Observation of sporadic E layer altitude partially modulated by the Traveling Ionospheric Disturbances at high latitudes over Zhongshan station

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
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Abstract

At Zhongshan (69° S, 76° E) Antarctica we investigate the sporadic E (Es)-layer virtual height modulation, observed by an ionosonde, during the passage of the Medium-Scale Traveling Ionospheric Disturbances (MSTIDs), observed by a SuperDARN radar. Two events were identified, on 04 October 2011 at 07:00 - 12:00 UT and 29 February 2012 at 00:00 - 04:00 UT with periods of 15.0 and 12.0 min, respectively. The magnitude of average height modulation of the Es-layer was 3.7 to 17.1 and 0.5 to 7.3 km, respectively, with the same periods as the MSTIDs. Ray tracing during the events shows that the likely MSTID propagation was up to 300 km in the ionospheric F-region. The computed ion vertical drift velocity using SuperDARN radar and magnetometer data, and Es-layer altitude modulation observed by the ionosonde have moderate to strong positive correlation of 0.71 ± 0.22 and 0.51 ± 0.16, respectively. We show that the MSTIDs polarization electric field, which is mapped down from the F-region along the near-vertical magnetic field, moderately contributes to the modulation of the Es layer altitude via the E×B drift mechanism.
在中山站上空观测到部分受高纬度移动电离层扰动调制的零星 E 层高度
在南极洲中山(南纬 69°,东经 76°),我们调查了电离层虚拟高度调制(由电离层探测仪观测)和中尺度移动电离层扰动(由超级雷达网雷达观测)通过期间的零星情况。确定了两个事件,分别发生在 2011 年 10 月 4 日世界时 07:00 - 12:00 和 2012 年 2 月 29 日世界时 00:00 - 04:00,周期分别为 15.0 分钟和 12.0 分钟。Es层的平均高度调制幅度分别为∼3.7至∼17.1和∼0.5至∼7.3 km,周期与MSTID相同。事件期间的光线跟踪显示,MSTID 在电离层 F 区域的传播可能高达 ∼300 公里。利用 SuperDARN 雷达和磁强计数据计算的离子垂直漂移速度与电离层高度调制观测到的电离层高度调制具有中等到较强的正相关性,分别为 0.71 ± 0.22 和 0.51 ± 0.16。我们的研究表明,MSTIDs极化电场是从F区沿近垂直磁场向下映射的,它通过E×B漂移机制对Es层高度的调制有适度的贡献。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
期刊介绍: The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them. The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions. Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.
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