activity
20152026
most citedWhy does the apparent mass of a coronal mass ejection increase?

32 citations · 302 across the 29 of their papers we have counts for

collaborators
Showing 2020Show all

5 papers · 1 filter

astro-ph.SR2020★ 10 cited

Three-Dimensional Reconstructions of Coronal Wave Surfaces Using a New Mask-Fitting Method

Li Feng, Lei Lu, Bernd Inhester +5

Coronal waves are large-scale disturbances often driven by coronal mass ejections (CMEs). We investigate a spectacular wave event on 7 March 2012, which is associated with an X5.4…

astro-ph.SR2020★ 9 cited

An investigation of flare emissions at multiple wavelengths

Dong Li, Alexander Warmuth, Lei Lu +1

We report multi-wavelength observations of four solar flares on 2014 July 07. We firstly select these flares according to the soft X-ray (SXR) and extreme ultraviolet (EUV) emissio…

astro-ph.SR2020★ 11 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★ 27 cited

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★ 29 cited

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-…