Radon Transformation
📂TomographyRadon Transformation
Definition
Let’s assume that a function f:D→R is defined on some 2D domain D⊂R2. The Radon transform Rf of f is defined as follows, for s∈R, θ=(cosθ,sinθ)∈S1,
Rf(s,θ):== t=−∞∫∞f(sθ+tθ⊥)dt t=−∞∫∞f(scosθ−tsinθ,ssinθ+tcosθ)dt
Explanation
Radon transform is a type of integral transform named after the Austrian mathematician Johann Radon (1887-1956).
The radioactive element radon is not named after the mathematician Radon, but rather its name comes from the word ‘radioactive’ with the inert gas suffix ‘-on’ added.
The geometric meaning of Rf(s,θ) is the integration of f at all points that are s away from the origin and perpendicular to θ.
While f is a function of Cartesian coordinates (x,y), the Radon transform Rf is a function of polar coordinates (s,θ).
The Radon transform is one of the core principles of CT and is based on the physical law known as Beer-Lambert’s law. This law states that the intensity of X-rays decreases differently depending on the type of medium they pass through. A reduction in the intensity of X-rays means that the medium has absorbed the X-rays. The extent to which a medium absorbs light is referred to as the attenuated coefficient, absorption coefficient, or absorbance. The fact that different media have different attenuation coefficients is utilized in non-destructive inspection using X-rays in CT. The reason why bones appear white in X-ray images is because bones absorb more X-rays than other materials.
Another Expression of the Definition
When ls,θ is considered as a line determined by polar coordinates (s,θ),
Rf(s,θ)=∫ls,θf
Thinking about the geometric meaning,
Rf(s,θ)=x⋅θ=s∫f(x)dx
When defined as θ⊥:={u:u⋅θ=0},
Rf(s,θ)=θ⊥∫f(sθ+u)du
Regarding the Dirac delta function δ,
Rf(s,θ)=R2∫f(x)δ(x⋅θ−s)dx
Generalization
For s∈R1, θ∈Sn−1, the Radon transform R:L2(Rn)→L2(Zn) is defined as follows.
Rf(s,θ)=x⋅θ=s∫f(x)dx
Here, Zn:=R1×Sn−1 is a unit cylinder in n+1 dimensions.
Derivation
Let’s designate x as the position, I(x) as the intensity of X-rays, and A(x) as the attenuation coefficient of the medium.
Beer-Lambert Law
The rate of change of the intensity of X-rays is as follows.
dxdI=−A(x)I(x)

Let x0 and x1 represent the starting and ending positions of the X-rays, respectively, and I0 and I1 represent the intensity of the X-rays at each point. When we separate the variables in (1) and integrate both sides, we obtain the following.
⟹⟹⟹∫x0x1I(x)1dIln(I1)−ln(I0)ln(I0I1)ln(I1I0)=−∫x0x1A(x)dx=−∫x0x1A(x)dx=−∫x0x1A(x)dx=∫x0x1A(x)dx
Looking at this equation, I0 is the intensity when the X-rays are shot, which is a known value. I1 is the intensity after the X-rays have passed through the object, and this value is measured by the detector located at x0. Therefore, the left side is a known value.
The range of integration on the right side is the path traveled by the X-rays we shot, so it is known. Hence, given the path L of the X-rays and the intensities I0, I1 at both ends, we can obtain the value obtained by integrating A(x) over the path L. This is referred to as the Radon transform of A(x).
Rf(L):=∫Lf(x)dx=ln(I1I0)
Properties
The basic properties of the Radon transform are as follows.
Linearity
R(αf+βg)=αRf+βRg
Shift Invariance
RTaf(s,θ)=Ta⋅θRf(s,θ)
Rotation Invariance
RAf=ARf
Dilation Invariance
RDrf=D1rRf