GEM Workshop on Intercalibrationg Cusp Signatures

第一个GEM（地球空间环境建模）理论- 观测活动解决了磁层顶的问题， 边界层，和他们的签名在尖点的 电离层 参加去年举行的观测讲习班的人员 1989年10月，在马里兰州大学， 战役的首要任务应该是确定 的尖点签名在地面和空中数据， 直接与航天器粒子数据相互校准 地面和空中设施的飞越。 的 相对容易识别的尖点粒子签名， 航天器仪器将作为罗塞塔石碑， 正在破译下面的签名 为此，一项试点数据- 收集程序发生在黑暗的尖点附近， 1990年1月16日，许多团体正在收集档案数据， 相互校准 这笔赠款是为了举办一个讲习班， 数据进行分析和理论解释。

The first GEM (Geospace Environment Modelling) theory- observing campaign addresses problems of the magnetopause, boundary layers, and their signatures in the cusp of the ionosphere. Participants in the observing workshop held last October 1989 at the University of Maryland determined that the first task of the campaign should be the confident identification of cusp signatures in ground-based and airborne data by intercalibrating with spacecraft particle data on direct overflights of the ground-based and airborne facilities. The relatively easily recognized cusp particle signatures from the spacecraft instruments would serve as a Rosetta stone for deciphering signatures below. To this end, a pilot data- gathering program took place in the vicinity of the dark cusp on January 16, 1990, and many groups are gathering archival data for intercalibration. This grant is for a workshop to bring these data together for analysis and theoretical interpretation.