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			<titleStmt><title level='a'>Site U1472</title></titleStmt>
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				<publisher>International Ocean Discovery Program</publisher>
				<date>05/04/2017</date>
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					<idno type="par_id">10580042</idno>
					<idno type="doi">10.14379/iodp.proc.359.110.2017</idno>
					<title level='j'>Proceedings of the International Ocean Discovery Program Expedition reports</title>
<idno>2377-3189</idno>
<biblScope unit="volume">359</biblScope>
<biblScope unit="issue">110</biblScope>					

					<author>C Betzler</author><author>GP Eberli</author><author>CA Alvarez_Zarikian</author><author>M Alonso-García</author><author>OM Bialik</author><author>CL Blättler</author><author>JA Guo</author><author>S Haffen</author><author>S Horozal</author><author>M Inoue</author><author>L Jovane</author><author>D Kroon</author><author>L Lanci</author><author>JC Laya</author><author>A Ling_Hui_Mee</author><author>T Lüdmann</author><author>M Nakakuni</author><author>BN Nath</author><author>K Niino</author><author>LM Petruny</author><author>SD Pratiwi</author><author>JJG Reijmer</author><author>J Reolid</author><author>AL Slagle</author><author>CR Sloss</author><author>X Su</author><author>PK Swart</author><author>Yao WrightJD</author><author>Young Z</author>
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			<abstract><ab><![CDATA[]]></ab></abstract>
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<div xmlns="http://www.tei-c.org/ns/1.0"><head>Background and objectives</head><p>Site U1472 (proposed Site MAL-06B) lies at 4&#176;46.2653&#8242;N, 073&#176;4.0111&#8242;E, at a water depth of 379.3 m in the middle of the south-ern transect (Figures <ref type="figure">F1</ref>, <ref type="figure">F2</ref>). It is located 9.2 km east of Site U1470 and 7.6 km west of Site U1471 in the southern branch of the Kardiva Channel, which connects the Inner Sea with the open Indian Ocean. The sediments of the Inner Sea are hemipelagic carbonates consist- 72&#176;45' 73&#176;5 &#176;5&#176;1 0&#176;N 70&#176;E 75&#176;0 &#176;4&#176;30' 5&#176;20' N 73&#176;35' 10 km U1472 Laccadive -Maldives Ridge Goidhoo atoll North Mal&#233; atoll Maalhosmadulu atoll Inner Sea Inner Sea ARI1 Indian Ocean K a rd iv a C h a n n e l K a rd iv a C h a n n e l Site U1472 IODP Proceedings 2 V o l u m e 3 5 9</p><p>ing of a mixture of components exported from the atolls and pelagic components (periplatform ooze). Site U1472 cores will therefore complement the record of the youngest paleoceanographic and sedimentological changes in the Maldives.</p><p>The site location was chosen based on an interpretation of seismic lines that show it lies on the apex of a Miocene-Pliocene shingled drift body that progrades to the east (Figure <ref type="figure">F2</ref>). The distal part of this drift was cored at Site U1471, where drift sequence (DS) DS1 and part of DS2 are of considerable thickness. At Site U1472, DS3-DS10 form the near-horizontal topsets of the prograding clinoforms within the drift. These clinoforms and the offlap pattern are reminiscent of geometries observed in prograding platform sequences <ref type="bibr">(Belopolsky and</ref><ref type="bibr">Droxler, 2004a, 2004b)</ref>. In DS3-DS6, these topsets contain wavy, laterally discontinuous reflections that represent either sand waves or deep-water coral bioherms.</p><p>The objectives for this site were (1) to constrain the ages of the drift depositional sequences; (2) to analyze the cyclostratigraphy of drift deposits, therefore reconstructing changes in the current regime and monsoon cyclicity; and (3) to retrieve the lithology of the wavy seismic facies to confirm their current-controlled deposition.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Operations</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Site U1472</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Hole U1472A</head><p>With limited time available because we needed to depart for Mal&#233; no later than 0200 h on Saturday 28 November 2015, we decided to move to Site U1472 and core one final advanced piston corer (APC) hole as deep as possible with the remaining expedition time. Site U1472 was originally a primary drill site for the expedition, but it was downgraded to alternate status as a result of a higher scientific priority to core at Site U1471.</p><p>An APC/extended core barrel (XCB) bottom-hole assembly (BHA) was made up as the ship moved 4.1 nmi in dynamic position-ing mode to Site U1472. The drill string was run to the seafloor, and Hole U1472A was started at 0415 h. We cut and recovered Cores 1H-34F from 0 to 251.9 mbsf, recovering 233.75 m of core (93%) (Table <ref type="table">T1</ref>; see Figure <ref type="figure">F1</ref> in the Expedition 359 summary chapter <ref type="bibr">[Betzler et al., 2017a]</ref>). None of the cores were oriented. The last core of Expedition 359 arrived on deck at 2015 h. The drill string was pulled up one last time, and all drilling equipment was secured. The seafloor-positioning beacon was released, but it did not come to the surface. Thrusters were raised, and at 0212 h on 28 November, we began the transit to Mal&#233;.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Transit to Mal&#233;</head><p>The transit ended at 0718 h on 28 November 2015, and at 0720 h the pilot came on board. The anchor was ultimately dropped in the Mal&#233; anchorage at 0806 h. As part of the Republic of Maldives drilling clearance, the ship was required to check in at Mal&#233;. The two observers were discharged, and the agent took everyone's passports ashore again to clear out of Maldivian waters. In addition, the Maldivian Minister of Fisheries and Agriculture came onboard for a meeting with the Co-Chief Scientists, who gave him a briefing on the expedition results. Passports were returned, and the pilot came aboard at 1430 h. At 1448 h on 28 November, the anchor was weighed, and at 1512 h, the pilot departed the ship, marking the beginning of the sea transit to Colombo, Sri Lanka.