The Aurora

The aurora is formed when protons and electrons from the Sun travel along the Earth's magnetic field lines. These particles from the Sun are very energetic. We are talking major-league energy, much more than the power of lightning: 20 million amps at 50,000 volts is channeled into the auroral oval. It's no wonder that the gases of the atmosphere light up like the gases of a streetlamp!

The aurora is also known as the northern and southern lights. From the ground, they can usually be seen where the northern and southern auroral ovals are on the Earth. The northern polar auroral oval usually spans Fairbanks, Alaska, Oslo, Norway, and the Northwest Territories. Sometimes, when the Sun is active, the northern auroral oval expands and the aurora can be seen much farther south.

The image to the left shows the northern oval where the aurora lights up the atmosphere, and the aurora which is found at the equator, called the equatorial arcs.

This left-hand image shows the northern auroral oval (the bright ring on the top of the silhouetted Earth) and the equatorial arcs (the red traces towards the center of the silhouetted Earth). The right image focuses on the northern auroral oval.
Click on image for full size version (55K GIF)
Image provided by Dynamics Explorer courtesy of L. Frank

Pictures of the Aurora

What is a Magnetosphere?

Find out more about the aurora in our Space Weather section

A Tale about the Aurora from the Menominee Tribe.





Last modified December 2, 1997 by the Windows Team

The source of this material is Windows to the Universe, at http://www.windows.ucar.edu/ at the University Corporation for Atmospheric Research (UCAR). ©1995-1999, 2000 The Regents of the University of Michigan; ©2000-01 University Corporation for Atmospheric Research. All Rights Reserved. Site policies and disclaimer