High-resolution palaeomagnetic results of Ethiopian trap series from Lima Limo section: implications for the Oligocene geomagnetic field behaviour and timing of volcanism

被引:6
作者
Ahn, Hyeon-Seon [1 ,2 ,3 ]
Kidane, Tesfaye [4 ]
Otofuji, Yo-ichiro [1 ,5 ]
Yamamoto, Yuhji [3 ]
Ishikawa, Naoto [6 ,7 ]
Yoshimura, Yutaka [8 ]
机构
[1] Kobe Univ, Dept Earth & Planetary Sci, Kobe, Hyogo 6578501, Japan
[2] Korea Inst Geosci & Mineral Resources KIGAM, Geol Div, Geol Res Ctr, Daejeon 34132, South Korea
[3] Kochi Univ, Ctr Adv Marine Core Res, Kochi 7838502, Japan
[4] Univ KwaZulu Natal, Sch Agr Earth & Environm Sci, Westville Campus, Durban, South Africa
[5] Inst GeoHist, Susai 1599, Akaiwa, Okayama 7012503, Japan
[6] Kyoto Univ, Grad Sch Human & Environm Studies, Kyoto 6068501, Japan
[7] Univ Toyama, Fac Sustainable Design, Dept Earth Syst Sci, Toyama 9308555, Japan
[8] Univ Tokyo, Atmosphere & Ocean Res Inst, Kashiwa, Chiba 2778564, Japan
关键词
Africa; Magnetostratigraphy; Palaeomagnetic secular variation; Palaeomagnetism; Large igneous provinces; Volcano/climate interactions;
D O I
10.1093/gji/ggaa557
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
We present high-resolution palaeomagnetic and rock magnetic results from 92 successive volcanic units on a 2 km tall Lima Limo (LL) section of the Oligocene Ethiopian flood basalts (OEFB). A total of 85 well-defined flow-mean characteristic remanent magnetization directions representing seven stable magnetic polarity zones with six transitional/excursional directions were determined. These results indicate the identification of four more polarity reversals than previous palaeomagnctic studies; the resulting magnetostratigraphy has, therefore, more polarity zonation. Comparison of this result with the most recently revised geomagnetic polarity time scale (GPTS, hereafter GPTS2016), by using available radiometric age data, could not find a unique correlation. Instead, it strongly suggests the recording of at least one very brief polarity chron or putative geomagnetic excursion. Our magnetostratigraphic interpretation infers that the relative timing between the OEFB eruptions and the Oi-2 global cooling estimated two possible scenarios: one where the lowermost reverse-polarity (R1) interval for the LL section is correlated to Chron C11r of GPTS2016, same as the interpretations of earlier studies, would make a causal linkage between the OEFB eruptions and the Oi-2 cooling less possible; and, the eruption timing estimated in another scenario correlating the R1 to Chron C12r might preserve the probability of its causal influence in the Oi-2 cooling. The resulting overall mean pole for the LI, section of this study, 78.2 degrees N in latitude and 213.0 degrees E in longitude (A(95) = 3.4 degrees, N= 79), is closer to other co-eval palaeomagnetic poles from different regions and the reference pole of Africa. Our analysis of geomagnetic palaeosecular variation (PSV) shows that, compared to the Plio-Pleistocene, the Early Oligocene has higher degrees of PSV but its slightly weaker latitude dependence.
引用
收藏
页码:311 / 328
页数:18
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