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Transit to Colombo</head><p>The transit to Colombo, Sri Lanka, was quick and uneventful. Shipboard clocks were advanced 30 min at 1400 h on 29 November 2015. Although the pilot was scheduled for 0700 h, it was not until 1013 h that the pilot actually boarded the ship. The ship entered the harbor, and the first line went ashore at the Unity Container Terminal berth at Colombo at 1100 h on 30 November, officially ending Expedition 359. -600 -800 -1000 -1200 -1400 -1600 0 500 1000 2000 m Two-way traveltime (ms) Platform Drift U1470 U1472 U1471 </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Lithostratigraphy</head><p>Site U1472 is the middle site in the southern transect and was drilled through a succession of drift and hemipelagic deposits (see Background and objectives). The site is comparable to the succession drilled at Site U1468 in the northern transect. Sites U1470 and U1471 were drilled to the west and east of this site, respectively. Re-sults from the east-west transect will help reconstruct the characteristics of drift sequences from the proximal to distal parts of a carbonate platform and determine the physical and climatic forcing processes driving the evolution of carbonate drift deposition. The sequence is divided into four lithostratigraphic units based on changes in texture, components, degree of lithification, and color (Figure <ref type="figure">F3</ref>).</p><p>Table T1. Site U1472 core summary. DRF = drilling depth below rig floor, DSF = drilling depth below seafloor, CSF = core depth below seafloor. NA = not applicable. H = advanced piston corer, F = half-length advanced piston corer. Download table in .csv format. Hole U1472A Latitude: 4&#176;46.2653&#8242;N Longitude: 073&#176;04.0111&#8242;E Water depth (m): 379.34 Date started (UTC): 1620 h; 26 November 2015 Date finished (UTC): 1515 h; 27 November 2015 Time on hole (days): 0.95 Seafloor depth DRF (m): 390.5 Rig floor to sea level (m): 11.16 Penetration DSF (m): 251.9 Cored interval (m): 251.9 Recovered length (m): 233.75 Recovery (%): 92 Drilled interval (m): NA Drilled interval (no.): 0 Total cores (no.): 34 APC cores (no.): 23 HLAPC cores (no.): 11 Core Top of cored interval DSF (m) Bottom of cored interval DSF (m) Interval advanced (m) Recovered length (m) Curated length (m) Recovery (%) Top of recovered core CSF-A (m) Bottom of recovered core CSF-A (m) Date (2015) Time UTC (h) 359-U1472A-1H 0.0 5.2 5.2 5.07 5.07 98 0.0 5.07 26 Nov 2H 5.2 14.7 9.5 9.47 9.47 100 5.2 14.67 27 Nov 3H 14.7 24.2 9.5 9.63 9.63 101 14.7 24.33 27 Nov 4H 24.2 33.7 9.5 9.14 9.14 96 24.2 33.34 27 Nov 5H 33.7 43.2 9.5 9.41 9.41 99 33.7 43.11 27 Nov 6H 43.2 52.7 9.5 9.42 9.42 99 43.2 52.62 27 Nov 7H 52.7 62.2 9.5 8.94 8.94 94 52.7 61.64 27 Nov 8H 62.2 71.7 9.5 9.57 9.57 101 62.2 71.77 27 Nov 9H 71.7 81.2 9.5 8.58 8.58 90 71.7 80.28 27 Nov 10H 81.2 90.7 9.5 9.39 9.39 99 81.2 90.59 27 Nov 11H 90.7 100.2 9.5 9.56 9.56 101 90.7 100.26 27 Nov 12H 100.2 109.7 9.5 9.60 9.60 101 100.2 109.80 27 Nov 13H 109.7 119.2 9.5 9.47 9.47 100 109.7 119.17 27 Nov 14H 119.2 128.7 9.5 9.67 9.67 102 119.2 128.87 27 Nov 15H 128.7 138.2 9.5 9.66 9.66 102 128.7 138.36 27 Nov 16H 138.2 147.7 9.5 9.84 9.84 104 138.2 148.04 27 Nov 17H 147.7 157.2 9.5 9.33 9.33 98 147.7 157.03 27 Nov 18H 157.2 166.7 9.5 9.60 9.60 101 157.2 166.80 27 Nov 19H 166.7 176.2 9.5 9.89 9.89 104 166.7 176.59 27 Nov 20H 176.2 185.7 9.5 9.81 9.81 103 176.2 186.01 27 Nov 21H 185.7 195.2 9.5 9.56 9.56 101 185.7 195.26 27 Nov 22H 195.2 198.2 3.0 3.19 3.19 106 195.2 198.39 27 Nov 23H 198.2 200.2 2.0 2.18 2.18 109 198.2 200.38 27 Nov 24F 200.2 204.9 4.7 0.91 0.91 19 200.2 201.11 27 Nov 25F 204.9 209.6 4.7 0.78 0.78 17 204.9 205.68 27 Nov 26F 209.6 214.3 4.7 4.55 4.55 97 209.6 214.15 27 Nov 27F 214.3 219.0 4.7 4.28 4.28 91 214.3 218.58 27 Nov 28F 219.0 223.7 4.7 4.19 4.19 89 219.0 223.19 27 Nov 29F 223.7 228.4 4.7 1.56 1.56 33 223.7 225.26 27 Nov 30F 228.4 233.1 4.7 4.03 4.03 86 228.4 232.43 27 Nov 31F 233.1 237.8 4.7 4.29 4.29 91 233.1 237.39 27 Nov 32F 237.8 242.5 4.7 3.68 3.68 78 237.8 241.48 27 Nov 33F 242.5 247.2 4.7 3.46 3.46 74 242.5 245.96 27 Nov 34F 247.2 251.9 4.7 2.04 2.04 43 247.2 249.24 27 Nov Hole U1472A totals: 251.9 233.75 233.75 Site U1472 IODP Proceedings 4 V o l u m e 3 5 9</p><p>Lithostratigraphic units</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Unit I</head><p>Interval: 359-U1472A-1H-1, 0 cm, to 7H-1, 0 cm Depth: 0-52.70 mbsf Unit I consists of unlithified packstone and grainstone and mudlean fine-to medium-grained grainstone with abundant fairly well preserved planktonic foraminifers (Figure <ref type="figure">F4</ref>) as the major skeletal component. The uppermost 2.6 m is dark medium-grained grayish brown unlithified grainstone that grades downhole to mud-lean unlithified packstone starting at 12.70 mbsf. Within the unlithified packstone, intercalations with a granular-grained floatstone texture occur with intraclasts up to 3 cm in size. These intraclasts occur at <ref type="bibr">4H-1, 14-24 cm (23.34-24.44 mbsf ), and 4H-1, 34-45 cm (24.54-25.65 mbsf )</ref>. Components include abundant planktonic foraminifers and well-preserved benthic foraminifers with common echinoderm spines, pteropods, sponge spicules (Figure <ref type="figure">F4A-F4B</ref>), calcareous nannofossils, whole gastropods and bivalves, and mollusk fragments. Intraclasts, fish teeth, otoliths, Halimeda fragments, pellets, and organic material are present. Some bioclasts have a yellow stain, which indicates reworking. Bioturbation is common to complete in this unit, often producing mottling.