Hai Luo1, Meining Chen1, Ziyue Wu2, Bei Lv1, Fei Peng1, Shijie Wang1, Wenkui Hou1, Weiqian Wang1, and Gaojie Zhu1
1AllTech Medical Systems, Chengdu, China, 2Marvel Stone Healthcare, Wuxi, China
Synopsis
Compared with magnitude value, phase of
MRI signal is more prone to be influenced by motion. A novel method,
sensitivity constrained phase update (sCPU) was proposed for robust and
efficient ghost artifacts reduction. Using coil sensitivities as constraints, a
synthetic image can be generated in which the
ghost is reduced due to phase cancelation. Phase error was first estimated from
the raw image and the synthetic image, and then was used to update the phase of
raw k-space. The results with simulated and in-vivo data show that the ghost artifacts
can be efficiently reduced after several iterations.
Introduction
Many techniques have been designed to
compensate for pseudo-periodic1-4 and rigid-body motion5. Some of these techniques
need to oversample the K-space data to estimate motion, such as PROPELLER4,5.
Another kind of retrospective techniques compensate
the motion in K-space, such as COCOA6 and PANDA7. Empirical thresholds are used
in these techniques to identify the corrupted data, which are hard to be
optimized for different clinical cases. Moreover, although these techniques are
effective against random or sudden movement, they are ineffective when there is
strong coherence of the ghost (Eg: rigid translation). Here a novel, sensitivity constrained
phase update method, is proposed for the reduction of different kinds of ghost
artifacts. Compared with magnitude
value, phase of MRI signal is more prone to be influenced by motion. So once the
phase error is corrected, the ghost artifacts can be largely suppressed. Method
For each individual coil image at position $$$y$$$, ghost artifacts were modulated by sensitivities, it could be written as $$m_i(y)=S_i(y)m_i(y)+\sum_{p=1}^{P}\omega_pS_i(y+\Delta y_p)m_k(y+\Delta y_p)\qquad(1)$$Here $$$S_i$$$ is the sensitivity, $$$y+∆y_p$$$ represents where the folded artifacts is come from and totally $$$P$$$ folded positions. $$$ω_p$$$ is the ghost level.Using sensitivities as a constraint, a synthetic image can be generated via equation (2) $$synm_i(y)=S_i(y)\frac{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}m_k(y)}{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}S_k(y)} \qquad(2)$$ $$$ψ_(j,k)$$$is the noise
correlation, combining equations (1) and (2),$$synm_i(y)=S_i(y)m_i(y)+S_i(y)\frac{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}[\sum_{p=1}^{P}\omega_pS_k(y+\Delta y_p)m_k(y+\Delta y_p)]}{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}S_k(y)} $$
$$=S_i(y)m_i(y)+S_i(y)\sum_{p=1}^{P}\omega_p{\chi} m_{k}(y+\Delta y_p) \qquad(3)$$
where$$\chi=\frac{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}S_k(y+\Delta y_p)}{\sum_{j,k}S_{j}^{*}(y)\psi_{j,k}S_k(y)}$$
For phase array coils, sensitivity is spatially varied that means $$$S_j (y)$$$ and $$$S_k (y+∆y_p )$$$ have different phase and magnitude. $$$\chi$$$ is much less than 1 due to high probability of phase cancellation. So, the ghost component in synthetic image is smaller while the true image component remains unchanged, as in Fig 1.
Fourier Transform of the difference of raw and synthetic image into frequency domain, we can get the phase error$$\Delta \varphi_i=\phi (F(m_i-synm_i)) \qquad(4)$$Where $$$F$$$ is the Fourier Transform operator and $$$ϕ$$$ is a phase operator. To control the noise amplification during the phase update, a magnitude weighted phase combination of all coils was performed. $$\Delta \varphi=\sum_{i}^{N}\lambda_i\Delta \varphi_i \qquad(5)$$Finally, phase error $$$\Delta \varphi$$$
can be subtracted
from the raw k-space to reduce the ghost artifact, the iterative update approach
could be written as$$ K_{n+1}=K_ne^{-i\Delta \varphi}\qquad(6)$$
Simulated and in-vivo data was used to
validate the proposed method. A standard head image and 8ch sensitivities (http://hansenms.github.io/sunrise/sunrise2013/) were used for simulation, with
both linear and random phase error to simulate motion induced artifacts. Also Gaussian
noise was simulated to verify the degradation due to noise.
Two in-vivo datasets, head T2 FSE
images and abdominal triggered T2 FSE images, were acquired on a 1.5T
whole-body scanner (Centauri, Alltech Medical Systems). For head imaging, acquisition
parameters were ETL 16, FOV 230mmx230mm, TR/TE 5000/90ms, matrix size 256*256
and 8 channel head coil. There were two intentional slight head shakes during
the scan. For abdominal imaging, acquisition parameters were ETL 16, FOV
300mmx350mm, TR/TE 3672/90ms, matrix size 240*256, 15 channel torso coil. Since
the volunteer’s breathing was very bad, there were obvious ghost artifacts. The sensitivity maps were calibrated via ESPIRiT8 with 6x6 kernel
from 24 calibration lines.Results
Fig. 2
shows the ghost reduction results with simulated data. Fig.2a & Fig.2d are
the simulated ghost images with linear and random phase error respectively.
Fig.2b & Fig.2e are the correction results and Fig.2c & Fig.2f are the
ghost map. The ghost artifact had almost been cleared in 10 iterations, but a
little noise amplification is seen.
Fig. 3
shows convergence performance and noise amplification during the iterations.
The algorithm converges very fast that the residual ghost is very small after
5~10 iterations while the noise amplification increases slowly with iteration. From this simulation, 5~10 iteration is a good compromise between ghost reduction
and noise amplification.
Fig.4&Fig.5
are the in-vivo application of the proposed method. The results show that the
ghost due to head shake or irregular breathing had been dramatically reduced.
The
computing time per 256x256 image for 10 iteration is about 500ms, using MATLAB
on a PC with Intel i7@3.6GHz and 16G RAM.Disscussion
Advantages: First of all, the proposed
method does not require extra hardware or additional data. Second, both
Cartesian and non-Cartesian acquisition are applicable. Third, this method is
fast and robust, ghost due to periodic or random motion can be efficiently
reduced.
Sensitivity map: Accurate and fast
varying receiver sensitivity map is the critical factor for estimating the
phase error. Since phase array coils were optimized for parallel imaging, the
sensitivity often varies fast. From our test results, sensitivity map via ESPIRiT
calibration is accurate enough in most cases.
Noise
amplification: There was a bit more noise amplification for large number
iteration. From the simulation, 5~10 iteration is a good compromise between
ghost reduction and noise amplification. Filtering or fitting the phase error can be implemented as a further work to control the noise amplification.Conclusion
A novel method, named sCPU, was proposed for robust and efficent ghost
reduction. Motion induced error was estimated from the raw image and a sensitivity constrained synthetic image, then it was subtracted from
the raw k-space to iteratively reduce ghost artifact. The results with simulated
and in-vivo datasets show that the ghost artifacts can be efficiently reduced after
several iterations.
(Code: https://github.com/concher009/MRI/tree/master/sCPU )Acknowledgements
No acknowledgement found.References
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