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Zoom-in to plasmapause-induced TEC enhancement - April 2001

Space weather events which disturb the plasmapause (displayed here as a green surface enclosing the Earth) can propagate down to the Earth's ionosphere. There they enhance the ionosphere electron content which can disrupt radio signals from satellites.

NOTE: This visualization shows the Earth's magnetic dipole field lines rotating rigidly with the Earth. Technically, this is inaccurate. Ions and electrons in the lower atmosphere can create currents which can make these lines 'drag' with Earth's rotation, but this will occur mostly near the Earth and not higher up. More details on this process can be found in the FAQ at the The Exploration of the Earth's Magnetosphere web site, Does the Earth's magnetic field rotate?.


Push-in view with time tags.    Push-in view with time tags.
Duration: 28.0 seconds
Available formats:
  320x240 (30 fps) MPEG-1   5 MB
  720x480 (29.97 fps) MPEG-2   24 MB
  640x480 (30 fps) MPEG-1   20 MB
  720x480 (29.97 fps) Frames (Pushin wdate)
  320x240     JPEG         32 KB
  640x480 (29.97 fps) MPEG-4   27 MB
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Push-in view without time tags.
   Push-in view without time tags.
Duration: 28.0 seconds
Available formats:
  320x240 (30 fps) MPEG-1   5 MB
  640x480 (30 fps) MPEG-1   20 MB
  720x480 (29.97 fps) MPEG-2   24 MB
  720x480 (29.97 fps) Frames (Pushin nodate)
  320x240     JPEG         38 KB
  640x480 (29.97 fps) MPEG-4   26 MB
How to play our movies


An overview of the pre-storm plasmasphere.
   An overview of the pre-storm plasmasphere.

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An overview of the pre-storm plasmasphere (without dates).    An overview of the pre-storm plasmasphere (without dates).

Available formats:
  2560 x 1920     TIFF 1 MB
  320 x 240         PNG 59 KB


Push-in to North America (no dates)    Push-in to North America (no dates)

Available formats:
  2560 x 1920     TIFF 4 MB
  320 x 240         JPEG 48 KB


Push-in to North America.    Push-in to North America.

Available formats:
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  320 x 240         JPEG 50 KB


The plasmasphere plume passes below the observer, enhancing the electron content of the ionosphere below it (no dates).    The plasmasphere plume passes below the observer, enhancing the electron content of the ionosphere below it (no dates).

Available formats:
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  320 x 240         JPEG 49 KB
  160 x 80           PNG 20 KB
  80 x 40             PNG   6 KB


The plasmasphere plume passes below the observer, enhancing the electron content of the ionosphere below it.    The plasmasphere plume passes below the observer, enhancing the electron content of the ionosphere below it.

Available formats:
  2560 x 1920     TIFF 4 MB
  320 x 240         JPEG 51 KB

Animation Number:3311
Animator:Tom Bridgman (SVS) (Lead)
Completed:2005-11-18
Scientists:Jerald Goldstein (SwRI)
 Marlene Colerico (MIT/Haystack)
 Anthea J. Coster (MIT/Haystack)
 Robert Robinson (NSF)
 Geoff Crowley (SwRI)
 John Foster (MIT/Haystack)
Instrument:IMAGE/EUV
Data set:World-wide GPS Receiver Network
Data Collected:2001/04/11T00:24:00Z - 2001/04/13T23:59:00Z
Series:Space Weather Cold Fronts
Keywords:
SVS >> Electron Fluxes
SVS >> Geomagnetic Field
SVS >> Plasmasphere
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Ionosphere/Magnetosphere Particles
GCMD >> EARTH SCIENCE >> Sun-earth Interactions >> Ionosphere/Magnetosphere Particles >> Electron Flux
GCMD >> Location >> Ionosphere
SVS >> Plasmapause
SVS >> Space Weather
More Information on this topic available at:
http://www.nasa.gov/vision/universe/solarsystem/cold_front_feature.html
Science paper:JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 110, A09S31, doi:10.1029/2004JA010928, 2005
 
 
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