Mathematical Analysis of the 08 May 2014 Weak Storm

Since the time scale of weak storms is about half the time scale of intense storms, it is troublesome and important to examine the solar wind parameters/interplanetary magnetic field (IMF) (E, v, P, T, N, and Bz) to evolve and affect to zonal geomagnetic indices (Kp, Dst, AE, and ap). In a severe st...

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Bibliographic Details
Published in:Mathematical problems in engineering 2021, Vol.2021, p.1-12
Main Author: Köklü, Kevser
Format: Article
Language:English
Subjects:
Charged particles
Electric fields
Flow velocity
Geomagnetism
Interplanetary magnetic field
Magnetic fields
Mathematical models
Mathematical problems
Parameters
Plasma
Principles
Software
Solar magnetic field
Solar wind
Storms
Time
Variables
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Summary:Since the time scale of weak storms is about half the time scale of intense storms, it is troublesome and important to examine the solar wind parameters/interplanetary magnetic field (IMF) (E, v, P, T, N, and Bz) to evolve and affect to zonal geomagnetic indices (Kp, Dst, AE, and ap). In a severe storm, which usually has two main phases, solar parameters have enough time to react, but weak storms cannot find this time. They have to yield their reaction in a short time. One can find a weak storm in order to reveal and discuss the consistency of models that have proven themselves in severe and moderate storms in this study. I discuss weak storm (Dst = −46) on May 8, 2014, via solar wind parameters and zonal geomagnetic indices. The goal of the work is to realize the models applicable to the moderate and the strong storms for a weak storm. Hereby, all possible correlations between solar parameters and zonal indices are discussed in depth. I tried to obey the cause-effect relationship while creating mathematical models while not ignoring the physical principles. Therefore, the physical principles govern the study. The results are visualized with tables and graphs for the understanding of the dynamic structure of the storm.
ISSN:1024-123X
1563-5147
DOI:10.1155/2021/9948745