The heating of the solar chromosphere and corona to the observed high temperatures, imply
the presence of ongoing heating that balances the strong radiative and thermal conduction …

Modern observatories have revealed the ubiquitous presence of magnetohydrodynamic
waves in the solar corona. The propagating waves (in contrast to the standing waves) are …

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 …

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 …

As a cool star evolves, it loses mass and angular momentum due to magnetized stellar
winds that affect its rotational evolution. This change has consequences that range from the …

The M dwarf star GJ 436 hosts a warm-Neptune that is losing a substantial amount of
atmosphere, which is shaped by the interactions with the wind of the host star. The stellar …

Our understanding of the formation and evolution of the corona and the heliosphere is linked
to our capability of properly interpret the data from remote sensing and in-situ observations …

Coronal mass ejections (CMEs) on stars other than the Sun have proven very difficult to
detect. One promising pathway lies in the detection of type II radio bursts. Their appearance …

The X-ray and extreme-ultraviolet (EUV) emissions from low-mass stars significantly affect
the evolution of the planetary atmosphere. However, it is observationally difficult to constrain …

The physical properties responsible for the formation and evolution of the corona and
heliosphere are still not completely understood. 3D MHD global modeling is a powerful tool …