Data for: New magnetobiostratigraphic results from the Ladinian of the Dolomites and implications for the Triassic geomagnetic polarity timescale

Supplementary Table S1: ChRM components from Rio Nigra and Rio Frommer stratigraphic sections. Data are in core, in situ, and tilt-corrected coordinates. Legend of the header is at the end of the table. Supplementary Table S2: Ages and durations of the chrons of the GPTS. The name of the chrons refers to the name of the magnetozones of origin. The mean polarity reversal rates for Early, Middle and Late Triassic (reversal/Myr) have been obtained through linear regression. Figure S1: Anisotropy of Magnetic Susceptibility carried out on the samples from Rio Nigra and Rio Frommer sections. Figure S2: Detail of the Middle Triassic interval of the GPTS/Age plot showing the error bars of the U-Pb zircon ages from Seceda (Wotzlaw et al., 2018) and Rio Nigra (Mietto et al., 2012).

补充表S1：里奥尼格拉（Rio Nigra）与弗罗姆尔河（Rio Frommer）地层剖面的特征剩磁（ChRM）组分。数据采用岩心、原位及经倾角校正的坐标系。表头图例详见表格末尾。
补充表S2：地磁极性年表（GPTS）各极性带的年龄与持续时长。各极性带名称与其对应起源磁极性带的名称一致。研究通过线性回归计算得到三叠纪早、中、晚三期的平均极性反转速率（反转/百万年）。
补充图S1：针对里奥尼格拉与弗罗姆尔河剖面样品开展的磁化率各向异性测试。
补充图S2：地磁极性年表/年龄图的三叠纪中期区间细节，展示了来自塞塞达（Seceda）（Wotzlaw等，2018）与里奥尼格拉（Mietto等，2012）的U-Pb锆石年龄误差棒。