | 7.9 | R9 | 2, 4, 8, 11, 12, 14, 15, 16, 21k |
ODP 625 | 28°50′N | 87°10′W | 889 | G. ruber, G. sacculifer | 3.7 | 4.3 | R33 | 3, 6, 7, 13, 17, 18, 22m |
ODP 704 | 46°53′S | 7°25′E | 2532 | G. bulloides, N. pachyderma | 3.0 | 6.0 | R15 | 2, 4, 11, 12, 14, 15, 16, 21o |
ODP 722 | 16°37′N | 59°48′E | 2028 | G. sacculifer | 2.7 | 12.1 | R15 | see datar |
ODP 758 | 5°23′N | 90°21′E | 2925 | G. sacculifer | 1.3 | 7.1 | R34, R35 | 2, 8, 11, 12, 14, 15, 16, 21k |
ODP 806 | 0°19′N | 159°22′E | 2520 | G. sacculifer | 3.3 | 3.5 | R36 | T. Bickert (personal communication, 2004)l |
ODP 851 | 2°46′S | 110°34′W | 3760 | G. sacculifer | 1.9 | 5.2 | R37 | see datal |
ODP 851 | 2°46′S | 110°34′W | 3760 | G. tumida | 1.9 | 5.1 | R37 | see datal |
ODP 851 | 2°46′S | 110°34′W | 3760 | N. humerosa, N. dutertrei | 1.9 | 6.7 | R37 | see datal |
ODP 925 | 4°12′N | 43°29′W | 3040 | G. sacculifer | 3.1 | 4.6 | R22, R38, R39s | see data |
ODP 999 | 12°44′N | 78°44′W | 2828 | G. sacculifer | 3.0 | 3.2 | R40 | see data |
ODP 1148 | 18°50′N | 116°34′E | 3294 | G. ruber, G. sacculifert,u | 2.5 | 9.8 | R31 | see data |
Temperature Proxy Records | ||||||||
DSDP 572 | 1°26′N | 113°51′W | 3893 | Ostracoda assemblages, SST | 1.4 | 18.2 | R41 | see dataq |
DSDP 607 | 41°00′N | 32°58′W | 3427 | Mg/Ca benthic foraminifera, BWT | 4.2 | 7.9 | R42 | Table 1l |
ODP 806 | 0°19′N | 159°22′E | 2520 | Planktonic foraminifera assemblages,v SST | 3.3 | 7.7 | R43 | T. Bickert (personal communication, 2004)l |
ODP 806 | 0°19′N | 159°22′E | 2520 | Mg/Ca benthic foraminifera, BWT | 3.3 | 254 | R44 | see data |
- a SST, sea surface temperature; BWT, bottom water temperature.
- b Average sedimentation rate within regression time interval.
- c Average temporal spacing within regression time interval.
- d R1, Shackleton and Opdyke [1977]; R2, Shackleton and Cita [1979]; R3, Keigwin [1982b]; R4, Oppo et al. [1995]; R5, Shackleton and Hall [1984]; R6, Curry and Miller [1989]; R7, Whitman and Berger [1992]; R8, Elmstrom and Kennett [1986]; R9, Keigwin [1986]; R10, Raymo et al. [1989]; R11, Raymo [1992]; R12, Lisiecki and Raymo [2005]; R13, Raymo et al. [1992]; R14, Tiedemann et al. [1994]; R15, Hodell and Venz [1992]; R16, Clemens et al. [1996]; R17, Chen et al. [1995]; R18, Shackleton et al. [1995a]; R19, Shackleton et al. [1995b]; R20, Mix et al. [1995]; R21, Bickert et al. [1997]; R22, Franz [1999]; R23, Billups et al. [1998a]; R24, Venz and Hodell [2002]; R25, Haug and Tiedemann [1998]; R26, Kwiek and Ravelo [1999]; R27, Lyle et al. [2000]; R28, Andreasen [2001]; R29, Ravelo et al. [2004]; R30, Tian et al. [2002]; R31, Jian et al. [2003]; R32, Prell [1985]; R33, Joyce et al. [1990]; R34, Farrell and Janecek [1991]; R35, Chen [1994]; R36, Jansen et al. [1993]; R37, Cannariato and Ravelo [1997]; R38, Chaisson and Ravelo [1997]; R39, Billups et al. [1998b]; R40, Haug et al. [2001]; R41, Hays et al. [1989]; R42, Dwyer et al. [1995]; R43, Andersson [1997]; R44, Lear et al. [2003].
