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Aberration-Corrected STEMs Open New Vistas

机译:像差校正的STEM开启了新的视野

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Since the electron microscope's inception in the 1930s, resolution limits imposed by electron lens aberrations have complicated its evolution. Compared with their visible-light counterparts, electron lenses are some 50x inferior. So while the ordinary microscope attained its resolution limit — close to the wavelength of visible light — about a century ago, this never quite happened for electron microscopy. Unsurprisingly, aberration correction became electron microscopy's Holy Grail because, although the wavelength used is several orders of magnitude smaller than that of light, it had not been possible to approach the wavelength of the electrons used (~0.03 A), which is considerably smaller than the average atom's diameter of 0.1-0.5 nm. Because e-beam resolution is limited to about 50 wavelengths, true atomic resolution was only achieved in the past couple of decades.
机译:自1930年代电子显微镜问世以来,电子透镜像差所施加的分辨率极限使它的发展变得复杂。与可见光相比,电子透镜的性能要差50倍。因此,尽管普通显微镜在一个世纪前达到了其分辨率极限(接近可见光的波长),但电子显微镜却从未发生过。毫不奇怪,像差校正成为电子显微镜的圣杯,因为尽管所使用的波长比光的波长小几个数量级,但不可能接近所用电子的波长(〜0.03 A),而该波长明显小于平均原子直径为0.1-0.5 nm。由于电子束分辨率仅限于约50个波长,因此仅在过去的几十年中才实现了真正的原子分辨率。

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