RIMI: Studies on Uranian and Neptunian Magnetospheres

9450454拟议的研究将研究决定海王星和天王星磁层等离子体形态的各种物理过程。拟议的项目是以旅行者号的观测为基础的，其中将包括：(1)指导带电粒子的中心运动和等离子体沿具有OTD和SH模型的磁场的磁层中的一条线的性质；(2)天王星和海王星的等离子体的理论模型；(3)天王星和海王星磁层中的动力学，特别是电流系统及其影响；(4)天王星和海王星磁层的等离子体的来源和输运过程。

9450454 The proposed research would study the various physical processes determining the plasma configurations of the Neptunian and Uranian magnetospheres. The proposed project is based on the Voyager observations and would include (1) Guiding center motion of charged particles and plasma bulk properties along a field line in the magnetospheres with a magnetic fields represented by both the OTD and SH models (2) Theoretical model of the plasmaspheres of Uranus and Neptune (3) Dynamics, especially current systems and their effects in the Uranian and Neptunian magnetospheres (4) Sources and transport processes of the plasmas of the Uranian and Neptunian magnetospheres.