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相关论文: Statistical properties of geomagnetic measurements…

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Records of Dst, Kp and Sym-H indexes are analyzed looking for evidences of possible precursors for magnetic storms. To accomplish this task the main magnetic storms were located and some periods immediately before storms and some periods…

地球物理 · 物理学 2007-05-23 Vitor H. A. Dias , Jorge O. O. Franco , Andres R. R. Papa

Geomagnetic storms are large-scale disturbances of the Earth's magnetosphere driven by solar wind interactions, posing significant risks to space-based and ground-based infrastructure. The Disturbance Storm Time (Dst) index quantifies…

计算工程、金融与科学 · 计算机科学 2025-04-28 Stefano Markidis , Jonah Ekelund , Luca Pennati , Andong Hu , Ivy Peng

Using the reconstruction of power input to the magnetosphere given in Paper 1 (arXiv:1708.04904), we reconstruct annual means of geomagnetic indices over the past 400 years to within a 1-sigma error of +/-20 pc. In addition, we study the…

地球与行星天体物理 · 物理学 2018-01-09 Mike Lockwood , Mathew J. Owens , Luke A. Barnard , Chris J. Scott , Clare E. Watt , Sarah Bentley

This paper presents an analysis on the distribution of periods between consecutive reversals of the Earth's magnetic field. The analysis includes the randomness of polarities, whether the data corresponding to different periods belong to a…

地球物理 · 物理学 2007-05-23 Cosme F. Ponte-Neto , Andres R. R. Papa

We show that distinctive alterations in scaling parameters of Dst index time series occur as a strong magnetic storm approaches. These alterations reveal a gradual reduction of complexity as the catastrophic event approaches. The increase…

地球物理 · 物理学 2007-05-23 G. Balasis , P. Kapiris , K. Eftaxias

In this paper we show that the simple analysis of the local geomagnetic field behaviour can serve as reliable imminent precursor for regional seismic activity increasing. As the first step the problem was investigated using one- component…

地球物理 · 物理学 2012-12-13 Strachimir Chterev Mavrodiev , Lazo Pekevski

We present geomagnetic storms (GSs) selected from three solar cycles, spanning the years 1995 to 2022. We studied the development of the main phase of storms within disturbance storm time (Dst) amplitudes ranging from Dst =-64 nT to Dst=-…

太阳与恒星天体物理 · 物理学 2024-02-07 Osman M. Ahmed , Badruudin Zaheer Ahmad , Moncef Derouich

Technical analysis is considered the oldest, currently omnipresent, method for financial markets analysis, which uses past prices aiming at the possible short-term forecast of future prices. In the frame of complex systems, methods used to…

数据分析、统计与概率 · 物理学 2021-06-02 Stelios M. Potirakis , Pavlos I. Zitis , Georgios Balasis , Konstantinos Eftaxias

Threshold systems appear to underlie the global behaviour of physical phenomena very unlike at a first look. The usual experimental fingerprint of threshold system grounded phenomena is the presence of power laws. Experimental evidence has…

地球物理 · 物理学 2007-05-23 Andres R. R. Papa , Luiz M. Barreto , Ney A. B. Seixas

Plasma pressure distribution in the inner magnetosphere is one of the key parameters for understanding the main magnetospheric processes including geomagnetic storms and substorms. However, the pressure profiles obtained from in-situ…

空间物理 · 物理学 2009-11-13 M. Stepanova , E. E. Antonova , J. M. Bosqued

Content. Solar flares are often used as precursors of geomagnetic storms. In particular, Howard and Tappin (2005) recently published in A&A a dependence between X-ray class of solar flares and Ap and Dst indexes of geomagnetic storms which…

空间物理 · 物理学 2009-12-02 Yu. I. Yermolaev , M. Yu. Yermolaev

Using the geomagnetic storm of July 15, 2000 as an example, we investigated the dependence of GPS navigation system performance on the nightside at mid-latitudes on the level of geomagnetic disturbance. The investigation was based on the…

地球物理 · 物理学 2007-05-23 E. L. Afraimovich , O. I. Berngardt , O. S. Lesyuta , A. P. Potekhin , B. G. Shpynev

Conditions in the solar wind resulting in magnetic storms on the Earth are a subject of long and intensive investigations. Recently Zhang et al. (2006), published a paper, where they used superposed epoch analyses method to study solar wind…

空间物理 · 物理学 2008-09-06 Yu. I. Yermolaev , M. Yu. Yermolaev , I. G. Lodkina

Geomagnetic storms (GS) occur when solar winds disrupt Earth's magnetosphere. GS can cause severe damages to satellites, power grids, and communication infrastructures. Estimate of direct economic impacts of a large scale GS exceeds $40…

机器学习 · 计算机科学 2024-01-22 Iris Yan

Understanding extreme space weather events is of paramount importance in efforts to protect technological systems in space and on the ground. Particularly in the thermosphere, the subsequent extreme magnetic storms can pose serious threats…

空间物理 · 物理学 2020-07-29 Denny M. Oliveira , Eftyhia Zesta , Hisashi Hayakawa , Ankush Bhaskar

In this paper we present an approach for forecasting the imminent regional seismic activity by using geomagnetic data and Earth tide data. The time periods of seismic activity are the time periods around the Sun-Moon extreme of the diurnal…

The main objective of the study is to determine the probability distributions of the geomagnetic Dst index as a function of the coronal mass ejection (CME) and solar flare parameters for the purpose of establishing a probabilistic forecast…

Forecasting geomagnetic storms is highly important for many space weather applications. In this study we review performance of the geomagnetic storm forecasting service StormFocus during 2011--2016. The service was implemented in 2011 at…

空间物理 · 物理学 2018-02-20 Tatiana Podladchikova , Anatoly Petrukovich , Yuri Yermolaev

Magnetic storms constitute the most remarkable large-scale phenomena of nonlinear magnetospheric dynamics. Studying the dynamical organization of macroscopic variability in terms of geomagnetic activity index data by means of complexity…

In this work 2D Ising systems were used to simulate the reversals of the Earth's magnetic field. Each spin was supposed to be a ring current in the Earth dynamo and the magnetization to be proportional to the field intensity. Given the…

地球物理 · 物理学 2007-05-23 Jorge O. O. Franco , Vitor H. A. Dias , Andres R. R. Papa
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