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    基于EMD分解的甘孜黄土磁化率记录的西南季风演化周期性

    刘冬雁 李巍然 乔彦松 王玲 彭莎莎

    刘冬雁, 李巍然, 乔彦松, 王玲, 彭莎莎, 2010. 基于EMD分解的甘孜黄土磁化率记录的西南季风演化周期性. 地球科学, 35(4): 533-541. doi: 10.3799/dqkx.2010.069
    引用本文: 刘冬雁, 李巍然, 乔彦松, 王玲, 彭莎莎, 2010. 基于EMD分解的甘孜黄土磁化率记录的西南季风演化周期性. 地球科学, 35(4): 533-541. doi: 10.3799/dqkx.2010.069
    LIU Dong-yan, LI Wei-ran, QIAO Yan-song, WANG Ling, PENG Sha-sha, 2010. The Periodicity of the Southwest Monsoon Revealed by the Magnetic Susceptibility of the Garzê A Loess-Paleosol Sequence Using EMD Method. Earth Science, 35(4): 533-541. doi: 10.3799/dqkx.2010.069
    Citation: LIU Dong-yan, LI Wei-ran, QIAO Yan-song, WANG Ling, PENG Sha-sha, 2010. The Periodicity of the Southwest Monsoon Revealed by the Magnetic Susceptibility of the Garzê A Loess-Paleosol Sequence Using EMD Method. Earth Science, 35(4): 533-541. doi: 10.3799/dqkx.2010.069

    基于EMD分解的甘孜黄土磁化率记录的西南季风演化周期性

    doi: 10.3799/dqkx.2010.069
    基金项目: 

    国家自然科学基金 40472088

    国土资源大调查项目 1212010911072

    详细信息
      作者简介:

      刘冬雁(1967-), 女, 副教授, 主要从事第四纪环境教学与科研.E-mail: dongyanliu67@126.com

    • 中图分类号: P539.3

    The Periodicity of the Southwest Monsoon Revealed by the Magnetic Susceptibility of the Garzê A Loess-Paleosol Sequence Using EMD Method

    • 摘要: 黄土磁化率可用以指示夏季风强度, 并已在中国风尘堆积的古气候演化周期研究中得到较好应用, 但迄今多集中于东南季风区.以青藏高原东南缘甘孜A黄土剖面磁性地层学研究为基础, 对1.16 Ma以来的磁化率记录进行经验模态分解(EMD), 探讨西南季风演化的多时间尺度周期性.结果表明: 偏心率、地轴倾斜、岁差的准周期成分在西南季风区黄土沉积中有明显反映, 指示西南季风的演化受天文因素控制; 出现岁差的拍频周期, 指示印度季风系统具有热带特征; 准200 ka周期是真实存在的, 但其成因机制需要进一步研究; 约400 ka周期波动, 可能对应理论值为准400 ka的偏心率长周期.西南季风演化的主要驱动因素可能是低纬太阳辐射.对于沉积记录的周期性研究来讲, 经验模态分解更切合实际, 它比传统谱分析方法有明显的优势和应用潜力.

       

    • 图  1  甘孜A剖面位置

      Fig.  1.  The location of the Garzê A section

      图  2  甘孜A剖面黄土-古土壤序列及其磁化率和磁性地层

      Fig.  2.  Loess-paleosol sequence and variations in the magnetic susceptibility and paleomagnetic records of the Garzê A section

      图  3  甘孜A剖面磁化率曲线

      Fig.  3.  Susceptibility curve of the Garzê A section

      图  4  甘孜A剖面磁化率指标EMD分解获得的7个模态和1个趋势项

      Fig.  4.  7 modes and a trend decomposed from susceptibility of the Garzê A section using EMD method

      图  5  甘孜A剖面磁化率功率谱(BT法)

      Fig.  5.  Spectral analysis of the magnetic susceptibility variations of the Garzê A section

      图  6  甘孜A剖面磁化率指标EMD分解的IMF1分量(a)与岁差理论值(b)的对比

      Fig.  6.  Susceptibility of the Garzê A section mode of IMF1 decomposed by EMD method (a) compared with orbital-precession (b)

      图  7  甘孜A剖面磁化率指标EMD分解的IMF2分量

      Fig.  7.  Susceptibility of the Garzê A section mode of IMF2 using EMD method

      图  8  甘孜A剖面磁化率指标EMD分解的IMF3分量(a)与偏心率短周期理论值的对比(b)

      Fig.  8.  Susceptibility of the Garzê A section mode of IMF3 decomposed by the EMD method (a) compared with orbital eccentricity (b)

      图  9  甘孜A剖面磁化率指标EMD分解的IMF4分量

      Fig.  9.  Susceptibility of the Garzê A section mode of IMF4 decomposed by EMD method

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    • 收稿日期:  2009-10-22
    • 刊出日期:  2010-07-01

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