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Chromatic spatial superresolution with infrared adaptive optics

机译:红外自适应光学装置实现彩色空间超分辨率

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Abstract: The diffraction-limited spatial cut-off frequency D/$lambda of a telescope aperture is not an absolute limit to imaging resolution, and various methods exist to obtain spatial information at frequencies much higher than D/$lambda under specialized circumstances. In particular, spectrally dissimilar objects can be discerned at separations far smaller than the Airy radius, by exploiting both the spatial and spectral information available. This general method is applied in differential speckle interferometry and chromatic position difference imaging. We describe proposed experiments, using the University of Durham's ELECTRA adaptive optics instrument, to perform a variant of chromatic position different imaging at IR wavelengths, but incorporating the very large resolution gain provided by AO image correction. This method, related in principle to differential speckle interferometry, involves measuring the shift of image centroid with wavelength across a spectrally dispersed image. The implementation of this experiment on ELECTRA requires only a simple modification to the standard ELECTRA optical configuration. The optical arrangement is described, and examples of astronomical applications are presented. !17
机译:摘要:望远镜孔径的衍射极限空间截止频率D / $ lambda并非对成像分辨率的绝对限制,在特殊情况下,存在各种方法来获取比D / $ lambda更高的频率的空间信息。尤其是,通过利用可用的空间和光谱信息,可以以远小于艾里半径的间距来识别光谱不相似的物体。该通用方法应用于差分散斑干涉测量和色差成像中。我们使用达勒姆大学的ELECTRA自适应光学仪器描述了拟议的实验,以执行红外波长处不同色度位置成像的变体,但结合了AO图像校正提供的非常大的分辨率增益。该方法原则上与差分散斑干涉法有关,涉及在整个光谱分散的图像上测量图像质心随波长的偏移。在ELECTRA上实施此实验仅需要对标准ELECTRA光学配置进行简单修改。描述了光学装置,并介绍了天文应用的示例。 !17

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