activity
20062021
most citedA Tracker Solution for a Holographic Dark Energy Model

125 citations · 620 across the 28 of their papers we have counts for

collaborators

28 papers

astro-ph.SR2021★ 4 cited

Spectral evolution of an eruptive polar crown prominence with IRIS observations

Jianchao Xue, Hui Li, Yang Su

Prominence eruption is closely related to coronal mass ejections and is an important topic in solar physics. Spectroscopic observation is an effective way to explore the plasma pro…

astro-ph.SR2021

High-Resolution Observations of Prominence Plume Formation with the New Vacuum Solar Telescope

Jian-Chao Xue, Jean-Claude Vial, Yang Su +5

Prominence plumes are evacuated upflows that emerge from bubbles below prominences, whose formation mechanism is still unclear. Here we present a detailed study of plumes in a quie…

astro-ph.SR2020

Simulations of stray light from the surface scattering of the Solar Corona Imager primary mirror

Jianchao Xue, Marco Romoli, Federico Landini +4

The Solar Corona Imager is an internally occulted coronagraph on board the ASO-S mission, which has the advantage of imaging the inner corona in H I {Lyman-\textalpha} (Ly-alpha) a…

astro-ph.SR2020★ 35 cited

Thermodynamical Evolution of Supra-Arcade Downflows

Jianchao Xue, Yang Su, Hui Li +1

Supra-arcade downflows (SADs) are dark, teardrop-shaped features descending upon flare arcades. They are thought to be the results of magnetic reconnection, but the detailed format…

astro-ph.SR2020★ 7 cited

Radiative Hydrodynamic Simulations of the Spectral Characteristics of Solar White-light Flares

Yu-Tong Yang, Jie Hong, Ying Li +2

As one of the most violent activities in the solar atmosphere, white-light flares (WLFs) are generally known for their enhanced white-light (or continuum) emission, which primarily…

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…