Collaborative Research: Imaging Auroral Radio Emissions: Multi-technique Investigations Employing Optical, Radar, and Satellite Instruments

合作研究：极光无线电发射成像：采用光学、雷达和卫星仪器的多种技术研究

• 批准号: 0243645
• 负责人: Allan Weatherwax
• 金额: --
• 依托单位: Siena College
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2003
• 资助国家: 美国
• 起止时间: 2003-04-01 至 2009-03-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0243645&HistoricalAwards=false
• 关键词: Collaborative; Research; Imaging; Auroral; Radio

The auroras are characterized not only be a variety of active optical emissions, but by a wide variety of radio emissions as well. The relationship between different optical features and different radio features, however, is poorly understood. Wave phenomena in the auroral regions play an important role in the energy flow between the magnetosphere and the ionosphere. In order to understand the relationships between optical and radio phenomena in the auroral region it is necessary to monitor the region with a variety of instruments. This project will utilize data from optical imaging instruments, radar backscatter from auroral features, and plasma wave, electric field, magnetic field and particle measurements from satellites crossing the auroral regions. Satellites which will be used in the study include the defense department DMSP satellites, NASA's FAST, WIND, POLAR, SAMPEX, and IMAGE satellites, and the European CLUSTER mission. A ground-based radio imaging system will be used to locate the regions producing auroral Medium Frequency (MF) radio emissions. The investigation will also contribute to studies of the timing and location of magnetic substorm onsets. The radio imaging instruments will be deployed at existing facilities in Alaska and Greenland. The data will be made available to all researchers, including those using the Alaska and Greenland facilities. The research project will also be integrated with educational activities being carried out by the three collaborating institutions (Dartmouth College, Siena College, and the Univ. of Alaska). In particular the educational effort at Dartmouth will include a focus toward the Dartmouth Women-in Science-Program (WISP). Students will be involved with both the engineering aspects of the new instrumentation as well as the analysis of the resulting scientific data.

极光的特征不仅是各种主动的光学排放，而且还通过各种无线电排放。 但是，不同的光学特征与不同的无线电特征之间的关系知之甚少。 极光区域的波现象在磁层和电离层之间的能量中起重要作用。 为了了解极光区域的光学现象与无线电现象之间的关系，有必要用各种仪器来监视该区域。 该项目将利用来自光学成像仪器的数据，来自极光特征的雷达反向散射以及等离子体波，电场，磁场，磁场和粒子测量的卫星，这些卫星穿越了极光区域。 该研究中将使用的卫星包括国防部DMSP卫星，NASA的快速，风，极地，Sampex和图像卫星以及欧洲集群任务。 基于地面的无线电成像系统将用于定位产生极光中频率（MF）无线电排放的区域。 该研究还将有助于研究磁性替代的时间和位置。 无线电成像仪器将部署在阿拉斯加和格陵兰的现有设施中。 数据将提供给所有研究人员，包括使用阿拉斯加和格陵兰设施的研究人员。 该研究项目还将与三个合作机构（达特茅斯学院，锡耶纳学院和阿拉斯加大学）进行的教育活动集成。 特别是，达特茅斯（Dartmouth）的教育工作将包括集中于达特茅斯女性科学计划（WISP）的重点。 学生将参与新仪器的工程方面以及对所得科学数据的分析。