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 …

Context. Solar coronal mass ejections (CMEs) can catch up and interact with preceding
CMEs and solar wind structures to undergo rotation and deflection during their propagation …

The Sun is a variable active-dynamo star, emitting radiation in all wavelengths and solar-
wind plasma to the interplanetary space. The Earth is immersed in this radiation and solar …

Coronal mass ejections (CMEs) are the major space weather drivers, and an accurate
modeling of their onset and propagation up to 1 AU represents a key issue for more reliable …

We present here an interesting two-step filament eruption during 14–15 March 2015. The
filament was located in NOAA AR 12297 and associated with a halo Coronal Mass Ejection …

We studied an Earth-directed coronal mass ejection (CME) that erupted on 2015 March 15.
Our aim was to model the CME flux rope as a magnetized structure using the European …

Interplanetary coronal mass ejections (ICMEs) are important drivers of space-weather
disturbances observed at the Earth. We use a parameterized ICME model to investigate the …

It is generally accepted that extreme space weather events tend to be related to strong flares
and fast halo coronal mass ejections (CMEs). In the present paper, we carefully identify the …

We investigate the solar wind structure for 11 cases that were selected for the campaign
study promoted by the International Study of Earth-affecting Solar Transients (ISEST) …

We present a magnetohydrodynamic model of solar eruption based on the dynamic state
transition from the quasi-static state to the eruptive state of an active region (AR) magnetic …