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武汉地区(30.5°N,114.4°E)钠流星尾迹激光雷达的初步观测
2010年
通过将Na激光雷达的积累时间设置为3.2s,我们在武汉地区(30.5°N,114.4oE)对原子流星尾迹进行了测量.在16个晚上166h的观测时间里,总共发现了125个Na流星尾迹事件.这些尾迹峰值密度变化范围为4040~39170cm–3,平均值为16430cm–3.出现高度范围为77.2~111.6km,质心高度为92.6km.钠尾迹高度分布的上边界与同时观测到的平均钠层剖面相类似.特别地,尾迹高度柱状图最大值出现在平均钠层峰值处.这表明流星体进入大气层后消融产生能被地基激光雷达探测到的流星尾迹,更多的出现在常规金属层的峰值附近.这与早期的K和Fe尾迹的激光雷达观测结果一致.观测发现,偶发钠层的形成往往伴随着钠流星尾迹群,这些尾迹出现高度与偶发钠层的高度一致.
谢秋洪易帆
Preliminary lidar observations of Na meteor trails at Wuhan (30.5°N, 114.4°E), China被引量:2
2010年
Na lidar measurements of atom meteor trails with an integration period of 3.2 s were conducted at Wuhan (30.5°N, 114.4°E), China. A total of 125 Na meteor trail events were registered from 166 hours (16 nights) of lidar data. These Na trails show peak densities ranging from 4040 to 39170 cm?3 with a mean of 16430 cm?3, while their occurrence altitudes vary from 77.2 to 111.6 km with a distribution centroid at 92.6 km. The upper edge of the Na trail altitude distribution resembles that of the altitude profile of the simultaneously observed mean Na layer. In particular, the trail altitude histogram maximum occurs around the mean Na layer peak. This is consistent with early lidar observations of K and Fe trails, which shows that meteoroids entering the atmosphere tend to yield more atom meteor trails detectable by ground-based lidars around the peak of the regular metal layers than elsewhere. It was found that the formation of the Nas layers was usually accompanied by a bunch of Na meteor trails, and that they occurred near the altitude of the Nas layer peak.
XIE QiuHong1,2,3 & YI Fan1,2,3 1 School of Electronic Information, Wuhan University, Wuhan 430079, China
关键词:钠层海拔高度激光雷达探测
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