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Optics physical limits

Abstract We explain the laser guide star concept and why we do need laser guide stars (LGS) to greatly enhance adaptive optics performances at large telescopes. Then we discuss the two physical limitations of LGS, which are the cone effect and the indetermination of the tilt of the incoming wavefront. Solutions to overcome them are explained. [Pg.249]

Polimeni JR, Granquist-Fraser D, Wood RJ, Schwartz EL. 2005. Physical limits to spatial resolution of optical recording clarifying the spatial structure of cortical hypercolumns. Proc Natl Acad Sd USA 102(11) 4158-4163. [Pg.15]

On the use of limited configuration interaction for many-body systems Journal of Physics B Atomic, Molecular Optical Physics 33 4735 (2000)... [Pg.62]

See other pages where Optics physical limits is mentioned: [Pg.2853]    [Pg.162]    [Pg.378]    [Pg.331]    [Pg.228]    [Pg.303]    [Pg.364]    [Pg.510]    [Pg.755]    [Pg.15]    [Pg.23]    [Pg.136]    [Pg.47]    [Pg.356]    [Pg.303]    [Pg.387]    [Pg.87]    [Pg.95]    [Pg.197]    [Pg.6382]    [Pg.615]    [Pg.25]    [Pg.606]    [Pg.331]    [Pg.4]    [Pg.80]    [Pg.224]    [Pg.140]    [Pg.101]    [Pg.625]    [Pg.351]    [Pg.2853]    [Pg.6381]    [Pg.606]    [Pg.224]    [Pg.131]    [Pg.209]    [Pg.341]    [Pg.351]    [Pg.538]    [Pg.287]    [Pg.5]    [Pg.117]    [Pg.671]    [Pg.5112]    [Pg.750]    [Pg.2016]    [Pg.177]   
See also in sourсe #XX -- [ Pg.23 , Pg.28 , Pg.43 ]



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