Quantifying Extreme Values in Geomagnetic Perturbations Using Ground Magnetic Records

Space Weather Pub Date : 2024-07-01 DOI:10.1029/2024sw003991
J. Rodríguez-Zuluaga, J. Gjerloev, S. Ohtani, Y. Zou, B. Anderson
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Abstract

We comprehensively analyzed geomagnetic perturbations using ground magnetic records from over 400 stations spanning four solar cycles, from 1976 to 2023. We assess the perturbations in the three magnetic components separately. Our study covers low, middle, and high magnetic latitudes in the northern magnetic hemisphere, with the primary objective of quantifying extreme values and evaluating their variability on magnetic latitude, local time, and solar cycle phases “minimum, ascending, maximum, and declining.” Our findings reveal spatial patterns to be less discernible as perturbations intensify, with distinct responses at middle and high latitudes. The extreme values, defined as percentiles 0 and 100, were observed to be localized and randomly distributed in local time, especially in the east magnetic component. Additionally, we observed dusk‐dawn asymmetries in the magnitude of perturbations related to the auroral electrojets, indicating complex interactions between the magnetosphere and ionosphere. Furthermore, the results reveal a preference for the most significant extreme values to occur in the declining phase of the solar cycle. These insights deepen our understanding of geomagnetic perturbations and their variability, contributing to space weather forecasting and mitigation strategies.
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利用地面磁场记录量化地磁扰动的极端值
我们利用从 1976 年到 2023 年跨越四个太阳周期的 400 多个站点的地面磁场记录,全面分析了地磁扰动。我们分别评估了三个磁成分的扰动。我们的研究涵盖了北磁半球的低、中、高磁纬度,主要目的是量化极端值,并评估它们在磁纬、当地时间和太阳周期阶段 "最小、上升、最大和衰减 "上的变化。我们的研究结果表明,随着扰动的加剧,空间模式的辨识度降低,中高纬度地区的反应截然不同。我们观察到,极端值(定义为百分位数 0 和 100)在当地时间内是局部和随机分布的,尤其是在东磁分量中。此外,我们还观察到与极光电喷有关的扰动幅度在黄昏和黎明时不对称,这表明磁层和电离层之间存在复杂的相互作用。此外,研究结果表明,最重要的极端值偏好出现在太阳周期的下降阶段。这些见解加深了我们对地磁扰动及其可变性的理解,有助于空间天气预报和减缓战略。
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