Mathematical Simulation of the Atmospheric Electric Field Disturbance during a Geomagnetic Storm on 17 March 2015

IF 1.4 4区 化学 Q4 PHYSICS, ATOMIC, MOLECULAR & CHEMICAL
S. S. Zamay, V. V. Denisenko, M. V. Klimenko, V. V. Klimenko, S. V. Anisimov
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Abstract

It follows from the observational data that variations of the atmospheric electric field occur during geomagnetic storms. In this paper, we present the simulation results of ionospheric electric fields during the main phase of the geomagnetic storm on March 17, 2015, within the framework of a quasi-stationary model of a conductor consisting of the atmosphere and the ionosphere. For this purpose, the satellite data on the global distribution of currents between the magnetosphere and the ionosphere are used to describe the magnetospheric source of the electric field. A variation of the electric potential in the ionosphere leads to a variation of the electric field in the entire atmosphere, including its surface layer. It is important that during a geomagnetic storm, the observatory in which the atmospheric electric field is measured significantly changes its position relative to the direction of the Sun. This leads to significant changes in the ionospheric conductivity above the observatory, which affects both the ionospheric electric field and the atmospheric part of the global electrical circuit (GEC). Therefore, when assessing the effect of a geomagnetic storm on the atmospheric electric field in a particular observatory, it is necessary to take into account the local time when comparing the measurement data with the geomagnetic activity indices. For the storm on March 17–18, 2015, we found that taking into account the variations of the ionospheric electric field when calculating the atmospheric electric field allowed us to reproduce the disturbances of the fair weather electric field observed at the Borok Geophysical Observatory. Based on the simulation results, it is shown that during extremely strong magnetic storms, additional atmospheric electric field variations in some places on the Earth have the same scale as the fair-weather field itself.

Abstract Image

2015 年 3 月 17 日地磁风暴期间大气电场扰动的数学模拟
摘要 根据观测数据,地磁暴期间会出现大气电场变化。本文介绍了 2015 年 3 月 17 日地磁风暴主要阶段期间电离层电场的模拟结果,该模拟是在由大气层和电离层组成的导体准静态模型框架内进行的。为此,利用磁层和电离层之间电流全球分布的卫星数据来描述磁层电场源。电离层电势的变化会导致整个大气层(包括其表层)电场的变化。重要的是,在地磁暴期间,测量大气电场的观测站相对于太阳方向的位置会发生显著变化。这会导致观测站上方的电离层电导率发生重大变化,从而影响电离层电场和全球电路(GEC)的大气部分。因此,在评估地磁暴对特定观测站大气电场的影响时,有必要在将测量数据与地磁活动指数进行比较时考虑当地时间。对于 2015 年 3 月 17-18 日的风暴,我们发现在计算大气电场时考虑电离层电场的变化,可以重现在博洛克地球物理观测站观测到的晴天电场干扰。模拟结果表明,在极强的磁暴期间,地球上某些地方的额外大气电场变化与公平天气电场本身的尺度相同。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Russian Journal of Physical Chemistry B
Russian Journal of Physical Chemistry B 化学-物理:原子、分子和化学物理
CiteScore
2.20
自引率
71.40%
发文量
106
审稿时长
4-8 weeks
期刊介绍: Russian Journal of Physical Chemistry B: Focus on Physics is a journal that publishes studies in the following areas: elementary physical and chemical processes; structure of chemical compounds, reactivity, effect of external field and environment on chemical transformations; molecular dynamics and molecular organization; dynamics and kinetics of photoand radiation-induced processes; mechanism of chemical reactions in gas and condensed phases and at interfaces; chain and thermal processes of ignition, combustion and detonation in gases, two-phase and condensed systems; shock waves; new physical methods of examining chemical reactions; and biological processes in chemical physics.
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