中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
GPS phase scintillation at high latitudes during geomagnetic storms of 7-17 March 2012-Part 2: Interhemispheric comparison

文献类型:期刊论文

作者Prikryl, P.1,10; Ghoddousi-Fard, R.2; Spogli, L.3; Mitchell, C. N.4; Li, G.5; Ning, B.5; Cilliers, P. J.6; Sreeja, V.7; Aquino, M.7; Terkildsen, M.8,9
刊名ANNALES GEOPHYSICAE
出版日期2015
卷号33期号:6页码:657-670
关键词Ionosphere ionospheric disturbances ionospheric irregularities polar ionosphere
DOI10.5194/angeo-33-657-2015
文献子类Article
英文摘要During the ascending phase of solar cycle 24, a series of interplanetary coronal mass ejections (ICMEs) in the period 7-17 March 2012 caused geomagnetic storms that strongly affected high-latitude ionosphere in the Northern and Southern Hemisphere. GPS phase scintillation was observed at northern and southern high latitudes by arrays of GPS ionospheric scintillation and TEC monitors (GISTMs) and geodetic-quality GPS receivers sampling at 1 Hz. Mapped as a function of magnetic latitude and magnetic local time (MLT), the scintillation was observed in the ionospheric cusp, the tongue of ionization fragmented into patches, sun-aligned arcs in the polar cap, and nightside auroral oval and subauroral latitudes. Complementing a companion paper (Prikryl et al., 2015a) that focuses on the high-latitude ionospheric response to variable solar wind in the North American sector, interhemispheric comparison reveals commonalities as well as differences and asymmetries between the northern and southern high latitudes, as a consequence of the coupling between the solar wind and magnetosphere. The interhemispheric asymmetries are caused by the dawn-dusk component of the interplanetary magnetic field controlling the MLT of the cusp entry of the storm-enhanced density plasma into the polar cap and the orientation relative to the noon-midnight meridian of the tongue of ionization.
WOS关键词INTERPLANETARY MAGNETIC-FIELD ; ELECTRON-CONTENT ; SOLAR MINIMUM ; AURORAL OVAL ; CONVECTION ; CONJUGATE ; IMF ; IONOSPHERE ; SUPERDARN ; PLASMA
WOS研究方向Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences
语种英语
WOS记录号WOS:000357118400004
资助机构Canada Foundation for Innovation ; Canada Foundation for Innovation ; New Brunswick Innovation Foundation ; New Brunswick Innovation Foundation ; National Science Foundation(PLR-1248062) ; National Science Foundation(PLR-1248062) ; NSF(AGS-0838219 ; NSF(AGS-0838219 ; national scientific funding agency of Australia ; national scientific funding agency of Australia ; national scientific funding agency of Canada ; national scientific funding agency of Canada ; national scientific funding agency of China ; national scientific funding agency of China ; national scientific funding agency of France ; national scientific funding agency of France ; national scientific funding agency of Japan ; national scientific funding agency of Japan ; national scientific funding agency of South Africa ; national scientific funding agency of South Africa ; national scientific funding agency of United Kingdom ; national scientific funding agency of United Kingdom ; national scientific funding agency of United States of America ; national scientific funding agency of United States of America ; Natural Resources Canada, Earth Sciences Sector (NRCan ESS)(20140371) ; Natural Resources Canada, Earth Sciences Sector (NRCan ESS)(20140371) ; AGS-0946900) ; AGS-0946900) ; Canada Foundation for Innovation ; Canada Foundation for Innovation ; New Brunswick Innovation Foundation ; New Brunswick Innovation Foundation ; National Science Foundation(PLR-1248062) ; National Science Foundation(PLR-1248062) ; NSF(AGS-0838219 ; NSF(AGS-0838219 ; national scientific funding agency of Australia ; national scientific funding agency of Australia ; national scientific funding agency of Canada ; national scientific funding agency of Canada ; national scientific funding agency of China ; national scientific funding agency of China ; national scientific funding agency of France ; national scientific funding agency of France ; national scientific funding agency of Japan ; national scientific funding agency of Japan ; national scientific funding agency of South Africa ; national scientific funding agency of South Africa ; national scientific funding agency of United Kingdom ; national scientific funding agency of United Kingdom ; national scientific funding agency of United States of America ; national scientific funding agency of United States of America ; Natural Resources Canada, Earth Sciences Sector (NRCan ESS)(20140371) ; Natural Resources Canada, Earth Sciences Sector (NRCan ESS)(20140371) ; AGS-0946900) ; AGS-0946900)
源URL[http://ir.iggcas.ac.cn/handle/132A11/62342]  
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.Nat Resources Canada, Geomagnet Lab, Ottawa, ON, Canada
2.Nat Resources Canada, Canadian Geodet Survey, Ottawa, ON, Canada
3.Ist Nazl Geofis & Vulcanol, Rome, Italy
4.Univ Bath, Dept Elect & Elect Engn, Bath BA2 7AY, Avon, England
5.Chinese Acad Sci, Inst Geol & Geophys, Beijing, Peoples R China
6.South African Natl Space Agcy, Space Sci Directorate, Hermanus, South Africa
7.Univ Nottingham, Nottingham Geospatial Inst, Nottingham NG7 2RD, England
8.Bur Meteorol, IPS Radio Serv, Haymarket, NSW, Australia
9.Bur Meteorol, IPS Space Serv, Haymarket, NSW, Australia
10.Univ New Brunswick, Dept Phys, Fredericton, NB E3B 5A3, Canada
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Prikryl, P.,Ghoddousi-Fard, R.,Spogli, L.,et al. GPS phase scintillation at high latitudes during geomagnetic storms of 7-17 March 2012-Part 2: Interhemispheric comparison[J]. ANNALES GEOPHYSICAE,2015,33(6):657-670.
APA Prikryl, P..,Ghoddousi-Fard, R..,Spogli, L..,Mitchell, C. N..,Li, G..,...&Romano, V..(2015).GPS phase scintillation at high latitudes during geomagnetic storms of 7-17 March 2012-Part 2: Interhemispheric comparison.ANNALES GEOPHYSICAE,33(6),657-670.
MLA Prikryl, P.,et al."GPS phase scintillation at high latitudes during geomagnetic storms of 7-17 March 2012-Part 2: Interhemispheric comparison".ANNALES GEOPHYSICAE 33.6(2015):657-670.

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来源:地质与地球物理研究所

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