中国科学院云南天文台机构知识库

地基太阳望远镜磁像仪在进行偏振测量时会受到大气湍流的影响，导致测量结果不准确。通过同步探测波前像差，对太阳窄带偏振图像退卷积重建的方法可以克服窄带滤光器带来的偏振测量通道光子数水平较低等问题，将高分辨图像重建算法应用到太阳偏振图像的重建中。在重建过程中，波前估计不准确会导致重建的偏振图像受到I的串扰，与真实的偏振信号之间存在一定偏差。为了研究同步重建过程中波前复原精度对偏振图像重建精度的影响，通过建立仿真模型，对不同视宁度和不同波前复原精度下I对偏振信号的串扰进行了仿真。结果表明，偏振图像的重建质量与波前复原精度正相关，在一定的条件下，增加用于图像重建的帧数和降低图像分辨率等方法也可以降低I对偏振信号的串扰。 

The magnetic imager of ground-based solar telescope will be affected by atmospheric turbulence during polarimetry, resulting in inaccurate measurement results. By synchronously detecting the wavefront aberration, and to use deconvolution reconstruction of the sun' s narrow band polarization image, the poor photons problem caused by the narrow band filter can be overcome. The high-resolution image reconstruction algorithm is applied to the reconstruction of the sun' s polarized image. During the reconstruction process, inaccurate wavefront sensing result can lead to I crosstalk between the reconstructed polarization image and the real polarization signal, resulting in certain difference. To study the impact of wavefront sensing accuracy on polarization image reconstruction accuracy during the reduction, a simulation model is established in this paper to study the I crosstalk of polarimetry results under different seeing and wavefront sensing accuracy. The results indicate that the reconstruction quality of polarized images is positively correlated with the accuracy of wavefront sensing. Under certain conditions, increasing the number of frames used for image reconstruction and reducing image resolution can also reduce the I →QUV crosstalk.