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Wavelet-Based Adaptive Optics

机译:基于小波的自适应光学

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Adaptive systems are useful when the signals or images are changing with time. For example, with adaptive wavelets, different filters are used for different parts of the signal: the signal itself should indicate whether a high or low order filter should be used. With adaptive optics, rapidly varying atmospheric wavefront distortions in a medium changing with time is reduced using optics: i.e. in astronomical adaptive optical systems, a system of control-driven de-formable mirrors eliminates distortion produced by a medium changing with time. Adaptive wavelets has the potential for achieving the same objective while reducing cost. Adaptive optics provides real-time compensation for aberrations produced by atmospheric turbulence, jitter, and the optics. The adaptive optics subsystem consists of a Wavefront Sensor, Real-Time Reconstructor and Server Compensator, Deformable Mirror, Tilt Correction, Optical Assembly, and Adaptive Optics Control. The Wavefront Sensor senses phase difference and wavefront tilts. The Real-Time Reconstructor and Servo Compensation system computes the Deformable Mirror actuator. The Tilt Correction system corrects wavefront tilt errors and angle of arrival jitter caused by atmospheric turbulence, mount vibration, wobble dynamics lag and system vibration. In summation, adaptive optics systems are highly complex and both assembly and maintenance very expensive. Adaptive wavelets offers the potential of simplifying the system and reducing the cost. The ultimate goal is higher image resolution. Adaptive systems are important when the signals or environments are changing in time. With adaptive lifting, the prediction/update filters or wavelet/ scaling functions are chosen in a fixed fashion. They can be chosen in such a way that a signal is approximated with very high accuracy using only a limited number of coefficients. Different prediction filters can be used for different parts of the signal. A high or low order prediction filter is chosen based on the signal itself. For example, the space-adaptive approach, the prediction filter depends on local information of the image pixels of one of two complementary groups. For applying adaptive wavelet lifting to optical images modulated by atmospheric turbulence, certain assumptions can be made: (1) the image is radially symmetric, and (2) the atmospheric turbulence is to some degree periodic. After that, choice of the prediction filter will take into account the characteristics of the optical image being investigated. Phase, for example, is never an easy problem.
机译:当信号或图像随时间变化时,自适应系统很有用。例如,对于自适应小波,信号的不同部分使用了不同的滤波器:信号本身应指示应使用高阶还是低阶滤波器。使用自适应光学器件,可以通过使用光学器件减少随时间变化的介质中迅速变化的大气波阵面畸变:即在天文自适应光学系统中,控制驱动的可变形反射镜系统消除了介质随时间变化而产生的畸变。自适应小波具有在降低成本的同时实现相同目标的潜力。自适应光学器件可为大气湍流,抖动和光学器件产生的像差提供实时补偿。自适应光学子系统由波前传感器,实时重构器和服务器补偿器,可变形镜面,倾斜校正,光学组件和自适应光学控制组成。波前传感器感测相位差和波前倾斜。实时重建器和伺服补偿系统计算可变形镜执行器。倾斜校正系统校正由大气湍流,安装振动,摆动动力学滞后和系统振动引起的波前倾斜误差和到达抖动角。总之,自适应光学系统非常复杂,并且组装和维护都非常昂贵。自适应小波具有简化系统和降低成本的潜力。最终目标是更高的图像分辨率。当信号或环境随时间变化时,自适应系统很重要。通过自适应提升,可以以固定方式选择预测/更新滤波器或小波/缩放函数。可以选择它们,使得仅使用有限数量的系数就可以非常高精度地逼近信号。不同的预测滤波器可用于信号的不同部分。根据信号本身选择高阶或低阶预测滤波器。例如,空间自适应方法,预测滤波器取决于两个互补组之一的图像像素的局部信息。为了将自适应小波提升应用于由大气湍流调制的光学图像,可以做出某些假设:(1)图像是径向对称的,并且(2)大气湍流在某种程度上是周期性的。在那之后,预测滤波器的选择将考虑所研究的光学图像的特性。例如,相位从来都不是容易的问题。

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