照片球与太阳色球在皮克杜米德天文台的光谱学研究（1956-2026）
70 years of spectroscopy of the photosphere and the solar chromosphere at the Pic du Midi Observatory (1956-2026)
AI总结：
皮克杜米德天文台自1956年以来持续进行太阳光球和色球的光谱学研究，通过建立实验室和升级设备，推动了太阳观测技术的发展。
摘要：
在皮克杜米德天文台开始对日冕进行观测的是伯纳德·利奥特和他的光谱日冕仪，该仪器安装在巴利亚德圆顶的多用途赤道 mounts 上。直到1956年，专门用于观测光球和色球的圆顶和仪器才出现。在国际地学年期间，一座太阳光谱学实验室在皮克杜米德天文台西侧建立，基于两台4米和9米焦距的光谱仪。1961年，一个塔式圆顶出现在皮克的东侧，后来配备了一台8米的光谱仪。大约1965年，巴利亚德圆顶最终专门用于日冕，配备了新的台面和新的光谱仪。同时，皮克的基础设施在几年内发生了革命性变化，我们也将展示太阳光谱仪及其目标。
英文摘要：
Observations of the solar corona at the Pic du Midi began with Bernard Lyot and his spectro coronagraph installed on the multi-purpose equatorial mount of the Baillaud cupola. It was not until 1956 that domes and instruments specifically dedicated to observations of the photosphere and the solar chromosphere appeared. On the occasion of the International Geophysical Year, a solar spectroscopy laboratory was created to the west of the Pic du Midi, based on two spectrographs of 4 m and 9 m focal length. In 1961 the turret dome appeared to the east of the Pic, later equipped with an 8 m spectrograph. Around 1965, the Baillaud dome finally specialized in the corona with a new table and new spectrographs. At the same time, a revolution in infrastructure took place at the Pic in a few years, which we present as well as the solar spectrographs and their goal.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
