Comparison of the observed topside ionospheric and plasmaspheric electron content derived from the COSMIC podTEC measurements with the IRI_Plas model results | |
Zhang, Man-Lian; Liu, Libo; Wan, Weixing; Ning, Baiqi | |
刊名 | ADVANCES IN SPACE RESEARCH |
2017-07-15 | |
卷号 | 60期号:2页码:222-227 |
关键词 | Total Electron Content (TEC) Topside ionosphere Plasmasphere COSMIC IRI_Plas model |
ISSN号 | 0273-1177 |
DOI | 10.1016/j.asr.2016.10.025 |
文献子类 | Article |
英文摘要 | In this paper, variations of the topside ionospheric and plasmaspheric electron contents (TPEC) in the altitude range of similar to 800 to 20,200 km are compared with the IRI_Plas model results for the low (2008) and high (2012) solar activity years using TEC data (pod-TEC) derived from the upward-looking precise orbit determination antenna on board COSMIC low Earth orbit (LEO) satellites tracking the GPS signals. For each year, the dataset were divided into groups according to four seasons: M-Equinox (March, April), J-Solstice (May June, July and August), S-Equinox (September, October) and D-Solstice (January, February, November, and December). Our study showed that the IRI_Plas model is able to reproduce reasonably well the main features of the observational TPEC's latitudinal, diurnal as well as seasonal variation tendency when no longitudinal difference is taken into account. However, there exist discrepancies between the observational TPEC and the model results. Except for the daytime hours in the Equinoctial seasons of the high solar activity year 2012 when the IRI_Plas model results showed an overestimation, in general, the IRI_Plas model results underestimate the observational ones, in particular at nighttime hours in the low-latitude region. When the longitudinal difference is taken into account, the comparison study showed that the longitudinal dependence effect shown in the observational TPEC's seasonal variations was not captured by the IRI_Plas model result. Moreover, the IRI_ Plas model results tend to show a double-peak structure in the low-latitude region, a feature not appearing in the observational results. (C) 2016 COSPAR. Published by Elsevier Ltd. All rights reserved. |
WOS关键词 | REPRESENTATION ; DENSITY ; NEQUICK ; TEC |
WOS研究方向 | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
语种 | 英语 |
出版者 | ELSEVIER SCI LTD |
WOS记录号 | WOS:000404318900003 |
资助机构 | National Natural Science Foundation of China (NSFC)(41274163) ; National Important Basic Research Project(2012CB825604) ; KIP Pilot of the Chinese Academy of Sciences(KZZD-EW-01-3) ; National Natural Science Foundation of China (NSFC)(41274163) ; National Important Basic Research Project(2012CB825604) ; KIP Pilot of the Chinese Academy of Sciences(KZZD-EW-01-3) ; National Natural Science Foundation of China (NSFC)(41274163) ; National Important Basic Research Project(2012CB825604) ; KIP Pilot of the Chinese Academy of Sciences(KZZD-EW-01-3) ; National Natural Science Foundation of China (NSFC)(41274163) ; National Important Basic Research Project(2012CB825604) ; KIP Pilot of the Chinese Academy of Sciences(KZZD-EW-01-3) |
内容类型 | 期刊论文 |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/51788] |
专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
通讯作者 | Zhang, Man-Lian |
作者单位 | Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China |
推荐引用方式 GB/T 7714 | Zhang, Man-Lian,Liu, Libo,Wan, Weixing,et al. Comparison of the observed topside ionospheric and plasmaspheric electron content derived from the COSMIC podTEC measurements with the IRI_Plas model results[J]. ADVANCES IN SPACE RESEARCH,2017,60(2):222-227. |
APA | Zhang, Man-Lian,Liu, Libo,Wan, Weixing,&Ning, Baiqi.(2017).Comparison of the observed topside ionospheric and plasmaspheric electron content derived from the COSMIC podTEC measurements with the IRI_Plas model results.ADVANCES IN SPACE RESEARCH,60(2),222-227. |
MLA | Zhang, Man-Lian,et al."Comparison of the observed topside ionospheric and plasmaspheric electron content derived from the COSMIC podTEC measurements with the IRI_Plas model results".ADVANCES IN SPACE RESEARCH 60.2(2017):222-227. |
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