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Simulated (STEREO) Views of the Solar Wind Disturbances Following the Coronal Mass Ejections of 1 August 2010 |
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| Authors: | Y. Zhang A. M. Du X. S. Feng W. Sun Y. D. Liu C. D. Fry C. S. Deehr M. Dryer B. Zieger Y. Q. Xie |
| Affiliation: | 1. Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, 100029, China 2. State Key Laboratory of Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, China 3. Geophysical Institute, University of Alaska, Fairbanks, AK, 99775-7320, USA 4. Space Sciences Laboratory, University of California, Berkeley, CA, 94720, USA 5. Exploration Physics International, Inc, Huntsville, AL, 35806, USA 6. Space Weather Prediction Center, Ret., National Oceanic and Atmospheric Administration, Boulder, CO, 80305, USA 7. Center for Space Physics, Boston University, 725 Commonwealth Ave, Boston, MA, 02215, USA 8. College of Meteorology and Oceanography, PLA University of Science and Technology, Nanjing, 211101, China |
| 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. |
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