Final answer:
The Solar Wind is created when particles from the Sun's fusion escape through the corona and attain sufficient speed to overcome the Sun's gravity. This stream of charged particles can then influence the tails of comets and cause phenomena such as the Aurora Borealis when interacting with Earth's atmosphere.
Step-by-step explanation:
Particles from fusion in the Sun escape through the corona and create the Solar Wind. The solar wind is a stream of charged particles, mainly protons and electrons, that flows outward from the sun into the solar system at considerable speeds. These particles originate from the Sun's corona, where the intense heat and rapid motion of gases allow them to overcome the gravitational pull of the Sun. As they travel through space, they can interact with objects they encounter, such as the tails of comets or the Earth's magnetosphere.
Comets often exhibit two tails due to the effects of solar wind and radiation pressure. The ion tail, composed of ionized gases, interacts electromagnetically with the solar wind and therefore always points away from the Sun. The second, a dust tail, is formed by dust particles affected by the Sun's radiation pressure rather than the solar wind. The northern and southern lights, known as auroras, are another spectacular display created when the solar wind particles collide with Earth's atmosphere.