• ISSN 2097-1893
  • CN 10-1855/P
李美, 阎泓竹, 张永仙. DEMETER 卫星离子浓度表征的电离层顶部结构季节变化特征[J]. 地球与行星物理论评, 2024, 55(5): 595-608. DOI: 10.19975/j.dqyxx.2023-059
引用本文: 李美, 阎泓竹, 张永仙. DEMETER 卫星离子浓度表征的电离层顶部结构季节变化特征[J]. 地球与行星物理论评, 2024, 55(5): 595-608. DOI: 10.19975/j.dqyxx.2023-059
Li M, Yan H Z, Zhang Y X. 2024. Inner properties of seasonal topside ionospheric structures determined via DEMETER ion perturbations. Reviews of Geophysics and Planetary Physics, 55(5): 595-608. DOI: 10.19975/j.dqyxx.2023-059
Citation: Li M, Yan H Z, Zhang Y X. 2024. Inner properties of seasonal topside ionospheric structures determined via DEMETER ion perturbations. Reviews of Geophysics and Planetary Physics, 55(5): 595-608. DOI: 10.19975/j.dqyxx.2023-059

DEMETER 卫星离子浓度表征的电离层顶部结构季节变化特征

Inner properties of seasonal topside ionospheric structures determined via DEMETER ion perturbations

  • 摘要: 本文利用DEMETER卫星约6年的在轨观测O+离子浓度数据,控制电离层扰动空间尺度在t=20~300 s条件下,软件自动探测和识别117718个电离层扰动. 去掉发生在Kp≥3的18169个扰动以消除磁暴对电离层的影响. 对剩余的99549个扰动,按季节和发生当地时间进行分组. 便于结果对比,只统计发生在夏季日侧、夏季夜侧、冬季日侧和冬季夜侧的四组电离层扰动. 不同变化幅度和空间尺度扰动的全球分布图显示,冬季赤道电离异常(EIA)发育,表现为磁赤道两侧低的电离层扰动密度,南北半球磁纬15°左右突然增强. 同时,日侧EIA异常主要表现为南北半球两侧边界扰动密度和空间尺度的同时增强,扰动空间尺度甚至超过200 s. 单从空间尺度角度,t=120 s是一个分界点,空间尺度小于这个点的扰动发生在日侧的概率大于夜侧,而大于这个点时,结论相反. 另外,大多数大空间尺度(t>200 s)的电离层扰动发生在日侧,尤其是夏季日侧,可能与强阳光照射引起电离层电离有关. 除了夏季日侧,威德尔海异常(WSA)在其余时段均显示清晰的轮廓. 在夏季日侧,在WSA地区的顶部电离层表现异常平静,没有变化幅度超过50%的正扰动和幅度超过100%的负扰动发生在这个区域. 而在冬季夜侧,绝大多数幅度超过100%的正扰动发生在这个区域.

     

    Abstract: In this investigation, 117718 ionospheric perturbations with a space size t = 20–300 s, but without a limit on amplitude (A), were automatically searched globally via software using ion density data measured by the Detection of Electromagnetic Emissions Transmitted from Earthquake Regions (DEMETER) satellite for approximately six years. After eliminating 18169 perturbations (PERs) that occurred in perturbed time (Kp ≥ 3) in order to avoid the global effects of geomagnetic storms, 99549 PERs were left. These PERs were divided into six groups with respect to local time and season, but only the summer and winter PERs were kept for good comparison. Each group of PERs was distributed on a map in terms of amplitude and space size. The distributions of all groups of plasma PERs showed that the equatorial ionization anomaly (EIA) structure developed well during the winter daytime. This structure is characterized by a low plasma PER density (Np) on both sides of the magnetic equator at low latitudes and a sudden enhancement of Np at a magnetic latitude of 15° at both sides of the magnetic latitudes. At the same time, this daytime anomaly was also clearly presented with a simultaneous enhancement in both Np and space size, even beyond 200 s along its boundary line. From the viewpoint of space size, there is a demarcation point, t = 120 s; the occurrence probabilities of day PERs are always higher than those at night before this point, whereas this result is reversed after this point. Another key point is that large spatial-scale perturbations (t > 200 s) present their major significance during daytime, especially during summer daytime, probably due to ionization under strong sunlight. The WSA (Wedell Sea Anomaly) phenomenon shows a clear configuration at all times except on the summer day. The topside ionosphere remained calm during the day in summer, and no positive PERs with a magnitude of more than 50% or a negative magnitude of more than 100% occurred in this WSA area. In winter nighttime, this WSA structure was characterized by major large positive PERs with a magnitude of more than 100%.

     

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