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  2. 地质与地球物理研究所
  3. 中国科学院地质与地球物理研究所
  4. 中国科学院地球与行星物理重点实验室
Challenges to Equatorial Plasma Bubble and Ionospheric Scintillation Short-Term Forecasting and Future Aspects in East and Southeast Asia

文献类型：期刊论文

作者Li, Guozhu2,3,4,10; Ning, Baiqi3,4,10; Otsuka, Yuichi9; Abdu, Mangalathayil Ali8; Abadi, Prayitno7; Liu, Zhizhao6; Spogli, Luca1,5; Wan, Weixing2,3,4,10
刊名SURVEYS IN GEOPHYSICS
出版日期2020-09-05
页码38
ISSN号0169-3298
关键词Ionospheric scintillation Equatorial plasma bubble Short-term variability The East and Southeast Asia
DOI10.1007/s10712-020-09613-5
英文摘要Equatorial plasma bubbles (EPBs) can cause rapid fluctuations in amplitude and phase of radio signals traversing the ionosphere and in turn produce serious ionospheric scintillations and disrupt satellite-based communication links. Whereas numerous studies on the generation and evolution of EPBs have been performed, the prediction of EPB and ionospheric scintillation occurrences still remains unresolved. The generalized Rayleigh-Taylor (R-T) instability has been widely accepted as the physical mechanism responsible for the generation of EPBs. But how the factors, which seed the development of R-T instability and control the dynamics of EPBs and resultant ionospheric scintillations, change on a short-term basis are not clear. In the East and Southeast Asia, there exist significant differences in the generation rates of EPBs at closely located stations, for example, Kototabang (0.2 degrees S, 100.3 degrees E) and Sanya (18.3 degrees N, 109.6 degrees E), indicating that the decorrelation distance of EPB generation is small (hundreds of kilometers) in longitude. In contrast, after the initial generation of EPBs at one longitude, they can drift zonally more than 2000 km and extend from the magnetic equator to middle latitudes of 40 degrees or higher under some conditions. These features make it difficult to identify the possible seeding sources for the EPBs and to accurately predict their occurrence, especially when the onset locations of EPBs are far outside the observation sector. This paper presents a review on the current knowledge of EPBs and ionospheric scintillations in the East and Southeast Asia, including their generation mechanism and occurrence morphology, and discusses some unresolved issues related to their short-term forecasting, including (1) what factors control the generation of EPBs, its day-to-day variability and storm-time behavior, (2) what factors control the evolution and lifetime of EPBs, and (3) how to accurately determine ionospheric scintillation from EPB measurements. Special focus is given to the whole process of the EPB generation, development and disruption. The current observing capabilities, future new facilities and campaign observations in the East and Southeast Asia in helping to better understand the short-term variability of EPBs and ionospheric scintillations are outlined.
WOS关键词F-REGION IRREGULARITIES ; FIELD-ALIGNED IRREGULARITIES ; TO-DAY VARIABILITY ; SANYA VHF RADAR ; SPREAD-F ; ELECTRIC-FIELD ; GPS SCINTILLATION ; STATISTICAL CHARACTERISTICS ; PREREVERSAL ENHANCEMENT ; DENSITY IRREGULARITIES
资助项目National Natural Science Foundation of China[41727803] ; National Natural Science Foundation of China[41422404] ; Hong Kong Research Grants Council (RGC)[B-Q61L PolyU 152222/17E] ; JSPS KAKENHI[15H05815] ; JSPS KAKENHI[16H05736] ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project
WOS研究方向Geochemistry & Geophysics
语种英语
出版者SPRINGER
WOS记录号WOS:000566698100001
资助机构National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; Hong Kong Research Grants Council (RGC) ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; JSPS KAKENHI ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project
源URL[http://ir.iggcas.ac.cn/handle/132A11/97793]  
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Li, Guozhu
作者单位1.Ist Nazl Geofis Vulcanol, Via Vigna Murata 605, I-00143 Rome, Italy
2.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing 100049, Peoples R China
3.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing 102212, Peoples R China
4.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing 100029, Peoples R China
5.SpacEarth Technol, Via Vigna Murata 605, I-00143 Rome, Italy
6.HongKong Polytech Univ, Dept Land Surveying & Geoinformat, Hung Hom, Kowloon, 181 Chatham Rd South, Hong Kong, Peoples R China
7.Indonesian Natl Inst Aeronaut & Space LAPAN, Ctr Space Sci, Bandung 40173, Indonesia
8.Inst Nacl Pesquisas Espaciais, Div Aeron, BR-12227010 Sao Paulo, Brazil
9.Nagoya Univ, Inst Space Earth Environm Res, Chikusa Ku, Furo Cho, Nagoya, Aichi 4648601, Japan
10.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing 100029, Peoples R China
推荐引用方式
GB/T 7714		 Li, Guozhu,Ning, Baiqi,Otsuka, Yuichi,et al. Challenges to Equatorial Plasma Bubble and Ionospheric Scintillation Short-Term Forecasting and Future Aspects in East and Southeast Asia[J]. SURVEYS IN GEOPHYSICS,2020:38.
APA Li, Guozhu.,Ning, Baiqi.,Otsuka, Yuichi.,Abdu, Mangalathayil Ali.,Abadi, Prayitno.,...&Wan, Weixing.(2020).Challenges to Equatorial Plasma Bubble and Ionospheric Scintillation Short-Term Forecasting and Future Aspects in East and Southeast Asia.SURVEYS IN GEOPHYSICS,38.
MLA Li, Guozhu,et al."Challenges to Equatorial Plasma Bubble and Ionospheric Scintillation Short-Term Forecasting and Future Aspects in East and Southeast Asia".SURVEYS IN GEOPHYSICS (2020):38.

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来源：地质与地球物理研究所

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