Supported by the National Basic Research Program(2012CB825602);National Natural Science Foundation of China(NNSFC,41204118,41231067);in part by the Specialized Research Fund for State Key Laboratories of China
By use of the global PPMLR Magnetohydrodynamics(MHD) model,a serial of quasisteady-state numerical simulations were conducted to examine the modulation property of the interplanetary magnetic field clock angle θ on t...
Supported by the National Basic Research Program(2012CB825602);National Natural Science Foundation of China(41231067,41174143);the Specialized Research Fund for State Key Laboratories of China
Kelvin-Helmholtz(K-H) waves are formed from the triggering of the K-H instability on the magnetopause,which is a candidate mechanism for solar wind entry into the magnetosphere,especially under northward interplanetar...
supported by the National Basic Research Program of China (2012CB825602);the National Natural Science Foundation of China (41231067 and 41204118);in part by the Specialized Research Fund for State Key Laboratories of China
The plasma transport between the plasmasphere and the ionosphere in response to the interplanetary conditions is still not fully understood until now.Simultaneous observations of the plasmasphere and ionosphere from t...