@article{oai:kanazawa-u.repo.nii.ac.jp:00060768,
 author = {臼井, 洋一 and Usui, Yoichi and Saitoh, Masafumi and Tani, Kenichiro and Nishizawa, Manabu and Shibuya, Takazo and Kato, Chie and Okumura, Tomoyo and Kashiwabara, Teruhiko},
 journal = {Physics of the Earth and Planetary Interiors},
 month = {Feb},
 note = {The ca. 3.47 Ga Duffer Formation has been considered to carry one of the oldest paleomagnetic records. Yet, the lack of rock magnetic data limits the interpretation of the nature of the remanence. We conducted a rock magnetic and paleomagnetic investigation on columnar dacite of the Duffer Formation. The main magnetic minerals are phenocrysts of titanomagnetite and magnetite, and secondary hematite in groundmass. Detailed thermal demagnetization revealed more complex natural remanence than previously estimated, consisting of four components with typical unblocking temperature of 200–350, 200–500, 590, and 690 °C. Combined with alternating field demagnetization and rock magnetic data, they are attributed to titanomagnetite, coarse-grained magnetite, fine-grained magnetite, and hematite, respectively. The comparison of unblocking temperature and coercivity suggests that the previously proposed secondary component is carried by fine-grained magnetite as well as hematite, while the putative primary component is carried by coarse-grained magnetite and titanomagnetite. Microscopic observations showed that coarse-grained magnetite and titanomagnetite are primary crystals, although this does not necessarily indicate they preserve primary remanence. The remanence directions of all components revealed higher scatter than the previous studies, suggesting the need for caution in interpretation. The low unblocking temperature of titanomagnetite suggests that if their remanence is truly primary, the rocks must have kept below ~ 250 °C for ~3.47 billion years. © 2020 Elsevier B.V., Embargo Period 24 months, 金沢大学理工研究域地球社会基盤学系},
 title = {Identification of paleomagnetic remanence carriers in ca. 3.47 Ga dacite from the Duffer Formation, the Pilbara Craton},
 volume = {299},
 year = {2020}
}