DSPographer
Senior Member
There are two main sources of black point noise. One is dark current which is a leakage of electrons in the photodetector in the absence of light which obeys Poisson statistics (it is an electron count) and the other is pre-amplifier noise. The RMS pre-amplifier noise is not at a level of the square root of the detected signal so it is not Poisson distributed; in general this noise is zero mean so it does not contribute to the mean black level measured. The total dark noise is the combination of these two independent noise sources (their variances add). If the black level is 25 e- (RMS noise of 5 e-) and the RMS pre-amplifier noise is 4 e- (I have seen numbers close to this level quoted for Canon's CMOS sensor pre-amplifiers) then the total dark noise is sqrt(5^2 + 4^2) or 6.4 e- RMS. This noise is still much less than the mean black level of 25 e- that is measured.