Paleomagnetic secular variation for a 21,000-year sediment sequence from Cascade Lake, north-central Brooks Range, Arctic Alaska

Two > 5-m-long sediment cores from Cascade Lake (68.38° N, 154.60° W), Arctic Alaska, were analyzed to quantify their paleomagnetic properties over the past 21,000 years. Alternating-field demagnetization of the natural remanent magnetization, anhysteretic remanent magnetization, isothermal remanent magnetization, and hysteresis experiments reveal a strong, well-defined characteristic remanent magnetization carried by a low coercivity magnetic component that increases up core. Maximum angular deviation values average < 2°, and average inclination values are within 4° of the geocentric axial dipole prediction. Radiometric ages based on 210Pb and 14C were used to correlate the major inclination features of the resulting paleomagnetic secular variation (PSV) record with those of other regional PSV records, including two geomagnetic field models and the longer series from Burial Lake, located 200 km to the west. Following around 6 ka (cal BP), the ages of PSV fluctuations in Cascade Lake begin to diverge from those of the regional records, reaching a maximum offset of about 2000 years at around 4 ka. Several correlated cryptotephra ages from this section (reported in a companion paper by Davies et al., this volume) support the regional PSV-based chronology and indicate that some of the 14C ages at Cascade Lake are variably too old.

On the relationship between paleomagnetic secular variation and excursions – records from MIS 8 - ODP Leg 172

Summary Paleomagnetic secular variation (PSV) and excursion data obtained across MIS 8 (243–300 ka) from the western North Atlantic Ocean—ODP Sites 1060–1063 show composite high-resolution PSV records (both directions and relative paleointensity) developed for each site and inter-compared. Two methods of chronostratigraphy allow us to date these records. First, we used published results that compared the calcium carbonate records of ODP Leg 172 sediments and tuned them with Milankovich cyclicity. We also compared our paleointensity records with the PISO-1500 global paleointensity record that was dated with oxygen isotope stratigraphy. We prefer the PISO-1500 record to date our cores. Two excursions are preserved in our PSV records—Excursions 8α and 9α. Our revised age estimates for both excursions are 8α (236.7–239.8 ka) and 9α (283.7–286.9 ka). We have compared shipboard measurements of the two excursions with u-channel measurements of selected excursion intervals. Excursion 8α is interpreted as a ‘Class II’ excursion (local reversal) with in-phase inclination and declination changes; Excursion 9α is a ‘Class I’ excursion with 90° out-of-phase inclination and declination changes. Averaged directions (after removal of true excursional directions) and relative paleointensity in 3 ka and 9 ka overlapping intervals show significant PSV directional variability over 104 yr time scales that is regionally correlatable among the four sites. A notable pattern of angular dispersion variability involves most time spent with low (∼10°) dispersion, with three shorter intervals of high (∼25°) dispersion. The relative paleointensity variability also shows significant variability over 104 yr time scales with three notable intervals of low paleointensity in all four records and a direct correspondence between the three low paleointensity intervals and the three intervals of high angular dispersion. The two magnetic field excursions occur in two of the three low-paleointensity/high-dispersion intervals. This suggests that the geomagnetic field operates in two states between reversals, one with regular to high paleointensity and low directional variability and one with low paleointensity and significantly higher directional variability and excursions.

Paleomagnetic secular variation records from Holocene sediments of Lake Victoria (0.5°S, 33.3°E)

We have conducted a paleomagnetic study of Holocene sediments from Lake Victoria in order to develop a high-resolution record of paleomagnetic secular variation (PSV). This study has recovered PSV records from two cores (V95-1P and V95-7P) in northern Lake Victoria (0.5°S). The PSV is recorded in fine-grained detrital magnetite/titanomagnetite grains, but the rock magnetic data suggest that significant magnetic mineral dissolution has occurred, which limits our paleomagnetic studies to the uppermost ~5 m of both cores. Detailed alternating field (af) demagnetization of the natural remanence (NRM) shows that a distinctive characteristic remanence (ChRM) is demagnetized from ~10 to 40 mT, which decreases simply toward the origin. The resulting directional PSV records for 1P and 7P are correlatable with 22 distinct inclination features and 19 declination features. Radiocarbon dating of the cores is based on eight radiocarbon dates from core 1P, which can be correlated into core 7P using both the PSV and rock magnetic/environmental measurements. The final PSV time series cover the last 11,000 years with an average sediment accumulation rate of ~40 cm/kyr. The Lake Victoria PSV records can be correlated with new PSV records from Lake Malawi. Comparison of the correlatable PSV feature ages between the two lakes indicates that the PSV records are not significantly different in age, although Lake Victoria PSV ages might average ~100 years younger. We think that the Lake Victoria and Lake Malawi PSV records, together, provide the most accurate, well-dated, and consistent record of Holocene PSV for Africa yet developed.