Is the Relatives Within Solar Wind Active Tension therefore the Magnetopause Standoff Range so Simple?
Is the Relatives Within Solar Wind Active Tension therefore the Magnetopause Standoff Range so Simple? We present results of global magnetohydrodynamic simulations which reconsider the relationship between the solar wind dynamic pressure (Pd) and magnetopause standoff distance (RSub). We simulate the magnetospheric response to increases in the dynamic pressure by varying separately the solar wind … Is the Relatives Within Solar Wind Active Tension therefore the Magnetopause Standoff Range so Simple?