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Comparing the Hinode and SOHO /MDI Data to the Simulated Large Scale Solar Convection

机译:将Hinode和SOHO / MDI数据与模拟大规模太阳对流进行比较

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Large-scale simulations of solar turbulent convection produce re-alistic data and provide a unique opportunity to study solar oscillations and test various techniques commonly used for the analysis of solar observations. We applied helioseismic methods to the sets of simulated as well as observed data and find remarkable similarities. Power spectra, k – v diagrams, time-distance diagrams exhibit similar details, although sometimes subtle differences are present.
机译:太阳能湍流对流的大规模模拟产生了重新实现的数据,并提供了学习太阳振荡的独特机会,并测试通常用于分析太阳观测的各种技术。我们将Helioseismic方法应用于模拟和观察到的数据集,并找到了显着的相似之处。功率谱,K-V图,时间距离图表具有相似的细节,但有时存在细微差异。

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