自动识别和数字化极光档案光学观测数据的软件

Andrei Vorobev, Alexander Lapin, Gulnara Vorobeva
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摘要

记录极光的主要工具之一是使用全天候相机在自动模式下对天空进行光学观测。观察结果记录在特殊的助记表中。阿斯卡图提供天空中不同部分的云层和极光有无的每日资料,传统上用于研究某一空间区域内极光的每日分布,以及根据地磁活动水平计算在其他区域观测到极光的概率。同时,ascaplot的处理目前是手工进行的,这与大量的时间成本和由于人为因素而导致的高比例错误相关。为了提高天文图像处理的效率,我们提出了一种自动识别和数字化极光光学观测数据的方法。提出了一种ascaplot结构的形式化方法,用于对ascaplot图像进行处理,提取相应的观测结果,形成结果数据集。该方法涉及使用机器视觉算法和使用专用掩码-用于数字化的调试图像,这是一个彩色图像,其中指定了ascaplot细胞的一般位置。提出的方法和相应的算法以软件的形式实现,该软件提供了对极光光学观测档案数据的识别和数字化。该解决方案是一个单用户桌面软件,允许用户以批处理模式将ascaplot图像转换为表,以供进一步处理和分析。计算实验结果表明,使用该软件,一方面可以避免天际线数字化过程中的错误,另一方面可以显著提高相应的计算运算速度。总的来说,这将提高处理ascaplot和进行相关领域研究的效率。
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Программное обеспечение для автоматизированного распознавания и оцифровки архивных данных оптических наблюдений полярных сияний
One of the main tools for recording auroras is the optical observation of the sky in automatic mode using all-sky cameras. The results of observations are recorded in special mnemonic tables, ascaplots. Ascaplots provide daily information on the presence or absence of cloud cover and auroras in various parts of the sky and are traditionally used to study the daily distribution of auroras in a given spatial region, as well as to calculate the probability of their observation in other regions in accordance with the level of geomagnetic activity. At the same time, the processing of ascaplots is currently carried out manually, which is associated with significant time costs and a high proportion of errors due to the human factor. To increase the efficiency of ascaplot processing, we propose an approach that automates the recognition and digitization of data from optical observations of auroras. A formalization of the ascaplot structure is proposed, which is used to process the ascaplot image, extract the corresponding observation results, and form the resulting data set. The approach involves the use of machine vision algorithms and the use of a specialized mask - a debug image for digitization, which is a color image in which the general position of the ascaplot cells is specified. The proposed approach and the corresponding algorithms are implemented in the form of software that provides recognition and digitization of archival data from optical observations of auroras. The solution is a single-user desktop software that allows the user to convert ascaplot images into tables in batch mode, available for further processing and analysis. The results of the computational experiments have shown that the use of the proposed software will make it possible to avoid errors in the digitization of ascaplots, on the one hand, and significantly increase the speed of the corresponding computational operations, on the other. Taken together, this will improve the efficiency of processing ascaplots and conducting research in the relevant area.
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