TITLE

Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010

AUTHOR(S)
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.
PUB. DATE
January 2014
SOURCE
Solar Physics;Jan2014, Vol. 289 Issue 1, p319
SOURCE TYPE
Academic Journal
DOC. TYPE
Article
ABSTRACT
Images 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.
ACCESSION #
91933470

 

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