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13 bytes added ,  03:30, September 11, 2007
Added reference to aurora australis. Changed description of auroral mechanism.
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An aurora, or polar aurora, is a glow in the sky, seen often in a ring-shaped region around the [[magnetic pole]]s ("auroral zone") and occasionally further equatorward. The name comes from an older one, "aurora borealis," [[Latin]] for "northern dawn," given because an aurora near the northern [[horizon]] (its usual location when seen in most of [[Europe]]) looks like the glow of the sky preceding [[sunrise]]. Also known as "northern lights," although it occurs both north and south of the [[equator]].
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An aurora ([[Latin]] for "dawn"), or polar aurora, is a glow in the sky, seen often in a ring-shaped region around the [[magnetic pole]]s ("auroral zone") and occasionally further equatorward. Auroras occur at both [[magnetic pole]]s of the Earth.  In the northern hemisphere, the phenomenon is referred to as the aurora borealis or the "northern lights".  In the southern hemisphere, it is called the aurora australis.
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The aurora is generally caused by fast [[electron]]s from space, guided earthward by magnetic field lines, and its light comes from collisions between such electrons and the [[atom]]s of the upper [[atmosphere]], typically 100 km (60 miles) above ground.
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Charged, energized particles from the sun, called the [[solar wind]], are captured by the Earth's magnetic field.  The particles collide with [[atom]]s in the upper [[atmoshpere]], causing the [[atom]]s to become energized.  These energized [[atom]]s then release their excess energy as light. 
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Auroras typically occur 100 km (60 miles) above ground.  
 
[[Category:Physics]]
 
[[Category:Physics]]

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