Phase-induced amplitude apodization complex mask coronagraph tolerancing and analysis

被引:4
|
作者
Knight, Justin M. [1 ,2 ]
Guyon, Olivier [1 ,2 ,3 ]
Lozi, Julien [3 ]
Jovanovic, Nemanja [4 ]
Males, Jared R. [2 ]
机构
[1] Univ Arizona, Coll Opt Sci, 1630 E Univ Blvd, Tucson, AZ 85719 USA
[2] Univ Arizona, Steward Observ, 933 N Cherry Ave, Tucson, AZ 85719 USA
[3] Natl Inst Nat Sci, Natl Astron Observ Japan, Subaru Telescope, 650 N Aohoku Pl, Hilo, HI 96720 USA
[4] CALTECH, Caltech Opt Observ, 1200 E Calif Blvd,MC 11-17, Pasadena, CA 91125 USA
基金
美国国家科学基金会;
关键词
stellar coronagraph; PIAACMC; focal plane mask; tolerancing; Monte Carlo;
D O I
10.1117/12.2314139
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Phase-Induced Amplitude Apodization Complex Mask Coronagraphs (PIAACMC) offer high-contrast performance at a small inner-working angle (< 1 lambda/D) with high planet throughput (> 70%). The complex mask is a multi-zone, phase-shifting mask comprised of tiled hexagons which vary in depth. Complex masks can be difficult to fabricate as there are many micron-scale hexagonal zones (> 500 on average) with continuous depths ranging over a few microns. Ensuring the broadband PIAACMC design performance carries through to fabricated devices requires that these complex masks are manufactured to within well-defined tolerances. We report on a simulated tolerance analysis of a "toy" PIAACMC design which characterizes the effect of common microfabrication errors on on-axis contrast performance using a simple Monte Carlo method. Moreover, the tolerance analysis provides crucial information for choosing a fabrication process which yields working devices while potentially reducing process complexity. The common fabrication errors investigated are zone depth discretization, zone depth errors, and edge artifacts between zones.
引用
收藏
页数:8
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