English

Phase-induced amplitude apodization complex mask coronagraph tolerancing and analysis

Instrumentation and Methods for Astrophysics 2018-07-13 v1 Earth and Planetary Astrophysics

Abstract

Phase-Induced Amplitude Apodization Complex Mask Coronagraphs (PIAACMC) offer high-contrast performance at a small inner-working angle (\approx 1 λ\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.

Keywords

Cite

@article{arxiv.1807.04379,
  title  = {Phase-induced amplitude apodization complex mask coronagraph tolerancing and analysis},
  author = {Justin M. Knight and Olivier Guyon and Julien Lozi and Nemanja Jovanovic and Jared R. Males},
  journal= {arXiv preprint arXiv:1807.04379},
  year   = {2018}
}

Comments

8 pages, 6 figures, SPIE Astronomical Telescopes + Instrumentation

R2 v1 2026-06-23T02:58:24.423Z