- e Benthic isotope data were adjusted to seawater equilibrium using corrections given by Shackleton and Hall [1984] or data references. Planktonic isotope data were adjusted to correct for species variations within a record, see data references.
- f Given numbers refer to events in Table 1, using absolute dates for magnetostratigraphic events (unless otherwise noted) and astronomically tuned dates for biostratigraphic events. For each record, data, and timescale references (or references cited therein) contain further information on magnetobiostratigraphy and tuning procedure. The average error between records owing to varying timescales (Table 1) is approximately 25 kyr [Mudelsee, 2005]. Records with hiatuses or a low time resolution can have significantly larger timescale errors (approximately 100 kyr).
- g Timescale uncertain in late part.
- h Combined record was constructed from low-resolution, absolutely dated part (< 2600 kyr) and high-resolution, tuned part (> 2600 kyr). A hiatus exists between 2188 and 2366 kyr.
- i Using astronomical dating for the interval up to 2100 kyr and magnetostratigraphic events Kaena Base and Gauss/Gilbert on the Cande and Kent [1992] timescale for the older interval. Hiatuses exist between approximately 2200 and 2300 kyr and between approximately 2700 and 2828 kyr.
- j Timescale uncertain in early part.
- k Ages in early part (at around MIS M2 to MG2) are approximately 50 kyr younger than ages in standard astronomically tuned timescales [Tiedemann et al., 1994; Shackleton et al., 1995b].
- l Timescale tuned to timescale of Shackleton et al. [1995b].
- m Timescale based wholly on biostratigraphy.
- n Biostratigraphic timescale correlated to standard astronomically tuned timescales [Tiedemann et al., 1994; Shackleton et al., 1995b] at around MIS 96–98–100.
- o Hiatus exists between approximately 2240 and 2700 kyr.
- p Hiatus exists between approximately 3278 and 3530 kyr.
- q The initial timescale was based on correlation of carbonate records between DSDP Sites 572 and 573 [Prell, 1985]; for DSDP 573 a magnetostratigraphy exists (events 2, 8, 11, 12, 14, 15, 16, and 21 in Table 1). The late part of the record (at around MIS 96–98–100) was subsequently correlated with standard astronomically tuned timescales [Tiedemann et al., 1994; Shackleton et al., 1995b].
- r Hiatus exists between approximately 2846 and 3323 kyr.
- s Very low resolution between 2 and approximately 2.6 Ma.
- t G. ruber was used in interval from 2 Ma to approximately 3.1 Ma; G. sacculifer was used in interval from approximately 3.1 to 4 Ma.
- u Low resolution between approximately 3 and 4 Ma.
- v Modern analog technique.
3. Methods
3.1. Regression
[7] We employed a simple parametric model of a climate change, a “ramp” [Mudelsee, 2000], to infer the start, end, and amplitude of the increase in mean δ18O and temperature from 2–4 Myr. Superimposed on this long-term (>1 Myr) trend are fluctuations, which come mainly from short-term (≤41 kyr) variations in ice volume and temperature. Such variations are partly induced by changes in the Earth's orbital parameters obliquity and precession [Berger et al., 1984]. Salinity effects [Whitman and Berger, 1992] and measurement uncertainties add some additional “noise.” To estimate the resultant uncertainties of the NHG parameters, start, end, and amplitude, we used extensive computer simulations that take data noise into account.
[8] Fits of the ramp regression model to the δ18O and temperature time series used a weighted least squares criterion for determining the amplitude combined with a brute force search for determining start and end [Mudelsee, 2000]. The increase in variability (time-dependent standard deviation, σ(t)) across the NHG was quantified by means of a running window. This allows not only to determine the weighting for the regression, but also to measure how much the size of the δ18O fluctuations increased as the ice sheets grew.
