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首页> 外文期刊>TAO: Terrastrial, atmospheric, and oceanic sciences >Daytime E-Region Irregularities During the 22 July 2009 Solar Eclipse over Chung-Li (24.9°N, 121.2°E), a Moderate Mid-Latitude Station
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Daytime E-Region Irregularities During the 22 July 2009 Solar Eclipse over Chung-Li (24.9°N, 121.2°E), a Moderate Mid-Latitude Station

机译:2009年7月22日,中度中纬度站中N(24.9°N,121.2°E)发生日食期间,日间电子区域异常

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The 22 July 2009 solar eclipse with an obscuration of > 83% at Chung-Li (24.9°N, 121.2°E, Dip 35°N) in Taiwan during noon hours has provided a unique opportunity for us to examine its impact on E-region irregularities which were observed simultaneously by the 52 MHz coherent radar and a co-located ionosonde. Significant observations revealed that the daytime E-region strong backscatter echoes at multiple heights and a sudden intensification of the weak sporadic E-layer during the 22 July 2009 solar eclipse. These results follow the research findings of Patra et al. (2009). As the incident solar radiation suddenly blocked by intruding Moon during solar eclipse events that would generally create night-like ionospheric conditions, it is surmised that the E-region irregularities were indeed induced by the eclipse associated effects. The induced effects resulted in faster recombination of molecular ions, generation of gravity waves and electric fields that could have created a conducive environment to excite plasma irregularities through a gradient-drift instability mechanism. The vertical shears of radar Doppler velocity and the peak radar backscatter at the node of Doppler velocity shear, as resolved by the coherent scatter radar with interferometer technique, were possibly due to the upward propagating gravity waves and wave-induced polarization electric fields. The present observational results should not only be highly useful to ascertain plausible mechanisms responsible for nighttime E-region irregularities, but also provided evidence that a solar eclipse could generate E-region plasma irregularities over temperate mid-latitudes for the first time.
机译:2009年7月22日中午在台湾中-(24.9°N,121.2°E,Dip 35°N)遮盖> 83%的日食为我们提供了一个独特的机会来研究其对E- 52 MHz相干雷达和共置离子探空仪同时观测到的区域不规则性。重大观测结果表明,2009年7月22日的日食期间,白天E区的强反向散射回波在多个高度发生,弱零星E层突然增强。这些结果遵循了Patra等人的研究发现。 (2009)。由于日食事件期间入射的太阳辐射突然被侵入的月亮所阻挡,通常会产生类似夜晚的电离层条件,因此推测E区不规则确实是由日食相关效应引起的。诱导的效应导致分子离子更快的重组,引力波和电场的产生,它们可能已经创建了一个有利的环境,可以通过梯度漂移不稳定性机制激发等离子体的不规则性。用干涉仪技术通过相干散射雷达解决的雷达多普勒速度的垂直切变和在多普勒速度切变的节点处的峰值雷达反向散射,可能是由于向上传播的重力波和波感应极化电场引起的。目前的观测结果不仅对确定造成夜间E区不规则现象的合理机制非常有用,而且还提供证据证明日食可在温带中纬度地区首次产生E区等离子不规则现象。

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