Supplementary Material to accompany: A 0.6-Million Year Record of Millennial-Scale Climate Variability in the Tropics Kelly Ann Gibson† and Larry C. Peterson, Rosenstiel School of Marine and Atmospheric Science, University of Miami, Miami, FL 33149, USA † Current address: Department of Earth and Ocean Sciences, University of South Carolina, Columbia, SC, 29208, USA Corresponding author: K.A. Gibson, Department of Earth and Ocean Sciences, University of South Carolina, Columbia, SC, 29208, USA (kgibson@geol.sc.edu) 1 Methods 2 Sediment Cores 3 Ocean Drilling Program Site 1002 (FS 1) (10°42.73’N, 65°10.18’W; 893 m water 4 depth) was the last of a program to study Caribbean ocean history drilled during ODP 5 Leg 165. The site was triple-cored to a sub bottom depth of ~170 m and recovered a 6 continuous, undisturbed sequence. This study utilizes sediments from Hole 1002C except 7 for a short disturbed interval in Core 1002C-9H, the result of a wireline failure during 8 core recovery that resulted in the core barrel falling back down to the bottom of the hole 9 [Peterson et al., 2000]. To avoid this disturbed interval, cores 9H and 10H from Hole 10 1002D were also XRF scanned and analyzed for δ18O stratigraphy and the results were 11 patched into the Hole 1002C record. 1 12 MD03-2622 (10o 42.37’N, 65o 10.15’W) was recovered in 2003 during the 13 IMAGES P.I.C.A.S.S.O. cruise from a location on the central basin saddle adjacent to 14 Site 1002. The 48.3 m-long giant Calypso core extends into Marine Isotope Stage 6. The 15 central saddle was selected as a coring location for both sites because it is less susceptible 16 to deposits from turbidity flows that are known to disturb sedimentation in the two deeper 17 subbasins. 18 19 20 Age Models The age model for MD03-2622 was made by correlating its lightness (L*) record 21 to that of nearby Calypso core MD03-2621 on the timescale of Deplazes et al. [2013]. 22 The age model for MD-2621 was generated by Deplazes et al. [2013] by correlating a 23 new, high-resolution (0.7μm step size) lightness (L*) record from MD03-2621 with an 24 AMS 14C-dated grayscale record [Hughen et al., 2004] from the Cariaco Basin, and then 25 the L* and a 1 mm resolution scanning-XRF record of Br from MD-2621 to the ice core 26 δ18O record of NGRIP on the Wolff et al. [2010] timescale using the program AnalySeries 27 [Paillard et al., 1996]. Parameters of sediment color in the Cariaco Basin (e.g., L*, % 28 reflectance, and grayscale) are primarily controlled by concentrations of organic matter, 29 which in turn appear to reflect variations in primary productivity. Independent calendar- 30 age chronologies for the last deglaciation have shown that abrupt changes in Cariaco 31 Basin L* values and Greenland δ18O were synchronous within dating uncertainties 32 (Hughen et al., 2000), giving confidence in the use of L* for age model creation. The 33 successful extension of radiocarbon calibrations into the last glacial using Site 1002 34 sediments by Hughen et al. (2004, 2006) further supports this contention, as does 2 35 recognition of century-scale “precursor” events in core MD03-2621 L* by Gaudenz et al. 36 (2013) previously identified only in Greenland ice cores and in European stalagmites. 37 The average sedimentation rate over the interval of study in MD03-2622 is ~30 cm/kyr. 38 The planktic δ18O stratigraphy from Peterson et al. [2000] that provided the first 39 age control for Hole 1002C was based on very low resolution sampling at 30 to 60- cm 40 intervals from MIS 1 to 5, and 150-cm sample spacing from Termination II to the base of 41 the sequence. Even with such a broad sampling interval, a recognizable δ18O stratigraphy 42 was achieved because of the high sedimentation rates. A much higher resolution δ18O 43 record for Hole 1002C is used in this study based on analysis of the shallow mixed-layer 44 dwelling foraminifer Globigerinoides ruber at approximately 10 to 20-cm intervals down 45 through MIS 12, and ~50-cm intervals for the remainder of the sequence. This new δ18O 46 record from Hole 1002C covers approximately the last 600 kyr, while the scanning XRF 47 data begin at ~111 ky BP and extend back through the four previous glacial-interglacial 48 cycles. 