日本地球惑星科学連合2018年大会

講演情報

[JJ] 口頭発表

セッション記号 S (固体地球科学) » S-GL 地質学

[S-GL32] 上総層群における下部-中部更新統境界GSSP

2018年5月24日(木) 15:30 〜 17:00 A10 (東京ベイ幕張ホール)

コンビーナ:岡田 誠(茨城大学理学部理学科)、菅沼 悠介(国立極地研究所)、亀尾 浩司(千葉大学理学研究科地球科学、共同)、久保田 好美(国立科学博物館)、座長:羽田 裕貴(茨城大学理工学研究科)、岡田 誠(茨城大学理学部)

16:00 〜 16:15

[SGL32-03] 下部ー中部更新統境界GSSP候補地である千葉複合セクションから得られた松山ーブルン境界の高解像度古地磁気変動記録

*岡田 誠1羽田 裕貴2菅沼 悠介3,4 (1.茨城大学理学部理学科、2.茨城大学理工学研究科、3.国立極地研究所、4.総合研究大学院大学)

キーワード:松山ーブルン境界、地磁気逆転、下部ー中部更新統境界

We report a high-resolution paleomagnetic direction and relative paleointensity records from a continuous marine succession , consisting of 55 meters in thickness, exposed on the Chiba composite section of the Kokumoto Formation, Kazusa Group, Japan. The Chiba composite section is a candidate for the Lower-Middle Pleistocene boundary GSSP. Our records provide detailed behaviors of the virtual geomagnetic poles (VGPs) and relative paleointensity changes during the Matuyama-Brunhes (M-B) polarity transition. The resultant relative paleointensity and VGP records show a significant paleointensity minimum near the M-B boundary, which is accompanied by a clear “polarity switch” like change in terms of the paleomagnetic direction. The relative paleointensity seems to keep in a low level for more than 10 thousand years associated with an unstable normal polarity. A high-resolution oxygen isotope chronology for the Chiba composite section indicates that the M-B boundary is located in the middle of Marine Isotope Stage (MIS) 19 and yields an age of 771.7 ka for the boundary. This age is consistent with those based on the latest astronomically tuned marine and ice core records and with the recalculated age of 770.9 ± 7.3 ka deduced from the U-Pb zircon age of the Byk-E tephra. Moreover, our relative paleointensity record exhibits a consistent variation with other paleointensity records including Be10 derived intensity proxy from deep sea and ice cores. Our paleomagnetic data especially for the relative paleointensity represent one of the most detailed records on this geomagnetic field reversal so far obtained from marine sediments and will therefore be key for understanding the dynamics of the geomagnetic dynamo and for calibrating the geological time scale.