IGGCAS OpenIR  > 地球与行星物理院重点实验室
IONISE: An Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia
Sun, Wenjie1,2,3; Wu, Baoyuan1; Wu, Zhi1; Hu, Lianhuan1,2,3; Zhao, Xiukuan1,2,3; Zheng, Jianchang1,2,3; Xie, Haiyong1,2,3; Yang, Sipeng1,2,3; Ning, Baiqi1,2,3; Li, Guozhu1,2,3,4
2020-08-01
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
ISSN2169-9380
Volume125Issue:8Pages:19
AbstractAn Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia (IONISE) is developed to identify and study the short-term and fine-scale ionospheric variations over China. The IONISE network mainly includes three crossed chains of Beidou geostationary satellite total electron content (TEC)/scintillation receivers along 110 degrees E, 23 degrees N, and 40 degrees N respectively, multistatic portable digital ionosondes and bistatic very high-frequency radars. Based on the IONISE observations, we report some preliminary results of ionospheric disturbances and irregularities, including (1) initially generated and zonally drifting equatorial plasma bubbles and related scintillations, (2) traveling ionospheric disturbances from middle to low latitudes, (3) drift of strong sporadic E structures over a wide area of more than 1,000 km, (4) fine-scale ionospheric perturbation and regional TEC gradient, and (5) general features of ionospheric response to geomagnetic storms. Possible mechanisms responsible for these ionospheric phenomena are discussed. The IONISE provides new data set for investigation on ionospheric disturbances of various scales in a broad region with dense observations along specific latitude/longitude. Plain Language Summary There are various types of ionospheric variations under different triggering conditions. To reveal possible sources responsible for short-term variability of ionosphere, trace the occurrence and movements of ionospheric irregularities and associated scintillations along the same longitude/latitude, and capture ionospheric disturbances of various scales over China, an Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia (IONISE), which consists of multiple types of instruments including Beidou geostationary (BD-GEO) total electron content (TEC)/scintillation receiver, portable digital ionosonde (PDI), and very high-frequency (VHF) radar, is developed. The BD-GEO TEC/scintillation measurements continuously made at the dense array of fixed ionospheric pierce points can track ionospheric disturbances of various scales along the same longitude/latitude, making it possible for investigation of different types of ionospheric disturbances. The Doppler velocity measurements by PDI are sensitive to ionospheric perturbations with weak amplitude which may be difficult to be detected from the general parameters such as F layer peak or virtual height derived from ionosonde observation. The spatially separated VHF radars with imaging capability of field aligned irregularities (FAIs) may capture the fine-scale evolution of FAIs. The preliminary results presented in this paper demonstrate the capability by IONISE for ionospheric disturbances of various scales such as equatorial plasma bubbles, traveling ionospheric disturbances, strong sporadic E structure, fine-scale ionospheric perturbation, regional TEC gradient, and ionospheric response to geomagnetic storms. It is expected that new observations from the IONISE will help to achieve a better understanding on the potential mechanisms for the multiscale ionospheric disturbances.
DOI10.1029/2020JA028055
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; 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 ; 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 ; 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 ; 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
WOS KeywordPOLARIZATION ELECTRIC-FIELD ; DIGITAL IONOSONDE ; PLASMA BUBBLES ; MAGNETIC STORM ; VHF RADAR ; F-REGION ; MIDLATITUDE ; DISTURBANCES ; DENSITY ; CHINA
Language英语
Funding ProjectNational Natural Science Foundation of China[41727803] ; National Natural Science Foundation of China[41422404] ; National Natural Science Foundation of China[41574149] ; Solar-Terrestrial Environment Research Network (STERN) of Chinese Academy of Sciences ; Chinese Meridian Project
Funding OrganizationNational Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; 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 ; 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 ; 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 ; 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
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000577125000029
PublisherAMER GEOPHYSICAL UNION
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.iggcas.ac.cn/handle/132A11/98309
Collection地球与行星物理院重点实验室
Corresponding AuthorLi, Guozhu
Affiliation1.Chinese Acad Sci, Inst Geol & Geophys, Beijing Natl Observ Space Environm, Beijing, Peoples R China
2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China
3.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China
4.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China
First Author AffilicationInstitute of Geology and Geophysics, Chinese Academy of Sciences;  Key Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Corresponding Author AffilicationInstitute of Geology and Geophysics, Chinese Academy of Sciences;  Key Laboratory of Earth and Planetary Physics, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Sun, Wenjie,Wu, Baoyuan,Wu, Zhi,et al. IONISE: An Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2020,125(8):19.
APA Sun, Wenjie.,Wu, Baoyuan.,Wu, Zhi.,Hu, Lianhuan.,Zhao, Xiukuan.,...&Li, Guozhu.(2020).IONISE: An Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,125(8),19.
MLA Sun, Wenjie,et al."IONISE: An Ionospheric Observational Network for Irregularity and Scintillation in East and Southeast Asia".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 125.8(2020):19.
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