Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan
文献类型:期刊论文
作者 | Wang, X. ; Shi, J. K. ; Wang, G. J. ; Gong, Y. |
刊名 | Advances in Space Research
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出版日期 | 2009 |
卷号 | 43期号:11页码:1812-1820 |
关键词 | Low-latitude ionosphere F2 peak parameters IRI model international reference ionosphere |
ISSN号 | 0273-1177 |
通讯作者 | 北京8701信箱 |
英文摘要 | Monthly median values of foF2, hmF2 and M(3000)F2 parameters, with quarter-hourly time interval resolution for the diurnal variation, obtained with DPS4 digisonde at Hainan (19.5 degrees N, 109.1 degrees E; Geomagnetic coordinates: 178.95 degrees E, 8.1 degrees N) are used to investigate the low-latitude ionospheric variations and comparisons with the International Reference Ionosphere (IRI) model predictions. The data used for the present study covers the period from February 2002 to April 2007, which is characterized by a wide range of solar activity, ranging from high solar activity (2002) to low solar activity (2007). The results show that (1) Generally, IRI predictions follow well the diurnal and seasonal variation patterns of the experimental values of foF2, especially in the summer of 2002. However, there are systematic deviation between experimental values and IRI predictions with either CCIR or URSI coefficients. Generally IRI model greatly underestimate the values of foF2 from about noon to sunrise of next day, especially in the afternoon, and slightly overestimate them from sunrise to about noon. It seems that there are bigger deviations between IRI Model predictions and the experimental observations for the moderate solar activity. (2) Generally the IRI-predicted hmF2 values using CCIR M(3000)F2 option shows a poor agreement with the experimental results, but there is a relatively good agreement in summer at low solar activity. The deviation between the IRI-predicted hmF2 using CCIR M(3000)F2 and observed hmF2 is bigger from noon to sunset and around sunrise especially at high solar activity. The occurrence time of hmF2 peak (about 1200 LT) of the IRI model predictions is earlier than that of observations (around 1500 LT). The agreement between the IRI hmF2 obtained with the measured M(3000)F2 and the observed hmF2 is very good except that IRI overestimates slightly hmF2 in the daytime in summer at high solar activity and underestimates it in the nighttime with lower values near sunrise at low solar activity. |
学科主题 | 空间物理 |
收录类别 | SCI |
原文出处 | http://www.sciencedirect.com/science?_ob=MImg&_imagekey=B6V3S-4V70RCR-3-K&_cdi=5738&_user=1999492&_orig=search&_coverDate=06%2F02%2F2009&_sk=999569988&view=c&wchp=dGLbVzW-zSkWz&md5=b5a710fa4bbb9ae27edc35b2f590f95e&ie=/sdarticle.pdf |
语种 | 英语 |
源URL | [http://ir.cssar.ac.cn/handle/122/1145] ![]() |
专题 | 国家空间科学中心_空间科学部 |
推荐引用方式 GB/T 7714 | Wang, X.,Shi, J. K.,Wang, G. J.,et al. Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan[J]. Advances in Space Research,2009,43(11):1812-1820. |
APA | Wang, X.,Shi, J. K.,Wang, G. J.,&Gong, Y..(2009).Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan.Advances in Space Research,43(11),1812-1820. |
MLA | Wang, X.,et al."Comparison of ionospheric F2 peak parameters foF2 and hmF2 with IRI2001 at Hainan".Advances in Space Research 43.11(2009):1812-1820. |
入库方式: OAI收割
来源:国家空间科学中心
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