Features of energetic particle radial profiles inferred from geosynchronous responses to solar wind dynamic pressure enhancements
Determination of the radial profile of phase space density of relativistic electrons at constant adiabatic invariants is crucial for identifying the source for them within the outer radiation belt. The commonly used method is to convert flux observed at fixed energy to phase space density at cons...
Main Authors: | Y. Shi, E. Zesta, L. R. Lyons |
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Format: | Article |
Language: | English |
Published: |
Copernicus Publications
2009-02-01
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Series: | Annales Geophysicae |
Online Access: | https://www.ann-geophys.net/27/851/2009/angeo-27-851-2009.pdf |
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