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Direct computation of myocardial deformation and strain from

tagged cine MRI

Citation for published version (APA):

Florack, L. M. J., & Assen, van, H. C. (2008). Direct computation of myocardial deformation and strain from

tagged cine MRI. (CASA-report; Vol. 0822). Technische Universiteit Eindhoven.

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Published: 01/01/2008

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and Strain from Tagged Cine MRI

Luc Florack1,2 and Hans van Assen2

1 Department of Mathematics and Computer Science, Eindhoven University of

Technology, The Netherlands, L.M.J.Florack@tue.nl

2 Department of Biomedical Engineering, Eindhoven University of Technology,

The Netherlands, H.C.v.Assen@tue.nl

Abstract. Myocardial deformation and strain can be investigated us-ing suitably encoded cine MRI that admits disambiguation of material motion. Practical limitations restrict the analysis to in-plane motion in cross-sections of the heart (2D+time), but the proposed method readily generalizes to 3D+time. Time evolution of the deformation tensor is gov-erned by a first order ordinary differential equation, which is completely determined by the velocity gradient tensor. We solve this matrix-ODE analytically, and present results obtained from healthy volunteers. The proposed method is robust and requires only off-the-shelf algorithms.

1

Introduction

Cine MRI [1], combined with (C)SPAMM3 encoding technology [2–4], admits disambiguation of local tissue motion, thus enabling the extraction of myocardial deformation and strain [5]. This can be achieved either without explicit a priori regularization, or through exploitation of sparse constraints combined with in-terpolation and/or regularization [3, 6–31]. Possible encodings are DENSE (Dis-placement ENcoding with Stimulated Echoes), and HARP (HARmonic Phase). Tagging based methods using HARP technology form our point of departure. Given a dense motion field within the myocardium, our aim is to devise an op-erational procedure for direct extraction of myocardial deformation and strain. By “direct” we mean that we seek to obviate sophisticated preprocessing steps, such as segmentation of, or interpolation between tag lines, finite element meth-ods explicitly coupled to the tagging pattern, etc. Although such sophisticated “indirect” procedures exist and have been proven powerful, they require spe-cific algorithmics that is neither trivially implemented nor readily available. In addition we aim to minimize the number of extrinsic control parameters. We

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believe that the parsimony of our method facilitates applicability and optimiza-tion, since only off-the-shelf algorithms (linear filtering and inversion of linear systems) are needed in our computation of myocardial deformation and strain.

2

Theory

2.1 Deformation

The velocity gradient tensor, with components Lα

βrelative to a coordinate frame,

relates the rate of change of a momentary infinitesimal line element d ˙xα to the

line element dxβitself. It can be shown that (employing summation convention)

d ˙xα= Lα

βdxβ with Lαβ =

∂vα

∂xβ (α, β = 1, . . . , n) . (1)

The numbers Lα

β constitute a matrix L with row and column index4 α, β. To

get an estimate of this tensor field we have applied the algorithm of Van Assen et al. and Florack et al. [9, 11], solving a linear system of algebraic equations. Tissue deformation can be described by a map f : M → N : x(X, t0) 7→ x(X, t), in which x(X, t) denotes the spatial position of a material point at time t, with reference position X = x(X, t0) at time t0(“Lagrange picture”). Domain M and codomain N are copies of the deformable tissue medium (a subset of IRn) at

times t0, respectively t ≥ t0. We fix t0so as to correspond to end-diastole. The associated differential map,

f∗≡ df : T MX −→ T Nx: v 7→ f∗(v) = viFiαfα, (2)

relative to a basis {fα} of T Nx, provides a local linearization of tissue

deforma-tion, the deformation tensor. Here T MXis the tangent space of M at the fiducial

point X = x(X, t0), and T Nxthat of N at the f -mapped point x = x(X, t). The

matrix F (t, t0) of this linear map relative to the local coordinate charts {xα, N }

and {Xi, M } is given by the Jacobian

i =

∂xα

∂Xi. (3)

By virtue of the chain rule, the relation between deformation and velocity gra-dient tensors, Eqs. (1) and (3), is given by the first order ODE [32]

˙

F = L F , (4)

