The 4 th International Workshop on MRI Phase Contrast & QSM (2016, Graz) hosted the first QSM challenge. A single-orientation GRE acquisition was provided, along with COSMOS and the χ 33 STI component as ground-truths. The submitted solutions differed more than expected depending on the error metric used for optimization and tended to over-regularization. This raised (unanswered) questions about the ground-truths and the metrics utilized.
We investigated the influence of background field remnants by applying additional filters. We also estimated the anisotropic contributions from the STI tensor to the apparent susceptibility, to amend the χ 33 ground-truth and to investigate the impact on the reconstructions. Lastly, we used forward simulations from the COSMOS reconstruction to investigate the impact that has noise on the metrics.
Reconstructions compared against the amended STI ground-truth returned lower errors. We show that the background field remnants had a minor impact in the errors. In the absence of inconsistencies, all metrics converged to the same regularization weights, whereas SSIM was more insensitive to such inconsistencies.