机译:极地帽中未触发的极光亚暴和长周期(1-4 mHz)地磁和极光亮度脉动
Schmidt Inst Phys Earth, Moscow, Russia;
Schmidt Inst Phys Earth, Moscow, Russia|Natl Res Nucl Univ MEPhI, Moscow, Russia;
Univ Ctr Svalbard, Svalbard, Norway|Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway|British Antarctic Survey, Cambridge, England;
Schmidt Inst Phys Earth, Moscow, Russia;
Univ Ctr Svalbard, Svalbard, Norway|Univ Bergen, Birkeland Ctr Space Sci, Bergen, Norway|British Antarctic Survey, Cambridge, England;
Schmidt Inst Phys Earth, Moscow, Russia|Russian Acad Sci, Space Res Inst, Moscow, Russia;
UiT Arctic Univ Norway, Tromso Geophys Observ, Tromso, Norway;
Magnetospheric physics (auroral phenomena);
机译:极帽中未触发的极光亚暴和长周期(1a ?? 4a?ˉmHz)地磁和极光亮度脉动
机译:极光亚暴期间与早晨扇形地磁Pc5脉动相关的等效电流
机译:极光亚暴期间与早晨扇区地磁Pc5脉动相关的等效电流
机译:亚暴活动期间午夜极光区极地电离层的精细结构:极光电喷流计与极光光度电离层电导率之间的关系
机译:声波波和极地电磁波
机译:同时观测极地卫星全球影像和地面全天空影像中的极光亚暴
机译:极帽中未触发的极光亚暴和长周期(1-4?mHz)地磁和极光亮度脉动
机译:利用地磁独立性对地磁暴和极光基质的相关比较。