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VaNDI: Variational Nonlinear Dipole Inversion enables QSM without free parameters
Daniel Polak1, Itthi Chatnuntawech2, Jaeyeon Yoon3, Siddharth Srinivasan Iyer1, Kawin Setsompop1, and Berkin Bilgic1

1Martinos Center for Biomedical Imaging, Charlestown, MA, United States, 2National Nanotechnology Center, Pathum Thani, Thailand, 3Department of Electrical and Computer Engineering, Seoul National University, Seoul, Korea, Democratic People's Republic of

Synopsis

We propose Nonlinear Dipole Inversion (NDI) for high-quality Quantitative Susceptibility Mapping (QSM) without additional regularization, while matching the RMSE of state-of-the-art regularized reconstruction techniques. In addition to avoiding over-smoothing these techniques often face, we also obviate the need for parameter selection. NDI is flexible enough to allow for reconstruction from an arbitrary number of head orientations, and outperforms COSMOS using as few as 2-direction data. This is made possible by a nonlinear forward-model that uses the magnitude as an effective prior, for which we derived a simple gradient descent update. We synergistically combine this physics-model with Variational Networks (VN) to leverage the power of deep learning in the VaNDI algorithm. VaNDI adopts this simple gradient descent rule and learns the network parameters during training, hence requires no additional parameter tuning.

Introduction

QSM solves a linear system, which relates the tissue phase $$$\phi$$$ to the unknown susceptibility $$$\chi:K\chi=\phi$$$. This ill-posed problem benefits from regularization,

$$\min_\chi||K\chi-\phi||_2^2+\lambda R(\chi)$$

This formulation assumes Gaussian noise, whereas phase noise distribution deviates from this especially in low-SNR regions (1). This has been recognized in nonlinear-MEDI (2), where a nonlinear fidelity term was utilized:

$$\min_\chi||W(e^{iK\chi}-e^{i\phi})||_2^2+\lambda ||MG\chi||_1$$

Here the magnitude $$$W$$$ serves as a noise weighting and allows derivation of a binary mask $$$M$$$ that weights the gradient computed with $$$G$$$ operator. Recently proposed FANSI algorithm (3) presents a rapid alternative to nonlinear-MEDI through parameter splitting (4,5), but comes at the cost of 3 parameters that need to be tuned. Herein, we develop a simple gradient-descent optimizer, Nonlinear Dipole Inversion (NDI), and show that magnitude weighting and nonlinear formulation act as inherent priors without need for additional regularization. NDI is simple, and can be flexibly extended to reconstruct multi-orientation data. We show that NDI matches the RMSE of FANSI without the need for parameter tuning, and without the vulnerability of over-smoothing the images. It outperforms COSMOS (6) in multi-head direction data, which is susceptible to streaking artifacts in data with small rotations. Further, we expand NDI to admit variational regularizers learned from training data. Our VaNDI outperforms NDI and FANSI, both in terms of reconstruction speed and quality.

Code/data: https://bit.ly/2RHeiF0

Theory

NDI uses gradient descent to minimize $$$f(\chi)=||W(e^{iK\chi}-e^{i\phi}||_2^2$$$, NDI uses gradient descent to minimize

$$f(\chi)=||W(\cos(K\chi)-\cos(\phi)||_2^2+||W(\sin(K\chi)-\sin(\phi))||_2^2$$

After simplifications, taking its derivative yields

$$\partial f(\chi)=2K^TW^2\sin(K\chi-\phi)$$

With this, the $$$t^{th}$$$ iteration of the reconstruction reduces to:

$$\chi^{t+1}=\chi^t-2\sum_{r=1}^NK_r^TW^2\sin(K_r\chi^t-\chi_i)$$

where we generalized the formula for multi-orientation reconstruction from $$$N$$$-directions, with $$$\phi_r$$$ and $$$K_r$$$ denoting tissue phase and dipole kernel belonging to $$$r^{th}$$$ head rotation.


Data Acquisition

QSMNet dataset (7) was used, where 3D-GRE data were acquired on 9 subjects at 5 head-orientations with 1mm3 resolution, 256x224x192 matrix, TE/TR=25/33ms (8). Multi-orientation data were processed using BET (9), and FLIRT (10), Laplacian unwrapping (11) and SMV filtering (12).

