The structure of the magnetic field surrounding the planet Mars has be
en investigated using a fully three-dimensional hybrid particle code.
The results of these Simulations are found to agree well with Phobos 2
data However, the results also indicate that the solar wind interacti
on with the planet Mars produces a magnetic environment around the pla
net that is unique among the planets of the solar system. This paper r
eports the findings from a series of large-scale, three-dimensional si
mulations and many two-dimensional simulations used to address numeric
al issues.