most citedTransverse coronal loop oscillations excited by homologous circular-ribbon flares

29 citations · 99 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.SR2021★ 29 cited

A unified model of solar prominence formation

C. J. Huang, J. H. Guo, Y. W. Ni +2

Several mechanisms have been proposed to account for the formation of solar prominences or filaments, among which direct injection and evaporation-condensation models are the two m…

astro-ph.SR2021★ 4 cited

Energy partition in a confined flare with an extreme-ultraviolet late phase

Q. M. Zhang, J. X. Cheng, Y. Dai +2

In this paper, we reanalyze the M1.2 confined flare with a large extreme-ultraviolet (EUV) late phase on 2011 September 9, focusing on its energy partition. The radiation (5.…

astro-ph.SR2020★ 29 cited

Transverse coronal loop oscillations excited by homologous circular-ribbon flares

Q. M. Zhang, J. Dai, Z. Xu +4

We report our multiwavelength observations of two homologous circular-ribbon flares (CRFs) in active region 11991 on 2014 March 5, focusing on the transverse oscillations of an ext…

astro-ph.SR2020★ 8 cited

Does a solar filament barb always correspond to a prominence foot?

Y. Ouyang, P. F. Chen, S. Q. Fan +2

Solar filaments are dark structures on the solar disk, with an elongated spine and several barbs extending out from the spine. When appearing above the solar limb, a filament is ca…

astro-ph.SR2020★ 29 cited

Longitudinal filament oscillations enhanced by two C-class flares

Q. M. Zhang, J. H. Guo, K. V. Tam +1

In this paper, we report the multiwavelength observations of a very long filament in active region (AR) 11112 on 2010 October 18. The filament was composed of two parts, the easter…