| タイトル | Protons and electrons in Jupiter's magnetic field - Results from the University of Chicago experiment on Pioneer 10 |
| 著者（英） | Mogro-Campero, A.; Perkins, M.; O'Gallagher, J. J.; Lentz, G.; Tuzzolino, A. J.; Mckibben, R. B.; Hamilton, D.; Simpson, J. A.; Pyle, K. R. |
| 発行日 | 1974-01-25 |
| 言語 | eng |
| 内容記述 | Fluxes of high energy electrons and protons are found to be highly concentrated near the magnetic equatorial plane from distances of about 30 to about 100 Jovian radii. The 10-hour period of planetary rotation is observed as an intensity variation, which indicates that the equatorial zone of high particle fluxes is inclined with respect to the rotation axis of the planet. At radial distances below 20 Jovian radii, the synchrotron-radiation-producing electrons with energies above 3 MeV rise steeply to a maximum intensity near the periapsis at 2.8 Jovian radii. The flux of protons with energies above 30 MeV reaches a maximum intensity at 3.5 Jovian radii, with the intensity decreasing inside this radial distance. |
| NASA分類 | SPACE SCIENCES |
| レポートNO | 74A18610 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/454107 |
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