Comparison of ionosphere characteristic parameters obtained by ionosonde with IRI-2007 model over Southeast Asia

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• 作者：N. Wichaipanich ; P. Supnithi ; T. Tsugawa ; T. Maruyama ; T. Nagatsuma
• 关键词：Conjugate points ; foF2 ; hmF2 ; IRI model ; Solar activity
• 刊名：Advances in Space Research
• 出版年：2013
• 出版时间：15 November, 2013
• 年：2013
• 卷：52
• 期：10
• 页码：1748-1755
• 全文大小：2356 K

文摘

In this work, the foF2 and hmF2 parameters at the conjugate points near the magnetic equator of Southeast Asia are studied and compared with the International Reference Ionosphere (IRI) model. Three ionosondes are installed nearly along the magnetic meridian of 100¡ãE; one at the magnetic equator, namely Chumphon (10.72¡ãN, 99.37¡ãE, dip angle 3.0¡ãN), and the other two at the magnetic conjugate points, namely Chiang Mai (18.76¡ãN, 98.93¡ãE, dip angle 12.7¡ãN) and Kototabang (0.2¡ãS, 100.30¡ãE, dip angle 10.1¡ãS). The monthly hourly medians of the foF2 and hmF2 parameters are calculated and compared with the predictions obtained from the IRI-2007 model from January 2004 to February 2007. Our results show that: the variations of foF2 and hmF2 predicted by the IRI-2007 model generally show the similar feature to the observed data. Both parameters generally show better agreement with the IRI predictions during daytime than during nighttime. For foF2, most of the results show that the IRI model overestimates the observed foF2 at the magnetic equator (Chumphon), underestimates at the northern crest (Chiang Mai) and is close to the measured ones at the southern crest of the EIA (Kototabang). For hmF2, the predicted hmF2 values are close to the hmF2(M3000F2_OBS) during daytime. During nighttime, the IRI model gives the underestimation at the magnetic equator and the overestimation at both EIA crests. The results are important for the future improvements of the IRI model for foF2 and hmF2 over Southeast Asia region.