Abstract

This paper presents the results of recording stars and space objects under daytime conditions, using a video camera with a silicon photodetector array. Algorithms for summing up to 300 frames of video images and two-point correction of spatial (geometrical) noise of the array are used in real time in the camera. They made it possible to reduce temporal and spatial noise, to increase the visualization threshold of magnitude, and to observe low-brightness stars and space objects with magnitudes of 8m–10m under daytime conditions from various sites in the northern hemisphere of the sky.

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

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.