Solar eruptive phenomena embrace a variety of eruptions, including flares, solar energetic
particles, and radio bursts. Since the vast majority of these are associated with the eruption …

Solar prominences are one of the most common features of the solar atmosphere. They are
found in the corona but they are one hundred times cooler and denser than the coronal …

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 …

The Sun, as an active star, is the driver of energetic phenomena that structure interplanetary
space and affect planetary atmospheres. The effects of Space Weather on Earth and the …

Current efforts in space weather forecasting of CMEs have been focused on predicting their
arrival time and magnetic structure. To make these predictions, methods have been …

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 …

Coronal mass ejections (CMEs) are relatively a recently discovered phenomenon—in 1971,
some 15 years into the Space Era. It took another two decades to realize that CMEs are the …

Solar coronal mass ejections (CMEs) are the most significant drivers of adverse space
weather on Earth, but the physics governing their propagation through the heliosphere is not …

We study the interaction of two successive coronal mass ejections (CMEs) during the 2010
August 1 events using STEREO/SECCHI COR and heliospheric imager (HI) data. We obtain …

PyThea is a newly developed open-source Python software package that provides tools to
reconstruct coronal mass ejections (CMEs) and shocks waves in three dimensions, using …