Modulation Transfer Function (MTF) is the measurement of a lens’ ability to transfer contrast at a particular resolution from the object to the image. It is the widely accepted fundamental parameter for the characterisation of optical systems worldwide. Knowledge of the MTF curves of the lenses and camera sensors involved in an optical system helps optimise optical system performance.
With LEO satellites, the image is moving on the surface of the detector, and thus MTF has to be measured dynamically. The CNES (French Space Agency) has built a bench to measure dynamic MTF of detectors (CCD and CMOS), especially those working in TDI (Time delay and integration) mode. It is based on a moving edge, synchronized with the movement of charges inside the TDI detector.
This document details how the MTF of the FINCH Eye Build I will be tested. This test will likely be executed in Spring 2023 and its results shall be compared to our requirement(s) obtained in collaboration with Data Processing.
For this test, we are not evaluating MTF at all spatial frequencies. The frequency of interest is the specific Nyquist frequency: $f_N=1/2a$ where a = pixel pitch.
One easy method for the MTF measurement at a defined frequency is the evaluation of the contrast. Here, we use an object made of black & white fringes. At Nyquist frequency, the image of a fringe has the same width as a pixel. The spatial resolution is directly linked to the capacity to distinguish the black from the white.
The image of this object on a pixel as a function of its position is a sine wave, so the Contrast Transfer Function (CTF) is easily calculated as:
where ϕ_dark = dark signal level