Having watched many Northern Lights (and one Southern Lights in Australia), I am fascinated by these dancing curtains of colour. This week came news that scientists looking at the Earth's Northern and Southern auroras have been surprised to find they are not mirror images of each other, as was once thought. The main cause behind the differences appears to be the interaction between the Sun's outer atmosphere and the Earth's magnetic field.
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, based on the tilt of the Earth's magnetic field toward the Sun and conditions in the Solar Wind.
By knowing how auroras react to the 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.
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 Earths 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 Suns 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.
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.
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