most citedA model for heating the super-hot corona in solar active regions

18 citations · 31 across the 6 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2024

Periodic Coronal Rain Driven by Self-consistent Heating Process in a Radiative Magnetohydrodynamic Simulation

Zekun Lu, Feng Chen, J. H. Guo +5

The periodic coronal rain and in-phase radiative intensity pulsations have been observed in multiple wavelengths in recent years. However, due to the lack of three-dimensional coro…

astro-ph.SR202418 cited

A model for heating the super-hot corona in solar active regions

Zekun Lu, Feng Chen, M. D. Ding +3

What physical mechanisms heat the outer solar or stellar atmosphere to million-Kelvin temperatures is a fundamental but long-standing open question. In particular, the solar corona…

astro-ph.SR20241 cited

Sun-as-a-star Study of an X-class Solar Flare with Spectroscopic Observations of CHASE

Y. L. Ma, Q. H. Lao, X. Cheng +5

Sun-as-a-star spectroscopic characteristics of solar flares can be used as a benchmark for the detection and analyses of stellar flares. Here, we study the Sun-as-a-star properties…

astro-ph.SR2024

Generalized Coronal Loop Scaling Laws and Their Implication for Turbulence in Solar Active Region Loops

Y. Dai, J. J. Xiang, M. D. Ding

Recent coronal loop modeling has emphasized the importance of combining both Coulomb collisions and turbulent scattering to characterize field-aligned thermal conduction, which inv…

astro-ph.SR2024

The White-light Emissions in Two X-class Flares Observed by ASO-S and CHASE

Ying Li, Zhichen Jing, De-Chao Song +9

The white-light continuum emissions in solar flares (i.e., white-light flares) are usually observed on the solar disk but, in a few cases, off the limb. Here we present on-disk as…

astro-ph.SR202412 cited

Three-dimensional velocity fields of the solar filament eruptions detected by CHASE

Ye Qiu, Chuan Li, Yang Guo +3

The eruption of solar filaments, also known as prominences appearing off-limb, is a common phenomenon in the solar atmosphere. It ejects massive plasma and high-energy particles in…