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Magnetic Reconnection 2

This is an update to an older magnetic reconnection animation (10072). The ionized wind from the Sun generates reconnection in the Earth's magnetic field. Particles leak in from the rediation belts producing the auroras.
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3-D Anaglyph Reconnection animation    3-D Anaglyph Reconnection animation
Duration: 44.3 seconds
Available formats:
  720x405     QT         89 MB
  720x405     MPEG-4   69 MB
  960x540     WEBM         6 MB
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Left Camera    Left Camera
Duration: 44.3 seconds
Available formats:
  720x405     QT         112 MB
  1920x1080 Frames (LeftCam)
  1920x1080 QT         66 MB
  960x540     WEBM         6 MB
  320x180     PNG           56 KB
How to play our movies


Right Camera    Right Camera
Duration: 44.3 seconds
Available formats:
  720x405     QT         111 MB
  1920x1080 Frames (RightCam)
  1920x1080 QT         69 MB
  960x540     WEBM         6 MB
How to play our movies

Short URL to This Page:http://svs.gsfc.nasa.gov/goto?20101
Animation Number:20101
Completed:2007-04-06
Animator:Walt Feimer (HTSI) (Lead)
Scientist:Nicola Fox (Johns Hopkins University/APL)
Please give credit for this item to:
NASA/Goddard Space Flight Center
Conceptual Image Lab
 
Keywords:
SVS >> Aurora
SVS >> Magnetic Fields
SVS >> Magnetosphere
NASA Science >> Earth
NASA Science >> Sun
 
 


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Many of our multimedia items use the GCMD keywords. These keywords can be found on the Internet with the following citation:
Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0

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