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On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015
Wang, Yuming; Zhang, Quanhao; Liu, Jiajia; Shen, Chenglong; Shen, Fang; Yang, Zicai; Zic, T.; Vrsnak, B.; Webb, D. F.; Liu, Rui; Wang, S.; Zhang, Jie; Hu, Qiang; Zhuang, Bin; Wang, YM (reprint author), Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei, Peoples R China.; Wang, YM (reprint author), Univ Sci & Technol China, Synerget Innovat Ctr Quantum Informat & Quantum P, Hefei, Peoples R China.
Department空间科学部
Source PublicationJOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS
2016
Volume121Issue:8Pages:7423-7434
ISSN2169-9380
Language英语
AbstractThe largest geomagnetic storm so far, called 2015 St. Patrick's Day event, in the solar cycle 24 was produced by a fast coronal mass ejection (CME) originating on 15 March 2015. It was an initially west-oriented CME and expected to only cause a weak geomagnetic disturbance. Why did this CME finally cause such a large geomagnetic storm? We try to find some clues by investigating its propagation from the Sun to 1 AU. First, we reconstruct the CME's kinematic properties in the corona from the SOHO and Solar Dynamics Observatory imaging data with the aid of the graduated cylindrical shell model. It is suggested that the CME propagated to the west similar to 33 degrees +/- 10 degrees away from the Sun-Earth line with a speed of about 817 km s(-1) before leaving the field of view of the SOHO/Large Angle and Spectrometric Coronagraph (LASCO) C3 camera. A magnetic cloud (MC) corresponding to this CME was measured in situ by the Wind spacecraft 2 days after the CME left LASCO's field of view. By applying two MC reconstruction methods, we infer the configuration of the MC as well as some kinematic information, which implies that the CME possibly experienced an eastward deflection on its way to 1 AU. However, due to the lack of observations from the STEREO spacecraft, the CME's kinematic evolution in interplanetary space is not clear. In order to fill this gap, we utilize numerical MHD simulation, drag-based CME propagation model (DBM) and the model for CME deflection in interplanetary space (DIPS) to recover the propagation process, especially the trajectory, of the CME from 30R(S) to 1 AU under the constraints of the derived CME's kinematics near the Sun and at 1 AU. It is suggested that the trajectory of the CME was deflected toward the Earth by about 12 degrees, consistent with the implication from the MC reconstruction at 1 AU. This eastward deflection probably contributed to the CME's unexpected geoeffectiveness by pushing the center of the initially west-oriented CME closer to the Earth.
Indexed BySCI
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/5632
Collection空间科学部
Corresponding AuthorWang, YM (reprint author), Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei, Peoples R China.; Wang, YM (reprint author), Univ Sci & Technol China, Synerget Innovat Ctr Quantum Informat & Quantum P, Hefei, Peoples R China.
Recommended Citation
GB/T 7714
Wang, Yuming,Zhang, Quanhao,Liu, Jiajia,et al. On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015[J]. JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,2016,121(8):7423-7434.
APA Wang, Yuming.,Zhang, Quanhao.,Liu, Jiajia.,Shen, Chenglong.,Shen, Fang.,...&Wang, YM .(2016).On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015.JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS,121(8),7423-7434.
MLA Wang, Yuming,et al."On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015".JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS 121.8(2016):7423-7434.
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