Radon transform

File:Radon transform.png

Radon transform. Maps f on the (x,Template:Nbspy)-domain to Rf on the (α,Template:Nbsps)-domain.

In mathematics, the Radon transform is the integral transform which takes a function f defined on the plane to a function Rf defined on the (two-dimensional) space of lines in the plane, whose value at a particular line is equal to the line integral of the function over that line. The transform was introduced in 1917 by Johann Radon,Template:Sfn who also provided a formula for the inverse transform. Radon further included formulas for the transform in three dimensions, in which the integral is taken over planes (integrating over lines is known as the X-ray transform). It was later generalized to higher-dimensional Euclidean spaces and more broadly in the context of integral geometry. The complex analogue of the Radon transform is known as the Penrose transform. The Radon transform is widely applicable to tomography, the creation of an image from the projection data associated with cross-sectional scans of an object.

Explanation

File:Sinogram - Two Square Indicator Phantom.svg

Radon transform of the indicator function of two squares shown in the image below. Lighter regions indicate larger function values. Black indicates zero.

File:Sinogram Source - Two Squares Phantom.svg

Original function is equal to one on the white region and zero on the dark region.

If a function<math>f</math> represents an unknown density, then the Radon transform represents the projection data obtained as the output of a tomographic scan. Hence the inverse of the Radon transform can be used to reconstruct the original density from the projection data, and thus it forms the mathematical underpinning for tomographic reconstruction, also known as iterative reconstruction.

The Radon transform data is often called a sinogram because the Radon transform of an off-center point source is a sinusoid. Consequently, the Radon transform of a number of small objects appears graphically as a number of blurred sine waves with different amplitudes and phases.

The Radon transform is useful in computed axial tomography (CAT scan), barcode scanners, electron microscopy of macromolecular assemblies like viruses and protein complexes, reflection seismology and in the solution of hyperbolic partial differential equations.

File:Radon transform sinogram.gif

Horizontal projections through the shape result in an accumulated signal (middle bar). The sinogram on the right is generated by collecting many such projections as the shape rotates. Here, color is used to highlight which object is producing which part of the signal. Note how straight features, when aligned with the projection direction, result in stronger signals.

File:Radon transform example.jpg

Example of reconstruction via the Radon transform using observations from different angles. The applied inversion to the projection data then reconstructs the slice image.<ref>Template:Cite thesis</ref>

Definition

Let <math>f(\textbf x) = f(x,y)</math> be a function that satisfies the three regularity conditions:Template:Sfn

1. <math>f(\textbf x)</math> is continuous;
2. the double integral <math>\iint\dfrac{\vert f(\textbf x)\vert }{\sqrt{x^2+y^2}} \, dx \, dy</math>, extending over the whole plane, converges;
3. for any arbitrary point <math>(x,y)</math> on the plane it holds that <math>\lim_{r\to\infty}\int_0^{2\pi} f(x+r\cos\varphi,y+r\sin\varphi) \, d\varphi=0.</math>

The Radon transform, <math>Rf</math>, is a function defined on the space of straight lines <math>L \subset \mathbb R^2</math> by the line integral along each such line as: <math display="block">Rf(L) = \int_L f(\mathbf{x}) \vert d\mathbf{x}\vert .</math>Concretely, the parametrization of any straight line <math>L</math> with respect to arc length <math>z</math> can always be written:<math display="block">(x(z),y(z)) = \Big( (z\sin\alpha+s\cos\alpha), (-z \cos\alpha + s\sin\alpha) \Big) \,</math>where <math>s</math> is the distance of <math>L </math> from the origin and <math>\alpha</math> is the angle the normal vector to <math>L</math> makes with the <math>X</math>-axis. It follows that the quantities <math>(\alpha,s)</math> can be considered as coordinates on the space of all lines in <math>\mathbb R^2</math>, and the Radon transform can be expressed in these coordinates by: <math display="block">\begin{align} Rf(\alpha,s) &= \int_{-\infty}^\infty f(x(z),y(z)) \, dz\\ &= \int_{-\infty}^\infty f\big( (z\sin\alpha+s\cos\alpha), (-z\cos\alpha+s\sin\alpha) \big) \, dz. \end{align}</math>More generally, in the <math>n</math>-dimensional Euclidean space <math>\mathbb R^n</math>, the Radon transform of a function <math>f</math> satisfying the regularity conditions is a function <math>Rf</math> on the space <math>\Sigma_n</math> of all hyperplanes in <math>\mathbb R^n</math>. It is defined by:

