most citedCharacteristics of events with metric-to-decahectometric type II radio bursts associated with CMEs and flares in relation to SEP events

12 citations · 23 across the 2 of their papers we have counts for

collaborators

7 papers

astro-ph.SR202011 cited

Extensive Study of a Coronal Mass Ejection with UV and WL coronagraphs: the need for multi-wavelength observations

Beili Ying, Alessandro Bemporad, Li Feng +3

Coronal Mass Ejections (CMEs) often show different features in different band-passes. By combining data in white-light (WL) and ultraviolet (UV) bands, we have applied different te…

astro-ph.SR2020

Observations of a quasi-periodic pulsation in the coronal loop and microwave flux during a solar preflare phase

Dong Li, Ying Li, Lei Lu +3

We report a quasi-periodic pulsation (QPP) event simultaneously detected from the spatial displacements of coronal loop at both EUV images and microwave emission during the preflar…

astro-ph.SR2020

Quasi-periodic pulsation detected in Lyman-alpha emission during solar flares

Dong Li, Lei Lu, Zongjun Ning +3

We investigated the quasi-periodic pulsation (QPP) in Lyman-alpha, X-ray and extreme-ultraviolet (EUV) emissions during two solar flares, i.e., an X-class (SOL2012-01-27T) and a C-…

astro-ph.SR201925 cited

Spectroscopic and Stereoscopic Observations of the Solar Jets

Lei Lu, Li Feng, Ying Li +3

We present a comprehensive study of a series of recurrent jets that occurred at the periphery of the NOAA active region 12114 on 2014 July 7. These jets were found to share the sam…

astro-ph.SR2019

Energy partition in two M-class circular-ribbon flares

Q. M. Zhang, J. X. Cheng, L. Feng +6

In this paper, we investigate the energy partition of two homologous M1.1 circular-ribbon flares (CRFs) in active region (AR) 12434. They were observed by \textit{SDO}, \textit{GOE…

astro-ph.SR2019

First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-Correlation Analysis

Beili Ying, Alessandro Bemporad, Silvio Giordano +5

The determination of the speed of Coronal Mass Ejections (CMEs) is usually done by tracking brighter features (such as the CME front and core) in visible light coronagraphic images…