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Divergent Geometries

For both equilinear (second generation) and equiangular (third, fourth, and fifth generation) geometries, the x-ray beams diverge from a single source to a detector array. In the equilinear mode, a single source produces a fan beam which is read by a linear array of detectors. If the detectors occupy an arc of a circle, then the geometry is equiangular.

Fan Beam Angle
For these divergent beam geometries, the fan beam angle needs to be calculated. For real-world CT scanners, this is fixed at the time of manufacture. CTSim, however, calculates the fan beam angle, alpha, from the scan diameter and the focal length as

alpha = 2 x asin ( (Sd / 2) / f)

Empiric testing with CTSim shows that for very large fan beam angles, greater than approximately 120 degrees, there are significant artifacts. The primary way to manage the fan beam angle is by varying the focal length since the scan diameter is usually fixed at the size of the phantom.

To illustrate, the scan diameter can be defined as

Sd = Sr x Vr x Pd

Further, the focal length can be defined as

F = FR x (VR x Pd)

Substituting these equations into the above equation, We have,

alpha = 2 sin (Sr / Fr)

Since in normal scanning s_r = 1, alpha depends only upon the focal length ratio in normal scanning.

Detector Array Size
In general, you do not need to be concerned with the detector array size -- it is automatically calculated by CTSim. For the particularly interested, this section explains how the detector array size is calculated.

For parallel geometry, the detector length is simply the scan diameter.

For divergent beam geometries, the size of the detector array also depends upon the focal length: increasing the focal length decreases the size of the detector array.

For equiangular geometry, the detectors are equally spaced around a arc covering an angular distance of alpha as viewed from the source. When viewed from the center of the scanning, the angular distance is
pi + alpha - 2 x acos ((Sd / 2) / C))
The dotted circle indicates the positions of the detectors in this case.

For equilinear geometry, the detectors are equally spaced along a straight line. The detector length depends upon alpha and the focal length. This length, Dl, is calculated as

2 x (F + C) x tan(alpha/2)