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 …

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 present a review of the different aspects associated with the interaction of successive
coronal mass ejections (CMEs) in the corona and inner heliosphere, focusing on the …

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 …

Solar eruptions are the main driver of space-weather disturbances at Earth. Extreme events
are of particular interest, not only because of the scientific challenges they pose, but also …

Coronal mass ejections (CMEs) are arguably the most violent eruptions in the solar system.
CMEs can cause severe disturbances in interplanetary space and can even affect human …

Magnetic flux ropes are characterized by coherently twisted magnetic field lines, which are
ubiquitous in magnetized plasmas. As the core structure of various eruptive phenomena in …

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 …

ICMEs (interplanetary coronal mass ejections), the heliospheric counterparts of what is
observed with coronagraphs at the Sun as CMEs, have been the subject of intense interest …

Coronal mass ejections (CMEs) play an important role in space weather. The propagation
characteristics of CMEs in the Corona and interplanetary space determine whether, when …