4 Our analysis is confined to a single short-axis plane, whence n = 2, i.e. we only

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subject to an initial condition, viz. F (t = t0, t0) = I. Equivalently, F (t, t0) = I +

Z t

t0

L(s) F (s, t0) ds . (5)

This induces an expansion known as the matricant, cf. Gantmacher [32]: F (t, t0) = I + Z t t0 L(τ ) dτ + Z t t0 L(τ ) Z τ t0 L(σ) dσ dτ + . . . (6) The matricant has the following property:

F (t, t0) = F (t, t1) F (t1, t0) (t0< t1< t) . (7) It follows that, if we split the interval [t0, t] into n parts by using intermediate points t1, . . . , tn−1separated by ∆tk = tk− tk−1(k = 1, . . . , n, with tn= t),

F (t, t0) = F (t, tn−1) . . . F (t1, t0) with t0< t1< . . . < tn−1< tn= t. (8)

For an infinitesimally narrow time interval [tk−1, tk] we have by approximation

F (tk, tk−1) = I + L(t∗k) ∆tk+ higher order terms in ∆tk, (9)

in which t∗

k is any point satisfying tk−1 ≤ t∗k ≤ tk. Eqs. (8–9) give rise to a

representation in terms of a so-called multiplicative integral [32]: F (t, t0) =∼ Z t t0 (I + L(τ ) dτ )def= lim ∆tk→0(I +L(t n) ∆tn). . .(I +L(t∗1) ∆t1) . (10) One recognizes the multiplicative counterpart of the Riemann sum approxima-tion for ordinary (“additive”) integrals. One can show that this is identical to

F (t, t0)[32]= ∼ Z t

t0

exp (L(τ ) dτ )def= lim

∆tk→0exp (L(t

n) ∆tn). . .exp (L(t∗1) ∆t1) . (11) Several properties of the deformation tensor are manifest in this representation. For instance, since for square matrices A, B, one has (i) det AB = det A det B, (ii) det(I + ²A) = 1 + ²tr A + O(²2), and (iii) det exp A = exp tr A, it shows that

det F (t, t0) =∼ Z t t0 (1 + tr L(τ ) dτ ) =∼ Z t t0 exp (tr L(τ ) dτ ) . (12) In particular, a divergence free velocity field (div v = tr L = 0) preserves volumes: det F (t, t0) = 1. Furthermore, exp A exp B = exp(A + B) if [A, B] = 0, whence for a stationary velocity field (L(t) = L0pointwise constant) one finds F (t, t0) = exp ((t − t0)L0). Finally, the multiplicative integral suggests a straightforward numerical approximation, viz. by using either Eq. (10) or (11) without limiting procedure. (In this case the two representations are of course no longer identical.)

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4

2.2 Strain

On the basis of the differential map f∗, Eq. (2), and its transpose f∗T, one defines

an intrinsic mapping on T MX, known as the Lagrangian strain tensor [33],

E ≡1 2(f

T

◦ f∗− idT MX) : T MX→ T MX: v 7→ E(v) = viEijej, (13)

relative to a basis {ej} of T MX, with mixed tensor components

Eij= 1 2 ³ g`jFα `hαβFiβ− δij ´ . (14)

Here gij are the components of the dual (Euclidean) metric tensor in domain

co-ordinates {Xi, M }, and h

αβ those pertaining to codomain coordinates {xα, N }.

Note that if f∗is an isometry, then E vanishes identically by construction. Thus

E captures nonrigid deformations only.

Below we consider a single Cartesian coordinate system for both domain and codomain. (In such a system the representations of the various metric tensors, gij and hαβ and their duals, gij and hαβ, all simplify to identity matrices.)

3

Experiment

Figure 1 illustrates various scalar fields extracted from the strain tensor field, Eqs. (13–14), by contraction with a pair of local unit vectors, viz. radial (r=radial) and azimuthal (c=circumferential) basis vectors of the polar coordinate system centered at the midpoint of the region of interest, and those defining the strain tensor’s eigensystem. If u, v ∈ T MX are two such unit vectors, then the local

scalar quantity derived from the strain tensor is given by the inner product (u, E(v)) = (E(u), v) = gjkukEijvi. Tensor components are evaluated in

Carte-sian coordinates. Figure 2 illustrates temporal evolutions of these quantities spatially averaged over the respective regions of interest, together with their standard deviations. Table 1 shows statistics for three healthy volunteers.

