日冕振荡观测周期的欠采样效应

Daye Lim, Tom Van Doorsselaere, Valery M. Nakariakov, Dmitrii Y. Kolotkov, Yuhang Gao, David Berghmans
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引用次数: 0

摘要

背景。最近对无衰减横向振荡的观测表明,周期与环长之间的关系有两个分支。一个是线性关系,被解释为驻留模式。另一种则几乎没有相关性,尚未得到最终解释。目的我们研究了取样不足对观测到的无衰减振荡周期的影响。方法。我们考虑了紧跟观测到的环长分布的振荡日冕环。假设所有振荡都是驻波,我们建立了一个代表无衰减振荡的信号模型,其中周期与环长成正比,振幅和相位是随机绘制的。通过不同的采样率,模拟望远镜的时间节奏,从原始信号中生成下采样信号,并使用快速傅里叶变换分析采样信号的周期。分析结果当采样频率越来越接近实际振荡周期时,高估短环路周期的趋势就会增强。环路长度与采样信号周期之间的关系显示出与观测结果相同的两个分支。结论我们发现,短环路中出现的长周期无衰减振荡可能是采样不足的结果。
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Undersampling effects on observed periods of coronal oscillations
Context. Recent observations of decayless transverse oscillations have shown two branches in the relationship between periods and loop lengths. One is a linear relationship, interpreted as a standing mode. The other shows almost no correlation and has not yet been interpreted conclusively. Aims. We investigated the undersampling effect on observed periods of decayless oscillations. Methods. We considered oscillating coronal loops that closely follow the observed loop length distribution. Assuming that all oscillations are standing waves, we modeled a signal that represents decayless oscillations where the period is proportional to the loop length and the amplitude and phase are randomly drawn. A downsampled signal was generated from the original signal by considering different sample rates that mimic temporal cadences of telescopes, and periods for sampled signals were analysed using the fast Fourier transform. Results. When the sampling cadence is getting closer to the actual oscillation period, a tendency for overestimating periods in short loops is enhanced. The relationship between loop lengths and periods of the sampled signals shows the two branches as in the observation. Conclusions. We find that long periods of decayless oscillations occurring in short loops could be the result of undersampling.
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