Figure 7. Relative illumination examples. Light collecting efficiency
Light collection efficiency is proportional to 1/ (f/#)2, where f/# = (focal length)/(aperture size). The smaller the f/#, the better the efficiency. There are some trade-offs with a small f/# optical system. As the aperture size increases, there tend to be more vignetting and aberrations, which make the optics more challenging to design. A low f/# system also tends to have shallower depth of field.
Relative illumination (RI) and chief ray angle (CRA) RI is defined as:
The sensor illuminance declines based on the (cos q) law, in a distortion and vignetting free lens system where q is the CRA incident angle on the sensor plane. The result is a relative darkening of the image toward the sensor border. The irradiance fall-off can be reduced by introducing negative distortion in the lens system. The max CRA at the sensor edge should be optimised based on the imager microlens array specification. A smaller CRA helps narrow the bandwidth of the BPF to achieve better ambient light immunity.
The following examples demonstrate how the CRA and the focused light cone sizes (effective f/#) across the field affect the RI. The lens system of Example 1 in Figure 7 has larger CRAs and gradually decreasing imaging cones (that is, increased f/#) as the field
Instrumentation Monthly April 2025
angle increases. The corresponding RI drops significantly with the field angle as shown in the corresponding RI plot. Example 2 in Figure 7 demonstrates that the RI can be well maintained by minimising the CRA as well as keeping uniform f/# across the field.
Stray light
Stray light is any unintended light in a system that could be detected by the sensor. Stray light can come from in or out of field sources that form a ghost image (for example, lens flare) through even numbers of reflections. Stray light can also emanate from opto-mechanical structures and any scattering surfaces. ToF systems are particularly sensitive to stray light because the multipath nature of stray light
Continued on page 50... 49
Page 1 |
Page 2 |
Page 3 |
Page 4 |
Page 5 |
Page 6 |
Page 7 |
Page 8 |
Page 9 |
Page 10 |
Page 11 |
Page 12 |
Page 13 |
Page 14 |
Page 15 |
Page 16 |
Page 17 |
Page 18 |
Page 19 |
Page 20 |
Page 21 |
Page 22 |
Page 23 |
Page 24 |
Page 25 |
Page 26 |
Page 27 |
Page 28 |
Page 29 |
Page 30 |
Page 31 |
Page 32 |
Page 33 |
Page 34 |
Page 35 |
Page 36 |
Page 37 |
Page 38 |
Page 39 |
Page 40 |
Page 41 |
Page 42 |
Page 43 |
Page 44 |
Page 45 |
Page 46 |
Page 47 |
Page 48 |
Page 49 |
Page 50 |
Page 51 |
Page 52 |
Page 53 |
Page 54 |
Page 55 |
Page 56 |
Page 57 |
Page 58 |
Page 59 |
Page 60 |
Page 61 |
Page 62 |
Page 63 |
Page 64 |
Page 65 |
Page 66 |
Page 67 |
Page 68 |
Page 69 |
Page 70 |
Page 71 |
Page 72 |
Page 73 |
Page 74 |
Page 75 |
Page 76 |
Page 77 |
Page 78 |
Page 79 |
Page 80