Interpretive Studies of Ionospheric Chemistry and Electrodynamics

该项目涉及使用理论建模， 结合观测约束来解释观测到的 不同电离层成分的全球分布，例如 如O+、H+和He+。 这些意见主要是组成部分 和结构的电离层等离子体观察到的各种 卫星：AE、DE和DMSP。 模型的应用和 地面观测的协作数据分析也是 为了研究决定 高纬对流型对气候变化的响应 磁活动和行星际条件。

This project involves the use of theoretical modeling which incorporates observational constraints to explain the observed global distributions of different ionospheric constituents, such as O+, H+ and He+. The observations are primarily of composition and structure of the ionospheric plasma as observed from various satellites: AE, DE and DMSP. Application of the modeling and collaborative data analyses to ground based observations is also planned in order to study the principal parameters determining the high latitude convection pattern response to changing magnetic activity and interplanetary conditions.