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激光测量局部区域性大气湍流特性技术
其他题名Laser measurement of local regional atmospheric turbulence characteristics
邓鉴
学位类型硕士
导师刘煜
2022-07-01
学位授予单位中国科学院大学
学位授予地点北京
培养单位中国科学院云南天文台
学位专业天文技术与方法
关键词局部大气湍流 视宁度 差分成像 天文选址
摘要坐落于地面的地基望远镜,对比空间望远镜,最大一个区别就在于受到大气的影响。遥远的星光经过大气时,由于大气湍流的存在,导致成像质量的退化,主要表现为下面四个方面:星象抖动,像面畸变,像质模糊和像闪烁。所以,为地基望远镜选择合适的站址是任何规模地基望远镜前期极为重要的基础性工作。一旦在良好的天文站址建设好望远镜后,望远镜安放的位置、高度都不能再随之改变。此时,圆顶局部视宁度对一台望远镜有着严重的影响,亟需进行人工测量和改善。目前,圆顶局部视宁度为代表的局部视宁度测量仪器除了微温脉动仪为主的气象学方法外,还缺少别的测量手段。长久以来,研究者主要把目光集中于研究整层大气湍流对望远镜的影响,并对整层大气湍流有了很深入的理解,却一直缺少对局部湍流进行单独、精确的光学评估测量手段。由于激光特有的高强度、高单色性、高相干性和高方向性等诸多特性,使其具有容量大、波束窄、增益高、速度快、抗干扰性强和保密性好等一系列优点。令激光探测成为大气探测的新方向。基于Kolmogorov的大气湍流理论,研制了一套使用多路非冗余基线激光测量局部湍流的仪器。相比于传统的微温脉动仪,该仪器不仅可以测量局部湍流的大气相干长度与视宁度,还能测量风速、外尺度和相干时间湍流参数,而且,该仪器方便灵活,可根据实际使用情况改变搭建方式,稍加改造后就可用于测量镜面湍流、管道湍流等局部湍流。不仅拥有广阔的应用前景还对我国局部湍流测量工作有着很好的研究意义及参考价值。
其他摘要One of the major differences between ground-based telescopes and space-based telescopes is the influence of the atmosphere. When distant starlight passes through the atmosphere, the presence of atmospheric turbulence leads to degradation of the image quality in four main ways: star jitter, image plane distortion, image quality blurring and image flicker. Therefore, the selection of a suitable site for a ground-based telescope is an extremely important fundamental task for any size of ground-based telescope.Once the telescope is built at a good astronomical site, the location and height of the telescope can no longer be changed. At this point, the dome local seeing have a serious impact on a telescope and need to be measured and improved manually. At present, there is a lack of measurement instruments for the local seeing represented by the dome local seeing other than the meteorological method based on the Micro-thermal Meter.For years, researchers have focused on studying the effects of whole-atmosphere turbulence on telescopes and have gained a deep understanding of whole-atmosphere turbulence, but there is a lack of separate and accurate optical evaluation measurements of local turbulence. Due to the unique characteristics of the laser, such as high intensity, high monochromaticity, high coherence, and high directionality, it has a series of advantages such as large capacity, narrow beam, high gain, fast speed, strong anti-interference, and good confidentiality, Thus laser detection has become a new direction of atmospheric detection. We developed an instrument to measure local turbulence using multiple non-redundant baseline lasers based on the theory of atmospheric turbulence. Compared with the traditional Micro-thermal Meter, this instrument can measure not only the atmospheric coherence length and seeing of local turbulence, but also wind speed, outer scale, and coherence time turbulence parameters. Moreover, the instrument is convenient and flexible, and the construction method can be changed according to the actual configuration; after slight modification, the instrument can be used to measure local turbulence such as mirror turbulence and tube turbulence. It not only has a broad application prospect but also has good research significance and reference value for local turbulence measurement in China.
学科领域天文学 ; 天体物理学 ; 实测天体物理学
学科门类理学 ; 理学::天文学
页数0
语种中文
文献类型学位论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25767
专题选址与日冕观测组
推荐引用方式
GB/T 7714
邓鉴. 激光测量局部区域性大气湍流特性技术[D]. 北京. 中国科学院大学,2022.
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