Using IRI and GSM TIP model results as environment for HF radio wave propagation model during the geomagnetic storm occurred on September 26-29, 2011
文献类型:期刊论文
作者 | Kotova, D. S.1,2; Klimenko, M. V.1,2; Klimenko, V. V.1; Zakharov, V. E.2; Ratovsky, K. G.3; Nosikov, I. A.1,2; Zhao, B.4,5 |
刊名 | ADVANCES IN SPACE RESEARCH
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出版日期 | 2015-11-01 |
卷号 | 56期号:9页码:2012-2029 |
关键词 | HF radio wave propagation model IRI model First principles model Ionosonde F3 layer Geomagnetic storm |
DOI | 10.1016/j.asr.2015.05.009 |
文献子类 | Article |
英文摘要 | This paper analyses the geomagnetic storm on September 26-29, 2011. We compare the calculation results obtained using the Global Self-consistent Model of the Thermosphere, Ionosphere and Protonosphere (GSM TIP) and IRI-2012 (Bilitza et al., 2014) model with ground-based ionosonde data of stations at different latitudes and longitudes. We examined physical mechanisms responsible for the formation of ionospheric effects during the main phase of geomagnetic storm that occurred at the rising phase of the 24th solar cycle. We used numerical results obtained from IRI-2012 and GSM TIP models as propagation environment for HF signals from an equatorial transmitter during quiet and disturbed conditions. We used the model of HF radio wave propagation developed in I. Kant Baltic Federal University (BFU) that is based on the geometrical optics approximation. We compared the obtained radio paths in quiet conditions and during the main and recovery storm phases and evaluated radio wave attenuation in different media models. (C) 2015 COSPAR. Published by Elsevier Ltd. All rights reserved. |
WOS关键词 | IONOSPHERIC F-REGION ; EQUATORIAL IONOSPHERE ; NUMERICAL-SIMULATION ; EARTHS IONOSPHERE ; ADDITIONAL LAYER ; ELECTRIC-FIELD ; PARAMETERS ; IONOGRAMS ; SYSTEM ; SECTOR |
WOS研究方向 | Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
语种 | 英语 |
WOS记录号 | WOS:000363345700023 |
资助机构 | RFBR Grant(14-05-00578) ; RFBR Grant(14-05-00578) ; (MK-4866.2014.5) ; (MK-4866.2014.5) ; RFBR Grant(14-05-00578) ; RFBR Grant(14-05-00578) ; (MK-4866.2014.5) ; (MK-4866.2014.5) |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/62202] ![]() |
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 |
作者单位 | 1.RAS, Pushkov Inst Terr Magnetism Ionosphere & Radio Wa, West Dept, Kaliningrad 236017, Russia 2.Immanuel Kant Balt Fed Univ, Dept Radiophys & Informat Safety, Kaliningrad 238300, Russia 3.Inst Solar Terr Phys SB RAS, Irkutsk 664033, Russia 4.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 100029, Peoples R China 5.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 | Kotova, D. S.,Klimenko, M. V.,Klimenko, V. V.,et al. Using IRI and GSM TIP model results as environment for HF radio wave propagation model during the geomagnetic storm occurred on September 26-29, 2011[J]. ADVANCES IN SPACE RESEARCH,2015,56(9):2012-2029. |
APA | Kotova, D. S..,Klimenko, M. V..,Klimenko, V. V..,Zakharov, V. E..,Ratovsky, K. G..,...&Zhao, B..(2015).Using IRI and GSM TIP model results as environment for HF radio wave propagation model during the geomagnetic storm occurred on September 26-29, 2011.ADVANCES IN SPACE RESEARCH,56(9),2012-2029. |
MLA | Kotova, D. S.,et al."Using IRI and GSM TIP model results as environment for HF radio wave propagation model during the geomagnetic storm occurred on September 26-29, 2011".ADVANCES IN SPACE RESEARCH 56.9(2015):2012-2029. |
入库方式: OAI收割
来源:地质与地球物理研究所
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