133 citations · 349 across the 5 of their papers we have counts for
10 papers
Explosive Chromospheric Evaporation in a Circular-ribbon Flare
Q. M. Zhang, D. Li, Z. J. Ning +3
In this paper, we report our multiwavelength observations of the C4.2 circular-ribbon flare in active region (AR) 12434 on 2015 October 16. The short-lived flare was associated wit…
On the Nature of the Extreme-Ultraviolet Late Phase of Solar Flares
Y. Li, M. D. Ding, Y. Guo +1
The extreme-ultraviolet (EUV) late phase of solar flares is a second peak of warm coronal emissions (e.g., Fe XVI) for many minutes to a few hours after the GOES soft X-ray peak. I…
On the Relationship Between a Hot-channel-like Solar Magnetic Flux Rope and its embedded Prominence
X. Cheng, M. D. Ding, J. Zhang +4
Magnetic flux rope (MFR) is a coherent and helical magnetic field structure that is recently found probably to appear as an elongated hot-channel prior to a solar eruption. In this…
Formation of a Double-decker Magnetic Flux Rope in the Sigmoidal Solar Active Region 11520
X. Cheng, M. D. Ding, J. Zhang +5
In this paper, we address the formation of a magnetic flux rope (MFR) that erupted on 2012 July 12 and caused a strong geomagnetic storm event on July 15. Through analyzing the lon…
Dynamic Evolution of an X-shaped Structure above a Trans-equatorial Quadrupole Solar Active Region Group
J. Q. Sun, X. Cheng, Y. Guo +2
In the solar corona, magnetic reconnection usually takes place at the singular configuration of magnetic field, in particular near a magnetic null owing to its high susceptibility…
Tracking the Evolution of A Coherent Magnetic Flux Rope Continuously from the Inner to the Outer Corona
X. Cheng, M. D. Ding, Y. Guo +6
The magnetic flux rope (MFR) is believed to be the underlying magnetic structure of coronal mass ejections (CMEs). However, it remains unclear how an MFR evolves into and forms the…