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首页> 外文期刊>Astronomy and astrophysics >Influence of phase-diversity image reconstruction techniques on circular polarization asymmetries
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Influence of phase-diversity image reconstruction techniques on circular polarization asymmetries

机译:相位分集图像重建技术对圆偏振不对称性的影响

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Context. Full Stokes filter-polarimeters are key instruments for investigating the rapid evolution of magnetic structures on the solar surface. To this end, the image quality is routinely improved using a-posteriori image reconstruction methods. Aims. We analyze the robustness of circular polarization asymmetries to phase-diversity image reconstruction techniques. Methods. We used snapshots of magneto-hydrodynamical simulations carried out with different initial conditions to synthesize spectra of the magnetically sensitive Fe i line at 5250.2 ?. We degraded the synthetic profiles spatially and spectrally to simulate observations with the IMaX full Stokes filter-polarimeter. We also simulated the focused/defocused pairs of images used by the phase-diversity algorithm for reconstruction and the polarimetric modulation scheme. We assume that standard optimization methods are able to infer the projection of the wavefront on the Zernike polynomials with 10% precision. We also consider the less favorable case of 25% precision. We obtain reconstructed monochromatic modulated images that are later demodulated and compared with the original maps. Results. Although asymmetries are often difficult to define in the quiet Sun due to the complexity of the Stokes V profiles, we show how asymmetries are degraded with spatial and spectral smearing. The results indicate that, although image reconstruction techniques reduce the spatial smearing, they can modify the asymmetries of the profiles, which are mainly caused by the appearance of spatially-correlated noise.
机译:上下文。 Full Stokes滤光片偏振仪是研究太阳表面磁性结构快速演变的关键工具。为此,通常使用后验图像重建方法来改善图像质量。目的我们分析了圆偏振不对称对相集图像重建技术的鲁棒性。方法。我们使用在不同初始条件下进行的磁流体动力学模拟快照来合成在5250.2?处的磁敏Fei谱线。我们在空间和光谱上对合成轮廓进行了降级,以模拟使用IMaX Full Stokes滤波器-旋光仪的观测结果。我们还模拟了相位分集算法用于重建和极化调制方案的聚焦/散焦图像对。我们假设标准优化方法能够以10%的精度推断波前在Zernike多项式上的投影。我们还考虑了25%精度的不利情况。我们获得重建的单色调制图像,随后将其解调并与原始地图进行比较。结果。尽管由于Stokes V轮廓的复杂性,通常很难在安静的太阳下定义不对称性,但我们展示了如何通过空间和频谱拖尾来降低不对称性。结果表明,尽管图像重建技术减少了空间拖尾现象,但它们可以修改轮廓的不对称性,这主要是由与空间相关的噪声的出现引起的。

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