Simon Schmidt1, Kristine John2, Martin Bruschewski2, Sebastian Flassbeck1, Mark E. Ladd1, Sven Grundmann2, and Sebastian Schmitter1,3
1Medical Physics in Radiology, German Cancer Research Center (DKFZ), Heidelberg, Germany, 2Institute of Fluid Mechanics, University of Rostock, Rostock, Germany, 3Physikalisch-Technische Bundesanstalt (PTB), Braunschweig and Berlin, Germany
Synopsis
In
this work, we successfully quantified the Reynolds stress tensor (RST) in a
well-known fluid-dynamic test case: the flow over periodic hills. This test
case was chosen because the turbulence in this kind of flow is strongly
inhomogeneous and anisotropic, representing a challenging measurement task. The
results indicate, in analogy to intravoxel velocity standard deviation (IVSD)
mapping, that RST quantification is highly susceptible to the applied
$$$m_1^{enc}~$$$value.
Furthermore, RST mapping inherently requires a higher dynamic range compared to
IVSD mapping, since the shear stresses are typically much lower than the normal
stresses.
Introduction
The relationship between the first gradient
moment m1 and the signal phase is used in flow MRI to quantify mean
velocities in each voxel. Additionally,
the velocity-encoding-related signal loss can be used to characterize
turbulence1-3 and to quantify the Reynolds stress tensor (RST)4, a
fluid-dynamic parameter that
characterizes the turbulent fluctuations in fluid momentum that might be of clinical interest in pathologies with altered
hemodynamics. For intravoxel velocity standard deviation (IVSD) mapping, i.e.
the quantification of the RST’s diagonal elements, it has been reported that
the choice of m1 influences the quantified turbulence3,
since low m1 values lead only to insignificant signal loss, whereas large m1 values result in strong signal dephasing such that
magnitude images reflect the noise floor. The same problem exists for the
quantification of the RST. Here, the normal stresses (diagonal elements) are
typically substantially higher than the shear stresses (off-diagonal elements),
which requires a high dynamic m1 range to correctly quantify the
full tensor.
In
this work, we examined a well-known fluid-dynamic test case, the flow
over periodic hills. This test case was chosen because the turbulence in this flow is strongly inhomogeneous and anisotropic, representing a challenging measurement task.Theory
Assuming a Gaussian intra-voxel velocity
distribution, the corresponding magnitude of an m1-encoded MRI
signal can be expressed as:
$$\left|S\left(\vec{k}_v\right)\right|=\left|S_0\right|\cdot\exp\left(-\frac{1}{2}\vec{k}_v~\Sigma^{-1}~\vec{k}_v\right)$$
where$$$~\vec{k}_v=\gamma\left[m_{1,x}~m_{1,y}~m_{1,x}\right]^{T}$$$, $$$\gamma$$$ the gyromagnetic ratio, $$$\Sigma$$$ the variance of the 3-dimensional Gaussian, and $$$S_0$$$ the signal of a velocity-compensated measurement.
Multiplying $$$\Sigma^{-1}~$$$by the fluid density $$$\rho~$$$is equal to the RST $$$\tau$$$. Typically, $$$\tau~$$$is obtained by fitting a 3-dimensional Gaussian to the data of six velocity-encoded measurements4 with the following encoding matrix $$$E$$$, according to the ICOSA65 encoding scheme and an additional compensated measurement:
$$E=m_1^{enc}\cdot\begin{bmatrix}0&0&0\\1/sqrt\left(1+\psi^2\right)&0&\psi/sqrt\left(1+\psi^2\right)\\1/sqrt\left(1+\psi^2\right)&0&-\psi/sqrt\left(1+\psi^2\right)\\\psi/sqrt\left(1+\psi^2\right)&1/sqrt\left(1+\psi^2\right)&0\\-\psi/sqrt\left(1+\psi^2\right)&1/sqrt\left(1+\psi^2\right)&0\\0&\psi/sqrt\left(1+\psi^2\right)&1/sqrt\left(1+\psi^2\right)\\0&-\psi/sqrt\left(1+\psi^2\right)&1/sqrt\left(1+\psi^2\right)\end{bmatrix}$$
where $$$\psi=\left(1+sqrt\left(5\right)\right)/2~$$$and $$$m_1^{enc}~$$$is the applied encoding moment. These measurements correspond to six points distributed on a shell with radius $$$m_1^{enc}$$$.Methods
An in-vitro
flow test case as shown in Fig.1A was used that consisted of 13 identical
consecutive hills with measurements performed between the 10th and
11th hill. Flow rate and temperature were kept constant at 255l/min
and 22°C, resulting in a Reynolds number of Re≈60000. Data were acquired on a 3T system (Magnetom Trio,
Siemens, Germany) with a custom phase-contrast sequence employing an ICOSA6
encoding with
values of [2.5,$$$~$$$5,$$$~$$$10,$$$~$$$15,$$$~$$$20,$$$~$$$25,$$$~$$$30,$$$~$$$35,$$$~$$$40,$$$~$$$45, $$$~$$$50,$$$~$$$60] mT/m·ms². Acquisition
parameters: resolution=1.0x1.0x6.0$$$\,$$$mm³, FOV=496x120$$$\,$$$mm², TE/TR=6.32/10.0$$$\,$$$ms,
averages=256.
