Cluster Redeploys For Another View Of Earth

TECH SPACE

Cluster Redeploys For A Better View

The four ESA Cluster satellites, launched into space in Summer 2000, are studying the Sun-Earth interaction in unprecedented detail. By flying in a unique formation that gives us four viewpoints instead of one, the Cluster quartet is helping to make the first detailed 3D map of the space environment closest to home and how the Sun affects it. Cluster's new constellation will provide information on a different part of our magnetosphere, which can stretch millions of kilometres out into space, to complete the picture. The Cluster mission, initially planned to operate in space for 2 years, was granted an extension of 3 extra years' peration early this year.

Paris - Jul 11, 2002
The Brazilian World Cup celebrations may have started to die down, but in space the never-ending football match between the Sun and Earth continues. And watching this match closely are Salsa, Samba, Rumba and Tango, the four satellites that make up the Cluster mission. They are performing their Brazilian dances 119 000 kilometres above our heads.

With all the grace and skill of the Brazilian players on the football field, the spacecraft making up the Cluster quartet are currently changing their tactical positions to get a different view of the Sun's effects on Earth's magnetosphere.

The Cluster spacecraft have been marking the activity of the Sun, and the powerful particles it kicks towards Earth, for two years. In particular, the four spacecraft are studying the outer edges of Earth's magnetosphere, which are stretched and pulled in different directions as they are bombarded by the Sun's particles.

As they dance around each other, the Cluster satellites can move close together with only 100 km between them to get a close-up view of these tiny particles. Then they can pull away from each other as far back as 20 000 km to get the bigger picture.

Breakthrough data from Cluster confirmed that the outer regions of the magnetosphere are constantly being rocked by 'big waves' that resemble ocean rollers.

For this particular dance step, Cluster will be withdrawing from a close-up formation to a distance of 3800 km. This is the third time that Cluster has changed its configuration since it began its operations.

Studying the physics of the magnetosphere is fundamental for us because although we rely on the Sun for its light and warmth, not all its gifts are so beneficial. The stream of invisible charged particles flashes towards Earth at speeds of up to 1000 kilometres per second, while explosions on the Sun regularly send millions of tonnes of gas our way.

If we did not have Earth's magnetosphere to protect us, our attitude towards the Sun would be very different. Even with this natural protective bubble wrapped around us, solar particles can sometimes enter Earth's upper atmosphere, creating enormous electrical currents around our planet, which can have dramatic consequences. As well as creating the beautiful coloured light displays of the auroras, or Northern and Southern Lights, these currents can in fact lead to widespread power blackouts, damage to communications satellites and navigation systems, and even corrosion in oil pipelines.

"The Sun and the Earth play a never-ending football game," says Philippe Escoubet, Cluster project scientist. "The Sun is kicking particles towards Earth, which is the goal, and our magnetosphere acts as the goalkeeper. Some of the particles are deflected by the magnetosphere, but some get past it, scoring goals which disrupt Earth's activities. Sometimes the Sun is very quiet, but when it's active we get a lot of balls flying in this direction."

SPACE SCIENCE

Cluster Tunes Into Radio Earth

Greenbelt - Dec 10, 2001
Researchers have known for three decades that the Earth is a potent radio transmitter, but they were never able to pinpoint where the noise was coming from. By using data from the four spacecraft of the European Space Agency's Cluster mission, NASA-funded scientists have now precisely located the source of that radio noise along magnetic field lines several thousand miles above bright regions in Earth's northern lights.

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