activity
20182026
most citedSolar Magnetic Flux Rope Eruption Simulated by a Data-Driven Magnetohydrodynamic Model

63 citations · 96 across the 9 of their papers we have counts for

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Showing astro-ph.SRShow all

10 papers · 1 filter

astro-ph.SR2026

Statistics of Solar Filament Mass based on CHASE Sun-as-a-star Spectroscopic Observations

T. Y. Xie, Z. H. Zhao, X. Cheng +5

Filaments are cool and dense plasmas suspended in the hot corona of the Sun and other stars. Accurately estimating their masses is of great significance for understanding subsequen…

astro-ph.SR2026

Limb Shift of the Fe I 6569 Å line on the Sun

H. C. Yu, M. D. Ding, J. Hong +2

The convective motions of solar granules generate a center-to-limb variation of Doppler velocity in the photospheric lines, known as the limb shift effect. This study presents a co…

astro-ph.SR2025

Data-constrained magnetohydrodynamic simulation of global solar corona including solar wind effects within 2.5

Yihua Li, Guoyin Chen, Jinhan Guo +6

Total solar eclipses (TSEs) provide a unique opportunity to observe the large-scale solar corona. The solar wind plays an important role in forming the large-scale coronal structur…

astro-ph.SR20253 cited

The Kinematical Behavior of Solar Eruptive Filaments Affected by the Poloidal Magnetic Field

Ye Qiu, Yang Guo, Mingde Ding +3

Kinematics of solar eruptive filaments is one of the important diagnostic parameters for predicting whether solar eruptions would induce geomagnetic storms. Particularly, some geom…

astro-ph.SR20257 cited

Observational Study of Recurrent Jets: Evolution of Magnetic Flux, Current, and Helicity

Chang Zhou, Yang Guo, Guoyin Chen +2

We observed three recurrent blowout jets in an active regio with Atmospheric Imaging Assembly (AIA) aboard the Solar Dynamics Observatory (SDO). Using Helioseismic Magnetic Imager…

astro-ph.SR2024

Developing an Automated Detection, Tracking and Analysis Method for Solar Filaments Observed by CHASE via Machine Learning

Z. Zheng, Q. Hao, Y. Qiu +3

Studies on the dynamics of solar filaments have significant implications for understanding their formation, evolution, and eruption, which are of great importance for space weather…