Wang S Y, Cowley J M
Department of Physics and Astronomy, Arizona State University, Tempe 85287.
Microsc Res Tech. 1995 Feb 1;30(2):181-92. doi: 10.1002/jemt.1070300208.
In a dedicated STEM instrument equipped with a field emission gun, shadow images are easily obtained and have many uses. They are very sensitive to misalignment of the instrument and astigmatism, and therefore can be used for rapid and accurate alignment of the microscope. For crystalline materials, the shadow image contains both the bright-field and dark-field images. It is a summation of the transmitted and diffracted beams, and is basically a kind of Gabor's in-line hologram. Under small or medium defocus, shadow images of a thin, well-orientated crystalline specimen take the characteristic form of Ronchigrams, which offer a unique means to calibrate the microscope operation parameters, such as the spherical aberration coefficient Cs and defocus settings of the objective lens, with high accuracy. With the calibrated values of Cs and delta, a transfer function of the objective lens may be generated. In the stage of numerical reconstruction, by adapting this transfer function to the experimentally recorded hologram the lens aberration introduced in forming the hologram may be corrected and an improved resolution may be achieved for electron microscope images.
在配备场发射枪的专用扫描透射电子显微镜(STEM)仪器中,很容易获得阴影图像且其用途广泛。它们对仪器的未对准和像散非常敏感,因此可用于显微镜的快速精确对准。对于晶体材料,阴影图像包含明场和暗场图像。它是透射光束和衍射光束的总和,基本上是一种伽柏同轴全息图。在中小离焦条件下,薄的、取向良好的晶体试样的阴影图像呈现出龙奇图的特征形式,这提供了一种独特的方法来高精度校准显微镜操作参数,如球差系数Cs和物镜的离焦设置。利用Cs和δ的校准值,可以生成物镜的传递函数。在数值重建阶段,通过将此传递函数应用于实验记录的全息图,可以校正形成全息图时引入的透镜像差,并提高电子显微镜图像的分辨率。