Abstract
The optical and technical characteristics of the tie-in between the chromospheric AFR-2 telescope and the digital camera Sony DSC-S85 are determined by computer simulation. The optimal layout of the camera, telescope optics, and collective lens is established. The modulation transfer function is used as an optimization parameter (quality criterion for the solar disk image in Hα).
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 callDisclaimer: 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.
