The magnetospheric simulation facility at the University of California
, Riverside (UCR) has been recently modified to improve scalings based
on magnetohydrodynamic (MWD) theory. In this facility a magnetized pl
asma stream interacts with a downstream dipole magnetic field simulati
ng the Earth's magnetosphere. Specific improvements include: higher st
ream-flow velocity, increased plasma density, more intense background
and dipole magnetic fields, and improved diagnostic capability. This p
aper briefly discusses MHD scaling requirements and measurements that
are relevant to the laboratory simulation; including a set of time-res
olved visible-light images showing the evolution of the model magnetos
phere.