Solar wind | Interplanetary Medium, Heliosphere, Plasma
https://www.britannica.com/science/solar-wind
WEBSolar wind, flux of particles, chiefly protons and electrons together with nuclei of heavier elements in smaller numbers, that are accelerated by the high temperatures of the solar corona, or outer region of the Sun, to velocities large enough to allow them to escape from the Sun’s gravitational.
DA: 60 PA: 25 MOZ Rank: 42