中文摘要：

为了解极光电集流在sawtooth事件期间的响应情形，本文利用北半球高纬地磁台站的磁场数据，建立了以球元基本电流系反演法求得大尺度电离层水平等效电流系分布的方法，以此研究了2000年9月30日同步轨道LANL卫星观测到的sawtooth事件期间极光电集流的变化．本文将sawtooth注入事件后极区电离层夜侧西向电集流增长的特征，与中低纬地基磁场北向分量正弯扰的特征做比较分析．两者的观测结果都表明在本sawtooth注入事件期间有电流楔的形成，且电流楔约有11h磁地方时（MLT）的宽度．此外，中低纬磁弯扰达到最大扰动值的时间一般比高纬电集流达到最大扰动值的时间长，说明影响中低纬磁弯扰变化的电流源较丰富．

英文摘要：

In order to study the response of auroral electrojets for a sawtooth event observed by LANL satellites on 30 September 2000, we obtain large scale 2-dimensional ionospheric equivalent current systems for the high-latitude ionosphere to study the variations of auroral electrojets during the sawtooth event using spherical elementary current system method with data of high-latitude magnetometers in the Northern Hemisphere. By comparing characteristics of enhancements of nightside ionospheric westward electrojets with those of positive magnetic bays in middle/low-latitude ground magnetic field H components after each sawtooth injection, it is demonstrated that there are current wedges formed during this sawtooth event. The local time width of current wedges suggested by the two observations are both around 11 hours （MLT）. In addition, time durations for middle/low-latitude magnetic bays to reach maximum variations were generally longer than those for high-latitude electrojets, implying that source currents for middle/ low-latitude magnetic bays are multiple.