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Trouble-Free Method of Coordinate Mapping and Spatial Calibration for All Sky Night Airglow Images

机译:所有夜空影像的坐标映射和空间校准的无故障方法

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The Number of observable facts and structures that are accessible with an airglow images which are captured by an All Sky Imager (ASI). All of these images are required to convert from the spherical coordinating system into the rectangular coordinating image system. The spatial calibration is also most important for the perfect measurement of gravity wave characteristics, plasma characteristics and OH emission parameters in the upper atmosphere, mesosphere, ionosphere study when that calibrations are used in real life dimensions. In this paper, we expressed an effective and simple technique for the coordinate mapping and the spatial calibration for accurate dimensions used in real world life and also implemented the same procedure by using Matlab R2013a. The pixel resolutions of OH image of 840 nm, a mesospheric image of 557.7 nm and ionospheric image of 630 nm are measured. These pixel resolutions are nearly same and measuring technique is very simple than other method used in the same area.
机译:可通过全天空成像仪(ASI)捕获的气辉图像访问的可观察事实和结构的数量。所有这些图像都需要从球坐标系转换为矩形坐标系。当在现实生活中使用校准时,空间校准对于在高层大气,中层层,电离层研究中完美测量引力波特性,等离子体特性和OH排放参数也是最重要的。在本文中,我们为现实生活中使用的精确尺寸表示了一种有效而简单的坐标映射和空间校准技术,并使用Matlab R2013a实施了相同的过程。测量了840 nm的OH图像,557.7 nm的中层图像和630 nm的电离层图像的像素分辨率。这些像素分辨率几乎相同,并且测量技术比同一区域中使用的其他方法非常简单。

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