Solar coronal mass ejections (CMEs) and flares have a statistically well-defined relationship,
with more energetic X-ray flares corresponding to faster and more massive CMEs. How this …

To better understand the physical connections in sympathetic solar eruptions, we
investigated the interaction between two nearby filaments and their successive partial …

Aims. This study focuses on the rapid evolution of the solar filament in active region 12975
during a confined C2 flare on 28 March 2022, which finally led to an eruptive M4 flare 1.5 h …

We present a multiwavelength analysis of two homologous, short-lived, impulsive flares of
GOES class M1. 4 and M7. 3 that occurred from a very localized minisigmoid region within …

In this article, we present a multi-wavelength and multi-instrument investigation of a halo
coronal mass ejection (CME) from active region NOAA 12371 on 21 June 2015 that led to a …

Although magnetic reconnection plays a key role in the formation of a solar filament, the
detailed formation process is still ambiguous. Combining the observational data from the …

We present an investigation of partial filament eruption on 2012 June 17 in the active region
NOAA 11504. For the first time, we observed the vertical splitting process during the partial …

We study a complex GOES M1. 1 circular ribbon flare and related pre-flare activity on 26
January 2015 [SOL2015-01-26T16: 53] in the solar active region NOAA 12268. This flare …

The decay index of solar magnetic fields is known as an important parameter in regulating
solar eruptions from the standpoint of the torus instability. In particular, a saddle-like profile …

Solar filament eruptions are often characterized by stepwise evolution due to the
involvement of multiple mechanisms, such as magnetohydrodynamic instabilities and …