Every radiometric measurement uses a detector in some way. This chapter discusses how they are described and delineates their most important properties with respect to radiometric measurements.
7.1 Detector Descriptions
The responsivity of a detector is the electrical output divided by the optical input. The inputs and outputs can take different forms. The output is often a voltage or a current, but sometimes it is a count of pulses or even a temporal frequency (which may have been generated by a voltage-to-frequency converter). In this text, for most purposes, the electrical output will be assumed to be either voltage or current. The input is a power or photon rate on the detector. It may be monochromatic, bandlimited, or cover the entire optical spectrum (say 95% to 99% of the radiation). The responsivity is almost always written as a script R, i.e., â. Thus the signal voltage can be written as V s =âÎ¦=â«â(Î»)Î¦(Î»)dÎ». The total noise arises from several sources, but, no matter how many and what kind, the total noise can be written V n =â«V 2 n (f)df − − − − − − − − − √ , where the spot noise, the noise at a given frequency, V n (f) , is the sum of all the noise components at that frequency. Therefore the signal-to-noise ratio, SNR, is given by SNR=V s V n =âÎ¦ V n =â«â(Î»)Î¦(Î»)dÎ» â«V 2 n (f)df √ .
Online access to SPIE eBooks is limited to subscribing institutions.