严重地磁暴期间中高纬度站上空宇宙射线的多分形分析

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Solar Physics Pub Date : 2024-10-23 DOI:10.1007/s11207-024-02393-w
Ashutosh Giri, Binod Adhikari, Subodh Dahal, K. S. S. Paula, M. J. A. Bolzan
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引用次数: 0

摘要

本研究探讨了在严重地磁暴期间从两个中纬度中子监测站(纽瓦克(NEWK)和伊尔库茨克 3 号(IRK3))以及两个高纬度监测站(图勒(THUL)和伊努维克(INVK))收集的宇宙射线(CR)计数的多分形特性。通过采用多分形和时间序列分析,我们对 CR 计数变化进行了深入研究,以证明这些方法在分析与天体物理和太阳现象相关的复杂信号方面的有效性。研究结果表明,不同纬度观测站的 CR 计数率呈现出多分形特征,反映了一系列缩放指数,捕捉到系统内不同程度的相关性和可变性。研究结果强调,太阳活动、地磁事件以及与地球磁场的相互作用在决定多分形方面的作用比测量站的地理位置更为重要。此外,研究还表明,地磁事件对 CR 计数值率的多分形特性的影响比测站地理位置的影响更大,突出了太阳风暴和地球磁场对 CR 分布和强度的影响。这项工作强调了多分形分析的价值,它是研究 CR 计数的复杂性质及其对外地和地面因素敏感性的有力工具。
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Multi-fractal Analysis of Cosmic Rays over Mid- and High-Latitude Stations During Severe Geomagnetic Storms

This study explores the multi-fractal properties of cosmic-ray (CR) counts collected from two mid-latitude neutron-monitor stations, Newark (NEWK) and Irkutsk 3 (IRK3), and two high-latitude stations, Thule (THUL) and Inuvik (INVK), during periods of severe geomagnetic storms. By employing multi-fractal along with time-series analysis, we did an in-depth examination of CR count variations to demonstrate the effectiveness of these methods in analyzing complex signals associated with astrophysical and solar phenomena. The findings reveal that CR count rates across stations at different latitudes exhibit multi-fractal characteristics, reflecting a range of scaling exponents that capture varying degrees of correlation and variability within the system. The results underscore that solar activity, geomagnetic events, and interactions with Earth’s magnetic field play a more crucial role in determining multi-fractality than the geographic location of the measurement station. Moreover, the study shows that geomagnetic events exert a stronger influence on the multi-fractal properties of CR count rate than the geographic location of station, underscoring the impact of solar storms and Earth’s magnetic field on the distribution and intensity of CRs. This work emphasizes the value of multi-fractal analysis as a powerful tool for investigating the complex nature of CR counts and its sensitivity to both extraterrestrial and terrestrial factors.

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来源期刊
Solar Physics
Solar Physics 地学天文-天文与天体物理
CiteScore
5.10
自引率
17.90%
发文量
146
审稿时长
1 months
期刊介绍: Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.
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