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|  |  |  |  | | | ESA’s Cluster flies through Earth’s electrical switch 19 May 2006
 | This sketch shows the various regions of Earth’s magnetosphere, being investigated by ESA’s Cluster mission. The position of the four satellites of the Cluster fleet is indicated by the red circle.
Credits: ESA |  |  |  |  |
| | | |  | This sketch shows a so-called electron diffusion region. It is a boundary just a few kilometres thick that occurs at an altitude of approximately 60000 kilometres above the Earth’s surface, where electrons can be accelerated to approximately one hundredth the speed of light. On 25 January 2005, and for nineteen times in one hour, the Cluster quartet found themselves engulfed in an electron diffusion region.
Credits: F.Mozer/UC Berkeley, USA |  |  |  |  |
| | | |  | In a plasma (a gas of charged particles), during magnetic reconnection, magnetic field lines of opposite direction break and then reconnect, forming an X-line magnetic topology. The newly reconnected field lines accelerate the plasma away from the X-line.
Credits: Center for Visual computing, Univ. of California Riverside |  |  |  |  |
| | | |  | | On 28 October 2003, the Sun released a coronal mass ejection of immense proportions which travelled in the direction of Earth. Bigger than the Sun itself, it hurtled towards Earth at a speed of over 2000 kilometres per second - five times the normal speed. |  |  |  |  |
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|  | More about... Magnetic reconnectionCluster factsheetRelated articles Cluster helps to protect astronauts and satellites against 'killer electrons'Satellites see largest jet of particles created between Sun and EarthCluster helps to protect astronauts and satellites against 'killer electrons'From ‘macro’ to ‘micro’ – turbulence seen by ClusterCluster's new view of near-Earth spaceHow the Sun affects us on EarthSpace weatherWhat are solar flares?Click here for a video of a 'Solar tantrum'Related links New microscopic properties of magnetic reconnection derived by ClusterESA's Space Weather pages
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