Responses of the wintertime auroral E-region neutral wind to varying levels of geomagnetic activity

IF 2.6 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Frontiers in Astronomy and Space Sciences Pub Date : 2023-10-23 DOI:10.3389/fspas.2023.1282724
Weijia Zhan, Stephen R. Keappler
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Abstract

Introduction: The auroral E-region is an important interface where forces from the magnetosphere and the lower atmosphere converge and have a significant effect on the vertical structure of the neutral winds. The resulting vertical neutral wind structure has been reported to be associated with altitude-dependent and nonlinear effects from different forces. We conduct a statistical examination of the reactions of wintertime neutral winds to four various degrees of geomagnetic activity, with a focus on the impacts of ion drag. Methods: We derive neutral winds using the PFISR measurements covering 2010–2019 and will give a statistical view of the auroral E-region neutral wind with a focus on the winter nighttime during different disturbed conditions. We investigate the effects of the geomagnetic activity on the neutral winds and the tidal components by dividing the dataset into 4 subsets. Tidal decomposition is conducted by least square fitting of the seasonal median winds to obtain the mean, diurnal amplitude, diurnal phase, semidiurnal amplitude, and semidiurnal phase. Results and discussion: We find that 1) when geomagnetic activity increases, dawn-dusk asymmetry exists in both zonal and meridional winds in the upper E-region with stronger zonal wind in the dusk sector than in the dawn sector and much stronger meridional wind in the dawn sector than in the dusk sector. 2) Tidal decomposition results reveal that geomagnetic activity has more significant effects on the meridional diurnal amplitude than zonal diurnal amplitude while the zonal and meridional semidiurnal amplitudes show similar changes when the geomagnetic activity increases. In addition, the maximum semidiurnal amplitude, particularly in the zonal direction, appears at a higher altitude with larger values as geomagnetic activity increases, indicating an ascending transition altitude for the semidiurnal oscillations. The ascending trend of maximum semidiurnal amplitude appearing at higher altitudes during more disturbed conditions has not been reported before. 3) Zonal wind over 110 km demonstrates increasing ion drag effects in the evening sector and the effects of coupled ion drag and other factors after midnight.
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冬季极光e区中性风对不同地磁活动水平的响应
极光e区是磁层和低层大气力汇聚的重要界面,对中性风的垂直结构有重要影响。据报道,由此产生的垂直中性风结构与不同力的高度依赖和非线性效应有关。我们对冬季中性风对四种不同程度地磁活动的反应进行了统计检查,重点研究了离子阻力的影响。方法:利用2010-2019年的PFISR观测数据推导中性风,并对不同干扰条件下冬季夜间的极光e区中性风进行统计分析。我们将数据集分为4个子集,研究了地磁活动对中性风和潮汐分量的影响。对季节中位风进行最小二乘拟合进行潮汐分解,得到平均、日幅、日相、半日幅和半日相。结果与讨论:1)地磁活动增加时,上e区纬向风和经向风均存在黎明-黄昏不对称性,黄昏扇区纬向风强于黎明扇区,黎明扇区经向风强于黄昏扇区。(2)潮汐分解结果表明,地磁活动对经向日振幅的影响比对纬向日振幅的影响更为显著,而随着地磁活动的增加,纬向和经向半日日振幅的变化趋势相似。此外,随着地磁活动的增加,最大半日振幅,特别是纬向的最大半日振幅出现在更高的高度和更大的值,表明半日振荡的过渡高度上升。在高海拔和高扰动条件下,最大半日日振幅呈上升趋势,以前没有报道过。③110 km以上纬向风在傍晚扇区离子阻力作用增强,午夜后离子阻力等因素的耦合作用增强。
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来源期刊
Frontiers in Astronomy and Space Sciences
Frontiers in Astronomy and Space Sciences ASTRONOMY & ASTROPHYSICS-
CiteScore
3.40
自引率
13.30%
发文量
363
审稿时长
14 weeks
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