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Träfflista för sökning "WFRF:(Dicker A. P.) srt2:(2020-2024)"

Search: WFRF:(Dicker A. P.) > (2020-2024)

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2.
  • Gudmundsson, Jón E., et al. (author)
  • The Simons Observatory : modeling optical systematics in the Large Aperture Telescope
  • 2021
  • In: Applied Optics. - 1559-128X .- 2155-3165. ; 60:4, s. 823-837
  • Journal article (peer-reviewed)abstract
    • We present geometrical and physical optics simulation results for the Simons Observatory Large Aperture Telescope. This work was developed as part of the general design process for the telescope, allowing us to evaluate the impact of various design choices on performance metrics and potential systematic effects. The primary goal of the simulations was to evaluate the final design of the reflectors and the cold optics that are now being built. We describe nonsequential ray tracing used to inform the design of the cold optics, including absorbers internal to each optics tube. We discuss ray tracing simulations of the telescope structure that allow us to determine geometries that minimize detector loading and mitigate spurious near-field effects that have not been resolved by the internal baffling. We also describe physical optics simulations, performed over a range of frequencies and field locations, that produce estimates of monochromatic far-field beam patterns, which in turn are used to gauge general optical performance. Finally, we describe simulations that shed light on beam sidelobes from panel gap diffraction.
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3.
  • Gallardo, P. A., et al. (author)
  • Optical design concept of the CMB-S4 large-Aperture telescopes and cameras
  • 2022
  • In: Proceedings of SPIE, the International Society for Optical Engineering. - : SPIE. - 0277-786X .- 1996-756X. ; 12190
  • Journal article (peer-reviewed)abstract
    • CMB-S4-the next-generation ground-based cosmic microwave background (CMB) experiment-will significantly advance the sensitivity of CMB measurements and improve our understanding of the origin and evolution of the universe. CMB-S4 will deploy large-Aperture telescopes fielding hundreds of thousands of detectors at millimeter wavelengths. We present the baseline optical design concept of the large-Aperture CMB-S4 telescopes, which consists of two optical configurations: (i) a new off-Axis, three-mirror, free-form anastigmatic design and (ii) the existing coma-corrected crossed-Dragone design. We also present an overview of the optical configuration of the array of silicon optics cameras that will populate the focal plane with 85 diffraction-limited optics tubes covering up to 9 degrees of field of view, up to 1.1 mm in wavelength. We describe the computational optimization methods that were put in place to implement the families of designs described here and give a brief update on the current status of the design effort. 
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4.
  • Xu, Zhilei, et al. (author)
  • The Simons Observatory : metamaterial microwave absorber and its cryogenic applications
  • 2021
  • In: Applied Optics. - 1559-128X .- 2155-3165. ; 60:4, s. 864-874
  • Journal article (peer-reviewed)abstract
    • Controlling stray light at millimeter wavelengths requires special optical design and selection of absorptive materials that should be compatible with cryogenic operating environments. While a wide selection of absorptive materials exists, these typically exhibit high indices of refraction and reflect/scatter a significant fraction of light before absorption. For many lower index materials such as commercial microwave absorbers, their applications in cryogenic environments are challenging. In this paper, we present a new tool to control stray light: metamaterial microwave absorber tiles. These tiles comprise an outer metamaterial layer that approximates a lossy gradient index anti-reflection coating. They are fabricated via injection molding commercially available carbon-loaded polyurethane (25% by mass). The injection molding technology enables mass production at low cost. The design of these tiles is presented, along with thermal tests to 1 K. Room temperature optical measurements verify their control of reflectance to less than 1% up to 65∘ angles of incidence, and control of wide angle scattering below 0.01%. The dielectric properties of the bulk carbon-loaded material used in the tiles is also measured at different temperatures, confirming that the material maintains similar dielectric properties down to 3 K.
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  • Result 1-4 of 4

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