The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD

Hiroaki Imada, Tadayasu Dotani, Takashi Hasebe, Masashi Hazumi, Junji Inatani, Hirokazu Ishino, Shingo Kashima, Nobuhiko Katayama, Kimihiro Kimura, Tomotake Matsumura, Ryo Nagata, Yutaro Sekimoto, Hajime Sugai, Aritoki Suzuki, Shin Utsunomiya

Research output: Chapter in Book/Report/Conference proceedingConference contribution

2 Citations (Scopus)

Abstract

The Lite satellite for the studies of B-mode polarization and Inflation from the cosmic microwave background (CMB) Radiation Detection (LiteBIRD) is a next generation CMB satellite dedicated to probing the inflationary universe. It has two telescopes, Low Frequency Telescope (LFT) and High Frequency Telescope (HFT) to cover wide observational bands from 34 GHz to 448 GHz. In this presentation, we report the optical design and characterization of the LFT. We have used the CODE-V to obtain the LFT optical design based on a cross- Dragonian telescope. It is an image-space telecentric system with an F number of 3.5 and 20 x 10 degrees2 field of view. The main, near and far side lobes at far-field have been calculated by using a combination of HFSS and GRASP 10. It is revealed that the LFT telescope has good main lobe properties to satisfy the requirements. On the other hand, the side lobes are affected by the stray light that stems from the triple reflection and the direct path from feed. In order to avoid the stray light, the way to block these paths is now under study.

Original languageEnglish
Title of host publicationSpace Telescopes and Instrumentation 2018
Subtitle of host publicationOptical, Infrared, and Millimeter Wave
EditorsGiovanni G. Fazio, Howard A. MacEwen, Makenzie Lystrup
PublisherSPIE
Volume10698
ISBN (Print)9781510619494
DOIs
Publication statusPublished - Jan 1 2018
Externally publishedYes
EventSpace Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave - Austin, United States
Duration: Jun 10 2018Jun 15 2018

Other

OtherSpace Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave
CountryUnited States
CityAustin
Period6/10/186/15/18

Fingerprint

Physical Optics
Physical optics
physical optics
Optical design
Optical Design
Telescopes
Telescope
telescopes
optics
Low Frequency
Stray light
lobes
low frequencies
Stray Light
Antenna lobes
Microwave
Microwaves
Satellites
Cosmic rays
cosmic microwave background radiation

Keywords

  • CMB space mission
  • Physical optics
  • Ray tracing
  • Wide field of view telescope

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Condensed Matter Physics
  • Computer Science Applications
  • Applied Mathematics
  • Electrical and Electronic Engineering

Cite this

Imada, H., Dotani, T., Hasebe, T., Hazumi, M., Inatani, J., Ishino, H., ... Utsunomiya, S. (2018). The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD. In G. G. