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 …

The Sun is an active star that can launch large eruptions of magnetized plasma into the
heliosphere, known as coronal mass ejections (CMEs). These can drive shocks that …

Context. Meter-wavelength type II solar radio bursts are thought to be the signatures of
shock-accelerated electrons in the corona. Studying these bursts can give information about …

Context. One of the most prominent sources for energetic particles in our Solar System are
huge eruptions of magnetised plasma from the Sun, known as coronal mass ejections …

We have investigated type II radio bursts in the solar corona using data from ground‐based
radio telescopes (> 18 MHz) and from the Radio and Plasma Wave experiment (WAVES) on …

Context. Coronal mass ejections (CMEs) are eruptive phenomena that can accelerate
energetic particles and drive shock waves. The CME-driven shocks propagate from the low …

Stellar coronal mass ejections (CMEs) remain observationally elusive, but could have
important implications for exoplanet habitability. Low-frequency radio bursts, known as Type …

Solar energetic particle (SEP) events are commonly separated in two categories: numerous
“impulsive” events of relatively short duration, and a few “gradual” events, where SEP …

Ground-based observations of metric (coronal) type II radio bursts are compared with
observations of coronal mass ejections (CMEs) obtained by the LASCO coronagraph …

Context. The Sun produces the most powerful explosions in the Solar System, solar flares,
which can also be accompanied by large eruptions of magnetised plasma, coronal mass …