Abstract
Taking the advantage of high temporal and spatial resolutions of the Solar Dynamics Observatory (SDO) observations, we study a solar corona extreme-ultraviolet (EUV) wave associated with the coronal mass ejection (CME) on 2014 January 7. Our main purpose is to investigate the driving mechanism of this EUV wave, by analyzing the relation between the CME and the onset time and initial location of the EUV wave. Our result indicates that the EUV wave should be driven by the associated CME. By analyzing the time-slice images, we find that the wave has a speed of over 1 200km·s−1. The observed fast EUV wave can be interpreted by the hybrid model proposed by Chen et al. (2002), and it corresponds to the fast component in Chen's model, i.e., the coronal Moreton wave.
Sign-in/Register to access full text options 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