49 The age model for the upper ~ 123 kyr for Hole 1002C was obtained by matching 50 the color record of Hole 1002C to the lightness record of MD03-2621 on its age model, 51 which is described above. For the record older than ~123 kyr, the remainder of the age 52 model was made by correlating the new planktic δ18O record with the Lisiecki and Raymo 53 [2005] benthic δ18O stack using the program AnalySeries [Paillard et al., 1996]. Anoxic 54 conditions in Cariaco Basin preclude generation of a continuous benthic record so we 55 must assume that δ18O variations in the planktic Hole1002C record are in phase with the 56 benthic Lisiecki-Raymo δ18O standard. 57 Prior to age model tuning, gas voids larger than 5 cm were removed from the 3 58 depth scale for Hole 1002C. A clear record of Marine Isotope Stages down through MIS 59 12 is obtained, with the lower resolution δ18O sampling below that hindering confident 60 identification of stages. Nonetheless, it appears that MIS 13-15 can be recognized though 61 the age model in this interval should be viewed with caution. Marine isotope stage 62 boundaries are after SPECMAP [Imbrie et al., 1984] applied to the Lisiecki and Raymo 63 [2005] age model. 64 65 Scanning XRF Analysis 66 Core sections from MD03-2622 and Site 1002 were run on an Avaatech XRF core 67 scanner for bulk elemental analysis in the Paleoclimatology Lab at RSMAS. Core MD03- 68 2622 was scanned in its entirety, which extends into MIS 6. From Hole 1002C, cores 69 representing sections 1002C-5H-4 through the end of 1002C-18H were scanned, which 70 together cover approximately 500 kyr of deposition from ~110 ky BP to ~600 ky BP. To 71 avoid scanning the disturbed interval in Hole 1002C mentioned above, cores 9H and 10H 72 from Hole 1002D were also scanned and patched into the Hole 1002C record. The results 73 from core MD03-2622 and Hole 1002C were spliced together at 115 ky BP, based on 74 matching patterns of Mo variability during Marine Isotope Stage (MIS) 5. 75 The archive sections from Hole 1002C and 1002D were photographed using a 76 Geoscan II color line-scan camera mounted on a GEOTEK Multi Sensor Core Logger in 77 the Paleoclimatology Lab at RSMAS. Core photographs were used to identify expansion 78 gaps and shrinkage cracks in both cores that could lead to low values in the XRF data. 79 Those data were subsequently removed so as to not misrepresent trends in elemental 80 variation. 4 81 Prior to analysis, cores were brought to room temperature for approximately one 82 hour to reduce condensation at the sediment surface during scanning. The core surface 83 was gently scraped with a glass slide to present a fresh surface for scanning, and covered 84 with 0.4 m-thick Ultralene® to prevent contact between the sediment surface and the 85 X-ray detector. The scanner was calibrated against a set of pressed powdered standards 86 prior to each run. All core sections were scanned at a 0.5 cm resolution downcore step 87 resulting in an average measurement spacing in time of ~16 yrs. Molybdenum was 88 measured as part of a 30kV run with a thin Pd filter, a measurement time of 10 seconds 89 and current of 1000 A. 90 Scanning-XRF results are presented here as counts per second (cps), which is the 91 standard output of the models that calculate the intensities of each elemental peak. 92 Arguments have been made for presenting scanning XRF data as ratios of elements 93 [Calvert and Pedersen, 2007] or as log ratios of elements [Weltje and Tjallingii, 2008]. 94 The bulk of the sedimentary Mo (97%) in the Cariaco Basin has been shown to be of 95 marine origin, with comparatively little contribution from a terrigenous or biogenic 96 source [Dean et al., 1999], suggesting that normalization of Mo with an element 97 indicative of terrigenous input (i.e. Al or Ti) is unnecessary. Comparison of plots of Mo 98 (cps) with Mo/Al and ln(Mo/Al) (FS 3) reveals very little variation between the three 99 different methods of reporting downcore variability in ventilation, so for simplicity sake, 100 the Mo record is presented as Mo in cps. 101 102 Wavelet Analysis 5 103 Wavelet analyses were performed using software provided by Grinstead et al. (available 104 at http://www.pol.ac.uk/home/research/waveletcoherence/) for MATLAB. Before 105 analysis, each time series was linearly interpolated at a constant 20-year timestep, with a 106 95% confidence interval set assuming a red noise model. The 20-year timestep very 107 closely approximates the average temporal sampling of the XRF data. 108 109 Supplemental Material References 110 Calvert, S. E., and T. F. Pedersen (2007), Elemental proxies for paleoclimatic and 111 palaeoceaongraphic variability in marine sediments: interpretation and applicaition, in 112 Proxies in late Cenozoic paleoceanography, edited by C. Hillaire-Marcel and A. de 113 Vernal, pp. 567-644, Elsevier, Oxford. 