For
velocity quantification, the phase data were corrected for background phases by
additional measurements without flow and averages=4 but otherwise identical
settings. The velocity vector field was then reconstructed from the data
corresponding to the five lowest
$$$m_1^{enc}~$$$values to minimize phase bias from higher orders of
motion (e.g. acceleration).
The RST was quantified by two different methods.
First, by fitting a 3-dimensional Gaussian to the magnitude data of the 12 ICOSA6-encoded measurements, normalized by the velocity-compensated measurements. To avoid
the offset due to the Rician nature of the magnitude noise, data points with
less than 10% normalized magnitude were excluded from the fit. Second, the RST
was calculated by fitting a 3-dimensional Gaussian individually for every
$$$m_1^{enc}~$$$value.Results
The three velocity vector field
components shown in Fig.1C illustrate that the velocities are restricted to the
x-y plane within the examined slice. Example magnitude images for all 12
shells along the second encoding direction are shown in Fig.2A, demonstrating
the high range of turbulence present in the test case. This finding is
supported quantitatively by Fig.2B, which displays the measured data of two regions
marked in Fig.2A with corresponding Gaussian fits. Note that here, only the
projection of the three-dimensional Gaussian along the second encoding
direction is shown. Additionally, Fig.2C+D show differences between the
Gaussian fit to the full dataset compared to individual Gaussian fits to two
example
$$$m_1^{enc}~$$$values. In the case of high turbulence (Fig.2D), the individual fit to
$$$m_1^{enc}$$$=45$$$\,$$$mT/m·ms² leads
to a substantial overestimation of
$$$\Sigma~$$$and
therefore to an underestimation of the RST (7-fold for$$$~\tau_{xy}$$$).
All six components of the RST, quantified by
the Gaussian fit to the full dataset, are illustrated in Fig.3A-F. As
expected,
$$$\tau_{xx}~$$$and
$$$\tau_{xy}~$$$are
the highest normal and shear stresses with peak values of 6.4$$$\,$$$m²/s² and 3.8$$$\,$$$m²/s²
respectively. In contrast, lower shear stresses of 0.7$$$\,$$$m²/s² and -1.0$$$\,$$$m²/s² are obtained for
$$$\tau_{xz}~$$$and $$$\tau_{yz}$$$. Additionally, the turbulent kinetic energy
(TKE), the trace of the RST (see Fig.3G), yielded peak values of 6$$$\,$$$kJ/m³.
Fig.4+5 display results from the individual
Gaussian fits to five example
$$$m_1^{enc}~$$$values, indicating amplified noise for low
$$$m_1^{enc}~$$$values and peak stress
underestimation for high
$$$m_1^{enc}~$$$of up to 3-fold for
$$$\tau_{xx}~$$$and the highest
$$$m_1^{enc}$$$. Furthermore, this method fails to correctly quantify the smallest
shear stress components
$$$\tau_{xz}~$$$and
$$$\tau_{yz}$$$.Discussion
In this work, we
successfully quantified the RST in a well-known fluid-dynamic test case that
produces stresses over a high range. However, additional data either from
simulations or other reference measurements would be needed to estimate the
method’s accuracy. The results indicate, in analogy to IVSD mapping, that RST
quantification is highly susceptible to the applied$$$~m_1^{enc}~$$$value.
Furthermore, RST mapping inherently requires a higher dynamic range compared to
IVSD mapping, since the shear stresses are typically much lower than the normal
stresses.
We speculate that multiple$$$~m_1^{enc}~$$$values
are in general necessary to correctly quantify all components of the RST, not only for this
particular test case.Acknowledgements
No acknowledgement found.References
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