scholarly journals Effects of Linewidth Broadening Method on Recoil of Sodium Laser Guide Star

Atmosphere ◽  
2021 ◽  
Vol 12 (10) ◽  
pp. 1315
Author(s):  
Xiangyuan Liu ◽  
Xianmei Qian ◽  
Rui He ◽  
Dandan Liu ◽  
Chaolong Cui ◽  
...  

The linewidth broadening of the circular-polarized continuous wave laser mitigates the recoil effects of the sodium laser guide star very well. By choice of the optimal laser linewidth, the relations between the laser intensity and average spontaneous emission rates are obtained. The numerically simulated results show that the 1–100 MHz linewidth broadening effectively weakens recoil and enhances the average spontaneous emission rates. For laser powers from 10 W to 60 W, considering the intensity distribution with random at the mesospheric sodium layer, when the laser linewidth is broadened to be 1–100 MHz from 0 MHz, increments of the return photons go up to 110% from 50% and do not have an effect on the spot sizes of the sodium laser guide star. Several cases have proven that the linewidth broadening method is correct. Further calculations show that the linewidth broadening method similarly applies to the case of the multi-mode laser. Furthermore, the linewidth broadening of re-pumping should be taken into account.

2003 ◽  
Vol 20 (10) ◽  
pp. 2093 ◽  
Author(s):  
Jean-Paul Pique ◽  
Sébastien Farinotti

2010 ◽  
Vol 511 ◽  
pp. A31 ◽  
Author(s):  
N. Moussaoui ◽  
B. R. Clemesha ◽  
R. Holzlöhner ◽  
D. M. Simonich ◽  
D. Bonaccini Calia ◽  
...  

1989 ◽  
Author(s):  
Chester S. Gardner ◽  
Byron M. Welsh ◽  
Laird A. Thompson

1999 ◽  
Author(s):  
David J. Butler ◽  
Richard I. Davies ◽  
Hayden Fews ◽  
Wolfgang K. P. Hackenberg ◽  
Sebastian Rabien ◽  
...  

2015 ◽  
Author(s):  
Feng Wang ◽  
Wei Zhang ◽  
Tianjiang Chen ◽  
Wenchao Zhou ◽  
Hong Yan

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.


1997 ◽  
Author(s):  
Andreas Quirrenbach ◽  
Wolfgang K. P. Hackenberg ◽  
Hans-Christoph Holstenberg ◽  
Norbert Wilnhammer

2015 ◽  
Author(s):  
Lu Feng ◽  
Edward Kibblewhite ◽  
Kai Jin ◽  
Suijian Xue ◽  
Zhixia Shen ◽  
...  

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