NSWP: Determining the Relationships between Promptly Penetrating, Daytime Low Latitude Electric Fields and Interplanetary Electric and Magnetic Field Conditions

由地球磁场和电离层电场（ExB）的相对方向和强度驱动的垂直等离子体漂移，以及这些漂移对行星际磁场（IMF）的敏感性是半经验建模的。 多元回归和神经网络分析适用于非相干散射雷达（ISR）的数据从Jicamarca，秘鲁雷达站点，低功率JULIA雷达数据从Jicamarca，磁强计数据从秘鲁和从菲律宾的网站，和ACE卫星数据，以提高我们的理解穿透电场。 赖斯对流模型也被用来提供理论洞察力的物理驱动程序，通过耦合到电离层电场耦合的IMF垂直离子漂移。 研究的重点是更准确地描述白天迅速穿透电场与行星际电场和磁场条件之间的时间依赖关系。 此外，IMF驱动的电场的纵向变化的确定。

Vertical Plasma drifts driven by the relative orientation and strengths of the Earth's magnetic field and ionospheric electric fields (ExB), and the sensitivity of those drifts to the interplanetary magnetic field (IMF) are modeled semi-empirically. Multiple-regression and neural network analyses are applied to incoherent scatter radar (ISR) data from the Jicamarca, Peru radar site, to low power JULIA radar data from Jicamarca, to magnetometer data from Peru and from the sites in the Philippines, and to ACE satellite data to improve our understanding of penetrating electric fields. The Rice Convection Model is also used to provide theoretical insight into physical drivers that couple the IMF to vertical ion drifts through coupling to ionospheric electric fields. The research focuses on more accurate descriptions of the time dependant relationships between promptly penetrating electric fields in the daytime and the interplanetary electric and magnetic field conditions. Also, the longitudinal variation of IMF driven electric fields is determined.