Aurora are bright glows caused by collisions between charged particles from the solar wind and atoms in the Earth's upper atmosphere. The solar wind carries the Sun's magnetic field and particles through space at around 400 km/s, shaping the Earth's magnetosphere into an elongated bubble. Under certain conditions, the solar wind's magnetic field can merge with Earth's, creating electrical currents that drive particles into the polar atmosphere, causing the visible auroral displays usually seen in night skies at high latitudes, known as the northern lights in the northern hemisphere and southern lights in the southern hemisphere.