Results

Multi-orientation: NDI vs COSMOS

Fig. 1 compares multi-orientation reconstructions using 2-, 3-, 4- and 5-direction data with NDI and COSMOS. COSMOS admits the closed form solution $$$\chi_{cosmos}=(\sum_rK_r^2)^{-1}\sum_rK_r^T\phi_r$$$, which is subject to artifacts if $$$\sum_rK_r^2$$$ is poorly conditioned in small rotation cases. NDI addresses this and improves reconstruction dramatically even from 2-directions.

Single-orientation: NDI vs TKD, L2 and FANSI

Fig. 2 compares 1-direction NDI against TKD (13), L2 (14) and FANSI (15), where the parameters of the latter three were tuned using the 5-direction COSMOS data. RMSEs are reported with respect to both the 5-direction COSMOS and 5-direction NDI reconstructions. NDI yields similar RMSE as FANSI, while achieving significantly sharper results, without the need for parameter tuning.

Variational NDI (VaNDI)

We developed VaNDI to further improve NDI using Variational Networks (VN) (16) by combining deep learning and nonlinear data fidelity (Fig. 3). This acts as an unrolled gradient descent with learned regularizers, where the step sizes, nonlinearities and convolutional filters are estimated during the training stage. We used an L2 loss to minimize the difference between 1-direction VaNDI and 5-direction NDI reference, with 1200 epochs, 7x7x7 kernels, and batch size of 1. Data from 8 subjects were used for training, while the 9thsubject was reserved for testing. Fig4 compares NDI (55.2% RMSE) and VaNDI (49.5% RMSE), where VaNDI further mitigated streaking artifacts and better completed the k-space.

Ultra-high resolution NDI at 7T

Multi-orientation NDI was also evaluated at 0.5 mm3 isotropic resolution at 7T and Wave-CAIPI (17)(R=15x, 5:13min/orientation), where a 32-ch coil [18] was used for high-quality imaging. This, however, limits the achievable head rotations (0, 7, 13 degrees) which makes reconstruction difficult. NDI still provides high-quality reconstruction as in Fig. 5.

Conclusion

We developed a robust and simple dipole inversion technique and demonstrated high-quality reconstructions. NDI has similar performance as FANSI, but is not vulnerable to over-smoothing since it does not require regularization or parameter tuning. VaNDI combined nonlinear data fidelity with learned regularizers to improve upon the state-of-the-art. VaNDI should have the flexibility to perform single-step reconstruction to estimate the susceptibility from raw phase, since the non-linear data fidelity is invariant to phase wraps and convolutional filters could learn SMV filters for background removal.

Acknowledgements

This work was supported in part by NIH research grants: R01EB020613, R01EB019437, R24MH106096, P41EB015896, and the shared instrumentation grants: S10RR023401, S10RR019307, S10RR019254, S10RR023043.

References

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Figures

Comparison of non-linear NDI vs linear COSMOS for different number of head orientations. NDI significantly reduced streaking artifacts and provides good results even at 2 head-directions.

Comparison of parameter-free NDI vs optimized TKD, L2, and FANSI. In comparison to TKD, NDI efficiently mitigates streaking artifacts while preventing large blurring as demonstrated in L2 and FANSI.

In the CNN part of the network (shown in blue) 3D convolutions (conv) and a non-linear activation (act) are learned for each gradient decent step GDtto increase the similarity between the output susceptibility and the 5-dir NDI.Moreover, a data-fidelity term (shown in orange) is integrated into the network to ensure agreement with the acquired data (phase). This term gets weighted by the parameter which is learned in training and can be interpreted as the gradient decent step size.

Single-orientation VaNDI further improved over NDI by reducing residual streaking artifacts. Moreover, VaNDI was able better at preserving the contrast in the basal ganglia (see zoom-in) and completed missing k-space data.

Ultra-high resolution QSM data was generated from multi-orientation scans at 0.5 mm3 isotropic resolution and R=15x acceleration using Wave-CAIPI encoding. As demonstrated in the zoom-ins, 3-dir NDI preserved the high spatial resolution of these acquisitions, while 3-dir COSMOS shows streaking artifacts and large amount of blurring at the gray-matter/white-matter boundary.

Proc. Intl. Soc. Mag. Reson. Med. 27 (2019)
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