[9] We estimated the persistence time, τ, of δ18O fluctuations by the decay period of the autocorrelation function [Mudelsee, 2002] fitted to the standardized regression residuals (a residual is given by the difference between the δ18O value and the ramp model value, divided by σ(t)). To detect outliers (positive and negative δ18O extremes), we adopted a ±3 σ(t) threshold.
[10] We performed computer simulations [Efron and Tibshirani, 1993; Mudelsee, 2000] as follows to derive parameter uncertainties: (1) Take fitted ramps, σ(t) and τ to produce a simulated time series with a random number generator. (2) Fit ramp to simulated data to obtain simulated parameters (start, end, amplitude). (3) Repeat steps 1 and 2 to produce 400 copies of simulated parameters. (4) Take standard deviation of each set of copies as uncertainty estimate.
[11] Comparing the mean of each set of copies with the original result showed that all estimations carried out had negligible bias. Because statistical uncertainties of start and end (Table 3) are clearly larger than timescale uncertainties (Table 2) the regressions do not require timescale simulations.
Recordb | Start, kyr | End, kyr | δ18O Amplitude, ‰ | Cooling, °C | τ, kyr |
---|---|---|---|---|---|
Benthic Records | |||||
606 b G.s. | 3506 ± 253 | 2753 ± 293 | 0.47 ± 0.12 | 0.4 ± 0.7 | 8.7 ± 2.0 |
606 b P.w. | 3440 ± 264 | 2545 ± 309 | 0.61 ± 0.13 | 1.2 ± 0.7 | 6.3 ± 1.5 |
607 b | 2903 ± 106c | 2720 ± 125 | 0.53 ± 0.06 | 0.62 ± 0.29 | 10.9 ± 1.4 |
610 b | 3347 ± 238 | 2831 ± 204 | 0.41 ± 0.09 | 0.1 ± 0.5 | 6.6 ± 1.0 |
659 b | 3459 ± 222 | 2084 ± 273d | 0.52 ± 0.09 | 0.7 ± 0.5 | 6.3 ± 0.8 |
662 b | 3191 ± 200 | 2463 ± 216 | 0.58 ± 0.13 | 1.0 ± 0.7 | 12.9 ± 2.2 |
722 b | 3499 ± 195 | 2077 ± 221d | 0.49 ± 0.07 | 0.5 ± 0.4 | 5.0 ± 0.9 |
758 b | 3502 ± 192 | 2150 ± 196 | 0.54 ± 0.07 | 0.8 ± 0.4 | 8.0 ± 1.3 |
806 b | 3695 ± 160 | 2639 ± 190 | 0.44 ± 0.06 | 1.0 ± 0.5 | 7.3 ± 0.8 |
846 b | 3700 ± 160 | 2462 ± 200 | 0.60 ± 0.07 | 1.1 ± 0.4 | 8.0 ± 0.9 |
849 b | 3176 ± 99 | 2446 ± 198 | 0.51 ± 0.07 | 0.7 ± 0.4 | 10.4 ± 1.3 |
925 b | 2732 ± 187c | 2532 ± 177 | 0.37 ± 0.07 | −0.1 ± 0.4 | 6.4 ± 0.8 |
929 b | 3747 ± 189 | 2930 ± 212 | 0.51 ± 0.08 | 0.7 ± 0.4 | 8.4 ± 1.0 |
982 b | 3827 ± 193d | 2095 ± 200d | 0.47 ± 0.06 | 0.4 ± 0.3 | 7.9 ± 0.9 |
999 b | 3861 ± 153d | 2090 ± 195d | 0.54 ± 0.06 | 0.8 ± 0.3 | 7.0 ± 0.8 |
1085 b | 3777 ± 147 | 2168 ± 193 | 0.53 ± 0.06 | 1.0e | 7.1 ± 0.8 |
1143 b | 3613 ± 138 | 2172 ± 165 | 0.69 ± 0.08 | 1.6 ± 0.4 | 5.4 ± 0.6 |
1148 b | 3734 ± 146 | 2492 ± 166 | 0.68 ± 0.07 | 1.6 ± 0.4 | 7.5 ± 1.4 |
Planktonic Records | |||||
572 p | 3152 ± 177 | 2830 ± 183 | 0.36 ± 0.06 | 0.12 ± 0.47 | 9.3 ± 1.5 |
606 p | 3760 ± 216 | 2001 ± 254d | 0.42 ± 0.06 | 0.2 ± 0.3 | 4.3 ± 0.9 |
625 p | 3992 ± 406d | 2013 ± 378d | 0.39 ± 0.07 | 0.0 ± 0.4 | 4.2 ± 0.5 |
758 p | 3050 ± 110 | 2692 ± 127 | 0.38 ± 0.04 | −0.1 ± 0.2 | 5.7 ± 0.9 |
806 p | 3936 ± 147d | 2000 ± 200d | 0.27 ± 0.04 | −0.85 ± 0.17 | 3.0 ± 0.3 |
851 p G.sac. | 3584 ± 236 | 2429 ± 225 | 0.51 ± 0.08 | 0.7 ± 0.4 | 6.5 ± 0.8 |
999 p | 3587 ± 188 | 2504 ± 193 | 0.46 ± 0.07 | 0.4 ± 0.4 | 4.5 ± 0.5 |
Averagef | 3606 ± 60g | 2384 ± 64g | 7.1 ± 0.4h |
