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CYRA - the cryogenic infrared spectrograph for the Goode Solar Telescope in Big Bear

机译:Cyra - 大熊队的Goode太阳能望远镜的低温红外光谱仪

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CYRA (CrYogenic solar spectrogRAph) is a facility instrument of the 1.6-meter Goode Solar Telescope (GST) at the Big Bear Solar Observatory (BBSO). CYRA focuses on the study of the near-infrared solar spectrum between 1 and 5 microns, an under-explored region which is not only fertile ground for photospheric magnetic diagnostics but also allows a unique window into the chromosphere lying atop the photosphere. CYRA is the first-ever fully cryogenic spectrograph in any solar observatory with its two predecessors, on the McMath-Pierce and Mees Telescopes, being based on warm optics except for the detectors and order sorting filters. CYRA is used to probe magnetic fields in various solar features and the quiet photosphere. CYRA measurements will allow new and better 3D extrapolations of the solar magnetic field and will provide more accurate boundary conditions for solar activity models. The superior spectral resolution of 150,000 and better allows enhanced observations of the chromosphere in the carbon monoxide (CO) spectral bands and will yield a better understanding of energy transport in the solar atmosphere. CYRA is divided into two optical sub-systems: The Fore-Optics Module and the Spectrograph. The Spectrograph is the heart of the instrument and contains the IR detector, grating, slits, filters, and imaging optics all in a cryogenically cooled Dewar (cryostat). The sensor is a 2048 by 2048 pixel HAWAII 2 array produced by Teledyne Scientific & Imaging, LLC. The cryostat interior and the readout electronics are maintained at 90 Kelvin by helium refrigerant-based cryo-coolers, while the IR array is cooled to 30 Kelvin. The Fore-Optics Module de-rotates and stabilizes the solar image, provides scanning capabilities and transfers the GST image to the Spectrograph. CYRA has been installed and is undergoing its commissioning phase. This paper reports on the design, implementation, and operation of CYRA in detail. The preliminary scientific results have been highlighted as well.
机译:Cyra(低温太阳能光谱仪)是大熊太阳能天文台(BBSO)的1.6米古德太阳能望远镜(GST)的设施仪器。 Cyra专注于近红外太阳光谱的研究1到5微米,这是一个探索的区域,这不仅是拍摄的射击磁性诊断的肥沃,而且还允许独特的窗户进入Photosphere上方的铬圈。 Cyra是任何太阳天文台的第一个完全低温的光谱仪,其两位前辈们在麦克马特 - 皮尔斯和Mees望远镜上,基于暖光学,除了探测器和订单分拣过滤器。 Cyra用于探测各种太阳能特征和静物电像篓的磁场。 CyRA测量将允许太阳能磁场的新和更好的3D外推,为太阳能活动模型提供更准确的边界条件。卓越的光谱分辨率为150,000,更好地允许在一氧化碳(CO)光谱带中的铬圈的增强观察,并将产生更好地理解太阳能大气中的能量运输。 CyRA分为两个光学子系统:前光模块和光谱仪。光谱仪是仪器的心脏,并包含IR探测器,光栅,狭缝,过滤器和所有在低温冷却的杜瓦(低温恒温器)中的成像光学器件。传感器是由Teledyne Scientific&Imaging,LLC生产的2048像素夏威夷2阵列。低温恒温器内部和读出电子器件由氦制冷剂的冷冻机维持在90个开尔文中,而红外阵列被冷却至30个开尔文。前光模块去旋转并稳定太阳能图像,提供扫描能力并将GST图像传送到光谱仪。 Cyra已安装并正在进行调试阶段。本文详细介绍了Cyra的设计,实施和操作。突出的科学结果也突出了。

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