scholarly journals Suppression of Rayleigh scattering noise in sodium laser guide stars by hyperfine depolarization of fluorescence

2006 ◽  
Vol 14 (24) ◽  
pp. 11494 ◽  
Author(s):  
Hugues Guillet de Chatellus ◽  
Ioana Moldovan ◽  
Vincent Fesquet ◽  
Jean-Paul Pique
Author(s):  
Felipe Pedreros Bustos ◽  
Ronald Holzlöhner ◽  
Domenico Bonaccini Calia ◽  
Joschua Hellemeier ◽  
Simon Rochester ◽  
...  

1991 ◽  
Author(s):  
Laird A. Thompson ◽  
Richard M. Castle ◽  
David L. Carroll

2020 ◽  
Vol 37 (4) ◽  
pp. 1208
Author(s):  
F. Pedreros Bustos ◽  
R. Holzlöhner ◽  
S. Rochester ◽  
D. Bonaccini Calia ◽  
J. Hellemeier ◽  
...  

2009 ◽  
Vol 17 (7) ◽  
pp. 4920 ◽  
Author(s):  
Fabien Marc ◽  
Hugues Guillet de Chatellus ◽  
Jean-Paul Pique

2014 ◽  
Vol 3 (3) ◽  
Author(s):  
Domenico Bonaccini Calia ◽  
Wolfgang Hackenberg ◽  
Ronald Holzlöhner ◽  
Steffan Lewis ◽  
Thomas Pfrommer

AbstractGround-based optical telescopes, in particular large ones, require adaptive optics to overcome the atmospheric seeing limit due to turbulence. Correcting the distorted wavefront necessitates bright stars in the field of view. The sky coverage can be greatly increased by using artificial sodium laser guide stars in addition to natural guide stars. We describe the underlying physics and technical considerations relevant to such systems before discussing the design of the four-laser guide star facility (4LGSF) which is currently under development for the ESO Very Large Telescope (VLT) on Cerro Paranal, Chile. The focus is upon the justification of the requirements and their technical solution.


2010 ◽  
Author(s):  
Wilhelm G. Kaenders ◽  
Axel Friedenauer ◽  
Vladimir Karpov ◽  
Vladimir Protopopov ◽  
Wallace R. L. Clements ◽  
...  

2015 ◽  
Vol 32 (12) ◽  
pp. 2425 ◽  
Author(s):  
Rachel Rampy ◽  
Donald Gavel ◽  
Simon M. Rochester ◽  
Ronald Holzlöhner

1995 ◽  
Vol 439 ◽  
pp. 455 ◽  
Author(s):  
M. Lloyd-Hart ◽  
J. R. P. Angel ◽  
B. Jacobsen ◽  
D. Wittman ◽  
R. Dekany ◽  
...  

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