In the field of materials sciences such as studies on ceramics, semi-conducting material and metals, role of light elements is important, because it is one of mainly composing elements or determiner of character i. e. dopants. The light elements at high resolution have been observed by ultrahigh voltage electron microscopy or aberration corrected electron microscopy in Transmission Electron Microscopy (TEM), since the visualization of light requires highly resolving power. Recently, a high angle annular dark field (HAADF) scanning transmission electron microscopy (STEM) has become widely used in this field because of high-resolution capability and easily interpretable image contrast, which is roughly proportional to square of atomic number Z (Z 2 ). However, the HAADF image sometimes gives lack of light element because of excess contrast originated from Z 2 , when the specimen contains the light and heavy elements. The TEM bright field imaging gives an image contrast roughly proportional to the Z, when the specimen is thin enough to be able to apply the 'thin film approximation'. We have examined to apply an STEM annular bright field (ABF) imaging, which is equivalent to TEM hollow cone illumination imaging technique [1-2], to the oxide or nitride samples for simultaneous visualization of light and heavier elements. According to the article on hollow cone illumination in TEM [2], the contrast transfer in ABF expected to give better resolution than conventional BF STEM and to give non-oscillating contrast transfer, which gives easily-interpretable images unlike the BF STEM. This paper reports characteristics and the experimental result of the ABF imaging technique.Experiments were performed with a new 200 kV microscope (JEM-ARM200F) equipped with an annular bright field and dark field detectors as well as a spherical aberration correction system for STEM [3]. Figure 1 shows a scheme for our experiment. This experimental configuration enables us to perform a simultaneous acquisition of annular dark and bright field images. The convergent angle of incident beam is limited with the aperture in condenser lens system. The inner and outer acceptance angle for HAADF image is limited with the camera length and size of the HAADF detector. Those for ABF image is limited with the camera length, size of the ABF detector and the size of preventing disc placed above the bright field detector. Figures 2 (a), (b) and (c) show the HAADF, conventional BF and ABF images of SrTiO 3 (001). And the model of SrTiO 3 (001) is illustrated in Fig. 2 (d). The experimental parameters for the observation are listed as follows. Detecting angle for HAADF, BF and ABF were 68 -200 mrad, 0-22 mrad, 11-22 mrad, respectively. The probe current and size were 24 pA and 0.1 nm. If we focus on the site of oxygen, the oxygen is invisible in the HAADF image ( Fig. 2(a)) and slightly visible in the BF image ( Fig. 2(b)). While in the ABF image (Fig. 2(c)), the oxygen is clearly visible. Additional experiments of focal dependency were performed with the th...

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