Abstract
Possibilities of the correction of the general wavefront tilt using a signal from a laser guide star (LGS) are analyzed. The quality of an image of an extraterrestrial object formed by an astronomic optical system through a turbulent atmosphere is analyzed. The efficiency of the adaptive correction of distortions for different LGS schemes is analyzed. Calculations are performed for different models of the vertical dependence of the structural parameter of the refractive index of the turbulent atmosphere.
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.
