Anders Dyhr Sandgaard1, Valerij G. Kiselev2, Noam Shemesh3, and Sune Nørhøj Jespersen1,4
1Department of Clinical Medicine, Center for Functionally Integrative Neuroscience, Aarhus University, Aarhus, Denmark, 2Medical Physics, Department of Radiology, Faculty of Medicine, University of Freiburg, Freiburg, Germany, 3Champalimaud Research, Champalimaud Centre for the Unknown, Lisbon, Portugal, 4Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark
Synopsis
Mapping tissue magnetic properties with MRI may improve
the diagnosis of diseases and enhance our understanding of their basic
mechanisms. However, MRI signals are sensitive to both structure and magnetic susceptibility,
the so-called “magnetic microstructure”, rendering accurate susceptibility
estimation a great challenge. Here, we present an analytical expression for the
Larmor frequency of a white matter model of myelinated axons with axially
symmetric microscopic susceptibility anisotropy and orientation dispersion. The
modelled axons are surrounded by microscopic spherical inclusions with a scalar
susceptibility. This goes beyond previous models of white matter magnetic microstructure.
Introduction
Magnetic susceptibility
of tissue contains valuable information about chemical composition, enabling
noninvasive mapping of de-myelination1, calcification2, iron-dyshomeostasis3. However,
accurate estimation of white matter (WM) constituents remains challenging, as
myelinated axons exhibit susceptibility tensor character4, are orientationally disperse5, and surrounded by iron-rich tissue6. Previous studies have modelled WM by the so-called generalized
mesoscopic Lorentzian tensor7,8, but such approaches were limited to parallel axons and or
low volume fractions. Here we relax these restrictions and present
an analytical expression for a system with two coexisting types of
inclusions; orientationally disperse, myelinated axons, and spherical
inclusions. Each axon is modeled by multiple concentric cylinders with axially
symmetric microscopic susceptibility anisotropy to mimic myelin layers; the randomly
positioned microscopic spherical inclusions with a scalar
susceptibility represent iron-rich sources residing outside the
cylinders with a scalar susceptibility.Theory
Magnetic microstructure
Figure 1 conceptualizes the magnetic microstructure. We model it as a porous medium embedded in an NMR-visible fluid8. The cylinders are infinitely long and randomly positioned (Figure 1A), described by the microscopic indicator function $$$\nu^C(\mathrm{r})$$$. They possess an axially symmetric microscopic susceptibility (Figure 1B),
$$\chi^C=\begin{pmatrix}\chi_\parallel&0&0\\0&\chi_\perp&0\\0&0&\chi_\perp\end{pmatrix}\qquad{(1)}$$
in the lipid eigen-frame ($$$\chi_\parallel$$$ is in the radial direction), and $$$\Delta\chi=\chi_\parallel-\chi_\perp$$$ defines the microscopic susceptibility anisotropy. Cylinders occupy the fraction $$$\zeta^C$$$ of the total volume $$$V$$$. Randomly positioned microscopic spherical inclusions with scalar susceptibility $$$\chi^S$$$ (Figure 1C) reside outside cylinders according to $$$\nu^S(\mathrm{r})$$$ and occupy a volume fraction $$$\zeta^S$$$.
Larmor frequency
When exposing the sample to an external magnetic field $$$\mathbf{B}_0=\mathrm{B}_0\hat{\mathbf{B}}$$$, inclusions become magnetized and induce a magnetic field, perturbing the Larmor frequency of the measured FID signal $$$S(t)$$$. In the fast diffusion regime and in the limit of small signal phase, this perturbation, $$$\Omega=\mathrm{arg}\{S(t)\}/t$$$, becomes
$$\Omega=\gamma{\mathrm{B}_{0}}{{\mathbf{\hat{B}}}^{\text{T}}}\frac{1}{\left(1-\zeta^S-\zeta^C\right)V}\int_Vd\mathbf{r}\left(1-\nu\left(\mathbf{r}\right)\right)\int_{V}{d\mathbf{{r}'}}\mathbf{\Upsilon}\left(\mathbf{r-{r}'}\right)\nu \left({\mathbf{{r}'}}\right)\mathbf{\chi}\left({\mathbf{{r}'}}\right)\mathbf{\hat{B}}.\qquad{(2)}$$
$$$\mathbf{\Upsilon}$$$ is the Lorentz-corrected dipole field9. As explained in previous studies8, and illustrated in Figure 2, $$$\Omega$$$ can be divided into two contributions: a mesoscopic, $$$\Omega^\mathrm{Meso}$$$, and a macroscopic, $$$\Omega^\mathrm{Macro}$$$ one, capturing magnetic field-effects at corresponding length scales, respectively: $$\Omega=\Omega^\mathrm{Meso}+\Omega^\mathrm{Macro}.\qquad{(3)}$$
We find $$$\Omega^\mathrm{Macro}$$$ depends on coarsed magnetic microstructure and overall sample shape
$$\Omega^\mathrm{Macro}=\gamma{\mathrm{B}_{0}}{{\mathbf{\hat{B}}}^{\text{T}}}\mathbf{\Upsilon}^{\mathrm{Macro}}\left(\zeta^C\chi_\perp+\zeta^S\chi^S+\zeta^C\Delta\chi\left(\sum_{m=-2}^2p^{2m}\mathbf{\mathcal{Y}}^{2m}-1\right)\right)\mathbf{\hat{B}},\qquad{(4)}$$
where $$\mathbf{\Upsilon}^{\mathrm{Macro}}=\frac{1}{V}\int_Vd\mathbf{r}\int_Vd\mathbf{r}'\mathbf{\Upsilon}(\mathbf{r}-\mathbf{r}')\qquad{(5)}$$
