Relative paleointensity estimates from magnetic anisotropy: Proof of concept

Relative paleointensity estimates from magnetic anisotropy: Proof of concept
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根据磁各向异性估计相对古强度:概念证明

DOI:
10.1016/j.epsl.2019.05.003
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发表时间:
2019
影响因子:
5.3
通讯作者:
Ježek
Ježek
中科院分区:
地球科学1区
文献类型:
--
作者:
Gilder;K. Wack;Ježek

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沉积岩的相对古强度数据对于破译地球发电机的工作原理和校正大气宇宙成因放射性核的产生发挥着重要作用,因此了解沉积物如何获得剩余磁化强度并更好地评估相对古强度数据的质量非常重要。我们展示了沉积在受控磁场中的沉积物的实验结果,以观察磁各向异性随施加场强从接近地球值到几乎完全饱和的函数的变化。在整个应用场强度范围内,相对古强度值遵循非常明确的幂律。剩磁织物从低场强时在沉积平面中具有最大各向异性轴的扁圆形演变为在高场强时最大各向异性轴平行于施加场方向的扁长形。磁化率各向异性也随着场强的变化而变化,但其相干性远不如剩磁各向异性。这些实验使用了特征良好的含有单域磁铁矿的天然沉积物,这使得对数据进行数值模拟成为可能。该模型使用一个简单的假设来匹配相对古强度和磁性织物发育的场依赖性,即沉积物中大部分(~80%)的剩磁载流子无法与磁场对齐,而一小部分可以自由对齐。因此,剩磁各向异性有望改进和评估相对古强度估计,并有助于改进沉积物磁记录的理论处理。
Relative paleointensity data from sedimentary rocks play an important role to decipher the workings of the geodynamo and to correct for atmospheric cosmogenic radionucleide production, so it is important to understand how sediments acquire remanent magnetizations and to better assess the quality of relative paleointensity data. We present experimental results from sediments deposited in controlled magnetic fields to observe the changes in magnetic anisotropy as a function of applied field strength going from near Earth-like values to almost full saturation. Relative paleointensity values followed a very well defined power law through the entire range of applied field intensities. Magnetic remanence fabrics evolved from oblate with maximum anisotropy axes in the sedimentary plane at low field strengths to prolate with maximum anisotropy axes parallel to the applied field direction at high fields. Anisotropy of magnetic susceptibility also evolved with field strength, but in a much less coherent manner than anisotropy of magnetic remanence. The experiments used well-characterized, natural sediments containing single domain magnetite, which made it possible to numerically model the data. The model matches the field dependency of both relative paleointensity and magnetic fabric development using a simple assumption that a large proportion (∼80%) of the remanence carriers in the sediments are unable to align with the magnetic field while a small fraction are free to align. Anisotropy of magnetic remanence thus holds promise to improve and assess relative paleointensity estimates and helps improve theoretical treatment of magnetic recording in sediments.
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