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An Aurora Watcher's Guide

What to look for when viewing these celestial dancing lights.

by Robert H. Eather

All-sky aurora
Finnish photographer Pekka Parviainen is known worldwide for his photographs of atmospheric and astronomical phenomena. This all-sky view shows the converging streamers that typify an auroral corona.
The earliest known references to auroras date back to the Old Testament, and in the 2,500 years since then the northern lights have fascinated casual skywatchers and scientists alike. But probably fewer than 5 percent of the Earth's inhabitants during this period have ever seen an aurora, since auroras usually appear only at high northern and southern latitudes, far from the world's population centers.

However, dedicated skywatchers who keep their eyes open have a much better chance than the public at large. And the odds of sighting an aurora on any given night are about at their best right now (2000) and will remain so through the next couple of years. Auroras make their way down to temperate latitudes during magnetic storms (temporary disturbances in the Earth's magnetic field) that originate from activity on the Sun.

Earth's magnetosphere
The solar wind transforms the Earth’s magnetic field into a weathervane, a long 'tear-drop' cavity confined by the solar wind and the magnetic field it carries with it. The bow of our magnetosphere bears the brunt of the solar gale and manages to splash the solar ions around and behind us. From time to time, some plasma reaches the Earth and enlivens the perpetual auroral circles around the magnetic poles.
Sky & Telescope: Gregg Dinderman.



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