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 …

This paper will review the input of 65 years of radio observations to our understanding of
solar and solar–terrestrial physics. It is focussed on the radio observations of phenomena …

Abstract We present the “Drag-Based Model”(DBM) of heliospheric propagation of
interplanetary coronal mass ejections (ICMEs). The DBM is based on the hypothesis that the …

Ensemble modeling of coronal mass ejections (CMEs) provides a probabilistic forecast of
CME arrival time that includes an estimation of arrival-time uncertainty from the spread and …

We present results from a set of numerical simulations aimed at exploring the mechanism of
coronal mass ejection (CME) suppression in active stars by an overlying large-scale …

Using the potential of two unprecedented missions, Solar Terrestrial Relations Observatory
(STEREO) and Reuven Ramaty High-Energy Solar Spectroscopic Imager (RHESSI), we …

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 …

We analyze the relationship between the coronal hole (CH) area/position and physical
characteristics of the associated corotating high-speed stream (HSS) in the solar wind at 1 …

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 …

Context. The propagation of interplanetary coronal mass ejections (ICMEs) and the forecast
of their arrival on Earth is one of the central issues of space weather studies. Aims. We …