Friday, December 19, 2014

Origin of Long-standing Space Mystery Revealed

The ESA/NASA Cluster and NASA's IMAGE missions were in a position around Earth on Sep. 15, 2005, to determine how solar material in the magnetic environment in near-Earth space creates a special kind of high-latitude aurora called a theta aurora. Image Credit: ESA/NASA/SOHO/LASCO/EIT

Auroras are the most visible manifestation of the Sun’s effect on Earth, but many aspects of these spectacular displays are still poorly understood. Thanks to ESA’s Cluster and NASA’s IMAGE satellites working together, a particular type of very high-latitude aurora has now been explained. Known as a theta aurora -- because seen from above it looks like the Greek letter theta, an oval with a line crossing through the center -- this type of aurora sometimes occurs closer to the poles than normal aurora. While the genesis of the auroral oval emissions is reasonably well understood, the origin of the theta aurora was unclear until now. A paper in the Dec. 19, 2014, issue of Science shows that hot plasma funneled into near-Earth space from the sun helps cause these unique aurora. “Previously it was unclear whether this hot plasma was a result of direct solar wind entry through the lobes of the magnetosphere, or if the plasma is somehow related to the plasma sheet on the night side of Earth," said Robert Fear of the University of Southampton in the UK, and the lead author of the Science paper. “One idea is that the process of magnetic reconnection on the night side of Earth causes a build-up of ‘trapped’ hot plasma in the higher latitude lobes.”

Although separated by some 150 million kilometres, the Sun and Earth are connected by the solar wind. This stream of plasma – electrically charged atomic particles – is launched by the Sun and travels across the Solar System, carrying its own magnetic field with it.

Depending on how this ‘interplanetary magnetic field’ is aligned with Earth’s magnetic field when it arrives, there can be various results.

“The possibilities have been debated since the first satellite observations of the phenomenon were made in the 1980s," said Fear.

At the point where the two fields meet, Earth’s magnetic field points north. If the interplanetary field is pointing south, then ‘magnetic reconnection’ can occur, where magnetic field lines pointing in opposite directions spontaneously break and reconnect with other nearby field lines.

The realignment opens the door so that solar wind material can funnel into the magnetosphere – the giant magnetic bubble surrounding Earth. This is what leads to the aurora, which is produced when the particles funnel down along Earth’s magnetic field lines and strike atoms high in the atmosphere. The interaction with oxygen atoms results in a green or, more rarely, red glow in the night sky, while nitrogen atoms yield blue and purple colors. Normally, the main region for this impressive display is the auroral oval, which lies at around 65–70 degrees north or south of the equator, encircling the polar caps.

But when the interplanetary magnetic field points northward, auroras can occur at even higher latitudes, sometimes resulting in theta aurora. Prior to the recent work, scientists suspected that theta aurora had something to do with the particles observed in the lobe regions of the magnetosphere. The plasma in the lobes is normally cold, but previous observations suggested that theta auroras are linked with unusually hot lobe plasma – but just how was unclear.

A theta aurora – so named because it looks like a Greek letter theta, a circle with a line through the middle -- as seen by NASA’s IMAGE satellite on Sep. 15, 2005. New research helps explains what causes these unique events. Image Credit: NASA/R. Fear et al (2014)
A theta aurora – so named because it looks like a Greek letter theta, a circle with a line through the middle -- as seen by NASA’s IMAGE satellite on Sep. 15, 2005. New research helps explains what causes these unique events. Image Credit: NASA/R. Fear et al (2014)

“The study highlights the intriguing process that can occur in the magnetosphere when the interplanetary magnetic field of the solar wind points northwards,” said Philippe Escoubet, ESA’s Cluster project scientist. “This is the first time that the origin of the theta aurora phenomenon has been revealed, and it is thanks to localised measurements from Cluster combined with the wide-field view of Image that we can better understand another aspect of the Sun–Earth connection.”

The mystery was finally solved by studying data collected simultaneously by the Cluster and IMAGE spacecraft on Sept. 15, 2005. While the four Cluster satellites were located in the southern hemisphere magnetic lobe, IMAGE had a wide-field view of the southern hemisphere aurora. As one Cluster satellite observed uncharacteristically energetic plasma in the lobe, IMAGE saw the arc of the theta aurora cross the magnetic footprint of Cluster.

The team found that the energetic plasma appeared on high-latitude magnetic field lines that had been closed by the process of magnetic reconnection driven by the northward pointed fields. This in turn caused the plasma to become relatively hot. Such observations support the idea that theta aurora are due to plasma trapped inside the magnetosphere, rather than material being directly pushed in from the solar wind.

"Solving the question of the origin of the theta aurora required Cluster’s high inclination orbit that sweeps over the region where the aurora are generated together with the imaging capability of IMAGE, which is no longer functioning," said Melvyn Goldstein, Cluster project scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "Hopefully, future missions will give comparable capabilities to view the polar regions of the magnetosphere."

ESA’s Cluster consists of four satellites flying in formation around Earth. The data presented in this report were collected by Cluster-1. The Cluster mission was launched in 2000 and is still operating.

NASA’s Imager for Magnetopause-to-Aurora Global Exploration (IMAGE) satellite was launched in 2000 and concluded operations at the end of 2005. The data presented in this report were collected by the satellite’s far-ultraviolet Wideband Imaging Camera.

Credit: ESANASAsouthampton.ac.uk

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