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We suggest a new approach that could be used for modeling both the largescale behavior of astrophysical jets and the magnetically dominated explosionsin astrophysics. We describe a method for modeling the injection of magneticfields and their subsequent evolution in a regime where the free energy ismagnetically dominated. The injected magnetic fields, along with theirassociated currents, have both poloidal and toroidal components, and they arenot force free. The dynamic expansion driven by the Lorentz force of theinjected fields is studied using 3-dimensional ideal magnetohydrodynamicsimulations. The generic behavior of magnetic field expansion, the interactionswith the background medium, and the dependence on various parameters areinvestigated.Comment: Accepted to ApJ, May 10, 2006 issue, 12 figures total (3 color  figures

Modeling the Large‐Scale Structures of Astrophysical Jets in the Magnetically Dominated Limit