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Unit II</head><p>Interval: 359-U1472A-7H-1, 0 cm, to 22H-1, 0 cm Depth: 52.70-195.20 mbsf Unit II is divided into two subunits.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Subunit IIA</head><p>Interval: 359-U1472A-7H-1, 0 cm, to 13H-3, 0 cm Depth: 52.70-112.7 mbsf 1H 2H 3H 4H 5H 6H 7H 8H 9H 10H 11H 12H 13H 14H 15H 16H 17H 18H 19H 20H 21H 22H 23H 24F 25F 26F 27F 28F 29F 30F 31F 32F 33F 34F 250 240 230 220 210 200 190 180 170 160 150 140 130 120 110 100 90 80 70 60 50 40 30 20 10 0 Recovery Core Depth (mbsf) Lithology and texture Mudstone Wackestone Packstone Grainstone Floatstone Rudstone Boundstone Grain size Components Lithification Clay Silt Very fine sand Fine sand Medium sand Coarse sand Granule Gravel Core photo Lith. unit Planktonic foraminifers Pteropods Halimeda Corals Benthic foraminifers Large benthic foraminifers Unlithified Partially lithified Lithified 40.0 20.0 0.0 NGR (cps) I A B III II IV Floatstone Grainstone Packstone Wackestone Mudstone Rudstone Boundstone Figure F4. Components of Unit I. A. Grainstone texture (359-U1472A-1H-3, 76-86 cm). B. 250 &#956;m sieve residue showing relatively pristine large fraction components such as planktonic foraminifers, pteropod fragments, stained lithoclasts, and mollusk fragments (1H-3).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>A A A A A A A A A A A A A A A A A A A A A A A A A A A B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B B</head><p>250 &#181;m cm C. Betzler et al.. Site U1472 IODP Proceedings 5 V o l u m e 3 5 9</p><p>The Unit I/II boundary is marked by a textural change from a grainstone-dominated succession to a packstone-dominated succession. Although the top of Subunit IIA is medium-grained unlithified grainstone, the major part of this unit consists of medium-to coarse-grained light gray to white unlithified mud-lean packstone. An interval with a floatstone texture occurs intercalated in the unlithified grainstone at <ref type="bibr">7H-1, 38-85 cm (53.08-53.55 mbsf)</ref>. Components include abundant planktonic foraminifers; common benthic foraminifers, mollusks, and echinoid fragments; and a few otoliths. Aggregate grains/intraclasts are abundant, and organic matter is present. A smear slide sample taken at 57.03 mbsf contains abundant calcareous nannofossils, aragonite needles, and calcite crystals. Apatite and organic matter are present, and dolomite rhombs are few. Bioclasts are overgrown with calcite.</p><p>Induration increases from Section 8H-6, 0 cm (69.7 mbsf ) downhole, and distinct partially lithified coarser grained intervals dominate the succession from Section 10H-1, 0 cm (81.2 mbsf ), downhole. Smear slide samples taken at 75.28 and 83.6 mbsf show an abundance of calcareous nannofossils and planktonic foraminifers. Aragonite needles are common, and dolomite rhombs, tunicates, and organic matter are present to rare. Most components show calcitic overgrowth.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Subunit IIB</head><p>Interval: 359-U1472A-13H-3, 0 cm, to 22H-1, 0 cm Depth: 112.7-195.20 mbsf A change to a packstone texture and interlayers with a wackestone texture together with an increase in lithification mark the Subunit IIA/IIB boundary. Subunit IIB is medium-to coarsegrained, light brownish gray to pale yellow and white, partially lithified to lithified planktonic foraminifer-rich wackestone and packstone. Components include abundant planktonic foraminifers, common benthic foraminifers and aggregate grains/intraclasts, and rare echinoid spines and shell fragments. Skeletal components have overgrowth, and skeletal assemblages are less diverse than those in Subunit IIA. Smear slide samples taken at 121.9 and 146.84 mbsf show an abundance of calcareous nannofossils, planktonic foraminifers, and calcite crystals. Benthic foraminifers and apatite are common. Tunicates, aragonite needles, and micritized grains are present. Bioclasts are severely overgrown with calcite crystals.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Unit III</head><p>Interval: 359-U1472A-22H-1, 0 cm, to 29F-1, 00 cm Depth: 195.20-223.7 mbsf The Unit II/III boundary is marked by a textural change to a succession dominated by a grainstone texture and the first occurrence of large benthic foraminifers. Unit III consists of partially lithified to lithified light grayish brown to light yellowish brown mediumgrained planktonic foraminifer-rich grainstone and interlayered fine-to medium-grained packstone. Contacts are sharp and represent changes in color and texture. Planktonic foraminifers are abundant. Benthic foraminifers, aggregate grains/intraclasts, and organic matter are common. Large benthic foraminifers are few to present and include Amphistegina and Lepidocyclina. A smear slide sample taken at 216.9 mbsf contains abundant aragonite needles, as well as calcite crystals and micritized grains. Calcareous nannofossils are distinctly absent. Components have calcite overgrowth and are poorly preserved. Fine carbonate crystallites seen in the overlying unit are nearly absent and are replaced by large benthic foraminiferal assemblages typical of neritic environments. Foraminiferal skeletons have overgrowths, masking their original shape and indicating alteration due to diagenesis (Figure <ref type="figure">F5</ref>).