首页> 外文会议>2011 30th URSI General Assembly and Scientific Symposium >1st Observations of SPEAR (Space Plasma Exploration by Active Radar) induced plasma line spectral enhancements in a naturally occurring sporadic E-region
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1st Observations of SPEAR (Space Plasma Exploration by Active Radar) induced plasma line spectral enhancements in a naturally occurring sporadic E-region

机译:在自然零星E区域中SPEAR(有源雷达进行的空间等离子体探测)引起的等离子体线光谱增强的1 st 观测

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This paper will present the 1st observations of sporadic E-layer heating at high latitudes (78°N) using the SPEAR heating facility and the EISCAT Svalbard Radar (ESR). During the experiment the SPEAR heating facility was transmitting with O-mode polarization in a field aligned direction with a constant ERP of ∼16MW. Results show distinct heating enhancements in the plasma line spectra, corresponding to the SPEAR heater frequency of 4.45MHz. High spatial resolution (100m) plasma line data indicate simultaneous enhancements at both the top and bottom side of the layer respectively (located at ∼107.5 and 109km altitude respectively). It is postulated that the results represent evidence of O to Z-mode conversion of the heater wave occurring at the bottom of the E-layer, allowing propagation through the layer resulting in simultaneous topside enhancements. The structure, both temporally and spatially, of these enhancements will be discussed in detail.
机译:本文将介绍使用SPEAR加热设备和EISCAT斯瓦尔巴德雷达(ESR)在高纬度(78°N)上零星E层加热的第一观察。在实验过程中,SPEAR加热设备以O型极化方式在磁场对准方向上传输,ERP恒定为〜16MW。结果显示等离子线光谱中明显的加热增强,对应于4.45MHz的SPEAR加热器频率。高空间分辨率(100m)的等离子线数据表明该层的顶侧和底侧分别有同时增强作用(分别位于约107.5和109km的高度)。据推测,该结果代表了在E层底部发生的加热器波从O到Z模转换的证据,从而允许通过该层的传播导致同时的顶面增强。这些增强的时间和空间结构都将详细讨论。

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