Laser Guide Star Adaptive Optical systems become an established technique at telescope facilities with large apertures. At these aperture diameters, such as 8m class telescope facilities, the finite distance and vertical extend of an artificial excited guide star result in perspective elongation, which produces errors in wave-front reconstruction and could influence the performance of adaptive optical systems seriously. In this paper, we shall briefly introduce and explain the effect of the perspective elongation, and show some results of theoretical simulation and experiment. First of all, we analyzed how the perspective elongation of sodium LGS changes, and gave the results of simulation which indicated the relation between the perspective elongation and some related parameters. The aberration caused by the elongation was analyzed, and the possibility of aberration correction was discussed. Based on the results of the theoretical simulation, we designed an experiment to observe the perspective elongation. A transmitting and receiving system has been set up. The system consisted of a 300mJ sodium LGS laser, a telescope with an aperture diameter of 450mm, a beam expander with an aperture diameter of 200mm, a LGS detecting device, etc. Based on the pulsed laser and the mobile LGS projector, we operated the experiment at different distance between the telescope and the laser projector. A series of elongated images, corresponding the distance from 5m to 30m, was obtained. The analytic results of the image data agreed with the theoretical simulation. Based on the experimental data, we deduced the aberration of wave-front at 30m separation. According to theoretical simulation of the perspective elongation, the effects including the aberration of wave-front could be achieved, which had been partially verified in the experiment. We suggest that one could improve the reconstruction accuracy in a sodium or Rayleigh LGS adaptive optical system by eliminating the influence of the perspective elongation in advance.
Using pulsed Sodium laser beacon,the exploration experiment of the return light measurement is carried out. The wavefront of Sodium laser beacon of one pulse and the wavefront of natural star of the same direction are measured using two Shack-Hartmann wavefront sensors simultaneously. The results of experimental data analysis show that the return photons numbers received of Shack-Hartmann wavefront sensor’s one subaperture are more than 200, and the intensity of Sodium laser beacon’s return light is even and steady. The signal-to-noise ratio of light spot distribution is about 3~5. The statistical variance of each order Zernike coefficient of Sodium laser beacon’s wavefront and natural star’s wavefront is consistent in the gross, and the pertinency of each order Zernike coefficient is well.
Wavefront sampling is important for beam parameters measurement. A new method to perform the
large aperture beam sampling with array-lens was put forward. A 25×25 array-lens of wavefront distortion
measurement was designed, and an experimental system was settled up. The perfect parallel beam is used to
demarcate the large aperture array-lens beam sampler. And a large aperture wavefront of distortion was measured by
the set. That the experiment result is in accordance with the theoretical calculation.