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首页> 外文期刊>Geophysical Research Letters >Gyrophase-restricted 100 keV-2 MeV ion beams near the foreshock boundary - art. no. 2049
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Gyrophase-restricted 100 keV-2 MeV ion beams near the foreshock boundary - art. no. 2049

机译:在前震边界附近受陀螺相位限制的100 keV-2 MeV离子束-艺术。没有。 2049年

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1] We report on gyrophase-restricted ion beams with energies extending from similar to 100 keV up to similar to 2 MeV, observed by Wind in the Earth's distant (similar to 65 R-E) foreshock. The ion gyrophases seen were nearly constant during periods when the distance to the shock contact point could be expected to vary by several RE, when there was no significant wave activity. At times the distributions had two peaks similar to 180degrees apart in gyrophase. These were consistent with a remotely-sensed energetic ion foreshock region having a thickness < 2 gyroradii (&SIM; 1.5 R-E for 0.5 MeV protons with pitch-angle α = 30&DEG;). In this picture, gaps in phase space would correspond to particles with guiding centers outside of the energetic foreshock region. Similar observations over a decade of energies ( 100 keV - 2 MeV) suggest that the region thickness scales with gyroradius. According to this interpretation, we have determined a rough range of geometries for which energetic particle production is favored. (Eg., θ(Bn) &SIM; 70 - 80&DEG; for 500 keV ions with α = 30&DEG;.) [References: 15
机译:1]我们报道了在地球遥远(类似于65 R-E)前风中观察到的,具有从约100 keV到约2 MeV的能量延伸的旋涡受限离子束。在没有明显的波活动的情况下,到震荡接触点的距离可以变化几个RE时,看到的离子旋涡相几乎是恒定的。有时,在旋相中,分布具有两个相距180度的峰。这些与厚度<2陀螺半径的遥感高能离子前震区(&SIM; 0.5 MeV质子的1.5 R-E,俯仰角α= 30&DEG)一致。在这张照片中,相空间中的间隙将对应于具有在高能前震区域之外的引导中心的粒子。在十多年的能量(100 keV-2 MeV)上进行的类似观察表明,该区域的厚度与陀螺半径成比例。根据这种解释,我们确定了有利于产生高能粒子的大致几何形状范围。 (例如,对于500 keV离子,θ=(Bn)&SIM; 70-80&DEG;α= 30&DEG;。)[参考:15

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