What Causes the Auroral Lights?


This animation demonstrates very simply how different elements at different heights, let off energy that we see as different colors. You'll notice in the static aurora picture, it almost seems as if there are layers of colors one on top of the other.
Movie adapted from original clips provided courtesy of Professor Patricia Reiff, Rice University Connections Program
High speed ions and electrons travel along magnetic field lines and impact the atmosphere in the region called the auroral oval. Atmospheric gases are excited by these high speed collisions and give off different types of light as they relax back to their normal states. The color and altitude of the aurora tell us which atmospheric gases are being excited.
  • Below 60 miles in altitude, nitrogen is responsible for blue and red auroral light.
  • Above this and upwards to 150 miles altitude, green light is produced by excited oxygen atoms.
  • Above 150 miles, red light from oxygen dominates the auroral glow.

Since blue, green and red light are being produced in various combinations at various altitudes, it mixes to give an incredible variety of colors (such as purple and pink).

Visit the Space Weather section to learn more about the aurora

You might also be interested in:

Traveling Nitrogen Classroom Activity Kit

Check out our online store - minerals, fossils, books, activities, jewelry, and household items!...more

AU

AU stands for Astronomical Units. Distances in space are too large to measure in Earth standards like miles or kilometers. For distances too large to measue in AU, we use light years. A light year is the...more

The Spiral of the IMF

The solar wind is formed as the Sun's topmost layer blows off into space carrying with it magnetic fields still attached to the Sun. Gusts and disturbances form in the solar wind associated with violent...more

Spiral Path of Material

For a planet to be affected by a blob of material being ejected by the sun, the planet must be in the path of the blob, as shown in this picture. The Earth and its magnetosphere are shown in the bottom...more

The SAR Arc

The aurora we are most familiar with is the polar aurora. This is what people are referring to when they speak of the northern or southern lights. But there are other less-known auroral activity, such...more

The Effect of Aurora on the Atmosphere

This figure shows the effect of the aurora on the atmosphere. When FAC's enter the atmosphere and create the aurora, they warm the atmosphere impulsively. This impulse travels throughout the atmosphere...more

The forming Aurora

This picture illustrates the streaming of particles into and out of the auroral zone, as Field-aligned currents (FAC's) short-circuit through the ionosphere. Some of the particles entering the auroral...more

The Expanding Auroral Oval

This figure shows a series of images of the auroral oval as it expands over the course of about an hour in response to a geomagnetic storm. This is an animation of the expanding auroral oval....more

Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part is sponsored in part through grants from federal agencies (NASA and NOAA), and partnerships with affiliated organizations, including the American Geophysical Union, the Howard Hughes Medical Institute, the Earth System Information Partnership, the American Meteorological Society, the National Center for Science Education, and TERC. The American Geophysical Union and the American Geosciences Institute are Windows to the Universe Founding Partners. NESTA welcomes new Institutional Affiliates in support of our ongoing programs, as well as collaborations on new projects. Contact NESTA for more information. NASA ESIP NCSE HHMI AGU AGI AMS NOAA