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 …

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 …

In this paper we present the results of a statistical study of the accelerations of coronal mass
ejections (CMEs). A CME usually undergoes a multiphased kinematic evolution, with a main …

Solar coronal mass ejections (CMEs) and flares have a statistically well-defined relationship,
with more energetic X-ray flares corresponding to faster and more massive CMEs. How this …

We present a statistical study of prominence and filament eruptions observed by the
Atmospheric Imaging Assembly (AIA) onboard the Solar Dynamics Observatory (SDO) …

Flares and coronal mass ejections (CMEs) are very powerful events in which energetic
radiation and particles are ejected within a short time. These events thus can strongly affect …

We examine the early phases of two near-limb filament destabilizations involved in coronal
mass ejections (CMEs) on 2005 June 16 and July 27, using high-resolution, high-cadence …

We re-examine observations bearing on the origin of metric type II bursts for six impulsive
solar events in November 1997. Previous analyses of these events indicated that the metric …

We explore the scenario of a coronal mass ejection (CME) being the cause of the observed
continuous X-ray absorption of the 1997 August 30 superflare on the eclipsing binary Algol …

Aims. We aim to examine the precursor phases and early evolution of a prominence
eruption associated with a M4-class flare and a partial halo coronal mass ejection (CME) …