- a The high-resolution records were analyzed to obtain NHG parameters start, end, δ18O amplitude within interval 2384–3606 kyr, and persistence time, τ. For the records 572 p, 607 b, 806 b, 806 p, and 1085 b the cooling of the water masses during this interval was determined via proxies (Figure 3). For the other records it was estimated by subtracting an ice volume signal of 0.39‰ from the δ18O amplitudes and using the δ18O temperature calibrations (section 3.2). Persistence time average results from using values from benthic records only.
- b Caption for Figure 1 contains the records' notation.
- c Start date is likely down biased because of midterm deviation at around 3100–3200 kyr (Figure 1).
- d Strongly skewed error distribution occurs because of solution near interval bound.
- e Error is not determined (likely > 50%).
- f Weighted 50%-trimmed mean with maximum of internal and external 1 − σ error. Trimming [Tukey, 1977] ensured that biased or strongly skewed individual results were excluded from averaging. Degree of trimming has little influence on result.
- g Internal error, superimposed is a timescale error of 25 kyr.
- h External error.
3.2. Calibration of δ18O Changes
[12] Calibration formulas are required to calculate temperature or salinity changes into δ18O changes, and vice versa. We used the calibration of temperature-related δ18O changes from modern and experimental data [Chen, 1994], Δδ18OT/ΔT = −0.234‰/°C. An estimation of the statistical error (1 − σ) of this formula yields 0.003‰/°C, which we inflated in a conservative approach to a value of 0.01‰/°C (S. Mulitza, Research Center Ocean Margins, personal communication, 2004) to take “species noise” and violations of the actualism assumption into account. The calibration of salinity-related δ18O changes, Δδ18OS/ΔT = 0.05‰/°C, assumes a linear relation between salinity and temperature changes and was developed for interpreting western equatorial Pacific δ18O amplitudes [Whitman and Berger, 1992]. Systematic errors caused by applying the calibration to other sites are likely small owing to the low signal proportion of Δδ18OS.
4. Results
4.1. NHG Start and End
[13] The results exhibit considerable variations in NHG start and end among the δ18O records (Figures 1 and 2and Table 3). The reason for this scatter is that the global ice volume signal of the NHG (δ18O increase), common to all records owing to an ocean mixing time of less than ∼2 kyr [Broecker et al., 1988, 2004], is obscured by noise, mainly of climatic origin (regional temperature and salinity fluctuations). We assume that the variations in estimated start and end cancel out when averaging the results from many records. This is a reasonable assumption, given climatological evidence for regional differences in temperature sensitivity [Ravelo et al., 2004] and the fact that our NHG δ18O database is so large. The average start and end values of the NHG ice volume increase are 3606 ± 60 kyr and 2384 ± 64 kyr, respectively, for the high-resolution records (Figure 1 and Table 3). The low-resolution records (Figure 2) yield an end date of 2510 ± 125 kyr that agrees within error bars, and a start date of 3350 ± 120 kyr that reflects minor systematic uncertainties. Sources of this error can be midterm deviations from the ramp form at around the start (see below) or underestimated influences of hiatuses in the low-resolution records.
