Study of the Optical Atmospheric Distortions using Wavefront Sensor Data

Study of the Optical Atmospheric Distortions using Wavefront Sensor Data
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DOI:
10.1007/s11182-021-02256-y
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发表时间:
2021-03-17
影响因子:
0.6
通讯作者:
Russkikh, I. V.
Russkikh, I. V.
中科院分区:
物理与天体物理4区
文献类型:
--
作者:
Kovadlo, P. G.;Shikhovtsev, A. Yu.;Russkikh, I. V.

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本文研究了贝加尔天文台大型太阳真空望远镜的光学湍流结构。给出了波前畸变研究的一些结果,以扩充数据库。讨论了利用增强的光学湍流强度探测大气层的可能性。计算了边界层内大气湍流层的高度。
The paper studies the optical turbulence structure at the Large Solar Vacuum Telescope of the Baikal Astrophysical Observatory. Some results on the study of the wavefront distortions are given to expand the data archive. The possibilities of detecting layers with enhanced optical turbulence intensity in the atmosphere are discussed. The altitudes of the atmospheric turbulent layers within the boundary layer are estimated.