The aurorae are generated by the solar wind-a stream of charged particles travelling from the outer layer of the sun, or corona, and slamming into Earth's magnetic field. The colors of the lights-which range from red, blue, and purple to green and yellow-depend on which gaseous molecules (mainly oxygen or nitrogen) collide with the solar particles as well as at what altitude that interaction takes place. (The Greek counterpart is Eos, whose name also means "dawn.") In Late Latin, borealis means "of the north," so aurora borealis literally translates as "dawn of the north." Its polar opposite, australis, means "of the south," giving rise to the name aurora australis, "dawn of the south." Both phenomenon are similar in their dazzling light shows made up of colors interacting in various forms, including vibrant rippling curtains, waving arcs, shimmering bands, and shooting rays. In Latin, aurora means "dawn," and in Roman mythology, Aurora is the personification of dawn. Auroras in the northern hemisphere are known as aurora borealis, or northern lights in the southern hemisphere, they are called aurora australis, or southern lights. Once there, they begin to collide and interact with gaseous atoms and molecules, and visible energy is released in the collisions, which gives observers an aural light show. Auroras on planet Earth have been found to be caused by energetically charged particles that travel from the sun to the Earth on solar wind, and are then magnetically drawn to the poles. In astronomy, an aurora is a luminous phenomenon that consists of streamers, arcs, or ripples of dancing vibrant light that appear in the upper atmosphere of a planet's magnetic polar regions.
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