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) were discovered in the early 1970s when space-borne
coronagraphs revealed that eruptions of plasma are ejected from the Sun. Today, it is known …

Magnetic fields suspend the relatively cool material of solar prominences in an otherwise hot
corona. A comprehensive understanding of solar prominences ultimately requires complex …

Abstract Coronal Mass Ejections (CMEs) are the key drivers of strong to extreme space
weather storms at the Earth that can have drastic consequences for technological systems in …

We present a clear case study on the occurrence of two successive X-class flares, including
a decade-class flare (X9. 3) and two coronal mass ejections (CMEs) triggered by shearing …

A key aim in space weather research is to be able to use remote-sensing observations of the
solar atmosphere to extend the lead time of predicting the geoeffectiveness of a coronal …

Coronal mass ejections (CMEs) are large-scale expulsions of coronal plasma and magnetic
field propagating through the heliosphere. Because CMEs are observed by white-light …

In this work, we present results of a time-dependent data-driven numerical simulation
developed to study the dynamics of coronal active region magnetic fields. The evolving …

Coronal mass ejections (CMEs) are large eruptions of plasma and magnetic field from the
low solar corona into the heliosphere. These eruptions are often associated with energetic …

We report a detailed analysis of interplanetary flux ropes observed at Venus and
subsequently at Earth's Lagrange L1 point between June 15 and 17, 2012. The observation …