Abstract
Through the aid of electronic light amplifiers, observers can view terrain on moonless nights with near-daylight acuity. This improvement in vision is obtained by using imaging sensors with larger lenses, greater quantum efficiencies, wider spectral responses, and larger photosensitive areas than those of the unaided eye. The observer’s improved resolving power using these sensors can be calculated in terms of a limiting resolution vs light level and an elemental signal-to-noise ratio at any operating point. The analysis facilitates the comparison of sensors on an equal basis and provides the system designer with more detailed sensor operating data. As examples, the limiting performance is calculated for the image orthicon and the secondary-electron conduction camera tube with and without cascaded image intensifiers. The calculated results are compared to those measured and are found to be in good agreement.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.