Collaborative Research: Ground-based Imager and Magnetometer Network for Auroral STudies (GIMNAST)

美国航天局的THEMIS使命（亚暴期间事件和大尺度相互作用的时间历史）包括支持覆盖北美极光区的扩展地面观测站网络。 每个观测站都配备了一台白光极光成像仪和一台磁力计，几乎覆盖全球范围的极光现象。 由于NASA的使命正在逐步结束，该项目将扩展THEMIS-GBO网络中由美国管理的部分的运行。 THEMIS-GBO系统的加拿大部分将在2012年得到资助，并可选择将其延长/继续到2015年。 该合同将使整个网络在2015年之前不间断运营。 THEMIS-GBO网络的观测与国家科学基金会和加拿大航天局支持的其他观测设施具有很强的协同作用。 在这些其他设施中，有位于扑克坪和雷索卢特湾的高级模块化非相干散射雷达（AMISR），以及位于北方半球的许多超级双极光雷达网（SuperDARN）相干散射雷达。 THEMIS-GBO网络的数据将提供给一般科学界，并将支持关于各种专题的科学研究，包括极光弧的出现和消失、小规模结构在极光弧中的作用、极光现象与大规模电离层对流之间的关系、极冠弧与开放和（或）封闭磁场线的关系、与极光弧相关的电流系统以及与太阳极小期相比太阳极大期磁亚暴的性质。 这些研究课题都与我们对空间气象和空间气象可能对技术系统产生的影响的认识有关。 该项目将为本科生提供直接的研究经验。

NASA's THEMIS mission (Time History of Events and Macroscale Interactions during Substorms) included support for an extended network of Ground-Based Observatories (GBOs) with coverage over the North American auroral regions. Each station is equipped with a white-light auroral imager and a magnetometer providing an almost global-scale coverage of auroral phenomena. This project will extend the operation of the US-managed portion of the THEMIS-GBO network now that the NASA mission is being phased out. The Canadian portion of the THEMIS-GBO system will be funded through 2012 with option to renew/continue it until 2015. This award will enable the uninterrupted operation of the entire network until 2015. The observations made by the THEMIS-GBO network are strongly synergistic with other observational facilities supported by NSF and by the Canadian Space Agency. Among these other facilities are the Advanced Modular Incoherent Scatter Radars (AMISR) located at Poker Flat and Resolute Bay, and the many Super Dual Auroral Radar Network (SuperDARN) coherent scatter radars located in the northern hemisphere. Data from the THEMIS-GBO network will be made available to the general science community and will support scientific research on a wide variety of topics, including the appearance and disappearance of auroral arcs, the role of small-scale structures in auroral arcs, the relationship between auroral phenomena and the large-scale ionospheric convection, the relationship of polar-cap arcs to open and/or closed magnetic field lines, the current systems associated with auroral arcs and the properties of magnetic substorms during solar maximum as compared to solar minimum. These research topics all have relevance to our understanding of space weather and the effects space weather can have on technological systems. The project will provide direct research experience for undergraduate students.