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Lines Determined by Polar Coordinates 📂Tomography

Lines Determined by Polar Coordinates

Description

Lines Determined by Polar Coordinates

그림1.png

A line, as shown in Figure (1), is determined by the slope aa and the yy intercept bb. It seems that all lines on a plane can be represented only by their slope and intercept, but this is not the case. Precisely, only lines can be depicted as functions. Therefore, a line perpendicular to the xx axis, as shown in Figure (2), cannot be represented by its slope and intercept.

그림2.png

Now, observe Figure (3). This line is perpendicular to the unit vector θ=(cosθ,sinθ)\boldsymbol{\theta} = (\cos \theta, \sin \theta) and is at a distance ss from the origin. Hence, we can understand that a line on a plane is determined by the polar coordinates (s,θ)(s, \theta). Additionally, unlike the method using slope and intercept, a line perpendicular to the xx axis, as shown in Figure (4), can also be expressed in polar coordinates.

This notation for lines is useful in expressing line integrals in cases like Radon Transform.

Points on a Line

그림3.png

As illustrated in the figure above, by adding the parameter tt, we can represent a point on a line. If we designate θ=(cosθ,sinθ)\boldsymbol{\theta}=(\cos \theta, \sin \theta), θ=(sinθ,cosθ)\boldsymbol{\theta}^\perp=(-\sin \theta, \cos \theta), we get:

P= sθ+tθ= (scosθ,ssinθ)+(tsinθ,tcosθ)= (scosθtsinθ,ssinθ+tcosθ) \begin{align*} P =&\ s\boldsymbol{\theta} + t \boldsymbol{\theta}^\perp \\ =&\ (s\cos\theta, s\sin\theta) + (-t \sin\theta, t \cos\theta) \\ =&\ (s\cos\theta-t \sin\theta, s\sin\theta+ t \cos\theta) \end{align*}

Then, a line ls,θl_{s, \theta} determined by ss and θ\theta is the same as the following set:

ls,θ={sθ+tθ:tR} l_{s, \theta} = \left\{ s\boldsymbol{\theta} + t \boldsymbol{\theta}^\perp : t \in \mathbb{R} \right\}

Moreover, since s(cos(θ+π),sin(θ+π))=s(cosθ,sinθ)-s \big(\cos(\theta + \pi), \sin (\theta + \pi)\big) = s(\cos \theta, \sin \theta), for a negative ss, it is defined as follows:

ls,θ+π:=ls,θ l_{-s, \theta+\pi} := l_{s, \theta}

Generalization

For Rn\mathbb{R}^{n}, a line that is perpendicular to the unit vector θSn1\boldsymbol{\theta} \in \mathbb{S}^{n-1} and is at a distance ss from the origin can be described as follows:

ls,θ={sθ+tθ:tR} l_{s, \boldsymbol{\theta}} = \left\{ s\boldsymbol{\theta} + t \boldsymbol{\theta}^\perp : t \in \mathbb{R} \right\}