denotes the sample-averaged dipole tensor, $$$p^{2m}$$$ are $$$l=2$$$ Laplace expansion coefficients of the fiber orientation distribution (fODF), $$$\mathcal{Y}^{2m}$$$ is the $$$l=2$$$ symmetric trace-free tensor representation of SO(3)10. For $$$\Omega^\mathrm{Meso}$$$ we find
$$\Omega^\mathrm{Meso}=-\gamma{\mathrm{B}_{0}}\left(\left(\zeta^C\chi_\perp-\tilde{\zeta}^S\chi^S\right)\sum_{m=-2}^2p^{2m}Y_2^m(\mathbf{\hat{B}})+\Delta\chi\frac{1}{3}\left(\frac{1}{6}\zeta^C-\tilde{\zeta}^C\right)\left(p^{2m}Y_2^m(\mathbf{\hat{B}})-1\right)
\right).\qquad{(6)}$$
$$$\tilde{\zeta}^C$$$ describes intra-cylindrical structure
$$\tilde{\zeta}^C=\frac{1}{1-\zeta^S-\zeta^C}\left(\sum_{m>w}\left(\zeta^C_{R_m}-\zeta^C_{r_m}\right)\mathrm{ln}\left(\frac{R_w}{r_w}\right)-\sum_w\mathrm{ln}\left(\frac{R_w}{r_w}\right)\right).\qquad{(7)}$$
$$$R_m$$$ denotes the radius of the outer layers of the mth shell with volume fraction $$$\zeta^C_{R_m}$$$, while $$$r_m$$$ denotes inner radii of each shell. $$$\tilde{\zeta}^S$$$ is an effective spherical weight defined by
$$\tilde{\zeta}^S=\zeta^S\frac{\zeta^C+\zeta^S\frac{\zeta^{EC}}{1-\zeta^{EC}}}{1-\zeta^S-\zeta^C},\qquad{(8)}$$
where $$$\zeta^{EC}$$$ denotes extra-cylindrical volume fraction.Methods
Validation
We
performed computer simulations to validate $$$\Omega^\mathrm{Meso}$$$ (Eq. (6)). $$$\Omega^\mathrm{Meso}$$$ was validated previously11 when $$$\Delta\chi=\chi^S=0$$$ in the presence of
orientation dispersion. Here we limit the validation to consider a multi-layer
cylinder surrounded by spherical inclusions (full description can be found in Figure 3) as a comprehensive numerical
validation is ongoing.
Predicted
Larmor frequency
We
considered the predicted behavior of $$$\Omega^\mathrm{Meso}$$$ for
cylinders with axially symmetric orientation dispersion surrounded by spherical
inclusions (a full description can be found in Figure 4). We varied 1) Orientation dispersion from
parallel to uniformly oriented; 2)
susceptibility anisotropy; and 3) sphere susceptibility.Results
Figure 3 shows simulations
validating $$$\Omega^\mathrm{Meso}$$$, while Figure 4 demonstrates the
predicted behavior of $$$\Omega^\mathrm{Meso}$$$. Its overall
functional behavior is $$$A\cdot\sin(\theta)^2+B$$$, where $$$\theta$$$ is the angle
between the mean cylinder axis and external field $$$\mathbf{\hat{B}}$$$. We find orientation dispersion dampens $$$\Omega^\mathrm{Meso}$$$ variation, while $$$\Delta\chi$$$ produces a non-zero $$$\Omega^\mathrm{Meso}$$$ (approx -0.1 of $$$\gamma\mathrm{B}_0\chi_\perp$$$ for this microstructure) for maximal dispersion and changes
the zero-crossing away from the magic angle. Spherical
inclusions produce a small contribution that
depends on the model fODF.
This stems from the correlation in the sphere positions induced by the presence
of cylinders via the restriction of no overlap.Discussion
Equations (6)-(8) reveal the behavior of $$$\Omega^\mathrm{Meso}$$$ for a WM model consisting of long cylinders and spherical
inclusions. $$$\Omega^\mathrm{Meso}$$$ depends on volume-weighted susceptibility parameters
describing the average magnetic response for each inclusion-type, while
their orientation is captured by $$$p^{2m}$$$ of the fODF.
Estimating $$$p^{2m}$$$ from diffusion MRI (dMRI), removes 5 structural parameters, which leaves only 3 undermined susceptibilities. Resolving all parameters would thus require
measuring $$$\Omega$$$ at multiple orientations or exploiting additional information from other contrasts
or modalities. The functional behavior
of $$$\Omega^\mathrm{Meso}$$$ (c.f. figure 4) agrees with
recent findings12 for the mesoscopic frequency from WM axons, and generalizes the mesoscopic Lorentzian tensor7,8 for this microstructure.
Limitations
Our model is a simplification of real WM microstructure, where axons exhibit axonal caliber-variation, undulation13,
and inclusions in all water
compartments. However, it captures important microstructural features
that have not been accounted for previously,
as current models assume parallel
cylinders and low volume fraction. Furthermore, our model can easily be
extended to include e.g., myelin-basic proteins, phospholipid-proteins within
the lipids and cylindrical inclusions such as unmyelinated axons,
neurofilaments and microtubules.Conclusion
We presented an expression for the Larmor
frequency of a WM model consisting of
multi-layer cylinders, with orientation dispersion and susceptibility
anisotropy, surrounded by spherical inclusions with isotropic susceptibility. This goes beyond previous models7,8 and relates orientation dependence to
the fODF, measurable with dMRI11,14-16. We believe this result brings susceptibility MRI one step closer
to becoming a useful tool in clinical research.Acknowledgements
This study is funded by the Independent Research Fund (grant 8020-00158B), Denmark, and by Helga & Peter Korning's Foundation.References
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