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Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010
Zhang, Y.; Du, A. M.; Feng, X. S.; Sun, W.; Liu, Y. D.; Fry, C. D.; Deehr, C. S.; Dryer, M.; Zieger, B.; Xie, Y. Q.; Zhang, Y (reprint author), Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029, Peoples R China.
Department空间科学部
Source PublicationSOLAR PHYSICS
2014
Volume289Issue:1Pages:319-338
ISSN0038-0938
Language英语
AbstractImages observed by the twin spacecraft Solar TErrestrial RElations Observatory (STEREO) A and B appear as complex structures for two coronal mass ejections (CMEs) on 1 August 2010. Therefore, a series of sky maps of Thomson-scattered white light by interplanetary coronal mass ejections (ICMEs) on 1 August 2010 are simulated using the Hakamada-Akasofu-Fry (HAF) three-dimensional solar-wind model. A comparison between the simulated images and observations of STEREO-A and -B clarifies the structure and evolution of ICMEs (including shocks) in the observed images. The results demonstrate that the simulated images from the HAF model are very useful in the interpretation of the observed images when the ICMEs overlap within the fields of view of the instruments onboard STEREO-A and -B.
Indexed BySCI
Funding Project中国科学院空间科学与应用研究中心
Document Type期刊论文
Identifierhttp://ir.nssc.ac.cn/handle/122/1507
Collection空间科学部
Corresponding AuthorZhang, Y (reprint author), Chinese Acad Sci, Inst Geol & Geophys, Beijing 100029, Peoples R China.
Recommended Citation
GB/T 7714
Zhang, Y.,Du, A. M.,Feng, X. S.,et al. Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010[J]. SOLAR PHYSICS,2014,289(1):319-338.
APA Zhang, Y..,Du, A. M..,Feng, X. S..,Sun, W..,Liu, Y. D..,...&Zhang, Y .(2014).Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010.SOLAR PHYSICS,289(1),319-338.
MLA Zhang, Y.,et al."Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010".SOLAR PHYSICS 289.1(2014):319-338.
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