Abstract

Control of phase contrast in electron microscope images is presently achieved by fine vernier control of the dc objective lens current. An incremental change δJ in lens current produces a corresponding increment δf in focal length and a focal separation in object space of δL o . L o is the distance from lens to conjugate object plane so that ΔL o is the axial separation of conjugate object plane and scattering specimen. The defocus phase at the image plane of a ray scattered at angle β relative to the axial ray is $\chi ={\vert K \vert \over 2} \triangle L_{\deg}\beta^{2} \qquad \eqno{hbox{(1)}}$ with |K| = 2π/λ. The phase contrast G in the image goes as $G \sim {\rm sin} \chi {\vert K \vert \over 2} \triangle L \deg \beta^{2} \qquad \eqno{\hbox{(2)}}$ ignoring spherical aberration, astigmatism, etc., for this purpose. Precise control of phase contrast for a spacing “a” = λβ−1 requires that the focal separation increments δL o be as small as 100 a and preferably less.1, 2

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