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Magnetostratigraphy and magnetic parameters of a sedimentary sequence in Punta San Andres, Buenos Aires, Argentina

机译:阿根廷布宜诺斯艾利斯蓬塔圣安德列斯的沉积层序的地磁和地磁参数

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This contribution focuses on polarity changes and magnetic parameters obtained in late Cenozoic sediments exposed on the cliffs in San Andres, Chapadmalal, Buenos Aires province. The sedimentary section studied comprises the Vorohue, San Andres, Miramar and Arroyo Seco Formations. The upper layers of Vorohu6 and the base of San Andres showed records of normal polarity and were attributed to the Gauss Normal Polarity Chron (>2.6 Ma). The main portion of San Andres Formation appears to have been deposited during lower and middle Matuyama Polarity Chron, including the Normal Polarity Subchron Olduvai (1.78-2.02 Ma). Miramar Formation contains polarity changes that should be assigned to Middle Matuyama/Jaramillo (1.05 Ma) and to Jaramillo/Upper Matuyama (0.99 Ma). The upper portion of the Miramar Formation and the lower one of the Arroyo Seco Formation show reverse polarity levels and were assigned to the Upper Matuyama (>0.78 Ma). Finally, the upper part of Arroyo Seco Formation seems to have been deposited during the Brunhes polarity chron (<0.78 Ma). Noticeable differences of magnetic records are obtained when comparing loess and paleosols values with calcic horizons values. LF susceptibility values range between 380 × 10~(-8) m~3/kg and 20 × 10~(-8)m~3/kg, of which the lowest values correspond to the calcic horizons. The outcome confirms previous results in the sense that neither of the existing magnetoclimatological models (wind and pedogenetic models) adequately account for the complexities of the Pampean loess. Clearly, the entrainment of dense magnetic iron oxides minerals was more efficient during stormy, dry (glacial) periods than during humid ones. Weathering and pedogenesis produce the decrease of susceptibility values, among other epigenetic processes. Thus, it follows that the decrease of magnetic values by weathering of parent materials depends on the geographic location of loess deposits.
机译:这一贡献集中于布宜诺斯艾利斯省查帕德马尔勒的圣安德列斯悬崖上暴露的晚新生代沉积物中的极性变化和磁参数。研究的沉积部分包括Vorohue,San Andres,Miramar和Arroyo Seco地层。 Vorohu6的上层和圣安德列斯的基底显示出正极性的记录,并归因于高斯正极性计时(> 2.6 Ma)。圣安德列斯组的主要部分似乎是在Matuyama极性下和中年代相期间沉积的,其中包括Normal Polarity Subchron Olduvai(1.78-2.02 Ma)。美丽华组的极性变化应分配给中部Matuyama / Jaramillo(1.05 Ma)和Jaramillo / Upper Matuyama(0.99 Ma)。 Miramar地层的上部和Arroyo Seco地层的下部显示出相反的极性水平,并被分配给上Matuyama(> 0.78 Ma)。最后,Arroyo Seco地层的上部似乎是在Brunhes极性年代(<0.78 Ma)沉积的。将黄土和古土壤值与钙质层位值进行比较时,会得到明显的磁记录差异。 LF磁化率值在380×10〜(-8)m〜3 / kg到20×10〜(-8)m〜3 / kg的范围内,其中最低值对应于钙质层位。该结果在某种意义上证实了先前的结果,即现有的磁气候模式(风和成岩模式)均不能充分说明潘普斯黄土的复杂性。显然,在暴风雨,干燥(冰川)时期,夹带磁性氧化铁矿物比在潮湿时期更有效。在其他表观遗传过程中,风化和成岩作用降低了磁化率值。因此,可以得出结论,由于母体材料的风化而引起的磁值的下降取决于黄土矿床的地理位置。

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  • 来源
    《Quaternary International》 |2012年第6期|p.91-103|共13页
  • 作者单位

    LEMIT, PALEOMAGNETISM, Comision de Investigaciones Cientificas de la Provincia de Buenos Aires, Calle 52 e/121 y 122, 1900 La Plata, Buenos Aires, Argentina;

    LEMIT, PALEOMAGNETISM, Comision de Investigaciones Cientificas de la Provincia de Buenos Aires, Calle 52 e/121 y 122, 1900 La Plata, Buenos Aires, Argentina;

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