Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK,rnEmail: jb@mssl.ucl.ac.uk;
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK;
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK;
Space Science and Technology Department, Rutherford Appleton Laboratory, Chilton, Didcot OX11 0QX, UK;
Space Science Laboratory, University of California, Berkeley, CA 94720, USA;
Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK;
Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK;
Max-Planck-Institut für Extraterrestrische Physik, D-85748, Garching, Germany;
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机译:关于高空停滞尖端的形成:聚类观察-艺术。没有。 L12101
机译:在西南IMF下的星群-FAST-SuperDARN- S?ndrestr?m结合期间,高空尖端向极边界的脉冲流以及相关的电离层对流和粒子特征
机译:在西南IMf下的簇-FAST-SuperDARN-Sondrestrom合流期间,高空尖端向极边界的脉冲流以及相关的电离层对流和粒子特征
机译:形成高空停滞的机制:群集和超级观测
机译:哈勃太空望远镜用中心密度尖端观察球状星团。
机译:非全局性捕获引起的源自左冠状动脉/右冠状动脉连合的特发性折返室性心动过速终止的两种机制
机译:高空停滞尖端的形成机理:簇和SuperDARN观测
机译:利用Interball和IsTp航天器观测高原尖点区域的理论研究