Volume: 03, Issue: 07 04/06/2005 
This view of the Aurora Australis, or Southern Lights, which was photographed by an astronaut aboard Space Shuttle Discovery (STS-39) in 1991, shows a spiked band of red and green aurora above the Earth's Limb. Image courtesy NASA.
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The NASA Polar spacecraft took this series of images of the aurora over the northern hemisphere. The most intense auroral activity appears in bright red or white. Image courtesy Univ. of Iowa/NASA Scientific Visualization Studio.
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This series of near-simultaneous auroras were observed between 6:24am and 7:10am ET on Oct. 23, 2002. Observations were made of the northern (left) and southern (right) hemispheres by IMAGE and Polar satellites, respectively. Image courtesy NASA.
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Other Articles in This Issue:
Space Shuttle Discovery Moves to Launch Pad
Spirit and Opportunity Head for Triple Overtime
Deep Impact Cruises toward Comet
Enhance Your Teaching Skills Online
 

Northern Lights and Southern Lights Are Not Mirror Images

Scientists gazing at Earth's Northern and Southern Lights were surprised to find they are not mirror images of each other, as was once thought. Instead, the auroras move and change independently based on the "tilt" of the Earth's magnetic field toward the Sun and conditions in the solar wind.

Analysis of the images from NASA's Polar spacecraft and the Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) spacecraft showed how the auroras move and change. The main cause behind the differences appears to be the interaction between the Sun's outer atmosphere and the Earth's magnetic field.

By knowing how auroras react to solar wind, scientists can better determine the impacts of space weather in the future. The new discovery by scientists from NASA, the University of Iowa, Iowa City, and the University of California at Berkeley, shows that auroras may be more complicated than previously thought.

The aurora form near-circular bands around both the northern and southern poles of the Earth, known as the auroral ovals. These phenomena also are known as the aurora borealis, or northern lights, and the aurora australis, or southern lights. It was expected that the auroral ovals would be mirror images of each other.

"This is the first analysis to use simultaneous observations of the whole aurora in both the Northern and Southern Hemispheres to track their locations," said lead author Timothy J. Stubbs of the Laboratory for Extraterrestrial Physics at NASA's Goddard Space Flight Center.

The Sun's outer atmosphere is an extremely thin electrified gas, or "plasma," better known as the "solar wind," since it blows constantly out from the Sun at around 250 miles per second. The Earth's magnetic field provides an obstacle in the solar wind flow and becomes compressed into an extended teardrop-shaped bubble known as the "magnetosphere."

The magnetosphere protects the Earth by shielding it from the solar wind. However, under certain conditions charged particles from the solar wind are able to penetrate this magnetic shield and become energized. Collisions between these charged particles and the Earth's upper atmosphere emit light which we observe as an "aurora."

Stubbs and his colleagues used data from the two spacecraft to study the auroras. By luck, the orbits of Polar and IMAGE were aligned so the entire auroral ovals in both hemispheres could be observed simultaneously in detail.

Stubbs and his colleagues noted four important items in their study of auroras observed in October 2002. As predicted, they observed the auroral ovals shift in opposite directions to each other depending on the orientation of the Interplanetary Magnetic Field (IMF). The IMF is the Sun's magnetic field that travels out into space with the solar wind.

They noted the auroral ovals also shift in opposite directions to each other depending on how far the Earth's northern magnetic pole is leaning toward the Sun (known as the "dipole tilt angle").

Following a change in the orientation of the IMF, they observed the southern auroral oval shift toward the Sun while the northern auroral oval remained in about the same location. The scientists believe the southern aurora moved because the solar wind was able to penetrate into the magnetosphere in the southern hemisphere, but not in the northern hemisphere.

What was most surprising was that both the northern and southern auroral ovals were leaning toward the dawn (morning) side of the Earth for this event. The scientists suspect the leaning may be related to "imperfections" of the Earth's magnetic field. The Earth has a similar type of magnetic field to that which occurs around a simple bar magnet, which causes iron filings to arrange themselves in loops around it.

"Because Earth's magnetic field is not a perfect dipole, we think this fact plays some role in causing the auroras to not be mirror images of each other," Stubbs said.

For more information and images related to this story on the Internet, visit http://www.nasa.gov/vision/earth/lookingatearth/dueling_auroras.html .

    
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