Three dimensional FLASH magneto-hydrodynamics(MHD) modeling is carried out to
interpret the OMEGA laser experiments of strongly magnetized, highly collimated
jets driven by a ring of 20 OMEGA beams. The predicted optical Thomson
scattering spectra and proton images are in good agreement with a subset of the
experimental data. Magnetic fields generated via the Biermann battery term are
amplified at the boundary between the core and the surrounding of the jet. The
simulation predicts multiple axially aligned magnetic flux ropes with
alternating poloidal component. Future applications of the hollow ring
configuration in laboratory astrophysics are discussed