4.2. Ice Volume Signal
[14] Extraction of the NHG ice volume signal within the interval 2384 to 3606 kyr cannot be achieved by averaging results from individual records because the noise components temperature and salinity would not cancel out but reflect an overall cooling. Evaluating the size of the ice volume amplitude alone on the basis of the δ18O results (Table 3) suggests an upper limit of around 0.4‰. This is indicated by values from records from several, low-latitude locations (925 b, 572 p, 625 p, 758 p, 806 p; see Figure 1 for notation), because a warming at all these sites across the NHG seems unlikely. More detailed information has to come from independent temperature proxy records from the same locations and water masses as the δ18O records. The problem is that these temperature records are scarce, which is the reason why we used all available records (including those with a low time resolution). The SST record (cold and warm season averaged) from DSDP 572 [Hays et al., 1989], based on ostracoda assemblages, shows a minimal cooling (Figure 3 and Table 3) during 2384–3606 kyr, equivalent to a δ18O increase of Δδ18OT = 0.03 ± 0.12‰. Adopting the linear relation of Whitman and Berger [1992] between temperature and salinity changes, the cooling relates to a salinity-related δ18O decrease, Δδ18OS = −0.01‰. Subtracting Δδ18OT and Δδ18OS from the 572 p amplitude of 0.36 ± 0.06‰ yields an NHG ice volume signal of Δδ18OI = 0.34 ± 0.13‰. The high-resolution SST record from ODP 806 [Andersson, 1997], based on foraminifera assemblages, reveals a remarkable warming of 0.85 ± 0.17°C, equivalent to Δδ18OT = −0.20 ± 0.04‰ and Δδ18OS = 0.04‰, converting the low 806 p amplitude (Table 3) into an ice volume signal of Δδ18OI = 0.43 ± 0.06‰. The BWT record from ODP 806 [Lear et al., 2003], based on Mg/Ca thermometry, reveals despite its low resolution that, while the surface waters warmed at the Ontong Java Plateau (western equatorial Pacific) across the NHG, the deep waters cooled (Δδ18OT = 0.24 ± 0.12‰, Δδ18OS = −0.05‰, and Δδ18OI = 0.25 ± 0.13‰). The Mg/Ca–derived BWT record from DSDP 607 [Dwyer et al., 1995], has Δδ18OT = 0.15 ± 0.07‰, Δδ18OS = −0.03‰, and Δδ18OI = 0.41 ± 0.09‰. The Mg/Ca–derived BWT decrease of 1°C between 3.7 and 2.5 Ma (not continuously measured) at site ODP 1085 (D. H. Andreasen, Rutgers University, personal communication, 2004), finally, translates into Δδ18OI = 0.35‰. It is remarkable that the few Pliocene temperature records available so far, derived from distributed geographical sites and water masses with different proxy techniques, reveal, within error bars, the same ice volume signal of the NHG between 3606 and 2384 kyr, namely, an increase of Δδ18OI = 0.39 ± 0.04‰ (weighted mean). The equivalent sea level lowering [Mix and Ruddiman, 1984] is 43 m, with an uncertainty of somewhat more than 5 m.
4.3. Climate Variability
[15] The time-dependent δ18O standard deviation, σ(t), measuring the size of shorter-term fluctuations in ice volume, temperature, and salinity, shows an increase across the NHG, from 3200 kyr and ∼0.2‰ to 2560 kyr and ∼0.3‰ (Figure 4). No significant differences were found between benthic and planktonic records. A qualitatively similar long-term increase in variability had previously been recognized in the benthic δ18O record from DSDP 552 [Shackleton et al., 1988]. The timing and slowness of the increase in standard deviation support the timing and slowness of the increase in mean ice volume in the Northern Hemisphere: Ice sheets have to exist before fluctuations in their size occur.
