Geomagnetic Disturbances and Midlatitude Airglow During the 20 December 2015 Magnetospheric Storm

IF 2.6 2区 地球科学 Q2 ASTRONOMY & ASTROPHYSICS
R. A. Marchuk, V. V. Mishin, Yu. V. Penskikh, Yu. Yu. Klibanova, A. V. Mikhalev
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Abstract

We report on the novel features of stormtime, midlatitude PiB/PiC geomagnetic pulsations, ionospheric and field-aligned currents, and oxygen, O1S and O1D, emissions at 557.7 and 630.0 nm, respectively. Those were observed during the main phase of the 20 December 2015 storm with significant variations of the solar wind dynamic pressure, Pd, and interplanetary magnetic field Bz. Intensifications of the shortest period, Т < 10 s, Pi1B pulsations and oxygen emissions marked the substorm onsets. The distinct characteristic of the strong substorm (SME = 2,910 nT) was the presence of bay-like geomagnetic variations with the X and Z components with the opposite signs in the northern and southern sections of the IMAGE chain near 18 MLT. Using the magnetogram inversion technique of our institute, we obtained the MLT-MLAT distribution (map) of equivalent and field aligned currents revealing an additional westward electrojet to the north of the eastward current. We have shown that such a current system provides the observed distribution of geomagnetic variations along the 18 MLT meridian during the 20 December 2015 strong substorm, including at the high-latitude half of the IMAGE chain of stations. These conclusions were clearly validated by our simple current system model. We also revealed a localized geomagnetic event during the SME decrease interval between two substorm activations, when the magnitudes of the H/X geomagnetic component, PiB/PiC pulsations, and oxygen emissions at mid latitudes were more than twice greater than during the strong substorm.

2015年12月20日磁层风暴期间的地磁扰动和中纬度气辉
我们报告了风暴时间,中纬度PiB/PiC地磁脉动,电离层和场向电流,以及氧,O1S和O1D,分别在557.7和630.0 nm发射的新特征。这些是在2015年12月20日风暴的主要阶段观测到的,太阳风动压,Pd和行星际磁场Bz发生了显著变化。最短周期强化,Т <;10 s, Pi1B脉动和氧气释放标志着亚暴的开始。强次暴(SME = 2910 nT)的显著特征是在18mlt附近,在IMAGE链的南北段出现了X和Z分量相反的海湾状地磁变化。利用本研究所的磁图反演技术,我们得到了等效电流和场向电流的MLT-MLAT分布图,揭示了东向电流的北面还有一个额外的西向电喷流。我们已经证明,这样一个电流系统提供了在2015年12月20日强亚暴期间沿18mlt子午线的地磁变化的观测分布,包括在IMAGE站链的高纬度部分。简单的电流系统模型清楚地验证了这些结论。我们还发现,在两次亚暴激活之间的SME减少间隔期间,中纬度地区的H/X地磁分量、PiB/PiC脉动和氧排放的强度比强亚暴期间大两倍以上。
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来源期刊
Journal of Geophysical Research: Space Physics
Journal of Geophysical Research: Space Physics Earth and Planetary Sciences-Geophysics
CiteScore
5.30
自引率
35.70%
发文量
570
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