The　initial　value　problems　of　bipolar　isentropic/non-isentropic　compressible　Navier-Stokes-Maxwell　(CNS-M)　systems　arising　from　plasmas　in　R-3　are　studied.　The　main　difficulty　of　studying　the　bipolar　isentropic/non-isentropic　CNS-M　systems　lies　in　the　appearance　of　the　electromagnetic　fields　satisfying　the　hyperbolic　Maxwell　equations.　The　large　time-decay　rates　of　global　smooth　solutions　with　small　amplitude　in　L-q(R-3)　for　2　＜=　q　＜=　infinity　are　established.　For　the　bipolar　non-isentropic　CNS-M　system,　the　difference　of　velocities　of　two　charged　carriers　decay　at　the　rate　(1　+　t)-　rate　(1　+　t)(-3/4+1/4q)　which　is　faster　than　the　rate　(1+t)(-3/4+1/4q)(ln　-3/+t))(1-2/q)　of　the　bipolar　isentropic　CNS-M　system,　meanwhile,　the　magnetic　field　decay　at　the　rate　(1　+　t)(-3/4+1/4q)(ln　-3/+t))(1-2/q)　which　is　slower　than　the　rate　(1　+t)-　34　+　4q　3　for　the　bipolar　isentropic　CNS-M　system.　The　approach　adopted　is　the　classical　energy　method　but　with　some　new　developments,　where　the　techniques　of　choosing　symmetrizers　and　the　spectrum　analysis　on　the　linearized　homogeneous　system　play　the　crucial　roles.　(C)　2021　Elsevier　Inc.　All　rights　reserved.