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“蜂群”卫星高度下南北半球地磁场波动的多重分形特征

Multifractal Characteristics of Geomagnetic Field Fluctuations for the Northern and Southern Hemispheres at Swarm Altitude.

作者信息

Toledo Benjamín, Medina Pablo, Blunier Sylvain, Rogan José, Stepanova Marina, Valdivia Juan Alejandro

机构信息

Departamento de Física, Facultad de Ciencias, Universidad de Chile, Las Palmeras 3425, Ñuñoa, Santiago 8370415, Chile.

Centro para el Desarrollo de la Nanociencia y la Nanotecnología (CEDENNA), Avenida Libertador Bernardo O'Higgins No. 3363, Estación Central, Santiago 8370415, Chile.

出版信息

Entropy (Basel). 2021 Apr 30;23(5):558. doi: 10.3390/e23050558.

DOI:10.3390/e23050558
PMID:33946286
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8146999/
Abstract

This paper explores the spatial variations of the statistical scaling features of low to high latitude geomagnetic field fluctuations at Swarm altitude. The data for this study comes from the vector field magnetometer onboard Swarm A satellite, measured at low resolution (1 Hz) for one year (from 9 March 2016, to 9 March 2017). We estimated the structure-function scaling exponents using the -leaders discrete wavelet multifractal technique, from which we obtained the singularity spectrum related to the magnetic fluctuations in the North-East-Center (NEC) coordinate system. From this estimation, we retain just the maximal fractal subset, associated with the exponent . Here we present thresholding for two levels of the Auroral Electrojet index and almost the whole northern and southern hemispheres, the exponent, the structure-function scaling exponent of order 2, and the multifractal width for the geomagnetic fluctuations. The latter quantifies the relevance of the multifractal property. Sometimes, we found negative values of , suggesting a behavior similar to wave breaking or shocklet-like propagating front. Furthermore, we found some asymmetries in the magnetic field turbulence between the northern and southern hemispheres. These estimations suggest that different turbulent regimes of the geomagnetic field fluctuations exist along the Swarm path.

摘要

本文探讨了在“蜂群”卫星高度上低纬度到高纬度地磁场波动统计标度特征的空间变化。本研究的数据来自“蜂群”A卫星上的矢量场磁力仪,以低分辨率(1赫兹)测量了一年(从2016年3月9日至2017年3月9日)。我们使用 - 领导者离散小波多重分形技术估计了结构函数标度指数,从中获得了与东北 - 中心(NEC)坐标系中磁波动相关的奇异性谱。通过该估计,我们仅保留了与 指数相关的最大分形子集。在此,我们给出了极光电集流指数两个水平以及几乎整个北半球和南半球的阈值、 指数、二阶结构函数标度指数以及地磁场波动的多重分形 宽度。后者量化了多重分形特性的相关性。有时,我们发现 的负值,这表明其行为类似于波破碎或类激波传播前沿。此外,我们发现北半球和南半球之间的磁场湍流存在一些不对称性。这些估计表明,沿着“蜂群”路径存在地磁场波动的不同湍流状态。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/7057e617ecd6/entropy-23-00558-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/ef8cecab8dd8/entropy-23-00558-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/32c03a042191/entropy-23-00558-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/4855b007fa26/entropy-23-00558-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/d60f18f3980d/entropy-23-00558-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/7057e617ecd6/entropy-23-00558-g005.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/ef8cecab8dd8/entropy-23-00558-g001.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/32c03a042191/entropy-23-00558-g002.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/4855b007fa26/entropy-23-00558-g003.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/d60f18f3980d/entropy-23-00558-g004.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/54fa/8146999/7057e617ecd6/entropy-23-00558-g005.jpg

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