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Development of model of atmospheric turbulence at Baikal Astrophysical Observatory site of the Large Solar Vacuum Telescope

机译:大型太阳能真空望远镜百吉岩天体医学观察仪的大气湍流模型的发展

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The Baikal Astrophysical Observatory of Institute Solar- Terrestrial Physics of Siberian Branch of Russian AcademySciences is located at an altitude of about 700 meter above sea level on the shore of Lake Baikal, Russian Federation.Large Solar Vacuum Telescope (LSVT) is the main telescope of the Baikal Astrophysical Observatory. We developmodels of vertical profile of atmospheric turbulence (the refractive-index structure constant) and wind speed at the BAOfor adaptive optical system design of LSVT. We also presented vertical profile wind speed and the refractive-indexstructure constant is obtained from NCEP /NCAR Reanalysis base.
机译:俄罗斯学院西伯利亚分公司研究所太阳能物理学的贝氏诗科学位于俄罗斯联邦湖泊湖岸边海拔大约700米的高度。大型太阳能真空望远镜(LSVT)是贝加尔人天体物理天文台的主望远镜。我们开发大气湍流垂直轮廓的模型(折射率结构常数)和鲍瓦的风速用于LSVT的自适应光学系统设计。我们还呈现了垂直轮廓风速和折射率结构常数从NCEP / NCAR再分析基础获得。

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