In this review, we explore advances in the study of solar eruptions in recent years from the perspective of observations from space using a multi-messenger and multi-viewpoint approach to the study of solar radiation, plasma and wind. Imaging the solar corona using different wavelengths and analyzing plasma properties, magnetic fields, and kinematic characteristics contributes to our understanding of the physics of the Sun. In addition, space observations of the Sun’s atmosphere
and interactions with the interplanetary environment define the new frontier of Space Weather.
Focusing on the solar perspective of phenomena relevant to Space Weather, coronal mass ejections are some of the most widely studied events from their initiation on the solar disk to interplanetary space. I will describe the approach used by the Solar Orbiter mission and in particular the Metis
coronagraph to derive valuable and innovative insight into formation, evolution, and impact of eruptive phenomena.

