Abstract
极区从电离层到磁层的上行粒子流探测研究是空间天气建模中的重要问题，其起源和加速机制是磁层-电离层-热层耦合小卫星星座计划的主要科学目标. 磁层-电离层-热层耦合小卫星星座计划拟定由两颗磁层星和两颗电离层/热层星组成星座对极区进行联合观测. 其中，上行粒子源区附近的就位探测是电离层-热层耦合机制研究的重点，也是电离层/热层星轨道设计的关键. 根据相关空间探测计划和卫星观测结果，通过比较圆轨道和椭圆轨道两种方案，确定电离层/热层星采用椭圆轨道.
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