Seasonal Variation of Post-sunset and Post-midnight Equatorial Plasma Bubble in Malaysia during Moderate Solar Activity Level

Nur Izzati Mohd Rosli, Nurul Shazana Abdul Hamid, M. Abdullah, S. M. Buhari, I. Sarudin
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Abstract

The equatorial plasma bubble (EPB) is a common event that occurred at the F-layer of the ionosphere due to plasma irregularities. Its occurrence can be observed around sunset and midnight hours, depending on the season. In this study, ROTI plot measurement was utilized in EPB detection, where the data was obtained from the Department of Survey and Mapping Malaysia (JUPEM). The seasonal variation of EPB in Langkawi, Malaysia was investigated for both post-sunset and post-midnight occurrence within the period of moderate solar activity year (2011). The result showed that EPB was varied with season, where both post-sunset and post-midnight EPB were highly observed during the equinoctial month (March and April) compared to June solstice. However, the post-sunset EPBs were found dominant during equinox while post-midnight EPBs were during June solstice.
中等太阳活动水平下马来西亚日落后和午夜后赤道等离子体泡的季节变化
赤道等离子体气泡(EPB)是电离层f层由于等离子体的不规则性而发生的一种常见现象。它的出现可以在日落和午夜左右观察到,这取决于季节。在本研究中,ROTI地块测量被用于EPB检测,其中数据来自马来西亚测绘部(JUPEM)。研究了马来西亚兰卡威在太阳活动中度年(2011年)日落后和午夜后发生的EPB的季节变化。结果表明:日强和午夜后的日强在春分月(3月和4月)比在6月至日高;然而,日落后的epb在春分期间占优势,而午夜后的epb在六月至期间占优势。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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