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Mars rover flyovers
Images taken by the Mars Reconnaissance Orbiter have been assembled to create these flyover animations of the Columbia Hills where the Spirit rover is exploring and the Opportunity rover at Victoria Crater.

 Spirit | Opportunity

Seas on Titan
NASA's Cassini spacecraft has found evidence for seas, likely filled with liquid methane or ethane, in the high northern latitudes of Saturn's moon Titan. This movie includes animation of the craft's encounters with Titan and an interview with insight into the science.

 Play

Atlas 5 launches STP 1
The United Launch Alliance Atlas 5 rocket with the U.S. military's Space Test Program 1 payload launches Cape Canaveral.

 Full Coverage

Atlantis rolls back
Battered by an intense hail storm six days earlier, space shuttle Atlantis retreated off launch pad 39A and returned to the cavernous Vehicle Assembly Building on March 4 to undergo thorough inspections and repairs.

 Video | Time-lapse

STS-112: ISS expansion
Atlantis made a week-long visit to the International Space Station in October 2002 that began the outward expansion of the outpost's truss backbone. Attachment of the 14.5-ton Starboard 1 segment was primary objective of the STS-112 mission. The astronauts tell the story of the flight in this post-flight movie.

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NASA budget hearing
This U.S. Senate space subcommittee hearing to examine NASA's proposed Fiscal Year 2008 budget features testimony from NASA Administrator Mike Griffin on February 28.

 Part 1 | Part 2

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Cluster opens a new window on near-Earth space
EUROPEAN SPACE AGENCY NEWS RELEASE
Posted: March 14, 2007

Plasma physicists have made an unprecedented measurement in their study of the Earth's magnetic field. Thanks to the European Space Agency's Cluster satellites they detected an electric field thought to be a key element in the process of 'magnetic reconnection'.

Thanks to these measurements, obtained by the eight PEACE electron sensors onboard the four spacecraft, scientists now have their first insight into magnetic reconnection's detailed behaviour.


This artist's impression shows the four ESA's Cluster satellites flying through the Earth's magnetosphere and observing the 'magnetic reconnection' process. Credit: ESA
 
Magnetic reconnection is a process that can occur almost anywhere that a magnetic field is found. In a reconnection event, the magnetic field lines are squeezed together somehow and spontaneously reconfigure themselves. This releases energy. When it occurs near the surface of the Sun, such an event powers giant solar flares that can release thousands of millions of tonnes of electrically charged particles into space.

The Earth's magnetic field creates a buffer zone, the magnetosphere, between our planet's atmosphere and the particles released during these eruptions. The Sun also releases a steadier flow of charged particles called the solar wind. On the large-scale, any heading this way buffet the magnetosphere, and are deflected by it. Plasma physicists describe this behaviour with a theory called 'magneto-hydrodynamics' (MHD).

On smaller scales, however, the picture becomes rather more complicated. The particles can actually flow across the magnetic field lines.This makes the mathematics of the behaviour more difficult. First to misbehave are the ions (positively charged particles). These break away from simple MHD on scales of less than a few hundred kilometres. On even smaller scales, less than 10 kilometres, the electrons (negatively charged particles) begin playing by other rules, too.

The new Cluster measurements reveal the electric field on the scale of a few hundred kilometres. "This is the first ever measurement of this term," says Paul Henderson, from University College London's Mullard Space Science Laboratory, UK, who led the investigation.

On 17 August 2003, Cluster was flying high above the night-time hemisphere of the Earth with an average separation of 200 kilometres between spacecraft. Data from several instruments shows that at 18:00 CET, a reconnection event took place and swept across the spacecraft.

Using data from Cluster's Plasma Electron and Current Experiment (PEACE) Henderson and collaborators calculated the pressure of electrons at each spacecraft and then calculated the difference between them and the variation with time. Using these quantities they calculated the electric field present near a reconnection site.

"This is an impossible calculation to make without four spacecraft," says Henderson. Now that the scientists can calculate the electric field in such a way, they have a new window into the process of magnetic reconnection.

Magnetic reconnection within Earth's magnetosphere regularly takes place on the night-time side of our planet, where the flow of the solar wind stretches out the magnetic field into a long tail. When the field reconnects in this region, it triggers jets of energetic particles that can cause auroral lights but can also damage satellites.

This new Cluster result takes scientists a step closer to seeing the precise details of magnetic reconnection. "When you think that the magnetosphere stretches over a million kilometres through space, we are actually looking at a minuscule part of it," says Henderson.

And that's exactly what plasma scientists want - the microphysics.