|
Auroras: billboards for electric space
Spectacular auroras are a phenomena whose beauty almost defies description. Triggered by disturbances in the solar wind and Earth's magnetosphere, these curtains of light occur when high energy electrons and ions in the magnetotail are energized and are guided towards the polar regions by Earth's magnetic field. At about 70 miles above the surface, fast moving electrons encounter Earth's upper atmosphere, where they slam into gas molecules, making them glow: oxygen molecules glow whitish-green, nitrogen molecules glow pink. Contrary to popular belief, aurora do not produce any sounds.
Satellites that orbit thousands of miles above Earth's surface can provide a global view of the aurora that neither the Space Shuttle nor ground observations can. These photographs show that the light of the aurora forms an oval shape - like a crown of light - high above and surrounding Earth's magnetic poles. The auroral oval or zone expands and contracts over a period of hours and days, depending on geomagnetic activity. The auroral zone is about six degrees wide, centered on a magnetic latitude of 67°.
Auroras act as a gauge of what's happening to Earth's magnetic field tens of thousands of miles away. On days that are calm, auroras are only slightly visible, even in the northern latitudes. But during magnetic storms, the auroral oval can grow until it can be seen as far south as Colorado or even Florida.
|
|
Copyright © 1998-1999 Space Science Institute, all rights reserved Comments? Send email to webmaster@spacescience.org. |