Density rendered slice ([g cm⁻³]) through the rotation axis, showing the early cloud structure of the strong field case μ = 2 before the formation of the disk. As the magnetic field is very strong, accretion will occur primarily along the field lines, creating an elongated cloud structure. Both high resolution cases (250³) of TSPH and GDSPH creates an elongated cloud structure, while in the low-resolution case (50³) only GDSPH forms the same cloud structure. TSPH instead forms a more compact central cloud, which as a consequence collapses faster than the GDSPH case and the high resolution cases.