Interplanetary coronal mass ejections (ICMEs) are large-scale heliospheric transients that
originate from the Sun. When an ICME is sufficiently faster than the preceding solar wind, a …

This work reviews factors which are important for the evolution of habitable Earth-like
planets such as the effects of the host star dependent radiation and particle fluxes on the …

Solar flares are often accompanied by filament/prominence eruptions (~ 104 K and~ 1010−
11 cm− 3), sometimes leading to coronal mass ejections that directly affect the Earth's …

The search for life in the Universe is a fundamental problem of astrobiology and modern
science. The current progress in the detection of terrestrial-type exoplanets has opened a …

The changing view of planets orbiting low mass stars, M stars, as potentially hospitable
worlds for life and its remote detection was motivated by several factors, including the …

Atmospheric erosion of CO2-rich Earth-size exoplanets due to coronal mass ejection (CME)-
induced ion pick up within close-in habitable zones of active M-type dwarf stars is …

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 …

The authors concentrate on observations that show the solar-stellar connection or point to
probable future stellar observations. Contents: 1. Introduction. 2. History of solar and stellar …

The first flare on the Sun was observed exactly 150 years ago. During most of the long
history, only secondary effects have been noticed, so flares remained a riddle. Now the …

Coherent radio bursts detected from M dwarfs have some analogy with solar radio bursts but
reach orders of magnitude higher luminosities. These events trace particle acceleration …