Abstract The Mars Atmosphere and Volatile Evolution mission has obtained comprehensive
particle and magnetic field measurements. The Solar Wind Electron Analyzer provides …

Our purpose is to characterize the evolution of the magnetopause Kelvin‐Helmholtz (KH)
wave activity with changes in thickness of the adjacent boundary layer, geomagnetic latitude …

We have studied the entry paths of solar wind plasma into the magnetosphere during an
extended period of northward IMF using an OpenGGCM MHD simulation of the cold dense …

The October 22–24, 2003 interplanetary magnetic cloud was characterized by an
exceptionally long interval (∼ 32 hours) of nearly purely northward interplanetary magnetic …

We have investigated the Geotail data statistically to understand the particle sources,
transport, and spatial distributions of the plasma sheet ions and electrons of different …

This study examines how solar wind plasma enters the magnetosphere under northward
interplanetary magnetic field (IMF) conditions, using the Open Geospace General …

The storm‐time ring current is formed by the inward convection of the near‐earth plasma
sheet, so understanding the changing source of the plasma sheet is key for understanding …

We have statistically analyzed Geotail data to investigate the processes that result in a
plasma sheet that is denser under a prolonged northward than southward interplanetary …

Two‐dimensional hybrid simulations are used to investigate how fast‐mode compressional
waves incident on a magnetopause current layer mode convert both linearly and nonlinearly …

A layer of nearly stagnant cold dense plasma is observed by THEMIS spacecraft in a closed
field region immediately inside the dayside magnetopause near the low‐latitude boundary …