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Magnetic fluid deformable mirror for correcting off-axis aberrations of liquid mirror telescope

机译:用于校正液体镜望远镜的轴外像差的磁性流体可变形镜

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Liquid mirror telescope (LMT) is a viable kind of telescope with a thin rotating mercury layer, which can generate excellent parabolic surface under the constant pull of gravity and a centrifugal acceleration. The cost of LMT is normally smaller than 1% of the cost of a traditional glass mirror telescope. However, the LMT cannot be tilted to observe larger field of sky due to the liquid property so that the field of view of LMT is very limit. In order to observe a larger field of the sky with LMT, the large off-axis aberrations must be compensated. Since the aberrations of a parabolic mirror increase rapidly with the increase of field angle, the classical correctors used in adaptive optics (AO) systems cannot correct the large off-axis aberrations of LMT when the field angles are significantly greater than 1 degree. In this paper, the magnetic fluid deformable mirror (MFDM) has been proposed as a new perspective to wavefront correction technology, which could produce a large stroke to compensate the large off-axis aberrations of LMT. The designed MFDM has a radius of 95 mm with 1141 actuators, which is able to correct the large off-axis aberrations of a 3-m f/4 LMT and permits the LMT to be operated at 10 degree off-axis observation from the zenith. The type and the order of off-axis aberrations generated by the liquid mirror telescope are first studied analytically and then the 3-m f/4 LMT operated at 10 degree off-axis observation is simulated in ZEMAX, where the off-axis aberrations and the Zernike coefficients of those aberrations are obtained from the simulation result. The required surface shape of MFDM can be calculated from the obtained Zernike coefficients of off-axis aberrations. Since the shape of the magnetic fluid surface is controlled by the combined magnetic field generated by a Maxwell coil and an array of micro-electromagnetic coils, the Maxwell coil and micro-electromagnetic coils are hence optimally designed to generate the required magnetic field. The correction performance of MFDM for the large off-axis aberrations of LMT is finally co-simulated by MATLAB, COMSOL and ZEMAX software. The simulation results show that the off-axis aberrations can be compensated with the designed MFDM and the Zernike coefficients of wavefront are substantially reduced.
机译:液体镜望远镜(LMT)是一种具有薄旋转汞层的可行望远镜,其可以在恒定的重力和离心加速下产生优异的抛物面。 LMT的成本通常小于传统玻璃镜望远镜成本的1%。然而,由于液体性质,LMT不能倾斜以观察到较大的天空领域,使得LMT的视野非常限制。为了观察LMT的天空的更大领域,必须补偿大的轴外像差。由于抛物线镜的像差随着场角的增加而迅速增加,所以在自适应光学(AO)系统中使用的经典校正器不能在场角显着大于1度时校正LMT的大轴上像差。本文已经提出了磁性流体可变形镜(MFDM)作为波前校正技术的新视角,这可能产生大行程以补偿LMT的大轴偏差像差。设计的MFDM具有95毫米的半径,具有1141个致动器,能够校正3米F / 4 LMT的大轴偏差,并允许LMT在Zenith的10度离轴观察中操作。首先在分析上研究由液体镜望远镜产生的轴外像差的类型和顺序,然后在Zemax中模拟在10度的轴外观察中操作的3-MF / 4 LMT,其中偏离轴像差从仿真结果获得这些像差的Zernike系数。可以根据所获得的Zernike系数的轴轴像差来计算MFDM所需的表面形状。由于磁性流体表面的形状由Maxwell线圈产生的组合磁场和微电磁线圈阵列,因此最佳地设计用于产生所需的磁场。 LMT的大型离轴像差MFDM的校正性能最终由Matlab,COMSOL和ZEMAX软件共同模拟。仿真结果表明,偏离轴像差可以用设计的MFDM补偿,并且波前的Zernike系数基本上减小。

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