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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.SR2024
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.SR2024
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…