4.4. Climate Persistence
[16] The estimated persistence time, τ, of δ18O fluctuations is of the order of a few kiloyears (Table 3). Correlation analyses showed that τ does not depend on the sedimentation rate (Table 2; r = 0.06) or the temporal spacing (Table 2; r = −0.04), which means that the sampling or effects within the sediment cores such as bioturbation likely did not influence τ. Rather, the persistence is thought to be of climatic origin and reflect the time constant [Imbrie and Imbrie, 1980] of the fluctuating part of the Antarctic and the developing Arctic ice sheets. The values are slightly smaller for planktonic than for benthic records, which we explain by a stronger “dilution” of the planktonic signal by short-term atmospheric interactions of surface waters. The benthic τ estimates, averaging to 7.1 ± 0.4 kyr, should come closest to the time constant of Pliocene ice sheets. This value is significantly smaller than the 17 kyr for the larger late Pleistocene ice sheets [Imbrie and Imbrie, 1980], in agreement with recent sedimentation modeling [Lisiecki and Raymo, 2005].
4.5. NHG Dynamics
[17] Over the 2–4 Myr interval, more or less all of the analyzed records (Figures 1, 2, and 3) exhibit a long-term trend, which is well described by the ramp model. There were few short excursions (extremes) and midterm deviations from this trend. The earliest δ18O extreme of likely global significance within 2–4 Myr was at marine isotope stages (MIS) M2–MG2 (3295–3340 kyr [Lisiecki and Raymo, 2005]), detected in 11 of 25 high-resolution records as a glacial event exceeding three standard deviations (Figure 1). Stage M2 seems to reflect a stronger glaciation than stage MG2 [Lisiecki and Raymo, 2005]. The global signature and IRD evidence from several sites in the North Atlantic/Nordic Seas [Kleiven et al., 2002] indicate a significant northern ice volume proportion. A systematic, midterm deviation from the glaciation trend was the Pliocene climate optimum [Dowsett et al., 1994], documented in 12 of 25 globally distributed, high-resolution records as an interval of lowered δ18O from ∼3250 kyr to ∼3050 kyr (Figure 1). Given the duration and the size of the δ18O decrease in many records (e.g., 607 b), a significant deglaciation seems likely. As regards the dispute about the stability of the Pliocene Antarctic ice shield [Shackleton et al., 1995a], our results combined with the IRD evidence [Kleiven et al., 2002] suggest that this deglaciation could have been a Northern Hemisphere event, leaving the Antarctic shield intact. Other, more heterogeneously distributed, shorter-term cold and warm extremes accompanied the long-term NHG glaciation trend (Figure 1) until a critical threshold was passed at 2.7 Ma [Haug et al., 1999] and strong glaciations (often exceeding 3 σ in Figure 1) at MIS 96–98–100 (2433–2523 kyr [Lisiecki and Raymo, 2005]) occurred. This heterogeneity and the above finding of spatial variations in start, end, and δ18O amplitude indicate differences on short-term to midterm timescales (∼41–100 kyr) among regional temperature histories across the NHG (Table 3). This supports the idea that during a global climate change, regional subsystems with varying feedback mechanisms emerge in response [Ravelo et al., 2004].
[18] In the geographical distribution of the long-term NHG temperature change (Figure 5), we see following provisional grouping. Bottom water cooling was, within the error ranges, more or less globally homogenous. Only 6 of 29 benthic records reflect larger deviations (Figure 5a), which may be due to reduced data quality (low-resolution records) or regional influences such as changes in upwelling (e.g., at DSDP 397 site). It is unclear why the result from the benthic record at site ODP 925 (0.1°C warming) deviates significantly from the results from nearby sites ODP 927 (0.9°C cooling) and ODP 929 (0.7°C cooling). The remaining 23 records have an average BWT decrease of ∼0.7°C.
[19] SST changes (Figure 5b) are divided into three groups. First, high latitudes likely cooled strongly (704 p). Second, at lower latitudes, the surface waters in the western Pacific region warmed significantly, by ∼0.7°C on average. Third, low-latitude surface waters elsewhere had, to first order, no long-term temperature change, which supports to some degree the hypothesis of a temperature buffer [Jenkins, 1992]. However, this does not apply to the western Pacific (warming) or some other regions (e.g., Sites 851 and 722). A more detailed picture of NHG temperature trends will emerge when more high-resolution BWT and SST records for the 2–4 Myr interval become available.