<math display="block">Rf(\xi) = \int_\xi f(\mathbf{x})\, d\sigma(\mathbf{x}), \quad \forall \xi \in \Sigma_n</math>where the integral is taken with respect to the natural hypersurface measure, <math>d \sigma</math> (generalizing the <math>\vert d\mathbf{x}\vert</math> term from the <math>2</math>-dimensional case). Observe that any element of <math>\Sigma_n</math> is characterized as the solution locus of an equation <math>\mathbf{x}\cdot\alpha = s</math>, where <math>\alpha \in S^{n-1}</math> is a unit vector and <math>s \in \mathbb R</math>. Thus the <math>n</math>-dimensional Radon transform may be rewritten as a function on <math>S^{n-1} \times \mathbb R</math> via: <math display="block">Rf(\alpha,s) = \int_{\mathbf{x}\cdot\alpha = s} f(\mathbf{x})\, d\sigma(\mathbf{x}).</math>It is also possible to generalize the Radon transform still further by integrating instead over <math>k</math>-dimensional affine subspaces of <math>\mathbb R^n</math>. The X-ray transform is the most widely used special case of this construction, and is obtained by integrating over straight lines.

Relationship with the Fourier transform

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File:Radon transform via Fourier transform.png

Computing the 2-dimensional Radon transform in terms of two Fourier transforms.

The Radon transform is closely related to the Fourier transform. We define the univariate Fourier transform here as: <math display="block">\hat{f}(\omega)=\int_{-\infty}^\infty f(x)e^{-2\pi ix\omega }\,dx. </math> For a function of a <math>2</math>-vector <math>\mathbf{x}=(x,y)</math>, the univariate Fourier transform is: <math display="block"> \hat{f}(\mathbf{w})=\iint_{\mathbb R^2} f(\mathbf{x})e^{-2\pi i\mathbf{x}\cdot\mathbf{w}}\,dx\, dy. </math> For convenience, denote <math>\mathcal{R}_\alpha[f](s)= \mathcal{R}[f](\alpha,s)</math>. The Fourier slice theorem then states: <math display="block"> \widehat{\mathcal{R}_{\alpha}[f]}(\sigma)=\hat{f}(\sigma\mathbf{n}(\alpha)) </math> where <math>\mathbf{n}(\alpha)= (\cos \alpha,\sin\alpha).</math>

Thus the two-dimensional Fourier transform of the initial function along a line at the inclination angle <math>\alpha</math> is the one variable Fourier transform of the Radon transform (acquired at angle <math>\alpha</math>) of that function. This fact can be used to compute both the Radon transform and its inverse. The result can be generalized into n dimensions: <math display="block">\hat{f}(r\alpha) = \int_{\mathbb R}\mathcal{R}f(\alpha,s)e^{-2\pi i sr} \, ds.</math>

Dual transform

The dual Radon transform is a kind of adjoint to the Radon transform. Beginning with a function g on the space <math>\Sigma_n</math>, the dual Radon transform is the function <math>\mathcal{R}^*g</math> on Rⁿ defined by: <math display="block">\mathcal{R}^*g(\mathbf{x}) = \int_{\mathbf{x}\in\xi} g(\xi)\,d\mu(\xi).</math>The integral here is taken over the set of all hyperplanes incident with the point <math>\textbf x \in \mathbb R^n</math>, and the measure <math>d \mu</math> is the unique probability measure on the set <math>\{\xi | \mathbf{x}\in\xi\}</math> invariant under rotations about the point <math>\mathbf{x}</math>.

Concretely, for the two-dimensional Radon transform, the dual transform is given by: <math display="block">\mathcal{R}^*g(\mathbf{x}) = \frac{1}{2\pi}\int_{\alpha=0}^{2\pi}g(\alpha,\mathbf{n}(\alpha)\cdot\mathbf{x})\,d\alpha.</math> In the context of image processing, the dual transform is commonly called back-projectionTemplate:Sfn as it takes a function defined on each line in the plane and 'smears' or projects it back over the line to produce an image.

