The Van Allen Probes (formerly Radiation Belt Storm Probes - RBSP) Explore the Earth's Radiation Belts
- Visualizations by:
- Tom Bridgman
- View full credits
In this region, many of the magnetic field lines intersect the surface of the Earth in the north and south. This means that lower energy ions and electrons, some 'boiled off' the Earth's ionosphere by solar ultraviolet radiation, can be trapped along these field lines. The charged particles spend their time bouncing between the 'mirror points' in the Earth's magnetic field. This trapped population forms the radiation belts around the Earth. The radiation created by this charged particle population can be hazardous to satellites and astronauts so it is important to understand their characteristics.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio
Animator
- Tom Bridgman (GST) [Lead]
Scientists
- David G. Sibeck (NASA/GSFC)
- Shrikanth G. Kanekal (NASA/GSFC)
Producers
- Genna Duberstein (ADNET)
- Scott Wiessinger (KBRwyle)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
Solar Anomalous and Magnetospheric Particle Explorer (SAMPEX) (Collected with the HILT sensor)
Dataset can be found at: http://sunland.gsfc.nasa.gov/smex/sampex/
See more visualizations using this data setSSCweb ephemerides (A.K.A. SSCweb)
Satellite ephemerides
Dataset can be found at: http://sscweb.gsfc.nasa.gov
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details nor the data sets themselves on our site.