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Last updated on April 17, 2014 at 11:49 EDT

Cluster’s Auroral Acceleration Campaign Yields Results

February 2, 2011

Auroras, more commonly known as the northern and southern lights, are one of the most beautiful and awe-inspiring natural phenomena. New insights into the processes that generate Earth’s auroras (and those of other planets) are now being provided by a flotilla of ESA satellites, known as the Cluster mission, as they sweep through the region of space where these colorful curtains of light are created. As they fly in formation above the planet’s poles, the Cluster spacecraft are gathering the first multi-point observations of auroral nurseries.

The red and green emissions are most commonly created by beams of electrons that are boosted to high velocities by quasi-static parallel electric fields in the auroral acceleration region (AAR), located between 4000 and 12 000 km above the poles. The downward-moving particles collide with the upper atmosphere at altitudes of around 100 km, producing shimmering patterns in the night sky.

“The AAR is a particle accelerator in space, similar to an electron gun in an old TV,” said Arnaud Masson, ESA’s deputy project scientist for Cluster. “It is fed by electrically charged particles that originate in the magnetotail, an elongated region of the magnetosphere located on the nightside of Earth.”

“The AAR is not permanent ““ it comes and goes,” continued Masson. “In the absence of the AAR and Alfv©n waves, the aurora is diffuse or spread out, and not always noticeable to the naked eye. When the AAR is present, bright, discrete arcs can be seen, sometimes with ‘black auroras’ embedded.”

The existence of the AAR has been known for decades. However, there are still many open questions about auroras, including the altitude distribution and stability of the electric fields which accelerate the particles inside these regions. Now, by analyzing the new data from Cluster, these open issues can be tackled for the first time.
Cluster multipoint studies

Since 2006, the Cluster satellites have slowly drifted away from their initial polar orbits. Meanwhile, the perigees (lowest points) of their orbits have decreased from 19 000 km to just a few hundred kilometers, giving Cluster access to new regions of near-Earth space. For the first time, in Spring 2009, scientists could make use of this natural orbital drift to obtain simultaneous measurements of the AAR with more than one satellite.

Some of the first results from the AAR data campaign are published by a team of European and American scientists in the 1 February 2011 issue of the prestigious journal Physical Review Letters. Their paper details the observations made by the Cluster C3 and C1 satellites on 5 June 2009, when they made an oblique crossing of the dusk-side auroral oval between 16:55 and 17:15 UT.

At that time, C1 was flying at an altitude of 9000 km, some 2600 km above its sister craft but lagging about 5 minutes behind. Subsequent analysis of data from the EFW electric field and waves, FGM magnetic field, PEACE electron and CIS ion instruments enabled the team to conduct a unique study of the physical state of the AAR during the flybys.

The dual observations revealed spatial and temporal variations in the electric fields and associated particle signatures For the first time it was possible to constrain the size and longevity of these regions. The data showed that the electric field structures measured at least 800 km across and remained stable for at least 5 minutes.

“The data from this and other events are revealing how the acceleration region and the associated electric potential pattern evolve in time and space, and the time scales over which they can be regarded as stable,” said Professor Göran Marklund from the Royal Institute of Technology, Stockholm, Sweden, who is lead author of the paper.

“These new results do not yet provide a complete explanation of the dynamics of the aurora, since the Cluster instruments are not optimized for measuring this region, but they provide important constraints on how these structures are created. They also provide inputs for simulations and for future multi-point missions that will explore near-Earth space. Similar space plasma processes occur throughout the Solar System, so a greater understanding of Earth’s auroras has implications far beyond our own planet,” he added.



Image 1 Caption: The dark band in the green aurora pictured here is an example of a black aurora. A black aurora isn’t an aurora at all; rather it is a lack of auroral activity. The black aurora is only visible to the naked eye if it is embedded in a region of diffuse (faint) aurora. (Credit: Jan Curtis)

Image 2 Caption: A schematic view of the Cluster C3 and C1 satellite trajectories between 16:55 and 17:15 UT on 5 June 2009. During this period, both satellites collected data from the auroral acceleration region (AAR) of Earth’s dusk-side aurora. C3 flew through the AAR at an altitude of about 6400 km (one Earth radius or RE), while C1 was flying at approximately 9000 km (1.4 RE) and lagging about 5 minutes behind. The blue ovals indicate the poleward half of the auroral oval, which is characterized by upward currents flowing along in the dusk-side magnetic field. (Credit: ESA)

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