2. Late Quaternary Paleomagnetic Secular Variation and Chronostratigraphy from Odp Sites 1233 and 12341
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Tiedemann, R., Mix, A.C., Richter, C., and Ruddiman, W.F. (Eds.) Proceedings of the Ocean Drilling Program, Scientific Results Volume 202 2. LATE QUATERNARY PALEOMAGNETIC SECULAR VARIATION AND CHRONOSTRATIGRAPHY FROM ODP SITES 1233 AND 12341 Steve P. Lund,2 Joseph Stoner,3 and Frank Lamy4 ABSTRACT During Ocean Drilling Program Leg 202, detailed shipboard paleo- magnetic measurements at Sites 1233 and 1234 identified a reproduc- ible high-resolution record of paleomagnetic secular variation (PSV) at each site. These records also contained evidence for three magnetic 1Lund, S.P., Stoner, J., and Lamy, F., field excursions. This paper summarizes the complete paleomagnetic 2006. Late Quarternary paleomagnetic record from Site 1233 and the paleomagnetic record for the uppermost secular variation and chronostratigraphy from ODP Sites 30 meters from Site 1234. We also establish a detailed PSV correlation 1233 and 1234. In Tiedemann, R., between the two sites, located ~500 km apart. Twenty-seven accelerator Mix, A.C., Richter, C., and Ruddiman, mass spectrometry radiocarbon dates permit us to develop time-depth W.F. (Eds.), Proc. ODP, Sci. Results, 202: plots and detailed PSV time series for the last ~50,000 yr at both sites. College Station, TX (Ocean Drilling Based on our chronostratigraphy, the most recent excursions occur at Program), 1–22. doi:10.2973/ α odp.proc.sr.202.208.2006 ~35,000 cal. yr before present (BP) (Excursion 3 ) and ~41,000 cal. yr BP 2Department of Earth Sciences, (Excursion 3β). The excursions were named for the oxygen isotope University of Southern California, Los stages within which they occur. These two excursions are not signifi- Angeles CA 90089-0740, USA. cantly different in age from the Mono Lake Excursion and Laschamp [email protected] 3 Excursion. A third, older excursion, which has not yet been adequately School of Oceanic and Atmospheric Sciences, Oregon State University, dated, also occurs at Site 1233. Corvallis OR 97331-5503, USA. 4GeoForschungsZentrum, Telegrafenberg, 14473 Potsdam, INTRODUCTION Germany. Our knowledge of detailed geomagnetic field secular variation in the Initial receipt: 4 November 2004 Acceptance: 23 February 2006 Southern Hemisphere is very limited during prehistoric times. A few Web publication: 1 December 2006 Ms 202SR-208 S.P. LUND ET AL. PALEOMAGNETIC SECULAR VARIATION AND CHRONOSTRATIGRAPHY 2 leomagnetic studies have developed reproducible Holocene paleomag- netic secular variation (PSV) records from Australia (Barton and McElhinny, 1981; Constable and McElhinny, 1985), New Zealand (Turner and Lillis, 1994), Argentina (Creer et al., 1983; Gogorza et al., 2000, 2002), and Antarctica (Brachfeld et al., 2000), but there is no re- producible detailed record of PSV from the entire Southern Hemisphere prior to ~18 ka. A gridwork of such records is essential for better under- standing the global space-time pattern of field variability between re- versals. Such a detailed knowledge of space-time field variability is particularly necessary to properly test newer, more realistic dynamo models of field variability (e.g., Kono and Roberts, 2002; Wicht and Ol- son, 2004) and better evaluate the relationship between magnetic field excursions and normal secular variation (e.g., Lund et al., 2001). During Leg 202, we recovered replicate high-resolution PSV records for the last ~70–150 ka from Sites 1233, 1234, and 1235 (Mix, Tiede- mann, Blum, et al., 2003). We present here a summary of the shipboard PSV data from replicate holes at Sites 1233 and 1234 for the last 50,000 yr. The PSV records from both sites contain evidence for two magnetic field excursions that are coeval with the Mono Lake (Benson et al., 2003) and Laschamp (Lund et al., in press) excursions, observed in the Northern Hemisphere. We also correlate the PSV records from Sites 1233 and 1234 and note their strong similarity even though they are lo- cated ~500 km apart. Finally, we integrate 27 radiocarbon dates recov- ered from Site 1233 to develop a revised chronostratigraphy at Sites 1233 and 1234 for the last 50,000 yr. PALEOMAGNETIC METHODS Shipboard paleomagnetic measurements were made on all cores re- covered during Leg 202. Individual cores, normally ~9.5 m in length, were cut into 1.5-m sections and split in half; each archive half was measured at 5-cm intervals on the shipboard 2-G Enterprises cryogenic magnetometer (Mix, Tiedemann, Blum, et al., 2003). The natural rema- nent magnetization (NRM) of each core segment was initially measured and then alternating-field (AF) demagnetization