Solar energetic and shock‐accelerated particles observed between 1 and 4 AU by the Kiel Electron Telescope (KET) on board Ulysses
Authors:
- 19 June 1992
- journal article
- Published by American Geophysical Union (AGU) in Geophysical Research Letters
- Vol. 19 (12) , 1279-1282
Abstract
We present observations of solar energetic particles and shock‐accelerated particles observed by the Kiel Electron Telescope (KET) on board the Ulysses spacecraft in the time interval 26 October 1990 to mid November 1991. Prompt events with diffusive propagation were observed mainly at small radial distances while at larger distances shock‐related events became dominant. Particularly high intensities of high energy electrons and >30 MeV/n nuclei are observed at merged or double shocks. Slowly‐varying populations (SVP) with long time scales neither related to prompt events nor to local shock effects are a new feature at these intermediate distances.Keywords
This publication has 7 references indexed in Scilit:
- Electron acceleration to relativistic energies by traveling interplanetary shocksJournal of Geophysical Research, 1989
- Shock acceleration of nuclei and electrons in the heliosphere beyond 24 AUThe Astrophysical Journal, 1984
- Characteristics of solar and heliospheric ion populations observed near earthAdvances In Space Research, 1984
- Transport coefficients of low‐energy cosmic rays in interplanetary spaceReviews of Geophysics, 1982
- The radial transport of energetic solar flare particles from 1 to 6 AUJournal of Geophysical Research, 1977
- Modulation of Jovian electron intensity in interplanetary space by corotating interaction regionsThe Astrophysical Journal, 1977
- Adiabatic Fermi acceleration of energetic particles between converging interplanetary shock wavesJournal of Geophysical Research, 1976