Intertwining property

Let <math>\Delta</math> denote the Laplacian on <math>\mathbb R^n</math> defined by:<math display="block">\Delta = \frac{\partial^2}{\partial x_1^2}+\cdots+\frac{\partial^2}{\partial x_n^2}</math>This is a natural rotationally invariant second-order differential operator. On <math>\Sigma_n</math>, the "radial" second derivative <math>Lf(\alpha,s) \equiv \frac{\partial^2}{\partial s^2} f(\alpha,s)</math> is also rotationally invariant. The Radon transform and its dual are intertwining operators for these two differential operators in the sense that:Template:Sfn <math display="block">\mathcal{R}(\Delta f) = L (\mathcal{R}f),\quad \mathcal{R}^* (Lg) = \Delta(\mathcal{R}^*g).</math>In analysing the solutions to the wave equation in multiple spatial dimensions, the intertwining property leads to the translational representation of Lax and Philips.<ref>Template:Cite journal</ref> In imaging<ref> Template:Cite journal</ref> and numerical analysis<ref>Template:Cite journal</ref> this is exploited to reduce multi-dimensional problems into single-dimensional ones, as a dimensional splitting method.

Reconstruction approaches

The process of reconstruction produces the image (or function <math>f</math> in the previous section) from its projection data. Reconstruction is an inverse problem.

Radon inversion formula

In the two-dimensional case, the most commonly used analytical formula to recover <math>f</math> from its Radon transform is the Filtered Back-projection Formula or Radon Inversion FormulaTemplate:Sfn: <math display="block">f(\mathbf{x})=\int^\pi_0 (\mathcal{R}f(\cdot,\theta)*h)(\left\langle\mathbf{x},\mathbf{n}_\theta \right\rangle) \, d\theta</math>where <math>h</math> is such that <math>\hat{h}(k)=|k|</math>.Template:Sfn The convolution kernel <math>h</math> is referred to as Ramp filter in some literature.

Ill-posedness

Intuitively, in the filtered back-projection formula, by analogy with differentiation, for which <math display="inline">\left(\widehat{\frac{d}{dx}f}\right)\!(k)=ik\widehat{f}(k)</math>, we see that the filter performs an operation similar to a derivative. Roughly speaking, then, the filter makes objects more singular. A quantitive statement of the ill-posedness of Radon inversion goes as follows:<math display="block">\widehat{\mathcal{R}^*\mathcal{R} [g]}(\mathbf{k}) = \frac{1}{\|\mathbf{k}\|} \hat{g}(\mathbf{k})</math> where <math>\mathcal{R}^*</math> is the previously defined adjoint to the Radon transform. Thus for <math>g(\mathbf{x}) = e^{i \left\langle\mathbf{k}_0,\mathbf{x}\right\rangle}</math>, we have: <math display="block"> \mathcal{R}^*\mathcal{R}[g](\mathbf{x}) = \frac{1}{\|\mathbf{k_0}\|} e^{i \left\langle\mathbf{k}_0,\mathbf{x}\right\rangle}</math> The complex exponential <math>e^{i \left\langle\mathbf{k}_0,\mathbf{x}\right\rangle}</math> is thus an eigenfunction of <math>\mathcal{R}^*\mathcal{R}</math> with eigenvalue <math display="inline">\frac{1}{\|\mathbf{k}_0\|}</math>. Thus the singular values of <math>\mathcal{R}</math> are <math display="inline">\frac{1}\sqrt{\|\mathbf{k}\|}</math>. Since these singular values tend to <math>0</math>, <math>\mathcal{R}^{-1}</math> is unbounded.Template:Sfn

Iterative reconstruction methods

{{#invoke:Labelled list hatnote|labelledList|Main article|Main articles|Main page|Main pages}} Compared with the Filtered Back-projection method, iterative reconstruction costs large computation time, limiting its practical use. However, due to the ill-posedness of Radon Inversion, the Filtered Back-projection method may be infeasible in the presence of discontinuity or noise. Iterative reconstruction methods (e.g. iterative Sparse Asymptotic Minimum Variance<ref name=AbeidaZhang>Template:Cite journal</ref>) could provide metal artefact reduction, noise and dose reduction for the reconstructed result that attract much research interest around the world.

