“…Ridge‐parallel abyssal hill patterns are distributed along the trace of this NTO, where several domed highs composed of ultramafic rocks are present, such as the 25°S OCC, Uraniwa Hills, and Phoenix knoll [ Kumagai et al ., ; Morishita et al ., ; Nakamura et al ., ; Sato et al ., ; Okino et al ., ] Between two nodal basins of CIR‐S1 and CIR‐S2, the Yokoniwa Rise occurs with a height of 1700 m from the rift valley floor as shallow dome‐like NTO massif [ Okino et al ., ; Fujii et al ., ]. Sea‐surface magnetic anomalies were identified along the Brunhes/Matuyama boundary in the eastern off‐axis area of CIR‐S1 and S2 far from the Yokoniwa Rise [ Honsho et al ., ; Sato et al ., ; Okino et al ., ]. These results suggest that the Yokoniwa Rise formed during the Brunhes normal chron (<0.78 Ma).…”