| タイトル | Energetic solar particle fluxes out to 3 AU during the 7 May 1978 flare event |
| 本文（外部サイト） | http://hdl.handle.net/2060/19850026509 |
| 著者（英） | Debrunner, H.; Lockwood, J. A. |
| 著者所属（英） | New Hampshire Univ. |
| 発行日 | 1985-08-01 |
| 言語 | eng |
| 内容記述 | Simultaneous solar proton flux measurements on IMP 7 and by the world wide neutron monitor network during the May 7, 1978 flare event led to conclusions that in the energy range from 50 MeV to 10 GeV: (1) the propagation of the flare particles in the interplanetary magnetic field (IMF) between the Sun and the Earth was nearly scatter free; and (2) therefore, the intensity time (IT) profiles of the solar proton fluxes observed at Earth for about one hour after onset represent the solar injection profiles even to energies as low as 50 MeV. Observations of the IMF at Helios A indicate that the IMF was undisturbed between the Sun and Helios A at the time of the May 7, 1978 flare event; and, therefore, the solar particle propagation was also scatter free from the Sun to Helios A. |
| NASA分類 | SOLAR PHYSICS |
| レポートNO | 85N34822
SH-3.2-6 |
| 権利 | No Copyright |
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