Inversion formulas

Explicit and computationally efficient inversion formulas for the Radon transform and its dual are available. The Radon transform in <math>n</math> dimensions can be inverted by the formula:Template:Sfn <math display="block">c_n f = (-\Delta)^{(n-1)/2}R^*Rf\,</math>where <math>c_n = (4\pi)^{(n-1)/2}\frac{\Gamma(n/2)}{\Gamma(1/2)}</math>, and the power of the Laplacian <math>(-\Delta)^{(n-1)/2}</math> is defined as a pseudo-differential operator if necessary by the Fourier transform: <math display="block">\left[\mathcal{F}(-\Delta)^{(n-1)/2} \varphi\right](\xi) = |2\pi\xi|^{n-1}(\mathcal{F}\varphi)(\xi).</math>For computational purposes, the power of the Laplacian is commuted with the dual transform <math>R^*</math> to give:Template:Sfn <math display="block">c_nf = \begin{cases} R^*\frac{d^{n-1}}{ds^{n-1}}Rf & n \text{ odd}\\ R^* \mathcal H_s\frac{d^{n-1}}{ds^{n-1}}Rf & n \text{ even} \end{cases} </math>where <math>\mathcal H_s</math> is the Hilbert transform with respect to the s variable. In two dimensions, the operator <math>\mathcal H_s\frac{d}{ds} </math> appears in image processing as a ramp filter.Template:Sfn One can prove directly from the Fourier slice theorem and change of variables for integration that for a compactly supported continuous function <math>f </math> of two variables: <math display="block">f = \frac{1}{2}R^{*}\mathcal H_s\frac{d}{ds}Rf.</math>Thus in an image processing context the original image <math>f </math> can be recovered from the 'sinogram' data <math>Rf </math> by applying a ramp filter (in the <math>s</math> variable) and then back-projecting. As the filtering step can be performed efficiently (for example using digital signal processing techniques) and the back projection step is simply an accumulation of values in the pixels of the image, this results in a highly efficient, and hence widely used, algorithm.

Explicitly, the inversion formula obtained by the latter method is:Template:Sfn <math display="block">f(x) = \begin{cases} \displaystyle - \imath 2\pi (2\pi)^{-n}(-1)^{n/2}\int_{S^{n-1}}\frac{\partial^{n-1}}{2\partial s^{n-1}}Rf(\alpha,\alpha\cdot x)\,d\alpha & n \text{ odd} \\ \displaystyle (2\pi)^{-n}(-1)^{n/2}\iint_{\mathbb R \times S^{n-1}}\frac{\partial^{n-1}}{q\partial s^{n-1}} Rf(\alpha,\alpha\cdot x + q)\,d\alpha\,dq & n \text{ even} \\ \end{cases}</math>The dual transform can also be inverted by an analogous formula: <math display="block">c_n g = (-L)^{(n-1)/2}R(R^*g).\,</math>

Radon transform in algebraic geometry

In algebraic geometry, a Radon transform (also known as the Brylinski–Radon transform) is constructed as follows.

Write

<math>\mathbf P^d \, \stackrel{p_1} \gets \, H \, \stackrel{p_2}\to \, \mathbf P^{\vee, d}</math>

for the universal hyperplane, i.e., H consists of pairs (x, h) where x is a point in d-dimensional projective space <math>\mathbf P^d</math> and h is a point in the dual projective space (in other words, x is a line through the origin in (d+1)-dimensional affine space, and h is a hyperplane in that space) such that x is contained in h.

Then the Brylinksi–Radon transform is the functor between appropriate derived categories of étale sheaves

<math> \operatorname{Rad} := Rp_{2,*} p_1^* : D(\mathbf P^d) \to D(\mathbf P^{\vee, d}).</math>

The main theorem about this transform is that this transform induces an equivalence of the categories of perverse sheaves on the projective space and its dual projective space, up to constant sheaves.<ref>Template:Harvtxt</ref>

See also

• Periodogram
• Matched filter
• Deconvolution
• X-ray transform
• Funk transform
• The Hough transform, when written in a continuous form, is very similar, if not equivalent, to the Radon transform.Template:Sfn
• Cauchy–Crofton theorem is a closely related formula for computing the length of curves in space.
• Fast Fourier transform

References

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Further reading

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External links

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