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首页> 外文期刊>Icarus: International Journal of Solar System Studies >Generating realistic synthetic meteoroid orbits
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Generating realistic synthetic meteoroid orbits

机译:产生现实的合成菱形轨道

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Highlights ? A method for generating synthetic sporadic meteoroid orbits is proposed. ? The method uses Kernel Density Estimation to model the sporadic background. ? The model is built using an existing meteoroid dataset of sporadic orbits. ? The model preserves the biases of the system the data was taken with. Abstract Context. Generating a synthetic dataset of meteoroid orbits is a crucial step in analysing the probabilities of random grouping of meteoroid orbits in automated meteor shower surveys. Recent works have shown the importance of choosing a low similarity threshold value of meteoroid orbits, some pointing out that the recent meteor shower surveys produced false positives due to similarity thresholds which were too high. On the other hand, the methods of synthetic meteoroid orbit generation introduce additional biases into the data, thus making the final decision on an appropriate threshold value uncertain. Aims. As a part of the ongoing effort to determine the nature of meteor showers and improve automated methods, it was decided to tackle the problem of synthetic meteoroid orbit generation, the main goal being to reproduce the underlying structure and the statistics of the observed data in the synthetic orbits. Methods. A new method of generating synthetic meteoroid orbits using the Kernel Density Estimation method is presented. Several types of approaches are recommended, depending on whether one strives to preserve the data structure, the data statistics or to have a compromise between the two. Results. The improvements over the existing methods of synthetic orbit generation are demonstrated. The comparison between the previous and newly developed methods are given, as well as the visualization tools one can use to estimate the influence of different input parameters on the final data. ]]>
机译:<![cdata [ 亮点 提出了一种生成综合散态环形轨道的方法。 方法使用内核密度估计来模拟零星背景。 该模型是使用零星轨道的现有的属性数据集构建。 模型保留系统的偏差数据。 < / ce:abstract-sec> 抽象 上下文。生成环形轨道的合成数据集是一个分析自动流星淋浴调查中的随机分组随机分组概率的关键步骤。最近的作品表明了选择菱形轨道的低相似性阈值的重要性,有人指出,最近的流星阵雨调查产生了由于过高的相似阈值而产生的误报。另一方面,综合性环形轨道生成方法将额外的偏差引入数据,从而使得最终决定在适当的阈值不确定。 目标。作为确定流星淋浴性质的性质的持续努力,提高自动化方法的一部分,决定解决合成的青色轨道轨道轨道的问题,主要目标是重现底层结构和综合轨道中观察到的数据的统计数据。 方法。介绍了使用内核密度估计方法产生合成菱形轨道的新方法。建议使用几种类型的方法,具体取决于一个努力保留数据结构,数据统计数据或两者之间存在妥协。 结果。对现有的合成轨道生成方法的改进进行了说明。给出了先前和新开发的方法之间的比较,以及可视化工具可以用于估计不同输入参数对最终数据的影响。 ]]>

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