首页> 外文期刊>Geological Magazine >Astronomical duration of polarity Chron C31r (Lower Maastrichtian): cyclostratigraphy of ODP Site 762 (Indian Ocean)and the Contessa Highway section (Gubbio, Italy)
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Astronomical duration of polarity Chron C31r (Lower Maastrichtian): cyclostratigraphy of ODP Site 762 (Indian Ocean)and the Contessa Highway section (Gubbio, Italy)

机译:极性Chron C31r(下马斯特里赫特)的天文学持续时间:ODP 762站(印度洋)和Contessa公路段(意大利古比奥)的旋回地层学

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摘要

The duration of polarity Chron C31r is estimated with a cyclostratigraphic approach. Two sites are investigated: ODP Site 762 (Indian Ocean) and the Contessa Highway section (Gubbio, Italy). Cyclostratigraphic analysis is performed on greyscale variations (Site 762) and magnetic susceptibility variations (Contessa section). Both sites reveal an astronomical control of the sedimentation, highlighted by the identification of all the orbital periodicities. Cyclostratigraphic signals are tuned on 405 ka eccentricity cycles extracted from the La04 astronomical solution. In both sites, cycle counting gives an estimate of the duration of polarity Chron C31r of about 2.09 ± 0.03 Ma.
机译:极性Chron C31r的持续时间通过旋回地层法估算。调查了两个地点:ODP 762地点(印度洋)和Contessa公路段(意大利古比奥)。对灰度变化(Site 762)和磁化率变化(Contessa部分)进行了旋回地层分析。这两个站点都揭示了对沉积的天文控制,所有轨道周期的确定都突显了这一点。在从La04天文解中提取的405 ka偏心周期上,对地层地层信号进行了调谐。在两个站点中,循环计数估计的极性Chron C31r的持续时间约为2.09±0.03 Ma。

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