An empirical model of the high‐energy electron environment at Jupiter
Autor: | Insoo Jun, Robin W. Evans, W. Kim, Chris Paranicas, Alexander Drozdov, Henry B. Garrett, M. de Soria-Santacruz |
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Rok vydání: | 2016 |
Předmět: |
Free electron model
Physics 010504 meteorology & atmospheric sciences Spacecraft 010308 nuclear & particles physics business.industry Plasma sheet Astronomy Magnetosphere 01 natural sciences Jovian Jupiter Geophysics Space and Planetary Science Planet Physics::Space Physics 0103 physical sciences Astrophysics::Earth and Planetary Astrophysics Geiger tube telescope business 0105 earth and related environmental sciences |
Zdroj: | Journal of Geophysical Research: Space Physics. 121:9732-9743 |
ISSN: | 2169-9402 2169-9380 |
Popis: | We present an empirical model of the energetic electron environment in Jupiter's magnetosphere that we have named the Galileo Interim Radiation Electron Model version-2 (GIRE2) since it is based on Galileo data from the Energetic Particle Detector (EPD). Inside 8RJ, GIRE2 adopts the previously existing model of Divine and Garrett because this region was well sampled by the Pioneer and Voyager spacecraft but poorly covered by Galileo. Outside of 8RJ, the model is based on 10-minute averages of Galileo EPD data as well as on measurements from the Geiger Tube Telescope onboard the Pioneer spacecraft. In the inner magnetosphere the field configuration is dipolar while in the outer magnetosphere it presents a disk-like structure. The gradual transition between these two behaviors is centered at about 17RJ. GIRE2 distinguishes between the two different regions characterized by these two magnetic field topologies. Specifically, GIRE2 consists of an inner trapped omnidirectional model between 8 to 17RJ that smoothly joins onto the original Divine and Garrett model inside 8RJ and onto a GIRE2 plasma sheet model at large radial distances. The model provides a complete picture of the high-energy electron environment in the Jovian magnetosphere from ∼1 to 50RJ. The present manuscript describes in great detail the data sets, formulation, and fittings used in the model and provides a discussion of the predicted high-energy electron fluxes as a function of energy and radial distance from the planet. |
Databáze: | OpenAIRE |
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