Properties of Meso-scale Polar Cap Structures and their Coupling to Nightside Auroral Dynamics

中尺度极冠结构的特性及其与夜间极光动力学的耦合

• 批准号: 1451911
• 负责人: Yukitoshi Nishimura
• 金额: $ 45.5万
• 依托单位: University of California-Los Angeles
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2015
• 资助国家: 美国
• 起止时间: 2015-09-01 至 2017-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1451911&HistoricalAwards=false
• 关键词: Properties; Meso; scale; Polar; Cap

The coupling of the solar wind with Earth's magnetic field gives rise to a range of disturbance effects in the space environment near Earth. Communications, navigation and energy production and distribution can be significantly affected by this space weather. The ability to forecast disturbances that may impact these technologies hinges upon detailed knowledge and understanding of the connected Sun-Earth system, including complicated coupling processes between the magnetosphere and ionosphere. A particular aspect of the latter is patches and arcs of auroral emissions observed in the polar cap. Some recent studies suggest that these structures, originating on the dayside, can drift across the polar cap and play a role in the creation and dynamics of space weather disturbances in the nightside ionosphere. Determining the precise nature of these polar cap structures and their relation to other dynamic features in the nightside ionosphere and magnetosphere is the main objective of this project. It will be attempted through a comprehensive analysis of simultaneous observations of the relevant phenomena from a variety of sources. The resulting understanding constitutes a critical step towards being able to include this effect in ionospheric space weather specification and forecast models. A graduate student will be trained as part of the research effort. This project aims to determine the properties of polar cap patches and arcs and their statistical association with auroral intensifications (PBIs) and streamers. Airglow 630.0 nm imagers will be used to track polar cap structures and determine the fraction of PBIs that are preceded by polar cap patches, and the fraction of polar cap patches that lead to PBIs. The properties of the polar cap patches/arcs such as size and speed will be determined with radar measurements, and the corresponding lobe measurements (flow, particle, FAC structure) determined with conjugate spacecraft. Specific project goals for the research effort include: (1) Establishing the airglow/arc-PBI connection statistically, (2) Determining the properties of the meso-scale structures in the polar cap, and (3) Establishing the possible magnetospheric counterpart for the ionospheric flow channels.

太阳风与地球磁场的耦合在地球附近的空间环境中产生了一系列的扰动效应。通信、导航、能源生产和分配都可能受到这种空间天气的显著影响。预测可能影响这些技术的干扰的能力取决于对连接的太阳-地球系统的详细知识和理解，包括磁层和电离层之间复杂的耦合过程。后者的一个特殊方面是在极帽中观察到的极光发射斑块和弧。最近的一些研究表明，这些起源于白天的结构可以在极帽中漂移，并在夜侧电离层的空间天气扰动的产生和动态中发挥作用。确定这些极帽结构的精确性质及其与夜侧电离层和磁层中其他动态特征的关系是该项目的主要目标。它将通过综合分析从各种来源同时观察到的有关现象来进行尝试。由此产生的理解是朝着能够将这种影响纳入电离层空间天气规范和预报模式迈出的关键一步。一名研究生将作为研究工作的一部分接受培训。该项目旨在确定极帽斑块和弧的性质及其与极光增强（pbi）和飘带的统计关联。Airglow 630.0 nm成像仪将用于跟踪极帽结构，并确定由极帽斑块引起的pbi的比例，以及导致pbi的极帽斑块的比例。通过雷达测量确定极帽斑块/弧的大小和速度等特性，通过共轭航天器确定相应的波瓣测量（流量、粒子、FAC结构）。具体的研究目标包括：(1)建立气辉/弧- pbi的统计联系；(2)确定极帽中尺度结构的性质；(3)建立电离层流动通道可能的磁层对应体。