测量尖端倾斜校正太阳偏振测量法中的视线诱发串扰。

Applied optics Pub Date : 2024-05-20 DOI:10.1364/AO.519245
Harsh Mathur, K Nagaraju, Hemanth Pruthvi, K Sagaynathan
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引用次数: 0

摘要

我们利用 Kodaikanal 塔隧道(KTT)望远镜同时记录的 H α 和 Ca ii 8662 Å 线对太阳黑子进行的分光测地观测,对视诱发的串扰进行了测量。Kodaikanal 塔隧道望远镜集成并安装了一个图像稳定系统,该系统由一个尖端倾斜装置和一个自动导向器系统组成。此外,KTT 的分光测偏仪也进行了升级,可同时记录三条光谱线的分光测偏观测数据。事实证明,尖端倾斜系统的截止频率为 80 赫兹,可有效减少测量斯托克斯参数中由视线引起的串扰,减少幅度至少为 2 倍。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Measurements of seeing-induced crosstalk in tip-tilt corrected solar polarimetry.

We present measurements of seeing-induced crosstalk using spectropolarimetric observations of sunspots recorded simultaneously in the H α and Ca ii 8662 Å lines with the Kodaikanal Tower Tunnel (KTT) telescope. The Kodaikanal Tower Tunnel telescope is integrated and installed with an image stabilization system consisting of a tip-tilt and an autoguider system. Additionally, the spectropolarimeter at KTT is upgraded to allow for the simultaneous recording of spectropolarimetric observations in three spectral lines. The tip-tilt system is shown to have a cutoff frequency of 80 Hz, effectively reducing the seeing induced crosstalk in the measured Stokes parameters by at least a factor of 2.

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