Wavefront corrective lens for the Subaru Laser Launching Telescope

被引:0
|
作者
Novi, A. [1 ]
Canestrari, R. [2 ,3 ]
Ghigo, M. [2 ]
Hayano, Y. [4 ]
机构
[1] Galileo Av, Via A Einstein 35, I-50013 Florence, Italy
[2] INAF, Osservatorio Astronom Brera, Merate, Italy
[3] Univ Studi Insubria, Comazzo, Italy
[4] NAOJ, SUBARU Telescope, Hilo, HI 96720 USA
关键词
Laser Launching Telescope; lightweighted mirror; aberration compensating optics; Ion Beam Figuring; WFE correction; removal function; spatial frequencies;
D O I
10.1117/12.787897
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
The optical quality of file LLT unit of SUBARU NAOJ telescope was improved by new athermalized supports of the optics, in order to operate at the best performance at temperatures below 0 degrees C. The ultimate wavefront correction of the whole LLT, that expands a laser beam from 40 mm to 500 mm, was made by Ion Beam Figuring oil the small 40 mm LLT entrance window. in accordance to the WFE measured in operating conditions. The correction of small Optics Including high spatial frequencies, resulting by the LLT expanding ratio, was possible by a special technique of IBF process developed at the Astronomical Observatory of Brera (INAF-OAB), using a concentrator of the ion beam size, able to force the broader beam emitted from an ion Source into a smaller spot having large removal rate.
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页数:7
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