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COMPARING SIMULATED EMISSION FROM MOLECULAR CLOUDS USING EXPERIMENTAL DESIGN

机译:使用实验设计比较分子团的模拟发射

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We propose a new approach to comparing simulated observations that enables us to determine the significance of the underlying physical effects. We utilize the methodology of experimental design, a subfield of statistical analysis, to establish a framework for comparing simulated position-position-velocity data cubes to each other. We propose three similarity metrics based on methods described in the literature: principal component analysis, the spectral correlation function, and the Cramer multi-variate two-sample similarity statistic. Using these metrics, we intercompare a suite of mock observational data of molecular clouds generated from magnetohydrodynamic simulations with varying physical conditions. Using this framework, we show that all three metrics are sensitive to changing Mach number and temperature in the simulation sets, but cannot detect changes in magnetic field strength and initial velocity spectrum. We highlight the shortcomings of one-factor-at-a-time designs commonly used in astrophysics and propose fractional factorial designs as a means to rigorously examine the effects of changing physical properties while minimizing the investment of computational resources.
机译:我们提出了一种比较模拟观察结果的新方法,使我们能够确定潜在物理效应的重要性。我们利用实验设计的方法(统计分析的一个子领域)来建立一个框架,用于相互比较模拟的位置-位置-速度数据立方体。我们基于文献中描述的方法提出了三种相似性度量:主成分分析,光谱相关函数和Cramer多元两样本相似性统计量。使用这些度量,我们可以相互比较从具有不同物理条件的磁流体动力学模拟生成的分子云的一组模拟观测数据。使用此框架,我们显示了所有三个指标对模拟集中的马赫数和温度变化均敏感,但是无法检测到磁场强度和初始速度谱的变化。我们强调了天体物理学中通常一次使用一次因子设计的缺点,并提出了分数阶乘设计作为一种在最小化计算资源投资的情况下严格检查物理性质变化的影响的方法。

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