SAMPEX - A Synoptic View of Earth's Electron Radiation Belts: North Pole Energetic Fluxes from HILT
The Solar Anomalous and Magnetospheric Particle Explorer, SAMPEX, measures fluxes of energetic particles from the sun, the Earth's magnetosphere, and cosmic ray sources over a broad range of energies.
The four instruments aboard SAMPEX are the Low-Energy Ion Analyzer (LEICA), The Heavy Ion Large Telescope (HILT), The Mass Spectrometer Telescope (MAST), and the Proton-Electron Telescope (PET).
Energetic electron fluxes (> 1 MeV) over the North Pole from the HILT solid state detector array during the period 7-6-1992 through 7-9-1993
Video slate image reads "SAMPEX
HILT Solid State Detector Array
> 1.0 MeV Electrons
North Pole".
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Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
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Animator
- Pamela ONeil (NASA)
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Scientists
- Dan Baker (University of Colorado)
- J. B. Blake (Aerospace Corporation)
- Linwood Callis (NASA/LaRC)
- Shrikanth G. Kanekal (University of Maryland)
- Berndt Klecker (Max Planck)
- Richard Mewaldt (CalTech)
Missions
This page is related to the following missions:Series
This page can be found in the following series:Datasets used
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[Solar Anomalous and Magnetospheric Particle Explorer (SAMPEX): HILT]
ID: 89This dataset can be found at: http://sunland.gsfc.nasa.gov/smex/sampex/
See all pages that use this dataset
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.
Release date
This page was originally published on Sunday, January 1, 1995.
This page was last updated on Wednesday, May 3, 2023 at 2:00 PM EDT.