作者: K.-P. Wenzel , R. P. Lepping , T. R. Sanderson , E. J. Smith , J. A. Slavin
DOI:
关键词: Computational physics 、 Earth's magnetic field 、 Magnetic reconnection 、 Heliospheric current sheet 、 Substorm 、 Plasma sheet 、 Geophysics 、 Magnetosphere 、 Interplanetary magnetic field 、 Physics 、 Magnetic cloud
摘要: The influence of the IMF orientation and magnitude substorm activity on magnetic configuration central plasma sheet at 20-240 earth radii down geomagnetic tail is investigated basis ISEE-3 data. results are presented graphically, high-speed antisolar bulk flows threaded by southward fields shown to be present in distant after periods Bz. effective dayside reconnection efficiency estimated as 25 + or - 4 percent, good agreement with theoretical models.