标题： 超星团磁场与10**(19) eV以上的宇宙射线各向异性 显示英文标题

标题： Supercluster Magnetic Fields and Anisotropy of Cosmic Rays above 10**(19) eV

摘要： 我们预测了能量高于 \(10^\{19\}\) eV 的质子和中子的能谱及其角分布，这些粒子来源于局部超星系团中的源，该超星系团还被认为含有强度在 0.05 到 0.5 微高斯之间的大尺度磁场。 我们表明，这个模型可以解释超高能宇宙线的所有现有特性，至少对于接近 0.5 微高斯的场强是如此。 该情景所预测的大尺度各向异性和聚类效应将使下一代实验能够强有力地排除其他模型。 显示英文摘要

摘要： We predict energy spectra and angular distributions of nucleons above 10**(19) eV that originate from sources distributed in the Local Supercluster, which is also supposed to contain a large scale magnetic field of strength between 0.05 and 0.5 micro Gauss. We show that this model can explain all present-day features of ultra-high energy cosmic rays, at least for field strengths close to 0.5 micro Gauss. The large-scale anisotropy and the clustering predicted by this scenario will allow strong discrimination against other models with next generation experiments.