A Double Disturbed Lunar Plasma Wake

This dataset is used and cited in the manuscript "A Double Disturbed Lunar Plasma Wake", Journal of Geophysical Research: Space Physics (2020). The Amitis hybrid-PIC code (Fatemi et al., 2017) is used here to model the lunar wake response to a passing CME while the Moon is crossing the geomagnetic tail. The data is composed of simulation results using nominal solar wind conditions and the double disturbed upwind boundary conditions extracted from ARTEMIS spacecraft data during the initial CME arrival.本数据集已被2020年刊载于《地球物理研究杂志：空间物理学》（Journal of Geophysical Research: Space Physics）的论文《双扰动月球等离子体尾迹》（A Double Disturbed Lunar Plasma Wake）使用并引用。本次研究采用Amitis混合粒子-细胞代码（hybrid-PIC code，Fatemi等，2017），对月球穿越地磁尾过程中，其等离子体尾迹对掠过的日冕物质抛射（Coronal Mass Ejection，CME）的响应进行建模。该数据集由两类模拟结果构成：一是基于标称太阳风条件的模拟结果，二是基于从ARTEMIS航天器（ARTEMIS）在初始CME抵达期间的探测数据中提取的双扰动上游边界条件的模拟结果。