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Towards Laser-Guide-Stars for Multi-Aperture Interferometry: an application to the Hypertelescope

机译:针对多孔径干涉测量的激光导星:a   应用于Hypertelescope

摘要

Optical interferometry has been successful at achieving milliarcsecondresolution on bright stars. Imaging performance can improve greatly byincreasing the number of baselines, which has motivated proposals to buildlarge (~ 100 m) optical interferometers with tens to hundreds of telescopes. Itis also desirable to adaptively correct atmospheric turbulence to obtain directphased images of astrophysical sources. When a natural guide star is notavailable, we investigate the feasibility of using a modified laser-guide-startechnique that is suitable for large diluted apertures. The method consists ofusing sub-sets of apertures to create an array of artificial stars in thesodium layer and collecting back-scattered light with the same sub-apertures.We present some numerical and laboratory simulations that quantify therequirements and sensitivity of the technique.
机译:光学干涉测量法已经成功地在明亮的恒星上实现了毫秒级的分辨率。通过增加基线数量可以大大提高成像性能,这促使人们提议使用数十到数百个望远镜来构建大型(〜100 m)光学干涉仪。还希望自适应地校正大气湍流以获得天体物理源的直接相位图像。当没有自然导星时,我们将研究使用适用于大稀释孔径的改良激光导星技术的可行性。该方法包括使用孔的子集在钠层中创建人造星的阵列,并收集具有相同子孔径的反向散射光。我们提供了一些数值模拟和实验室模拟,以量化该技术的要求和灵敏度。

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