首页> 外文会议>2013 US National Committee of URSI National Radio Science Meeting >A meteor wind radar measurement campaign using the Colorado Software Defined Radar with meteor trial echoes interpreted under a modern diffusion theory
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A meteor wind radar measurement campaign using the Colorado Software Defined Radar with meteor trial echoes interpreted under a modern diffusion theory

机译:使用科罗拉多软件定义的雷达进行流星风雷达测量活动,并根据现代扩散理论解释流星试验回波

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This talk presents various interesting characteristics within data collected during a recent campaign using the Colorado Software Define Radar (CoSRad) system. First, a brief system description illustrates how CoSRad is configured for interferometric meteor wind radar mode, where nearly all echoes originate from specular meteor trails. A schematic showing the primary CoSRad hardware setup provides context in interpreting the continuously-recorded data in RTI format. A visualization depicting CoSRad's all-sky specular echo detection strategy prepares us to examine a number of echoes observed during a recent campaign at Platteville, CO (Aug 20 – Sep 1). After a brief look at the canonical meteor trail echo, a number of ostensibly geophysical non-meteoric echoes are presented. In addition to their scientific interest, these echoes convey CoSRad's system capabilities. We first investigate non-specular echo occurrence rates as a function of k-vector geometry with respect to the earth's magnetic field (Oppenheim et. al. 2000, Close et. all. 2000). Next, specular trail echoes are interpreted with respect to Dimant and Oppenheim's (2006) theory predicting depletions in the background plasma surrounding meteor trails. Unlike earlier theories of meteor trail evolution, Dimant and Oppenheim consider the trail's interaction with the existing background ionosphere plasma. Their theory predicts that background plasma is drawn into the trail edges resulting in an electron depletion region around the trail. A number of echoes are presented containing a clear electron depletion region around the trail echo's perimeter. Instrumental effects are discussed and shown to be independent of the observed depletion regions. Finally, we show the depletion phenomenon's correlation with height and time of day. The talk concludes with how the CoSRad architecture has enable these measurements, and touches on how rapid and reconfigurable deployment enables CoSRad to perform similar- measurement campaigns using many existing systems around the world.
机译:该演讲介绍了在最近的一次活动中使用Colorado Software Define Radar(CoSRad)系统收集的数据中的各种有趣特征。首先,简要的系统描述说明了如何将CoSRad配置为干涉式流星风雷达模式,其中几乎所有回波都来自镜面流星轨迹。显示主要CoSRad硬件设置的示意图为解释RTI格式的连续记录数据提供了上下文。描绘CoSRad的全天候镜面反射检测策略的可视化图像使我们能够检查在最近一次科罗拉多州普拉特维尔运动(8月20日至9月1日)期间观察到的大量反射。在简要浏览了典型的流星迹回波之后,提出了许多表面上非地球物理的回波。这些回声除了具有科学意义外,还传达了CoSRad的系统功能。我们首先研究相对于地球磁场,非镜面回波的发生率与k矢量几何的关系(Oppenheim等,2000; Close等,全部2000)。接下来,根据Dimant和Oppenheim(2006)的理论解释了镜面反射回波,该理论预测了流星沿周围的背景等离子体中的损耗。与早期的流星轨迹演化理论不同,Dimant和Oppenheim认为该流星与现有背景电离层等离子体的相互作用。他们的理论预测,背景等离子体被拖入尾迹边缘,从而在尾迹周围形成电子耗尽区。呈现了许多回波,在回波的周界周围包含一个清晰的电子耗尽区。讨论并显示出仪器效果与观察到的耗尽区无关。最后,我们显示了损耗现象与一天中的身高和时间的关系。演讲以CoSRad架构如何实现这些测量为结束,并谈到了快速和可重新配置的部署如何使CoSRad使用世界各地的许多现有系统执行类似的测量活动。

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