at one or two steps up to 25 mT was applied; the NRM was remeasured after each AF demagne- tization step. Individual core segments were not demagnetized at higher AF because the archive halves were to be further sampled for more detailed paleomagnetic studies after the completion of Leg 202. The limited shipboard AF demagnetization up to 25 mT, however, did a good job of removing a strong but soft viscous overprint that is often noted in cores collected during Ocean Drilling Program (ODP) legs (Mix, Tiedemann, Blum, et al., 2003; Lund et al., 2003). More detailed paleomagnetic measurements have been made in three selected 1.5-m intervals using U-channels that were collected from the centers of ar- chive core halves. These results, reported in a companion article (Lund et al., this volume), corroborate the shipboard paleomagnetic measure- ments presented here. All holes at each site have been correlated based on a variety of ship- board stratigraphic measurements and normalized to a common depth scale (meters composite depth [mcd]) for comparison (Mix, Tiedemann, Blum, et al., 2003). A composite splice section has been chosen from the replicate holes that best represents the observed variability at each site. These independent correlations were used to reconstruct the decli- nation record at each site. The declination records have been modified S.P. LUND ET AL. PALEOMAGNETIC SECULAR VARIATION AND CHRONOSTRATIGRAPHY 3 by first rotating the average declination for each core to 0° and then F1. Site 1233 PSV records, 0–30 slightly varying each core’s average declination to best match the decli- mcd, p. 11. A Composite PSV splice Hole 1233A Hole 1233B Hole 1233C Hole 1233D Hole 1233E nation trends between adjacent cores from each hole based on the ob- -80° -60° -60° -60° -60° -60° -60° -40° -20° 0 I1 260 I2 I3 1,180 I4 1,980 I5 3,820 5 I6 I7 5,040 I8 served declination variability in the other holes using the splice I9 5,590 I10 7,090 I11 10 8,780 I12 I13 I14 10,040 correlations. I16 I15 15 I18 I17 I19 12,260 I20 I21 20 I22 Sediment depth (mcd) 13,620 I23 I23 ‘ I24 I25 25 I26 17,240 I27 19,680 I28 Cal. yr BP 30 RESULTS B Composite PSV splice Hole 1233B Hole 1233C Hole 1233D Hole 1233E -20°0° 20° 0° 20° 0° 20° 0° 20° 0° 20° 0 260 D2 D1 D3 1,180 D4 1,980 D5 3,820 5 D6 D7 5,040 D8 5,590 D9 D10 7,090 10 8,780 Site 1233 Paleomagnetic Secular Variation Records D11 10,040 15 D12 D13 D14 12,260 D15 D16 20 Sediment depth (mcd) 13,620 D17 D17 ‘ D18 The AF demagnetized paleomagnetic directional records from Holes D19 25 D20 17,240 D21 D22 19,680 D23 Cal. yr BP D24 1233A–1233E (41.0°S, 74.45°W; 838 m water depth) are displayed in 30 D25 Figures F1, F2, F3, F4, and F5. The solid lines represent a seven-point running average of the directional data. Selected inclination (I1–I106) F2. Site 1233 PSV records, 30–60 and declination features (D1–D111) are noted based on their appear- mcd, p. 12. ance in records from multiple holes. Normally, directional features were A Composite PSV splice Hole 1233B Hole 1233C Hole 1233D Hole 1233E -80°-60° -60° -60° -60° -60° -40° 30 I29 I30 ( I31 ) 21,480 replicated in at least three holes, but selected features (in parentheses) ( I32 ) 35 I33 22,510 I34 I35 40 23,860 were only replicated in two holes. The boundaries between successive I36 I37 I38 26,050 I39 45 cores are evident in Figures F1, F2, F3, F4, and F5 as gaps in the direc- I39 ‘ 28,830 I40 29,510 I41 Sediment depth (mcd) 50 ( I42 ) 29,780 ( I43 ) tional records. The paleomagnetic directional record from the splice is ( I44 ) ( I44 ‘) 55 I45 I46 32,340 I47 I48 I49 36,360 I50 Cal. yr BP shown at the left in Figures F1, F2, F3, F4, and F5. The splice directional 60 B Composite PSV splice Hole 1233B Hole 1233C Hole 1233D Hole 1233E -20° 0° 20° 0°20° 0° 20° 0° 20° 0° 20° 40° 60° 80° 30 record represents our best composite record of the PSV recorded at Site D26 D27 21,480 35 D28 D29 22,510 1233, based on shipboard measurements. D30 40 D31 23,860 D32 D33 ° ° 26,050 B B D34 The inclinations at Site 1233 typically vary from 70 to 30 with an 45 D35 D35 ‘ 28,830 D36 29,510 D37 ° ° Sediment depth (mcd) 50 B D38 29,780 average near 55 . The observed average inclination is ~5 less than the Interval of D39 more uncertain D40 correlations 55 D41 32,340 D41 ‘ ° D42 expected axial-dipole inclination for the site latitude and ~10 less than D43 Excursion 3α 36,360 D44 Cal. yr BP 60 the average inclination expected for this site based on long-term lati- tude-dependent nondipole effects (ΔI anomaly) (e.g., Lund, 1993; Mer- rill et al., 1996). The slightly lower than expected inclinations are F3. Site 1233 PSV records, 60–90 probably a result of the presence of some residual viscous overprint mcd, p.