对于大口径地基开放式太阳望远镜,热光阑温升将导致其像质劣化。尤其是,热光阑通光孔紧挨成像光束,其与环境的温度差对像质影响很大。这是中国巨型太阳望远镜(Chinese Giant Solar Telescope,CGST)计划面临的诸多问题之一。解决热光阑...对于大口径地基开放式太阳望远镜,热光阑温升将导致其像质劣化。尤其是,热光阑通光孔紧挨成像光束,其与环境的温度差对像质影响很大。这是中国巨型太阳望远镜(Chinese Giant Solar Telescope,CGST)计划面临的诸多问题之一。解决热光阑温控问题的具体方法是设计整体冷却效率高且在关键位置得到进一步强化的热光阑结构,以达到温控均匀的目的。本文提出倒锥导流式热光阑设计方案,该方案有利于降低通光孔位置温度,使温度极高点离开通光孔。对流换热系数和光阑温度场仿真结果证明此方案明显优于目前常用的方法。倒锥导流式热光阑的极限温升为3℃,优于GREGO的极限温升(7℃);实测温度场与仿真温度场进行对照,结果在误差范围内。结果证明导流式倒锥结构具有较好的温控效果。展开更多
The Chinese Giant Solar Telescope(CGST)low-dispersion spectrograph requires a large field-of-view(FOV)and high spatial resolution,which can be addressed by a carefully designed image slicer system.Our proposed design ...The Chinese Giant Solar Telescope(CGST)low-dispersion spectrograph requires a large field-of-view(FOV)and high spatial resolution,which can be addressed by a carefully designed image slicer system.Our proposed design divides the rectangular 50″×20″FOV at the telescope focal plane into four 50″×5″subfields.Each subfield undergoes optical reconstruction using its independent collimator-camera system(F/36-F/25.79),achieving vertical alignment and focal reduction of subfields to form a pseudo-slit.Using tilt mirrors for scanning allows simultaneous acquisition of spectral data with both a large FOV and a high angular resolution of 0.05″.This resolves manufacturing challenges for an image slicer,avoiding the requirement for hundreds of elements,multi-angle configurations,and compact dimensions,and also provides effective technical support for engineering work on the CGST.展开更多
文摘对于大口径地基开放式太阳望远镜,热光阑温升将导致其像质劣化。尤其是,热光阑通光孔紧挨成像光束,其与环境的温度差对像质影响很大。这是中国巨型太阳望远镜(Chinese Giant Solar Telescope,CGST)计划面临的诸多问题之一。解决热光阑温控问题的具体方法是设计整体冷却效率高且在关键位置得到进一步强化的热光阑结构,以达到温控均匀的目的。本文提出倒锥导流式热光阑设计方案,该方案有利于降低通光孔位置温度,使温度极高点离开通光孔。对流换热系数和光阑温度场仿真结果证明此方案明显优于目前常用的方法。倒锥导流式热光阑的极限温升为3℃,优于GREGO的极限温升(7℃);实测温度场与仿真温度场进行对照,结果在误差范围内。结果证明导流式倒锥结构具有较好的温控效果。
基金supported by National Key Research and Development Programme‘Frontier Research on Large Scientific Devices’Key Special Project(2024YFA1612000)Sino-German Science Foundation Program(M-0086)Yunnan Science and Technology Leading Talent Program(202105AB160001).
文摘The Chinese Giant Solar Telescope(CGST)low-dispersion spectrograph requires a large field-of-view(FOV)and high spatial resolution,which can be addressed by a carefully designed image slicer system.Our proposed design divides the rectangular 50″×20″FOV at the telescope focal plane into four 50″×5″subfields.Each subfield undergoes optical reconstruction using its independent collimator-camera system(F/36-F/25.79),achieving vertical alignment and focal reduction of subfields to form a pseudo-slit.Using tilt mirrors for scanning allows simultaneous acquisition of spectral data with both a large FOV and a high angular resolution of 0.05″.This resolves manufacturing challenges for an image slicer,avoiding the requirement for hundreds of elements,multi-angle configurations,and compact dimensions,and also provides effective technical support for engineering work on the CGST.