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Unit IV</head><p>Interval: 359-U1472A-29F-1, 0 cm, to 34F-CC, 17 cm Depth: 224.22-249.24 mbsf The Unit III/IV boundary is marked by a significant increase in the abundance of benthic foraminifers and in the diversity of skeletal components. Unit IV is characterized by medium-to coarsegrained partially lithified and unlithified planktonic foraminiferrich grainstone and interlayered unlithified medium-grained packstone. Components include abundant planktonic foraminifers, benthic foraminifers, and aggregate grains/intraclasts. Large benthic foraminifers including Amphistegina, Lepidocyclina, and Miogypsina are common. Mollusk fragments, gastropods, lithoclasts, and echinoid fragments are present to common. Coral fragments, Halimeda plates, Chlamys, and red algae also occur at the top of this succession (29F-1, 52-91 cm).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Discussion</head><p>Unit I contains carbonate sand with well-preserved planktonic foraminifers as the dominant skeletal component. It also contains pteropods, otoliths, echinoid fragments, shell fragments, and other components (Figure <ref type="figure">F4</ref>) typical of a hemipelagic sedimentary environment. The facies of Unit I is similar to the top units of all the sequences drilled in this area. The occurrence of yellow-stained bioclasts and the presence of a solitary coral (Core 359-U1472A-4H; Figure <ref type="figure">F6</ref>) and a cold-water coral (Core 6H) indicate some reworking. The light gray to brownish gray color of the sediment may be a consequence of the high content in organic matter and iron in reduced form, in response to bottom water redox conditions. An interpretation of suboxic conditions is supported by higher natural gamma radiation (NGR) (Figure <ref type="figure">F3</ref>). Varying gray-brown color changes associated with a cyclic pattern of lightness (L*) and NGR may indicate cyclic changes in bottom water oxygenation conditions.</p><p>Textural changes and degree of lithification are the primary criteria considered for marking the Unit I/II boundary. Unit I has a grainstone to packstone texture, and Unit II has a packstone to wackestone texture. Unit II has similar skeletal components to those in Unit I, but a distinct difference is the absence of pteropods. NGR values in Unit II are distinctly lower than those in Unit I (Figure <ref type="figure">F3</ref>). The top of Unit II contains large bioclasts and shells (Figure <ref type="figure">F7</ref>), indicating a phase of intensified bottom currents. Although the entire  unit has similar components, Unit II is divided into two subunits on the basis of differences in texture, grain size, and degree of preservation of skeletal components. Subunit IIA has a predominantly uniform packstone texture, indicating relatively stable energy conditions prevalent during deposition. The occurrence of aggregate grains and an increased degree of cementation also document early marine diagenesis. Compared to Subunit IIA, Subunit IIB has variable texture alternating between packstone and wackestone with more coarsegrained intervals and increased lithification. The subunit has abundant calcitic needles (Figure <ref type="figure">F5</ref>), and the calcareous skeletons have overgrowths. The variable texture and grain size are similar to those observed in Unit II at Site U1468 and can be attributed to waxing and waning intervals of monsoon-induced currents/energy conditions at the seafloor and/or changes in sea level <ref type="bibr">(Betzler et al., 2009;</ref><ref type="bibr">L&#252;dmann et al., 2013)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A A</head><p>The transition from packstone to grainstone texture and the grain size change from predominantly medium-to coarse-grained sand define the top of Unit III (Figure <ref type="figure">F3</ref>). The textural, grain size, and biota assemblage changes collectively indicate that this unit represents a shallowing-upward succession, possibly due to sea level fall, and increased energy conditions leading to winnowing conditions.</p><p>Unit IV is marked by a transition to predominantly coarsegrained partially lithified grainstone. Texture, grain size, bioclast components and the inclined contacts of layers with coarse sand (Figure <ref type="figure">F8</ref>) document a high-energy condition typical for the top of the contourite fan drift sequence (e.g., <ref type="bibr">Betzler et al., 2014)</ref>. The occurrence of reef material along with large benthic foraminiferal spe-cies typical of inner to middle neritic environments (see Biostratigraphy) indicates that this succession represents material reworked from shallow-water environments and deposited at Site   </p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>A A A A A A A A A A A A A A A A A A A</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>A A A A A A A</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>A A A A A A A A A A A A</head><p>A A A B B B C C C C C C C C C C C C C C C C C C C C C C C C C D D D D D D D D D D D D D D D D D D D D 2 mm 2 mm cm cm Site U1472 IODP Proceedings 7 V o l u m e 3 5 9</p><p>U1472 by prevalent strong currents. The fining-upward succession (Figure <ref type="figure">F8</ref>) within the unit indicates a reduction in current strength or may represent the sand wave type morphology registered at this depth in the seismic profile. In summary, a 251.9 m hole was drilled at Site U1472, recovering a ~234 m long sequence dating back to the late Miocene (see Biostratigraphy) and evolving from a high-energy, shallow-marine environment (neritic) to a hemipelagic sedimentary system, recording changes in sea level and current regime likely driven by varying monsoonal strength. Hemipelagic components such as planktonic foraminifers are present throughout the sequence, but they are in varying states of preservation as a consequence of diagenesis.