首页> 外文期刊>Advances in space research >Comments on the percentage of occurrence methodology used in 'a study of L band scintillations during the initial phase of rising solar activity at an Indian low latitude station' by H J Tanna, S P Karia and K N Pathak
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Comments on the percentage of occurrence methodology used in 'a study of L band scintillations during the initial phase of rising solar activity at an Indian low latitude station' by H J Tanna, S P Karia and K N Pathak

机译:H J Tanna,S P Karia和K N Pathak对“印度低纬度站太阳活动上升初期的L波段闪烁研究的研究”中使用的发生方法百分比的评论

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摘要

Following Tanna et al. (2013), we computed the percentage of occurrence of S-4 index for the period of 2012-2015 using the data of the dual frequency GPS receiver at the Tripura University, Agartala station (23.76 N, 91.26 degrees E) situated at the northern crest of the equatorial ionization anomaly (EIA) region of the Indian Subcontinent. We have observed discrepancy in the results contradicting the actual scintillation occurrence. The distinctly noticeable discrepancy is that the maximum occurrence month is shifted to April 2013 instead of March 2014. The problem arises due to the denominator term used in the percentage of occurrence ratio i.e. the total number of days of observed scintillation activity during the complete period under consideration. But the conventional percentage of occurrence methodology uses the number of days of observation (the total number of days for which data is available) during each month in the denominator. It correctly assigns the maximum occurrence to March 2014 instead of April 2013 and the obtained monthly statistics follow the solar activity during this period. (C) 2018 COSPAR. Published by Elsevier Ltd. All rights reserved.
机译:继Tanna等。 (2013年),我们使用位于北部的阿加尔塔拉大学Tripura大学双频GPS接收器(23.76 N,91.26度E)的双频GPS接收器的数据,计算了2012-2015年期间S-4指数的发生百分比印度次大陆的赤道电离异常(EIA)区域的波峰。我们已经观察到与实际闪烁发生相矛盾的结果差异。明显不同的是,最大发生月份从2013年4月而不是2014年3月开始。出现问题的原因是分母项占发生率的百分比,即在整个观测期间内闪烁活动的总天数考虑。但是传统的发生百分比方法使用分母中每个月的观察天数(可获得数据的总天数)。它正确地将发生次数最多的事件分配给了2014年3月,而不是2013年4月,并且获得的月度统计数据遵循了此期间的太阳活动。 (C)2018年COSPAR。由Elsevier Ltd.出版。保留所有权利。

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