The Northern Lights
Brandy Bones
Issue date: 11/12/04 Section: Arts & Features
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The most impressive view was to the north, where the aurora borealis, as it is properly known, seemed to be vibrating to an intense rhythm while refracting spectacular colors up its length. It was a clear night with a few clouds poetically interrupting the beams of light. As if this was not enough to complete our weekend and happily begin our Monday, one friend saw a shooting star streak across the sky. We took it in for 20 minutes or so, satisfied that we had caught the best of the Earth's laser show. By the time we left, the Northern Lights were still visible, but the sky had calmed down a bit; the tempo of the beams had lessened and the colors had relaxed.
"The aurora seen on Sunday night lasted throughout the night until dawn on Monday," explained Professor of Physics and Astronomy Thomas J. Balonek. "This was the most spectacular aurora seen from Colgate since the early 90's." (Some previous intense Northern Lights displays in the last several years were clouded out in Hamilton.) "At its peak, the lights covered about two-thirds of the sky, stretching down to the middle of the southern sky. The entire northern sky was full of rapidly changing types of auroral activity."
The aurora borealis phenomenon is caused when material thrown off the surface of the sun collides with the atmosphere of the Earth. Highly charged electrons from the solar winds leave the sun at speeds of one million miles per hour, and reaching the earth and following the magnetic force of the Earth's core. When these electrons enter the upper atmosphere, they collide with different atoms and give off this energy as light: oxygen gives off green and red light, while nitrogen gives off blue and purple. The light is created in much the same way that a neon sign functions, with electrons passing through gases in tubes. The reverberations of the Northern Lights are caused by the constantly changing combination of magnetic and electrical forces.
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