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Biostratigraphy</head><p>A ~233.75 m sequence was recovered at Site U1472. Calcareous microfossils are present throughout the sequence, with good preservation in the upper 100 m and poor to very poor preservation below. Several biostratigraphic events were identified, allowing for the construction of a reasonable biostratigraphic model for the site. Calcareous nannofossil biostratigraphy suggests a late Miocene age for the bottom of the sequence. Based on the absence of radiolarians at previous sites, we did not expect to find them at Site U1472, and core catcher samples were not studied for these microfossils.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Age model</head><p>The sequence of recognized events is summarized in Table <ref type="table">T2</ref> and plotted in Figures <ref type="figure">F9</ref> and <ref type="figure">F10</ref>.</p><p>Through the Quaternary and early Pliocene, there is a useful sequence of biostratigraphic events, and a fairly clear age model was established. As at other sites, planktonic foraminifers consistently indicate older ages and therefore indicate lower sedimentation rates than those suggested by calcareous nannofossils. A compromise regression line based on both groups gives a sedimentation rate of ~2.6 cm/ky (Figure <ref type="figure">F10</ref>). This sedimentation rate continues to the bottom of the hole.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Calcareous nannofossils</head><p>Calcareous nannofossils are abundant and well preserved in the first two cores of Hole U1472A (Table <ref type="table">T3</ref>). In subsequent cores, nannofossil preservation deteriorates, becoming moderate to poor, and abundances decrease. Principal marker events (the first occurrence <ref type="bibr">[FO]</ref> of Emiliania huxleyi and the last occurrences [LOs] of Pseudoemiliania lacunosa, Discoaster brouweri, and Discoaster pentaradiatus) were placed in the upper ~100 m through the LO of Sphenolithus abies (3.54 Ma), which occurs between Samples 359-U1472A-9H-CC and 10H-CC (Table <ref type="table">T2</ref>). Below this depth, most samples have only rare nannofossils, and assemblages are dominated by very small (&lt;3 &#956;m) Reticulofenestra and S. abies. Virtually no discoaster specimens were observed below Sample 13H-CC; consequently, the LO of Discoaster quinqueramus, usually one of the most reliable events, could not be placed.</p><p>In Samples 20H-CC to 27H-CC, coccoliths are frequent or common and dominated by small reticulofenestrids (&lt;6 &#956;m), clearly from the small Reticulofenestra interval or above (i.e., &lt;8.8 Ma). Samples 27H-CC to 29H-CC are barren or have only very rare coccoliths. The basal part of the recovered sequence shows assemblages in a few samples (30H-CC, 32H-CC, and 34H-CC) that include a significant proportion of large Reticulofenestra specimens (6-9 &#956;m), suggesting these assemblages are below the small Reticulofenestra event <ref type="bibr">(Young, 1990;</ref><ref type="bibr">Rio et al., 1990)</ref> and are therefore older than 8.8 Ma <ref type="bibr">(Hilgen et al., 2012)</ref>. Hence, the base of the small Reticulofenestra event was placed between Samples 27H-CC and 30H-CC (Table <ref type="table">T2</ref>).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Planktonic foraminifers</head><p>Planktonic foraminifers were examined in Hole U1472A core catcher samples (35 samples). Additionally, the mudline sample was also recovered and examined. Planktonic foraminifers show good preservation from the mudline to Sample 359-U1472A-12H-CC (109.8 mbsf ), where foraminifers start to show calcite overgrowth. Planktonic foraminifers are abundant in all samples except for the bottom six (Samples 29H-CC to 34H-CC), which are characterized by high amounts of large benthic foraminifers.</p><p>Four Pleistocene bioevents were identified in Hole U1472A: the LO of Globigerinoides ruber pink (0.12 Ma) between the Hole U1472A mudline sample and Sample 1H-CC (2.6 mbsf ), the LO of Globorotalia tosaensis (0.61 Ma) between Samples 1H-CC and 2H-CC (9.9 mbsf ), the LO of Globigerinoides fistulosus (1.88 Ma) between Samples 5H-CC and 6H-CC (47.9 mbsf ), and the LO of Table <ref type="table">T2</ref>. Biostratigraphic events, Site U1472. FO = first occurrence, LO = last occurrence. N = nannofossil, PF = planktonic foraminifer. The age of the events is based on the list compiled by <ref type="bibr">Gradstein et al. (2012)</ref>. Ages are based on <ref type="bibr">Gradstein et al. (2012)</ref>. See <ref type="bibr">Raffi et al. (2006)</ref> for a review of nannofossil events and original sources for correlations to magnetostratigraphic timescales. Download table in .csv format. Event Abbreviation Fossil group Age (Ma) Age reference Core, section, interval (cm) last sample above event Core, section, interval (cm) first sample below event Top depth (mbsf ) Bottom depth (mbsf) Midpoint depth (mbsf) 359-U1472A-359-U1472A-LO Globigerinoides ruber pink L G.rp PF 0.12 Thompson et al. (1979) 1H-1, mudline 1H-CC 0.05 5.07 2.6 FO Emiliania huxleyi F E.h N 0.29 Hilgen et al. (2012) 1H-CC 2H-CC 5.07 14.67 9.9 LO Pseudoemiliania lacunosa L P.l N 0.44 Hilgen et al. (2012) 1H-CC 2H-CC 5.07 14.67 9.9 LO Globorotalia tosaensis L G.t PF 0.61 Lourens et al. (2004) 1H-CC 2H-CC 5.07 14.67 9.9 LO Globigerinoides fistulosus L G.f PF 1.88 Lourens et al. (2004) 5H-CC 6H-CC 43.11 52.62 47.9 LO Discoaster brouweri L D.b N 1.93 Hilgen et al. (2012) 5H-CC 6H-CC 43.11 52.62 47.9 LO Discoaster pentaradiatus L D.p N 2.39 Hilgen et al. (2012) 6H-CC 7H-CC 52.62 61.64 57.1 LO Globorotalia limbata L G.l PF 2.39 Lourens et al. (2004) 5H-CC 6H-CC 43.11 52.62 47.9 LO Dentoglobigerina altispira L D.a PF 3.47 Lourens et al. (2004) 7H-CC 8H-CC 61.64 71.77 66.7 LO Sphenolithus abies L S.a N 3.54 Hilgen et al. (2012) 9H-CC 10H-CC 80.28 90.56 85.4 LO Globorotalia margaritae L G.m PF 3.85 Lourens et al. (2004) 8H-CC 9H-CC 71.77 80.28 76.0 LO Globoquadrina dehiscens L G.d PF 5.92 Wade et al. (2011) 14H-CC 15H-CC 128.87 138.36 133.6 Start small Reticulofenestra event S sR N 8.8 Hilgen et al. (2012) 27H-CC 30H-CC 218.58 232.43 225.5 Site U1472 IODP Proceedings 8 V o l u m e 3 5 9 Globorotalia limbata (2.39 Ma) between Samples 5H-CC and 6H-CC (47.9 mbsf ). Within the Pliocene, we identified the LO of Dentoglobigerina altispira (3.47 Ma) between Samples 7H-CC and 8H-CC (66.7 mbsf ), the LO of Globorotalia margaritae (3.85 Ma) between Samples 8H-CC and 9H-CC (76 mbsf), and the LO of Globoquadrina dehiscens (5.92 Ma) between Samples 14H-CC and 15H-CC (133.6 mbsf ) (Tables <ref type="table">T2</ref>, <ref type="table">T4</ref>). Constraints on this event are limited because only a few specimens of G. dehiscens were identified.