Using a (3+1)-D hydrodynamic model CLVisc, we study the directed flow () of light hadrons produced in Au+Au, Ru+Ru and Zr+Zr collisions at 200 GeV. The evolution of tilted energy density, pressure gradient and radial flow along the -direction are systematically investigated. Counter-clockwise tilt of initial fireball is shown to be a vital source of the directed flow for final light hadrons. A good description of directed flow is provided for light hadrons in central and mid-central Au+Au and isobar collisions at RHIC. Our numerical results show a clear system size dependence for light hadron across different collision systems. We further study the effect of nuclear structure on the directed flow and find that the for light hadrons is insensitive to the nuclei with quadrupole deformation.

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