4

Conclusion

We have proposed a simple and robust linear model for extracting myocardial deformation and strain. Material motion and gradient velocity are determined by a multi-scale linear system of algebraic equations. We have analytically solved the linear matrix-ODE governing myocardial deformation. By discretizing the closed-form solution we have subsequently solved for the induced Lagrangian strain tensor field, yielding results that are typical for healthy volunteers, cf.

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Garot et al. [12], thus demonstrating the feasibility of our method. An advantage of our method is that only off-the-shelf algorithms are needed. This serves clarity, facilitates optimization, and enables implementation on dedicated hardware. Of course, our quantitative results demand evaluation by a more comprehensive benchmarking on in vivo as well as carefully controlled synthetic or phantom data. Moreover, by virtue of the transparent mathematical framework, it is pos-sible to assess tolerances on the basis of theoretical error propagation models. Future investigation will be needed to pursue these recommendations, and com-pare theoretically predicted and experimentally observed performance measures. Acknowledgments. The Netherlands Organisation for Scientific Research (NWO) is gratefully acknowledged for financial support. Jos Westenberg has provided the MR data used in our experiments.

base mid apex

I II III I II III I II III

−0.16±0.13 −0.17±0.11 −0.19±0.11 −0.19±0.09 −0.17±0.08 −0.15±0.09 −0.16±0.16 −0.20±0.09 −0.19±0.13

0.20±0.25 0.16±0.21 0.14±0.25 0.04±0.20 0.14±0.15 0.03±0.15 0.07±0.23 0.20±0.23 −0.02±0.18 0.02±0.15 −0.04±0.12 −0.07±0.13 0.01±0.07 −0.02±0.09 −0.06±0.11 0.07±0.14 −0.03±0.11 −0.05±0.12 0.25±0.22 0.19±0.20 0.18±0.23 0.07±0.17 0.16±0.15 0.09±0.16 0.15±0.21 0.22±0.22 0.05±0.19

−0.22±0.11 −0.21±0.09 −0.24±0.09 −0.23±0.09 −0.19±0.08 −0.21±0.07 −0.26±0.12 −0.23±0.09 −0.27±0.09

Table 1. Average and standard deviation of strains from three healthy volunteers (labels I,II,III) over base, mid, and apex short-axis cross-sectional ROIs at that time frame at which Emaxhas attained its maximum in mid-slice (tI= 16, tII= 15, tIII= 14).

Rows correspond to, from top to bottom, Ecc, Err, Ecr, Emax, and Emin.

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8 -0.3 0.3 0 -0.3 0.3 0 -0.3 0.3 0 -0.3 0.3 0 -0.3 0.3 0

Fig. 1. Color-coded strain fields in short axis mid-slice cross-sections, time frames 1, 6, 11, 16, 21 (a full heart cycle subtends 42 frames), regularized through Gaussian blurring with spatial scale σ = 1.0, for one healthy volunteer. First row: Circumferential strain Ecc. Second row: Radial strain Err. Third row: Shear strain Ecr. Fourth row:

Minimal strain eigenvalue Emin. Fifth row: Maximal strain eigenvalue Emax.

5 10 15 20 -0.3 -0.2 -0.1 0.0 0.1 0.2 0.3 Time Frame Strain MID slice Ecc Err Ecr 5 10 15 20 -0.3 -0.2 -0.1 0.0 0.1 0.2 0.3 Time Frame Strain MID slice Emax Emin

Fig. 2. Temporal evolution of scalar strain quantities over the first half of the heart cycle (i.e. mostly systolic) in mid-slice cross-section. Error bars indicate standard de-viations over the spatial ROI in each time frame, thus capture all sources of variation due to noise, numerics, and true spatial variability. Legends explain the various graphs. Notice the strong correlation between the extrinsic (polar system related) and instrinsic (eigensystem related) strains. (In the eigensystem, shear strain vanishes identically.)

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