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Benthic foraminifers</head><p>Eleven core catcher samples were investigated for benthic foraminifers. Pleistocene benthic foraminifers are abundant, and preservation ranges from very good to good (Table <ref type="table">T5</ref>). Pliocene to Pleistocene benthic foraminifers present include Cibicidina walli, Cibicidoides robertsonianus, Bolivina sp. (smooth flat), and Uvigerina proboscidea, indicating a middle neritic to upper bathyal depositional environment. The lithology shows a change in Sample 359-U1472A-15H-CC, where foraminifer-rich sediments partially lithified. Below Sample 20H-CC, the benthic foraminifer assemblage notably changes to one dominated by Amphistegina sp., Discogypsina sp., and fragments of large benthic foraminifers (Lepidocyclina sp.), which points to an inner neritic to middle neritic depositional environment.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Geochemistry</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Interstitial water chemistry</head><p>A total of 25 interstitial water (IW) samples were obtained from Site U1472 by whole-round squeezing. Chloride and alkalinity titrations were performed, but no additional IW analyses were completed because of time constraints. Concentrations of all measured species are given in Table <ref type="table">T6</ref>. Alkalinity concentrations decrease from 3.43 mM at the surface to 2.66 mM at the bottom (239 mbsf ) of Hole U1472A (Figure <ref type="figure">F11</ref>). On the other hand, Cl -concentrations steadily increase from 559 to 573 mM throughout Hole Depth (mbsf) PT1 Pleistocene PL5 M14 NN21 Pliocene PL4-PL3 NN18-NN16 Poor preservation (cemented specimens) continues downhole late Miocene NN19 NN15-NN10B Middle neritic to upper bathyal PL2-PL1 Inner neritic to middle neritic Moderate preservation NN10A-NN9 Planktonic foraminifers Calcareous nannofossils Benthic foraminifers Chrono-stratigraphy 0 20 40 60 80 100 120 140 160 180 200 220 240 U1472A Core Recovery 1H 2H 3H 4H 5H 6H 7H 8H 9 H 10H 11H 12H 13H 14H 15H 16H 17H 18H 19 H 20H 21H 22H 23H 24F 25F 26F 27F 28F 29 F 30F 31F 32F 33F 34F Figure F10. Age-depth plot, Site U1472. Details of each event plotted are given in Table T2. Calcareous nannofossils Planktonic foraminifers Age (Ma) Sed. rate (cm/ky) F E.h L D.b L P.l L D.p L S.a L G.rp L G.f L G.l L D.p S sR L G.d Pleistocene Pliocene late Miocene 2.6 Bottom (~240 mbsf) 0 20 40 60 80 100 120 140 160 180 200 220 240 260 280 0 1 2 3 4 5 6 7 8 9 10 L G.m L G.t Depth (mbsf)</p><p>Table T3. Nannofossil range chart, Hole U1472A. Download table in .csv format. Table T4. Planktonic foraminifer range chart, Hole U1472A. Download table in .csv format. Table T5. Benthic foraminifer range chart, Hole U1472A. Download table in .csv format. Site U1472 IODP Proceedings 9 V o l u m e 3 5 9</p><p>U1472A with some variations. Similar to Cl -, salinity also increases from 35 at the surface to 36 at the bottom. The range of pH is 7.4 to 7.8.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Bulk sediment geochemistry</head></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>X-ray diffraction</head><p>Sedimentary mineralogy was determined by X-ray diffraction (XRD) from squeeze cake samples for a total of 25 samples. In contrast to Sites U1467 and U1471, where aragonite decreases in the upper 100 mbsf, aragonite remains abundant at Site U1472 throughout the sampled interval, constituting 15% to 50% of the sediment (Figure <ref type="figure">F12</ref>; Table <ref type="table">T7</ref>). One sample from 200.2 mbsf is even predominantly composed of aragonite (82.5%). High-Mg calcite (HMC) is present in the uppermost sample only at 2.63 mbsf, and dolomite is present up to 6% in pre-Pleistocene sediments. The remainder of the sediment is composed of low-Mg calcite (LMC).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Volatile hydrocarbons</head><p>Headspace samples for the analysis of methane, ethene, ethane, propene, and propane were obtained from 34 sediment samples at Site U1472. Methane concentrations remain low between 1.51 and 2.59 ppmv (Figure <ref type="figure">F13</ref>; Table <ref type="table">T8</ref>). No heavier hydrocarbons (C 2+ ) were detected at this site.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Discussion</head><p>The slight increase in the concentration of Cl -at Site U1472 is higher than the increase observed at Site U1471 but not as strong as that found at Sites U1466 or U1468. This increases may be a relict signal of Last Glacial Maximum seawater (see Geochemistry in the Site U1467 chapter <ref type="bibr">[Betzler et al., 2017b]</ref>) that has not yet diffused away. The constant alkalinity concentrations with depth indicate negligible rates of bacterial sulfate reduction relative to advection of seawater at Site U1472.