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Eliminating the static aberrations in an MCAO system

机译:消除MCAO系统中的静态像差

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Within the last years, the Adaptive Optics (AO) systems built or designed are growing in complexity: their optics are numerous and they aim at better performances on-axis and/or in the Field of View. A limiting factor to those performances can be the Non-Common Path Aberrations (NCPA), i.e. static aberrations present in the optical path of the instrument after the dichroic, which therefore are not seen by the AO Wave Front Sensor. Since long the Deformable Mirror of the system has been used to partially compensate for them, in a more or less efficient and complex way. This paper will present a rapid to implement, rather simple and all-measured method of compensation for the NCPA tanks to the use of Phase Diversity and of a calibration matrix of the modes constituting the aberrations. Moreover for systems composed of several DMs, we will present how a clever use of those can reduce significantly the aberrations in the whole FoV. All those techniques will be illustrated by their application to ESO'S MCAO Demonstrator (MAD).
机译:在过去的几年中,构建或设计的自适应光学(AO)系统的复杂性不断提高:它们的光学系统众多,它们的目标是在轴上和/或视场中具有更好的性能。这些性能的限制因素可能是非公共路径像差(NCPA),即二向色性后仪器光路中存在的静态像差,因此AO Wave Front Sensor无法看到。长期以来,系统的可变形镜已被用来以某种或多或少的效率和复杂的方式对它们进行部分补偿。本文将介绍一种快速实施,相当简单和全面的补偿方法,用于使用相差和构成像差模式的校准矩阵对NCPA储罐进行补偿。此外,对于由多个DM组成的系统,我们将介绍如何巧妙地使用它们可以显着降低整个FoV中的像差。所有这些技术将通过在ESO的MCAO演示器(MAD)中的应用进行说明。

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