Tomographic wave-front sensing with a single guide star

Tomographic wave-front sensing with a single guide star

Adaptive optics or numerical restoration algorithms that restore high resolution imaging through atmospheric turbulence are subject to isoplanatic wave-front errors. Mitigating those errors requires that the wave-front aberrations be estimated within the 3D volume of the atmosphere. Present techniqu...

Full description

Bibliographic Details
Main Authors: Hart, Michael, Jefferies, Stuart, Hope, Douglas
Other Authors: Univ Arizona, Coll Opt Sci
Language:en
Published: SPIE-INT SOC OPTICAL ENGINEERING 2016
Subjects:
wave-front sensing
tomography
anisoplanatism
telescopes
Online Access:Michael Hart ; Stuart Jefferies and Douglas Hope " Tomographic wave-front sensing with a single guide star ", Proc. SPIE 9982, Unconventional Imaging and Wavefront Sensing XII, 998207 (November 1, 2016); doi:10.1117/12.2257358; http://dx.doi.org/10.1117/12.2257358
http://hdl.handle.net/10150/622717
http://arizona.openrepository.com/arizona/handle/10150/622717

Internet

Michael Hart ; Stuart Jefferies and Douglas Hope " Tomographic wave-front sensing with a single guide star ", Proc. SPIE 9982, Unconventional Imaging and Wavefront Sensing XII, 998207 (November 1, 2016); doi:10.1117/12.2257358; http://dx.doi.org/10.1117/12.2257358
http://hdl.handle.net/10150/622717
http://arizona.openrepository.com/arizona/handle/10150/622717

Similar Items