5. Conclusions
[20] The schematic view of the NHG (Figure 6) underlines that this climate transition was gradual. The amplitude of the change in mean ice volume (0.39‰) is only one to two times stronger than the average noise level, and is up to two times weaker than the largest glacial δ18O excursions (∼0.8‰) from the long-term trend (Figures 1 and 2). (The low signal-to-noise ratio of the climate transition is an a posteriori confirmation of our approach to construct and analyze a large database.) The timing of the change in mean ice volume (from 3.6 to 2.4 Ma) allows us to evaluate the feasibility of causal explanations of the NHG.
[21] A recent paper [Knie et al., 2004] proposed that a supernova explosion occurred close to the solar system, at 2.8 Ma, based on iron isotope data in a manganese crust. This could have led to an enhanced cosmic ray flux for a few 100 kyr. It was cautiously suggested that, provided there is a negative correlation between cosmic ray flux and Earth's surface temperature, “this supernova could have triggered a climatic change” [Knie et al., 2004, p. 171103-3], that is, the NHG. In light of our finding that the NHG began at 3.6 Ma, the supernova explanation becomes unlikely.
[22] Willis et al. [1999] noted spectral power at periods less than or equal to 15 kyr in a climate record based on pollen data from the Pula maar, Hungary, which spans the interval between 3.05 and 2.6 Ma. Willis et al. [1999, p. 571] proposed that “a nonlinear response at sub-Milankovitch frequencies may have been responsible for the initiation of the NHG.” The early start of the NHG at 3.6 Ma (Figure 6) again does not support this view. Other attempts to relate the initiation of the NHG to changes in spectral power are also not compatible with the early cooling trend documented here. For example, Maslin et al. [1998] proposed that an increase in obliquity minima from 3.2 to 2.5 Ma may have triggered the NHG. We do not dispute that Milankovitch variability may have influenced Pliocene to Pleistocene climate evolution; however, we do not believe such variability was the trigger for the NHG. The initiation of NHG was a long-term climate change, affecting such important variables as ice volume and temperature, and numerous feedback effects likely occurred from 3.6 to 2.4 Myr ago.
[23] The slow ice buildup (Figure 6) indicates a slow, tectonic mechanism as the probable root cause of NHG. The shoaling of the Central American Seaway in the Pliocene was suggested by Keigwin [1982a]. This tectonic movement led to a restricted water mass exchange between the Atlantic and the Pacific Oceans and to an intensified Gulf Stream, which brought moisture to high northern latitudes [Keigwin, 1982a]. However, a comparison of Atlantic/Pacific records of neodymium and lead isotopes [Frank et al., 1999] revealed that the restriction in water mass exchange was essentially complete by 5 Ma. Although the present study sets the NHG start earlier than previous work, we think that the disagreement in timing is still a strong argument against invoking the shoaling of the Central American Seaway as the explanation of NHG. Furthermore, two modeling studies [Nisancioglu et al., 2003; Klocker et al., 2005] show that an enhanced northward moisture transport is accompanied by enhanced heat transport, which can delay the start of a glaciation as originally proposed by Berger and Wefer [1996].
[24] Another tectonic mechanism is Tibetan uplift, proposed to have led to weathering-induced atmospheric carbon dioxide removal [Raymo et al., 1988]. Here the precise timing of when this movement became climatologically effective is not accurately constrained and might have been well before the NHG start [Raymo and Ruddiman, 1992; Molnar et al., 1993; Spicer et al., 2003]. Carbon dioxide proxy records are also needed to test this hypothesis directly. Currently available records employ the stomata index in oaks [Kürschner et al., 1996], or boron and carbon isotopes in marine matter [Raymo et al., 1996; Pagani et al., 1999; Pearson and Palmer, 2000]. These records suggest that Miocene-Pliocene carbon dioxide concentrations were not doubled but were possibly 30% higher than preindustrial levels. This evidence is not sufficient to accept or reject the Tibetan uplift hypothesis.
