3 papers
astro-ph.SR2019
Synthesising Solar Radio Images From Atmospheric Imaging Assembly Extreme-Ultraviolet Data
Z. F. Li, S. H. Hua, X. Cheng +1
During non-flaring times, the radio flux of the Sun at the wavelength of a few centimeters to several tens of centimeters mostly originates from the thermal bremsstrahlung emission…
astro-ph.SR2018
Two Types of Long-duration Quasi-static Evolution of Solar Filaments
Chen Xing, Haochuan Li, Bei Jiang +2
In this Letter, we investigate the long-duration quasi-static evolution of 12 pre-eruptive filaments (4 active region and 8 quiescent filaments), mainly focusing on the evolution o…
astro-ph.SR2018
Unambiguous Evidence of Filament Splitting-Induced Partial Eruptions
X. Cheng, B. Kliem, M. D. Ding
Coronal mass ejections are often considered to result from the full eruption of a magnetic flux rope (MFR). However, it is recognized that, in some events, the MFR may release only…