Development of LabVIEW based data acquisition unit for Compact photometer for terrestrial and planetary emissions

B. Madhava Reddy, V. Elamaran, C. Vineeth, T. Pant
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Abstract

The study of atmospheric emissions like Airglow, Aurora etc, are essential to understand the theory and behavior of atmosphere. The Compact Airglow photometer (CAP) is one of the Fabry-Perot (FP) etalon based optical instruments which is capable of detecting the faint airglow emissions from sky in the presence of bright background light (which may be Sun or moon light). This is achieved by capturing the circular fringes of the required emissions, formed by the Fabry-Perot (FP) etalon as images along with the background using a Charge Coupled Device (CCD). The paper purports to the development of data acquisition unit for Compact photometer for terrestrial and planetary emissions using LabVIEW Software. The data acquisition unit interfaces CCD with any personal computer. The system is capable of subtracting the dark noise from each CCD frame (obtained at every 100 ms minimum) and integrating them for the desired time. It is also capable of selecting and counting the photons falling on two rectangular portions at any region in the CCD image plane separately. For each wavelength, two regions, one with fringe (Signal + Background) and other without fringe (Background alone) have been identified. Subtraction of the latter from the former will give the intensities of the airglow emissions at desired wavelengths (signal).
基于LabVIEW的小型地球和行星发射光度计数据采集单元的开发
对气辉、极光等大气排放物的研究,对于理解大气的理论和行为是至关重要的。紧凑型气辉光度计(CAP)是一种基于法布里-佩罗(FP)标准子的光学仪器,能够在明亮的背景光(可能是太阳或月亮的光)存在的情况下检测来自天空的微弱气辉发射。这是通过使用电荷耦合器件(CCD)捕获所需发射的圆形条纹来实现的,该条纹由Fabry-Perot (FP)标准子形成,作为图像与背景一起使用。本文旨在利用LabVIEW软件开发用于地球和行星发射的紧凑型光度计的数据采集单元。数据采集单元将CCD与任何个人计算机连接起来。该系统能够从每个CCD帧(至少每100毫秒获得一次)中减去暗噪声,并在所需时间内对它们进行积分。它还能够分别选择和计数落在CCD图像平面上任意区域的两个矩形部分上的光子。对于每个波长,确定了两个区域,一个有条纹(信号+背景),另一个没有条纹(背景单独)。前者减去后者将得到气辉在所需波长(信号)下的发射强度。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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