A new view of the particle acceleration theory for the neutron star magnetosphere

费米伽马射线观测站提供了关于脉冲星磁层的大量数据和新事实。这些天的情况，加上其他波长的各种观测结果，都需要新的理论和模型。在这个项目中，我们试图建立一个关于脉冲星磁层中粒子加速的新观点和新理论。

Fermi gamma-ray observatory yields a great expansion of data and new fact on the pulsar magnetosphere. This situation of these days, together with variety of observational results in other wave length, requires new theories and models. In this project, we are attempting to construct such a new view and a new theory for the particle acceleration in the pulsar magnetosphere.