Context. Type II radio bursts are a type of solar radio bursts associated with coronal shocks.
Type II bursts usually exhibit fine structures in dynamic spectra that represent signatures of …

On 21 April 2023, a significant M1. 7 solar flare erupted from Active Region 13283,
accompanied by a filament eruption and a full-halo Coronal Mass Ejection, which reached …

Context. Fast coronal mass ejections (CMEs) can drive shock waves capable of accelerating
electrons to high energies. These shock-accelerated electrons act as sources of …

We select and investigate six global solar extreme-ultraviolet (EUV) wave events using data
from the Solar Dynamics Observatory and the Solar and Heliospheric Observatory. These …

Coronal mass ejections (CMEs) are often associated with X-ray (SXR) flares powered by
magnetic reconnection in the low corona, while the CME shocks in the upper corona and …

Aims. Solar radio type II bursts are often associated with coronal shocks driven by solar
eruptions. In this study, we report a type II burst associated with filament–filament interaction …

Since fast head-on coronal mass ejections and their associated shocks represent potential
hazards to the space environment of the Earth and even other planets, forecasting the arrival …

In this paper, we present for the first time a comprehensive statistical study between type II
radio bursts from the metric (m) to the dekameric–hectometric (DH) domain and their …

In this study, we compile a catalog of metric type II radio bursts using the Radio Solar
Telescope Network (RSTN) to study the occurrence, associations, and properties of the …

Understanding and predicting the geoeffectiveness of solar activity on Earth is crucial for
space weather. Therefore, predicting the impact of coronal mass ejections (CMEs) and their …