Climatology of equatorial and low-latitude F region kilometer-scale irregularities over the meridian circle around 120 degrees E/60 degrees W
文献类型:期刊论文
作者 | Zhao, Xiukuan3,4,5,6; Xie, Haiyong3,4,5,6; Hu, Lianhuan3,4,5,6; Sun, Wenjie3,4,5,6; Hao, Xiqing6; Ning, Baiqi4,5,6; Takahashi, Hisao2; Li, Guozhu1,4,5,6 |
刊名 | GPS SOLUTIONS |
出版日期 | 2021 |
卷号 | 25期号:1页码:14 |
ISSN号 | 1080-5370 |
关键词 | Equatorial plasma bubble irregularity Long-term occurrence characteristics South American and East Asian low latitudes |
DOI | 10.1007/s10291-020-01054-2 |
英文摘要 | The occurrences of equatorial plasma bubble (EPB) irregularities over Asian and American sectors often show a different behavior due to significantly different geometries of the geomagnetic field. By using the GPS total electron content observations over equatorial and low latitudes sectors of Asian (about 120 degrees E) and American (about 60 degrees W) during 1997-2018, we present a comparative study of long-term occurrences of EPB kilometer-scale irregularities over the two longitude sectors. The results show that post-sunset EPB irregularities over the Asian sector were positively correlated with solar activity. However, in the American sector, such a positive dependence was not apparent in 2000-2002, which could be partly induced by limited data available during the high occurrence season of solar maximum when the GPS receivers frequently lost lock. The geomagnetic disturbance tends to inhibit the generation of EPB irregularities over both sectors during post-sunset but enhance their generation during post-midnight. The latitudinal distribution of EPB irregularities exhibited a double-peak structure centered within +/- 10 degrees (dip lat.), with the latitudinal limit below +/- 25 degrees at solar maximum in both sectors and below +/- 20 degrees and +/- 10 degrees at solar minimum in American and Asian sectors, respectively. Specifically, in the American sector, the occurrence rates were about two times higher than those in the Asian sector, and the occurrence rates in the northern hemisphere were apparently lower than those in the southern hemisphere. The enhanced ionization by particle precipitation over the South Atlantic Magnetic Anomaly region could cause the north-south asymmetry of occurrence rates of EPB irregularities. The results help in designing experiments to understand better the generation of EPB irregularities under the future international meridian circle project. |
WOS关键词 | VERTICAL PLASMA DRIFT ; BUBBLES ; SOLAR ; SCINTILLATIONS ; STORM ; RECEIVERS |
资助项目 | National Natural Science Foundation of China[41727803] ; National Natural Science Foundation of China[41904141] ; National Natural Science Foundation of China[42020104002] ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Chinese Meridian Project |
WOS研究方向 | Remote Sensing |
语种 | 英语 |
出版者 | SPRINGER HEIDELBERG |
WOS记录号 | WOS:000592139700001 |
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 ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the 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 the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the 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 the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the 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 the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Solar-Terrestrial Environment Research Network (STERN) of the Chinese Academy of Sciences ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project ; Chinese Meridian Project |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/98723] |
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.Univ Chinese Acad Sci, Coll Earth & Planetary Sci, Beijing, Peoples R China 2.Inst Nacl Pesquisas Espaciais, Div Aeron, Sao Jose Dos Campos, Brazil 3.Natl Earth Syst Sci Data Ctr, Geophys Ctr, Beijing, Peoples R China 4.Chinese Acad Sci, Innovat Acad Earth Sci, Beijing, Peoples R China 5.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China 6.Chinese Acad Sci, Beijing Natl Observ Space Environm, Inst Geol & Geophys, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Zhao, Xiukuan,Xie, Haiyong,Hu, Lianhuan,et al. Climatology of equatorial and low-latitude F region kilometer-scale irregularities over the meridian circle around 120 degrees E/60 degrees W[J]. GPS SOLUTIONS,2021,25(1):14. |
APA | Zhao, Xiukuan.,Xie, Haiyong.,Hu, Lianhuan.,Sun, Wenjie.,Hao, Xiqing.,...&Li, Guozhu.(2021).Climatology of equatorial and low-latitude F region kilometer-scale irregularities over the meridian circle around 120 degrees E/60 degrees W.GPS SOLUTIONS,25(1),14. |
MLA | Zhao, Xiukuan,et al."Climatology of equatorial and low-latitude F region kilometer-scale irregularities over the meridian circle around 120 degrees E/60 degrees W".GPS SOLUTIONS 25.1(2021):14. |
入库方式: OAI收割
来源:地质与地球物理研究所
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