The AFI sequence is a robust flip angle mapping method and is used within quantitative MRI protocols. AFI is a modified spoiled gradient echo (SPGR) sequence, employing interleaved TR times of different lengths. It is well known that SPGR signal behaviour is sensitive to Magnetization Transfer effects, so in this work we used a two-pool model to derive signal equations for AFI that include MT. We found that MT will lead to an underestimation of flip angle by up to 6% in white matter and that longer TR and lower RF energy lead to larger bias.
MT effects can be well described using a “two-pool” model in which longitudinal magnetization has two components $$$\mathbf{M_z}=[M_z^f M_z^r]^T$$$ where $$$M_z^f$$$ is ‘free’ (observable) magnetization and $$$M_z^r$$$ is ‘restricted’ magnetization associated with macromolecules and not directly observed. During evolution periods the modified Bloch equations12 are written $$$\mathbf{\dot{M}_z}=\mathbf{\Lambda M_z +C}$$$ where:
$$\mathbf{\Lambda} = \begin{bmatrix} -R_1^f-k & k/f \\ k & -R_1^r -k/F\end{bmatrix}$$
and
$$\mathbf{C}=\begin{bmatrix} R_1^f M_0^f \\ R_1^r M_0^r \end{bmatrix}$$
Each pool has its own relaxation rate $$$R_1^{f,r} $$$; k is the exchange rate from free to restricted pool; and F is the ratio of pool sizes $$$\frac{M_0^r}{M_0^f}$$$. An RF pulse of flip angle $$$\alpha$$$ rotates the free-pool and saturates the bound-pool, so $$$\mathbf{M_z \rightarrow \Theta M_z}$$$. Here $$$\mathbf{\Theta}=\begin{bmatrix} \cos\alpha & 0\\ 0 & e^{-\pi\gamma^2 G E_{rf}}\end{bmatrix}$$$ where G is the absorption rate of the tissue13 and $$$E_{rf}$$$ is RF pulse energy in units $$$\mu T^2 ms$$$. Figure 1 shows a sequence diagram. Steady-state expressions for magnetization at points 1 and 2 (i.e. directly before each RF pulse) are:
$$\mathbf{ M_z^1 = \left(1 - \Xi_2\Theta\Xi_1\Theta\right)^{-1}\left(\Xi_2\Theta\left(\Xi_1-1\right)+\left(\Xi_2-1\right)\right)\Lambda^{-1}C }$$
$$\mathbf{ M_z^2 = \Xi_1\Theta M_z^1 + \left(\Xi_1-1\right)\Lambda^{-1}C }$$
where $$$\mathbf{\Xi_{1,2}} = \exp\left(\mathbf{\Lambda}TR_{1,2}\right)$$$.
Apparent flip angle $$$\hat{\alpha}$$$ was estimated using the standard AFI formula3 on the ratio $$$\frac{M_z^{f,2}}{M_z^{f,1}}$$$ . MT parameters for white matter (k=4.3s-1,F=0.132;T1=779ms) and gray matter (k=1.8s-1,F=0.062,T1=1211ms) were taken from Gloor et al14. Following Gloor et.al, we fix $$$R_1^f=R_1^r$$$ and $$$T_2^r=12\mu s$$$. A single healthy adult volunteer was imaged at 3T using AFI with $$$\alpha=60°$$$, $$$E_{rf}=48.7\mu T^2ms$$$, resolution 1.5x1.5x3mm3, 30mm slab size for TR1=30,50,60 and 80ms with n=5. Strong gradient spoiling was employed.
This work was supported by the Wellcome EPSRC Centre for Medical Engineering at Kings College London (WT 203148/Z/16/Z), MRC strategic grant MR/K006355/1, EPSRC fellowship award (EP/L00531X/1) and by the National Institute for Health Research (NIHR) Biomedical Research Centre based at Guy’s and St Thomas’ NHS Foundation Trust and King’s College London. The views expressed are those of the authors and not necessarily those of the NHS, the NIHR or the Department of Health.
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