</p><p>Neomorphism of aragonite to LMC does not appear to occur with the same intensity as at other Expedition 359 sites. The high abundance of aragonite even at 200 mbsf is unique to this site and might be related to the general lack of modern, active diagenesis inferred from constant pore fluid profiles. We lack data on the concentration of Sr 2+ in IW samples that could indicate if carbonate neomorphism is currently occurring. The constant alkalinity at Site U1472 also suggests that the small amounts of dolomite present in the sediments are the result of previous episodes of alteration and are not actively forming in the modern sediment column. Carbonate diagenesis and dolomitization must have occurred in previous time intervals but unusually do not seem to have resulted in aragonite neomorphism to LMC.</p><p>Table T6. Interstitial water chemistry, Site U1472. Download table in .csv format. Figure F11. IW Cl -, alkalinity, and hydrogen (pH), Site U1472. late Miocene Pliocene Pleist. 500 550 600 0 50 100 150 200 250 Cl -(mM) Depth (mbsf) 0 2 4 Alk (mM) 7 7.5 8 pH I II III Age Lith. unit Figure F12. Relative concentrations of aragonite, HMC, LMC, dolomite, and quartz measured using XRD, Site U1472. 0 50 100 150 200 0 20 40 60 80 100 Depth (mbsf) Mineralogy (%) late Miocene Pliocene Pleistocene I II III Aragonite HMC LMC Dolomite Quartz Age Lith. unit Table T7. XRD results, Site U1472. Download table in .csv format. Figure F13. Methane in head space samples, Site U1472. late Miocene Pliocene Pleistocene 0 1 2 3 4 5 0 50 100 150 200 Methane (ppmv) Depth (mbsf) I II III Lith. unit Age Table T8. Headspace hydrocarbons, Site U1472. Download table in .csv format. Site U1472 IODP Proceedings 10 Volume 359</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Paleomagnetism</head><p>Natural remanent magnetization (NRM) was measured on 23 APC cores and 17 half-length APC (HLAPC) cores from Hole U1472A at 15 cm intervals using the superconducting rock magnetometer. Cores were subjected to stepwise alternating field (AF) demagnetization at 15 and 30 mT. The first and second sections of each core were generally skipped for efficiency and because they were generally affected by drill pipe contamination and thus rendered useless for paleomagnetic purposes (see Paleomagnetism in the Site U1467 chapter <ref type="bibr">[Betzler et al., 2017b]</ref>). Results are summarized in Figure <ref type="figure">F14</ref>. 10 -6 10 -4 10 -2 Intensity (A/m) 120 100 80 60 40 20 0 Depth (mbsf) 360 270 180 90 0 Declination (&#176;) after 30 mT AF demag -90 90 -60 -30 0 30 60 Inclination (&#176;) after 30 mT AF demag Flux jump Flux jump 10 -6 10 -4 10 -2 Intensity (A/m) 240 220 200 180 160 140 Depth (mbsf) 360 270 180 90 0 Declination (&#176;) after 30 mT AF demag -90 90 -60 -30 0 30 60 Inclination (&#176;) after 30 mT AF demag Flux jump Flux jump Magnetization intensity after demagnetization at 30 mT and removing the high-intensity sections is rather low, averaging 2.34 &#215; 10 -5 A/m, and similar to that observed at previous sites in the same condition (same demagnetization steps and removal of high peaks). Occasional "flux jumps" in the y-axis superconducting quantum interference device (SQUID) sensor were observed at about 21, 37, 160, and 173 mbsf. Measurements from this site were not affected by the declination bias observed at previous sites.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Paleomagnetic results</head><p>Nearly vertical and negative inclinations were found in the upper 30 mbsf of Hole U1472A (Figure <ref type="figure">F14</ref>), which could be interpreted as a coring disturbance in these soft and water-trenched sediments. The rest of the inclination record is generally shallower but still shows erratic behavior that is not easily interpretable as a sequence of reversals.</p><p>The declination record, which is not oriented, is also scattered and difficult to interpret. An equal-area projection of the paleomagnetic directions from Hole U1472A shows, in fact, nearly uniformly dispersed directions (Figure <ref type="figure">F15</ref>).</p><p>In principle, geomagnetic reversals can be deduced from nearly antipodal changes in declination and can be occasionally observed in Figure <ref type="figure">F14</ref>; however, the interpretation of these features did not give any reasonable results, suggesting that they are either a strongly incomplete record (i.e., not all reversals are recorded) or simply stochastic fluctuations.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Physical properties</head><p>NGR, magnetic susceptibility (MS; with the magnetic susceptibility loop <ref type="bibr">[MSL]</ref> or WRMSL MS), gamma ray attenuation (GRA) bulk density, and P-wave velocity were measured on whole-round cores from Hole U1472A (0-252 mbsf ). Magnetic susceptibility point (MSP or Section Half Multisensor Logger [SHMSL] MS) and color reflectance were performed on archive-half sections. P-wave velocity measurements were also conducted on working-half sections in the core liner. Porosity and density from moisture and density (MAD), thermal conductivity, and shear strength were not measured at this site. Based on variations of physical properties, especially NGR, three petrophysical (PP) units were distinguished (Figure <ref type="figure">F16</ref>). Unit 1, comprising two subunits, spans from the seafloor to ~124 mbsf. Unit 2 extends from ~124 to ~200 mbsf, and Unit 3 covers ~200 to 251.9 mbsf.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Natural gamma radiation</head><p>Petrophysical Unit 1 NGR values display large-scale fluctuations with some relatively small-scale excursions superimposed (Figure <ref type="figure">F16</ref>). Subunit 1A extends from ~0 to 52 mbsf and shows relatively high values that range from ~10 to 40 counts/s. NGR in the top of Subunit 1B shifts abruptly to lower values (&lt;20 counts/s) at 52 mbsf but increases to 20 to 30 counts/s from 81 to 124 mbsf. Another decrease in NGR marks the top of Unit 2 at 124 mbsf, and variability increases downhole to the base of this unit. In Unit 3, NGR values exhibit relatively small-scale excursions and remain relatively low (&lt;25 counts/s).