Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

This review article summarizes the advancement in the studies of Earth-affecting solar
transients in the last decade that encompasses most of solar cycle 24. It is a part of the effort …

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 …

Much progress has been made in the study of coronal mass ejections (CMEs), the main
drivers of terrestrial space weather thanks to the deployment of several missions in the last …

Our host star, the Sun, is a middle-aged main sequence G type star whose activity varies.
These variations are primarily governed by solar magnetic fields which are produced in the …

Magnetic flux rope (MFR) is the core structure of the greatest eruptions, that is, the coronal
mass ejections (CMEs), on the Sun, and magnetic clouds are posteruption MFRs in …

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 …

The magnetic flux rope is among the most fundamental magnetic configurations in plasma.
Although its presence after solar eruptions has been verified by spacecraft measurements …

Episodic ejections of blobs (episodic jets) are widely observed in black hole sources and
usually associated with flares. In this paper, by performing and analyzing three-dimensional …

We provide evidence for particle acceleration up to∼ 5 MeV at reconnecting current sheets
in the solar wind based on both case studies and a statistical analysis of the energetic ion …