GEM: Examination of Substorm Trigger and Development Mechanisms Based on Multisatellite Observations in the Near Earth Tail

GEM：基于近地尾部多卫星观测研究亚暴触发和发展机制

• 批准号: 9501546
• 负责人: Shinichi Ohtani
• 金额: $ 19.5万
• 依托单位: Johns Hopkins University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 1995
• 资助国家: 美国
• 起止时间: 1995-09-01 至 1999-08-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9501546&HistoricalAwards=false
• 关键词: GEM; Examination; Substorm; Trigger; Development

In this project the investigators will study tail current disruption during substorms by making use of multisatellite observations. Tail current disruption plays an important role in releasing magnetic energy which has been stored in the near-Earth tail before a substorm onset. Recent observations have shown that tail current disruption initiates in the near-Earth magnetotail and then expands both azimuthally and radially, corresponding to the expansion of substorm activities at the ionosphere. Thus, the spatial expansion of tail current disruption is one of the most essential features associated with substorms. The main objectives of the project are (1) to find the dependence of the spatial developmental of tail current disruption on tail magnetic configurations, and (2) to find magnetic conditions that are necessary for triggering the (local) onsets of tail current disruption. To achieve these objectives the investigators will focus on preonset magnetic conditions . Data to be used include: magnetic field data from geostationary satellites and elliptically orbiting satellites. Magnetic signatures will be interpreted in terms of the tail field configuration and the enhancement in the tail current intensity. This study is the first attempt to statistically examine the mechanisms of the trigger and the spatial development of current disruption in terms of preonset magnetic configurations. The understanding of such mechanisms is one of the main goals of magnetospheric physics. The results of this project will put important constraints on future theoretical and observational studies of substorm physics, and will be useful as an input for more global studies, such as coordinated ground and satellite data analyses and global simulations of magnetospheric substorms.

在这个项目中，研究人员将利用多卫星观测来研究亚暴期间尾流的破坏。 尾流扰乱对于释放亚暴爆发前储存在近地尾部的磁能起着重要作用。 最近的观测表明，尾流扰乱始于近地磁尾，然后在方位角和径向上扩展，对应于电离层亚暴活动的扩展。 因此，尾流扰动的空间扩展是与亚暴相关的最重要特征之一。 该项目的主要目标是（1）找到尾电流干扰的空间发展对尾磁配置的依赖性，以及（2）找到触发尾电流干扰（局部）发生所需的磁性条件。 为了实现这些目标，研究人员将重点关注爆发前的磁条件。 所使用的数据包括：来自地球静止卫星和椭圆轨道卫星的磁场数据。 磁特征将根据尾场配置和尾电流强度的增强来解释。 这项研究是首次尝试从预发作磁配置方面统计检查电流干扰的触发机制和空间发展。 了解此类机制是磁层物理学的主要目标之一。 该项目的结果将对未来亚暴物理的理论和观测研究产生重要约束，并将有助于作为更多全球研究的输入，例如协调地面和卫星数据分析以及磁层亚暴的全球模拟。