</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Density</head><p>GRA density measurements on whole-round cores generally increase downhole from ~1.4 to 2.1 g/cm 3 (Figure <ref type="figure">F16</ref>). Unit 1 bulk density tracks NGR and is subdivided into Subunits 1A and 1B based on two increasing trends with depth. In Unit 2, bulk density remains relatively constant with an average of ~1.8 g/cm 3 followed by another increase to 2.1 g/cm 3 in Unit 3.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>P-wave velocity</head><p>P-wave velocities were measured using the P-wave logger (PWL) on the WRMSL. PWL values are usually lower than velocities measured with the P-wave caliper (PWC), most likely due to high water content of the sediments. PWL measurements on wholeround cores roughly increase from ~1600 m/s at the seafloor to 1975 m/s at the bottom of Hole 1472A (Figure <ref type="figure">F16</ref>). In Unit 3, PWC values vary more than in Units 1 and 2. From the seafloor through most of Unit 2 (~190 mbsf ), PWL values increase with a trend similar to that of the PWC values. PWL values in the lower portion of Unit 2 and throughout Unit 3 are offset to low values relative to PWC and display greater variability because of the poor coupling between the core and the core liner.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Color reflectance</head><p>In Unit 1, L* values generally increase downhole from 0 to 124 mbsf (Figure <ref type="figure">F17</ref>). Minor fluctuations on the order of 5-10 m are superimposed on this trend. Variability is reduced in Subunit 1B, reflecting more homogeneous sediment color in the unit. In Units 2 and 3, L* values decrease slightly, showing broader deviation. These two units are separated by an abrupt shift toward higher values at ~200 mbsf, but the base of Unit 3 returns to values encountered in the lower part of Unit 2.</p><p>In Unit 1, a* values show a broad trend of first decreasing and then increasing between 0 and 60 mbsf. Below a sharp decrease at the top of Subunit 1B, values remain stable toward the ba=se of the subunit. In the lower portion of Unit 2 and into Unit 3, a* again displays a broad shift to higher values. b* mostly ranges from approximately -5 to 15 and shows an inverse relationship with a*. N = 1073 C. Betzler et al.. Site U1472 IODP Proceedings 12 Volume 359</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Magnetic susceptibility</head><p>Magnetic susceptibility was measured on whole-round and split cores, recording contamination from the drilling process, probably rust from the drill string. Many of these contaminated values were manually removed from the raw data. However, this process was conservative, and some peaks with relatively high values remain. Most MSL values are very low (-2.5 to 0 IU), as are MSP values (-12 to -5 IU) (Figure <ref type="figure">F17</ref>). MSL and MSP values decrease slightly from the seafloor to the middle of Unit 2 (~150 mbsf), followed by some excursions in the lower portion of Unit 2 and the entire Unit 3. Depth (mbsf) 0 20 40 60 80 100 120 140 160 180 200 220 240 U1472A Core Recovery 1H 2H 3H 4H 5H 6H 7H 8H 9H 10H 11H 12H 13H 14H 15H 16H 17H 18H 19H 20H 21H 22H 23H 24F 25F 26F 27F 28F 29F 30F 31F 32F 33F 34F 0 20 40 60 NGR (cps)</p><p>1.2 1.4 1.6 1.8 2.0 2.2 1000 1500 2000 2500 PWL PWC GRA bulk density (g/cm 3 ) P-wave velocity (m/s) 1A 2 PP unit 3 1B Site U1472 IODP Proceedings 13 Volume 359</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Seismic stratigraphy</head><p>Site U1472 is located on the southern platform-basin transect between Sites U1470 and U1471. The subsurface stratigraphic packaging is comparable to northern transect Site U1468 but comprises an undisturbed succession of all drift sequences (DS1-DS10) (Figure <ref type="figure">F18</ref>). DS3-DS10 have lower sedimentation rates at this site than at basinal Site U1467 <ref type="bibr">(L&#252;dmann et al., 2013)</ref>. Because of time limitations at the end of the expedition, we only drilled about 252 mbsf into DS3.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Time-depth conversion</head><p>Because of time restrictions, neither downhole logging nor a check shot survey was performed at this site. Because of the proximity of Sites U1472 and U1470, we used the check shots from Site U1470 as a reference to adapt the velocity model. Computed interval velocities are shown in Figure <ref type="figure">F19</ref>. Figure <ref type="figure">F20</ref> shows the timedepth conversion, and Table <ref type="table">T9</ref> shows the depths of DS4-DS10.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>Seismic facies and geometries</head><p>DS7-DS10 are well-stratified, medium-to low-amplitude continuous reflections and are interpreted to be sheeted drifts. They pass basinward into elongated mounded separate drifts where they were drilled at Site U1467. DS3-DS6 show different facies and geometry. They are characterized by subparallel reflections of predominantly high amplitude. Toward the base of DS3, the reflections became chaotic and low in amplitude. DS5 and DS6 are sheet-like, whereas DS3 and DS4 have a divergent pattern and thicken basinward. 20 40 60 80 Reflectance L* 0 1 2 3 4 5 Reflectance a* -10 -5 0 5 10 15 Reflectance b* Magnetic susceptibility (IU) Depth (mbsf) 0 20 40 60 80 100 120 140 160 180 200 220 240 U1472A Core Recovery 1H 2H 3H 4H 5H 6H 7H 8H 9H 10H 11H 12H 13H 14H 15H 16H 17H 18H 19H 20H 21H 22H 23H 24F 25F 26F 27F 28F 29F 30F 31F 32F 33F 34F WRMSL SHMSL -15 -10 -5 0 5 1A 2 PP unit 3 Table T9. Drift sequence boundaries, Site U1472. Download table in .csv format. Sequence (bottom) TWT (ms) Depth (mbsf) DS10 38.5 33.5 DS9 63 54 DS8 113 100 DS7 154 135 DS6 193.5 168 DS5 198 176 DS4 256 223</p></div></body>
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