One of the fundamental problems in modern astrophysics is the propagation of cosmic rays in turbulent magnetic fields, which can be studied by way of in-situ measurements of energetic particles in the heliosphere. Between 1 and 10 AU Jovian and galactic particles contribute continuously to the few-MeV electron intensities. As a result of this a 13 month period in the MeV electron intensity time profiles is observed at Earth. During its recent ascend to high latitudes the Ulysses spacecraft approached the planet Jupiter within 1 AU. 3-20 MeV-electrons were measured by the Kiel Electron Telescope (KET) on-board Ulysses from 1990 to 2006. At solar maximum Jovian electrons could unambiguously be identified at heliographic latitudes beyond 40°N and 10 AU from the planet. In this contribution we will present results of an analysis of Ulysses KET MeV electron measurements from the recent third out-off-ecliptic path and compare these data with observations obtained from 1992 to 1994 when the spacecraft was leaving the planet.
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机译：现代天体物理学中的一个基本问题是宇宙射线在湍流磁场中的传播，这可以通过在氦层中的能量粒子的原位测量来研究。在1到10之间的Au Jovian和银河系颗粒之间连续贡献几种MeV电子强度。因此，在地球上观察到MEV电子强度的13个月内。在最近向高纬度的上升期间，尤利西斯航天器在1 AU内接近行星Jupter。从1990年到2006年的基尔电子望远镜（KET）板载尤利尔斯测量了3-20mev-Electrons。在太阳能最大的时，Jovian电子可以明确地在从行星中超过40°N和10 Au的光学纬度鉴定。在这一贡献中，我们将呈现来自最近的第三个外偏见的ulysses Ket Mev电子测量的分析结果，并将这些数据与1992年至1994年获得的观察结果进行比较，当航天器离开行星时。
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