![](https://webarchive.library.unt.edu/eot2008/20080921082720im_/http://veimages.gsfc.nasa.gov//14572/magnetoplasmaHR_Oblique.0000_web.thumb.png)
Images & Animations
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Credit
NASA/Goddard Space Flight Center Scientific Visualization Studio
Earth's Radiation Belts Tremble Under Impact of Solar Storm
Radiation Belts and Plasmapause Fluctuate Under Solar Storm
Under the wave of energetic particles from the Halloween 2003 solar storm events, the Earth's radiation belts underwent significant changes in structure. This visualization is constructed using daily-averaged particle flux data from the SAMPEX satellite installed in a simple dipole model for the Earth's magnetic field. The toroidal structure of the belts corresponds to regions with electron fluxes in excess of 100 electrons/s/cm^2/steradian with energies of 2-6 MeV. The color-scale on the cross section is violet for low flux and white for high flux. The translucent grey arcs represent the fields lines of the Earth's dipole field. The 3-dimensional structure was built from the SAMPEX measurement by propagating the particle flux values along field lines of a simple magnetic dipole.
In this visualization, we see the interaction of the radiation belts (violet/white), the plasmapause (green surface) and magnetopause (grey surface).
As the particle events saturate the SAMPEX detectors, the radiation belt measurements develop a high level of noise that generates a 'blown-out' view in this model of the belts. The plasmasphere is still in its steady configuration.
Metadata
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Sensor
SAMPEX/PET, IMAGE/EUV -
Animation ID
3049 -
Video ID
None -
Start Timecode
00:00:00:00 -
End Timecode
00:00:00:00 -
Animator
Tom Bridgman, James W. Williams, Greg Shirah -
Studio
SVS -
Visualization Date
2004/12/01 -
Scientist
Daniel Baker (LASP), Shrikanth Kanekal (NOAA), Jerald Goldstein (SwRI) -
Keywords
Geomagnetic Field, Radiation Belts, Plasmapause, HDTV -
DLESE Subject
Space science -
Data Date
2003/10/29 - 2003/10/31 -
Pao ID
G04-071 -
Animation Type
Regular