114 Dean, W. E., D. Z. Piper, and L. C. Peterson (1999), Molybdenum accumulation in 115 Cariaco Basin sediment over the past 24 k.y.; a record of water-column anoxia and 116 climate, Geology, 27, 507-510. 117 Deplazes, G., et al. (2013), Links between tropical rainfall and North Atlantic climate 118 during the last glacial period, Nature Geosci, 6(3), 213-217. 119 Imbrie, J., J. D. Hays, D. G. Martinson, A. McIntyre, A. C. Mix, J. J. Morely, N. G. 120 Pisias, W. L. Prell, and N. J. Shackleton (1984), The orbital theory of Pleistocene 121 climate: Support from a revised chronology of the marine δ18O record, in Milankovitch 122 and Climate: Understanding the Response to Astronomical Forcing, edited by A. Berger, 123 D Reidel Pub Co, Higham, MA. 124 Lisiecki, L. E., and M. E. Raymo (2005), A Pliocene-Pleistocene stack of 57 globally 125 distributed benthic δ18O records, Paleoceanography, 20(1), 1-17. 6 126 Paillard, D., L. Labeyrie, and P. Yiou (1996), Macintosh program performs time-series 127 analysis, EOS Transations, 77(379). 128 Peterson, L. C., G. H. Haug, R. W. Murray, K. M. Yarincik, J. W. King, T. J. Bralower, 129 K. Kameo, S. D. Rutherford, and R. B. Pearce (2000), Late Quaternary stratigraphy and 130 sedimentation at Site 1002, Cariaco Basin (Venezuela), Proceedings of the Ocean 131 Drilling Program, Scientific Results, 165, 85-99. 132 Weltje, G. J., and R. Tjallingii (2008), Calibration of XRF core scanners for quantitative 133 geochemical logging of sediment cores: Theory and application, Earth and Planetary 134 Science Letters, 274(3-4), 423-438. 135 Wolff, E. W., J. Chappellaz, T. Blunier, S. O. Rasmussen, and A. Svensson (2010), 136 Millennial-scale variability during the last glacial: The ice core record, Quaternary 137 Science Reviews, 29(21-22), 2828-2838. 138 139 Supplementary Figure Captions 140 Fs01 141 a. Position of the Cariaco Basin (indicated by the yellow star) with respect to summer 142 (Sept) and winter (March) position of the ITCZ (indicated by the dashed white line). b. 143 Location of Cariaco Basin and of cores utilized in this study. The lightest color on the 144 bathymetric map indicates water <100 m deep. Major contributing rivers to terrigenous 145 sedimentation are indicated. 146 147 Fs02 148 The age model for Hole 1002C was made by tuning the ODP Hole 1002C G. ruber δ18O 7 149 record to the Lisiecki-Raymo [2005] stacked benthic δ18O record. Additional age control 150 for the upper 125 kyr of the age model was added by matching the reflectance record 151 from Hole 1002C with the well-dated L* record of MD-2621 [Deplazes et al., 2013]. The 152 age model for MD-2622 was also made by correlating the MD-2622 L* record with the 153 dated MD-2621 L* record. Purple triangles indicate tiepoints used in construction of the 154 Hole 1002C age model. The age depth plot to the right shows that the stratigraphic 155 sequence in the Cariaco Basin is continuous with no hiatuses or disturbed intervals and 156 relatively constant sedimentation rates that average 30-40 cm/ky. 157 158 Fs03 159 Running averages (10 pt smooth) of Mo (cps) in blue, Mo/Al in black, and ln(Mo/Al) in 160 red. Normalization of Mo with Al would provide a record of “excess Mo,” that which is 161 not delivered to the sediment in the terrigenous fraction; however, 97% of the Mo in the 162 Cariaco Basin is hosted in the marine fraction [Dean et al., 1999]. Therefore, 163 normalization does not significantly alter the downcore appearance of Mo variability. 164 Similarly, the log ratio of Mo/Al does not significantly change the downcore appearance 165 of Mo variability. For simplicity sake, the results here are presented as Mo (cps). 166 8