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首页> 外文期刊>Annals Of Geophysics >The study of equatorial plasma bubble during January to April 2012 over Kolhapur (India)
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The study of equatorial plasma bubble during January to April 2012 over Kolhapur (India)

机译:2012年1月至2012年4月在印度Kolhapur进行的赤道等离子体气泡研究

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Over 53 nights of all sky airglow imager data collected during January-April 2012 from the low latitude station Kolhapur (16.68°N, 74.26°E; 10.6°N dip latitude) have been analyzed to study the F-region dynamics through the imaging of OI 630 nm emission line. The observed night airglow data were supported by the ionosonde measurements from Tirunelveli (8.7°N, 77.8°E; 0.51°N dip latitude). Well defined magnetic field aligned depletions were observed during the observation period. Out of 53 nights, 40 nights exhibited the occurrence of north-south aligned equatorial plasma bubbles. These plasma bubbles were found moving towards east with drift speed in range between 70 to 200 m s -1 . We have analyzed the zonal drift velocity variation and relation of bubble occurrence with the base height of the ionosphere together with the effects of the geomagnetic Ap and solar flux F 10.7 cm index in its first appearance.
机译:在2012年1月至4月期间,从低纬度站Kolhapur(北纬16.68°,东经74.26°;倾角为10.6°N)收集的所有天气成像仪数据中,经过53个晚上的分析,通过对F区域的成像进行研究OI 630 nm发射线。观测到的夜间气辉数据由Tirunelveli(8.7°N,77.8°E; 0.51NN纬度)的离子探空仪测量结果支持。在观察期间观察到明确定义的磁场对准的耗尽。在53个晚上中,有40个晚上出现了南北对齐的赤道等离子气泡。发现这些等离子气泡向东移动,漂移速度在70到200 m s -1之间。我们分析了纬向漂移速度的变化以及气泡出现与电离层基本高度的关系,以及首次出现时地磁Ap和太阳通量F 10.7 cm指数的影响。

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