期刊
PHYSICS OF THE EARTH AND PLANETARY INTERIORS
卷 328, 期 -, 页码 -出版社
ELSEVIER
DOI: 10.1016/j.pepi.2022.106864
关键词
Paleomagnetic secular variation; Calabrian ridge excursion; Brunhes; Paleointensity; ODP Leg 172; Excursion
This paper summarizes the paleomagnetic secular variation (PSV) and excursions recorded from sediment measurements in the western North Atlantic Ocean at ODP Sites 1060, 1061, 1062, and 1063. It identifies various features and dates the records using different methods. The records from Sites 1062 and 1063 are found to be the most consistent and high-resolution.
This paper summarizes paleomagnetic secular variation (PSV) and excursions recorded from MIS 9-10 (300-374 ka) shipboard measurements of sediments from the western North Atlantic Ocean at ODP Sites 1060, 1061, 1062, and 1063. We have identified 33 inclination features, 31 declination features, and 12 paleointensity features that are reproducible among the four ODP Sites. We have dated these records based on estimates of Milankovich carbonate cyclicity in Grutzner et al. (2002). We also dated these records by comparison with the PISO-1500 global paleointensity record (Channel et al., 2009). The two methods give comparable age estimates for this time interval.. We have also recovered a 9-m PSV record from u-channel studies of Hole 1062H. This record is almost identical to the shipboard paleomagnetic results from Site 1062. All records show evidence for the Calabrian Ridge Excursion (329 +/- 3 ka); Sites 1062 and 1063 contain the most consistent and high-resolution paleomagnetic records of the excursion. The Calabrian Ridge excursion is associated with a narrow (similar to 12 ky) interval of high angular dispersion and low paleointensity. We have also carried out a statistical study of the PSV records after removing all true excursional directions (Lund, 2018). There is significant PSV directional variability over 104 yr time scales that is common to all four sites. The pattern of angular dispersion variability is bimodal with most time spent with low (similar to 10 degrees) dispersion, with two shorter intervals of high (similar to 25) dispersion. The high-dispersion intervals are associated with low intensity intervals and excursions.
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