[25] Tibetan uplift could also have resulted in other important changes to the climate system. For instance, a sudden, tenfold increase in atmospheric dust load at 3.6 Ma has been related to aridification due to Tibetan uplift [Rea et al., 1998]. This increase, in good agreement with the NHG start, could have been responsible for the cooling that permitted increased snow and ice buildup on Northern Hemisphere land surfaces [Rea et al., 1998]. A strengthening of the east Asian monsoon from 3.6 to 2.6 Ma [Zhisheng et al., 2001] could also have strengthened the weathering process. The above dates correspond with the inferred NHG initiation (Figure 6) and suggest Tibetan uplift may have affected global climate evolution at this time.
[26] A final tectonic mechanism that fits our derived NHG time frame is the proposed restriction of the Indonesian Seaway between 4 and 3 Myr ago [Cane and Molnar, 2001]. This event could have reduced the atmospheric heat transport from the tropics to higher northern latitudes in the Pacific region. It could also explain the observed NHG warming of surface waters in the western Pacific region (Figure 5b) by the accumulation of westward flowing, equatorial surface waters.
[27] Two major causes for explaining the Pliocene warmth interval (3.25 to 3.05 Ma) have been brought forward. The first, elevated atmospheric CO2 levels, is problematic because it is not well corroborated by data [see also Crowley, 1996]. Elevated CO2 is also difficult to reconcile with the Tibetan uplift NHG explanation. The required positive, ∼200-kyr-long CO2 deviation from a long-term downward trend could have come from a variation in terrestrial plant biomass, as was suggested for the late Pleistocene glacial-interglacial cycle [e.g., Shackleton, 1977]. If so, one should search for evidence for significant Pliocene biomass changes. These could be a consequence of the NHG initiation. The second cause, stronger oceanic heat transport, is not feasible to explain a global warming event because, to first order, it merely redistributes heat on the planet [Crowley, 1996]. Since the results of the PRISM group [Dowsett et al., 1994, 2005] show that the Pliocene climate optimum occurred at a wide spatial scale, this explanation is thus problematic. However, surface waters at site ODP 806 in the western equatorial Pacific exhibit a pronounced cooling during the Pliocene warmth (Figure 3). This can be interpreted as heat that was transported steadily away from that region. Transport direction was predominantly northward. This heat may have melted parts of the newly built up Northern Hemisphere ice sheets (see section 4.5 and Haywood and Valdes [2004]). The ice-albedo feedback would have enhanced this midterm Pliocene warming signal [Haywood and Valdes, 2004]. Another transport mechanism could have been enhanced heat transport by winds. Long-term changes in wind properties can be induced by orographic changes. The feasibility of such scenarios in context of the NHG and the Pliocene warmth could be analyzed using coupled global climate models (GCMs). For example, Chandler et al. [1994], Sloan et al. [1996], and Haywood and Valdes [2004] studied the middle Pliocene climate using GCMs.
[28] The long-term glaciation trend of the Northern Hemisphere eventually led to thresholds in the climate system being exceeded and thereby shorter-term, positive feedback mechanisms initiated. Such feedbacks could have been a shift toward stratification in the polar ocean at 2.7 Myr ago, which may have trapped additional carbon dioxide in the abyss [Haug et al., 1999; Sigman et al., 2004] and also provided moisture to northern North America [Haug et al., 2005]. The strong glaciation at MIS 110 [Haug et al., 1999] would have been a consequence of this amplification of the long-term glaciation trend. The climate system finally came into a new, quasi-stable state with Milankovitch-type glacial-interglacial cycles [Berger et al., 1984], which have persisted to the present.
Acknowledgments
[29] We gratefully acknowledge the remarks by an anonymous reviewer and the Editor, L. Sloan. We thank C. Andersson, D. Andreasen, W. Berger, T. Bickert, K. Billups, J. Chen, S. Clemens, W. Curry, J. Farrell, G. Haug, Z. Jian, L. Lisiecki, A. Mix, D. Oppo, W. Prell, A. Ravelo, R. Tiedemann, and the ODP data librarian for the release of published and unpublished data and S. Cande, B. Clement, G. Haug, S. Mulitza, D. Schrag, and M. Schulz for comments. Supported by DFG research grant MU 1595/2 (M.M.).