Collaborative Research: A New 50 MHz Radar for Meteor and Aeronomical Science

合作研究：用于流星和航空科学的新型 50 MHz 雷达

• 批准号: 0638624
• 负责人: Julio Urbina
• 金额: $ 37.17万
• 依托单位: Pennsylvania State Univ University Park
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2007
• 资助国家: 美国
• 起止时间: 2007-06-01 至 2014-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0638624&HistoricalAwards=false
• 关键词: Collaborative; Research; New; 50; MHz

The investigators will develop a prototype of next generation meteor radars with improved ability for deriving neutral winds, temperatures and individual meteor properties. The data will be used to determine a more accurate characterization of the global meteor flux and its effect on upper atmospheric physics. The radar will be operated at a site in Pennsylvania and will be capable of observing at least two of three primary types of meteor reflection: 1) the commonly used specular meteor trails; 2) the recently understood non-specular trails, which result from plasma instability and turbulence generated field aligned irregularities (FAI); and 3) meteor head-echoes, which are a radar target moving at the speed of the meteoroid. Since the system can detect and resolve in time and space at least two mechanisms, we can study the observation biases introduced by each technique. These biases plague our current characterization of the meteor input function into the upper atmosphere, introducing uncertainties in the estimates of atmospheric parameters. Additionally, the detailed radio signature produced by both head echoes and non-specular trails are far more complex than specular echoes. The system will be designed using the latest digital technology, improving the available data for the study of both meteors, and the dynamics and energetics of themesosphere and lower thermosphere (MLT) atmospheric region. The investigators have built strong domestic and international collaborations that will be crucial in achieving the scientific and educational goals of the program. The research will provide undergraduate and graduate students exposure to a wide variety of fields including aeronomy, meteor science, design and construction of radar systems, radio frequency engineering, and software radar.

研究人员将开发下一代流星雷达的原型，改进获取中性风、温度和单个流星特性的能力。 这些数据将用于更准确地确定全球流星通量及其对高层大气物理学的影响。 该雷达将在宾夕法尼亚州的一个地点运行，并将能够观测三种主要流星反射类型中的至少两种：1）通常使用的镜面流星尾迹; 2）最近了解的非镜面尾迹，这是由等离子体不稳定性和湍流产生的场向不规则性（FAI）造成的;（3）流星头回波，即雷达目标以流星速度运动。 由于该系统可以在时间和空间上检测和解决至少两种机制，因此我们可以研究每种技术引入的观测偏差。 这些偏见困扰我们目前的流星输入功能到高层大气的特性，引入大气参数估计的不确定性。 此外，由头部回波和非镜面反射尾迹产生的详细无线电特征比镜面反射回波复杂得多。 该系统的设计将使用最新的数字技术，改进流星研究以及中层和低热层大气区域动力学和能量学研究的现有数据。 研究人员已经建立了强有力的国内和国际合作，这对实现该计划的科学和教育目标至关重要。 该研究将为本科生和研究生提供广泛的领域，包括高空气象学，流星科学，雷达系统的设计和建造，射频工程和软件雷达。