The phenomenon of quasi-periodic pulsations (QPPs) in solar and stellar flares has been
known for over 50 years and significant progress has been made in this research area. It has …

The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …

Magnetic reconnection is a multi-faceted process of energy conversion in astrophysical,
space and laboratory plasmas that operates at microscopic scales but has macroscopic …

摘要随着空间光学技术的快速发展以及光电探测器件性能的不断提升, 高分辨率, 多光谱,
低探测阈值的遥感系统在航空, 航天等领域的应用越来越广泛, 对光电载荷的杂光抑制能力与 …

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime
possibility to heat the low corona to millions of degrees. Here, we present ultra-high …

Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As
they are driven by their footpoint motions on the solar surface, which transport energy from …

Magnetic reconnection is a fundamental process of topology change and energy release,
taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory …

Coronal mass ejections (CMEs) and solar flares are the large-scale and most energetic
eruptive phenomena in our solar system and able to release a large quantity of plasma and …

Abstract The Solar Upper Transition Region Imager (SUTRI) onboard the Space Advanced
Technology demonstration satellite (SATech-01), which was launched to a Sun …

We present a clear case study on the occurrence of two successive X-class flares, including
a decade-class flare (X9. 3) and two coronal mass ejections (CMEs) triggered by shearing …