As observed in Thomson-scattered white light, coronal mass ejections (CMEs) are manifest
as large-scale expulsions of plasma magnetically driven from the corona in the most …

We review and summarize the applications of the Grad-Shafranov (GS) reconstruction
technique to space plasma structures in the Earth's magnetosphere and in the interplanetary …

Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding
CMEs and solar wind structures to undergo rotation and deflection during their propagation …

An extreme geomagnetic storm has the potential to affect various technologies and activities
in space and on the ground, eg, power grids, oil and gas industries, communications …

Using multi-instrument and multiwavelength observations, we studied a coronal mass
ejection (CME) that led to an intense geomagnetic storm on 2023 April 23. The eruption …

An unexpected strong geomagnetic storm occurred on 2018 August 26, which was caused
by a slow coronal mass ejection (CME) from a gradual eruption of a large quiet-region …

Forecasting the geomagnetic effects of solar storms, known as coronal mass ejections
(CMEs), is currently severely limited by our inability to predict the magnetic field …

The flux of Galactic cosmic rays (GCRs) can undergo a Forbush decrease (FD) during the
passage of a shock, sheath region, or magnetic flux rope associated with a coronal mass …

Context. Rising concerns about the impact of space-weather-related disruptions demand
modelling and reliable forecasting of coronal mass ejection (CME) impacts. Aims. In this …

We develop an approach of the Grad–Shafranov (GS) reconstruction for toroidal structures
in space plasmas, based on in situ spacecraft measurements. The underlying theory is the …