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 …

Abstract Space weather refers to dynamic conditions on the Sun and in the space
environment of the Earth, which are often driven by solar eruptions and their subsequent …

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 …

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 …

Abstract Interplanetary Coronal Mass Ejections (ICMEs), their possible shocks and sheaths,
and co-rotating interaction regions (CIRs) are the primary large-scale heliospheric structures …

Forecasting the in situ properties of coronal mass ejections (CMEs) from remote images is
expected to strongly enhance predictions of space weather and is of general interest for …

We use observations from the MErcury Surface, Space ENvironment, GEochemistry, and
Ranging (MESSENGER) spacecraft, in orbit around Mercury, to investigate interplanetary …

We investigate how coronal mass ejections (CMEs) propagate through, and interact with, the
inner heliosphere between the Sun and Earth, a key question in CME research and space …

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 …