no code implementations • 24 Oct 2020 • Guiping Zhou, Guannan Gao, Jingxiu Wang, Jun Lin, Yingna Su, Chunlan Jin, Yuzong Zhang
By revisiting the successive eruptions on 2012 March 7, fast-mode shocks are identified to account for the X5. 4 flare-related EUV wave with a velocity of 550 km/s, and appeared faster than 2060$\pm$270 km/s at the front of the corresponding coronal mass ejection in the slow-rising phase.
Solar and Stellar Astrophysics
no code implementations • 5 Mar 2012 • Jingxiu Wang, Guiping Zhou, Chunlan Jin, Hui Li
Each of the clusters is characterized by a few well-developed ERs that are partially or fully co-aligned in magnetic axis orientation.
Solar and Stellar Astrophysics
