STRUCTURE, PROPAGATION, AND EXPANSION OF A CME-DRIVEN SHOCK IN THE HELIOSPHERE: A REVISIT OF THE 2012 JULY 23 EXTREME STORM

	STRUCTURE, PROPAGATION, AND EXPANSION OF A CME-DRIVEN SHOCK IN THE HELIOSPHERE: A REVISIT OF THE 2012 JULY 23 EXTREME STORM
	Liu, Ying D.; Hu, Huidong; Zhu, Bei; Luhmann, Janet G.; Vourlidas, Angelos
刊名	ASTROPHYSICAL JOURNAL
	2017
卷号	834 期号:2 页码:158
关键词	shock waves solar-terrestrial relations solar wind Sun: coronal mass ejections (CMEs) Sun: radio radiation
ISSN号	0004-637X
英文摘要	We examine the structure, propagation, and expansion of the shock associated with the 2012 July 23 extreme coronal mass ejection. Characteristics of the shock determined from multi-point imaging observations are compared to in situ measurements at different locations and a complex radio type II burst, which according to our definition has multiple branches that may not all be fundamental-harmonic related. The white-light shock signature can be modeled reasonably well by a spherical structure and was expanding backward even on the opposite side of the Sun. The expansion of the shock, which was roughly self-similar after the first similar to 1.5 hr from launch, largely dominated over the translation of the shock center for the time period of interest. Our study also suggests a bowshockmorphology around the nose at later times due to the outward motion in combination with the expansion of the ejecta. The shock decayed and failed to reach Mercury in the backward direction and the Solar Terrestrial Relations Observatory B (STEREO B) and Venus in the lateral directions, as indicated by the imaging and in situ observations. The shock in the nose direction, however, may have persisted to the far outer heliosphere, with predicted impact on Dawn around 06: 00 UT on July 25 and on Jupiter around 23: 30 UT on July 27 by a magnetohydrodynamic model. The type II burst shows properties generally consistent with the spatial/temporal variations of the shock deduced from imaging and in situ observations. In particular, the low-frequency bands agree well with the in situ measurements of a very low density ahead of the shock at STEREO A.
收录类别	SCI
语种	英语
内容类型	期刊论文
源URL	[http://ir.nssc.ac.cn/handle/122/5810]
专题	国家空间科学中心_空间科学部
推荐引用方式 GB/T 7714	Liu, Ying D.,Hu, Huidong,Zhu, Bei,et al. STRUCTURE, PROPAGATION, AND EXPANSION OF A CME-DRIVEN SHOCK IN THE HELIOSPHERE: A REVISIT OF THE 2012 JULY 23 EXTREME STORM[J]. ASTROPHYSICAL JOURNAL,2017,834(2):158.
APA	Liu, Ying D.,Hu, Huidong,Zhu, Bei,Luhmann, Janet G.,&Vourlidas, Angelos.(2017).STRUCTURE, PROPAGATION, AND EXPANSION OF A CME-DRIVEN SHOCK IN THE HELIOSPHERE: A REVISIT OF THE 2012 JULY 23 EXTREME STORM.ASTROPHYSICAL JOURNAL,834(2),158.
MLA	Liu, Ying D.,et al."STRUCTURE, PROPAGATION, AND EXPANSION OF A CME-DRIVEN SHOCK IN THE HELIOSPHERE: A REVISIT OF THE 2012 JULY 23 EXTREME STORM".ASTROPHYSICAL JOURNAL 834.2(2017):158.