Variations of ionospheric slab thickness over the magnetic equator of Southeast Asia

P. Jamjareegulgarn, P. Supnithi, K. Watthanasangmechai, T. Yokoyama, T. Tsugawa, M. Ishii, C. Nayak
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Abstract

In this paper, the diurnal and seasonal variations of the ionospheric slab thickness in an ionosonde chain over magnetic equator of Southeast Asia are studied. Three ionosonde stations of SEALION project located along the magnetic meridian of 100°E are selected to investigate, including two stations in Thailand, namely Chumphon and Chiang Mai, and one station in Indonesia, namely Kototabang. The monthly hourly medians of the foF2 from three ionosonde stations in 2010 are used to compute the observed NmF2. Refer to the TEC data; it can be obtained directly from GPS receiver at Chumphon station since the TEC data in 2010 were observed completely. In contrast, the TEC data at Chiang Mai station lost extremely and those at Kototabang station were unavailable. Hence, the TEC data used for these two stations are obtained from the International GNSS service (IGS). Our results show that 1) for all seasons, the NmF2 values during daytime have the successive decreasing values from Chiang Mai, Kototabang, and Chumphon. While the NmF2 values at three stations are almost identical during nighttime; 2) for all seasons at these three stations, the TEC values in the daytime are larger than those in the nighttime and their maximum values in the equinox and winter are higher than those in the summer; 3) the slab thickness values in all seasons during nighttime are generally larger than those during daytime for all three stations. Meanwhile, during daytime for all seasons, the slab thickness at Chumphon station is the highest among these three stations due to the fountain effect over magnetic equator.
东南亚磁赤道上空电离层板厚的变化
本文研究了东南亚磁赤道上一条电离层探空链中电离层板厚度的日变化和季节变化。选择SEALION项目沿100°E磁子午线的三个电离层探空站进行考察,其中两个站位于泰国春丰和清迈,一个站位于印度尼西亚科托塔邦。利用2010年三个电离层探空站逐月逐时中值计算NmF2的观测值。参照TEC数据;由于2010年的TEC数据已经完全观测到,因此可以直接从春丰站的GPS接收器获得。相比之下,清迈站的TEC数据丢失极为严重,Kototabang站的数据则无法获得。因此,这两个台站使用的TEC数据是从国际全球导航卫星系统(IGS)获得的。结果表明:①白天NmF2值从清迈、科托塔邦到春丰依次递减;而夜间三个站点的NmF2值几乎相同;2) 3个站点的TEC值在所有季节中白天大于夜间,春分和冬季的最大值大于夏季;3) 3个站点夜间各季节的板厚值均大于白天。同时,由于磁赤道上的喷泉效应,春丰站在白天的板厚是三个站点中最高的。
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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