While the curtain-like auroras we see at Earth are green at the bottom and red at the top, NASA’s Cassini spacecraft has shown us similar curtain-like auroras at Saturn that are red at the bottom and purple at the top. This is how the auroras would look to the human eye.
The color difference occurs because Earth’s auroras are dominated by excited nitrogen and oxygen atoms and molecules, and Saturn’s auroras are dominated by excited forms of hydrogen. Within each element, colors can differ because of atmospheric density, the levels of the atomic version of an element versus the molecular version, and the energy of impacting electrons.
The height of this particular part of the aurora is about 870 miles (1,400 kilometers).
This image from Cassini’s imaging cameras shows particularly bright auroras on Nov. 29, 2010. Star tracks appear in the clear sky due to the spacecraft’s motion. Color was derived from the measurements in red, green and blue filters. In the annotated version, the longitude and latitude are marked on the planet with white dashed lines. An unannotated version is also available.
The Cassini Solstice Mission is a joint United States and European endeavor. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter was designed, developed and assembled at JPL. The imaging team consists of scientists from the US, England, France, and Germany. The imaging operations center and team lead (Dr. C. Porco) are based at the Space Science Institute in Boulder, Colo.
Excerpt from above, is from the page of Cassini Solstice Mission visit http://ciclops.org, http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.
Released: February 11, 2014