On the Application Limits of the \({{D}_{{{{V}_{2}}}}}\) Parameter in the Study of Variations of the Ancient Geomagnetic Field

IF 0.9 4区 地球科学 Q4 GEOCHEMISTRY & GEOPHYSICS
D. A. Ushakov, V. E. Pavlov
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引用次数: 0

Abstract—To describe secular geomagnetic variation on geological timescales, statistical models have been widely used in recent decades. Currently, the most popular among these is the TK03 model (Tauxe and Kent, 2004). As other statistical models, TK03 numerically characterizes the amplitude of secular geomagnetic variation and the shape of the distribution of paleomagnetic directions which are thought to directly reflect the directions of the geomagnetic field on the considered interval of geological time. For this purpose, three main parameters are used: the scatter Sb (or S) of the virtual geomagnetic poles, the elongation E of the distribution of paleomagnetic directions, and the elongation direction \({{D}_{{{{V}_{2}}}}}\) of the distribution of paleomagnetic directions. The correct use of these parameters to describe paleosecular variation requires the fulfillment of certain, sometimes rather strict conditions. These conditions for parameters Sb and E were considered in a number of previous publications, while the limits and conditions of application of \({{D}_{{{{V}_{2}}}}}\) have not been studied in detail so far. The results of mathematical modeling presented in this paper allow us to evaluate the stability of the calculated parameter values as a function of sampling latitude, the number of samples used to determine this parameter, the length of the time series from which this parameter is estimated, as well as the inclination shallowing and the degree of averaging if \({{D}_{{{{V}_{2}}}}}\) is estimated from sedimentary rocks. We also consider the extent to which the \({{D}_{{{{V}_{2}}}}}\) parameter can be sensitive to the presence and characteristics of the equatorial dipole component in the total geomagnetic field.

Abstract Image

Abstract Image

论 $${{D}_{{{{V}_{2}}}}}$ 参数在古代地磁场变化研究中的应用极限
摘要--为了描述地质时间尺度上的世俗地磁变化,近几十年来统计模型得到了广泛应用。目前,其中最流行的是 TK03 模型(Tauxe 和 Kent,2004 年)。与其他统计模型一样,TK03 以数值形式描述了地磁世俗变化的幅度和古地磁方向分布的形状,这些被认为直接反映了所考虑的地质时间间隔内的地磁场方向。为此,使用了三个主要参数:虚拟地磁极的散度 Sb(或 S)、古地磁方向分布的伸长率 E 和古地磁方向分布的伸长方向 \({{D}_{{{{V}_{2}}}}}\)。正确使用这些参数来描述古地磁变化需要满足某些条件,有时是相当严格的条件。之前的一些出版物考虑了参数 Sb 和 E 的这些条件,而 \({{D}_{{{{V}_{2}}}}}\) 的应用限制和条件迄今为止尚未得到详细研究。本文介绍的数学建模结果使我们能够评估计算参数值的稳定性,它是采样纬度、用于确定该参数的样本数量、估算该参数的时间序列长度以及从沉积岩中估算 \({{D}_{{{{V}_{2}}}}}\)时的倾斜浅度和平均程度的函数。我们还考虑了 \({{D}_{{{{V}}_{2}}}}}\) 参数对总地磁场中赤道偶极分量的存在和特征的敏感程度。
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来源期刊
Izvestiya, Physics of the Solid Earth
Izvestiya, Physics of the Solid Earth 地学-地球化学与地球物理
CiteScore
1.60
自引率
30.00%
发文量
60
审稿时长
6-12 weeks
期刊介绍: Izvestiya, Physics of the Solid Earth is an international peer reviewed journal that publishes results of original theoretical and experimental research in relevant areas of the physics of the Earth''s interior and applied geophysics. The journal welcomes manuscripts from all countries in the English or Russian language.
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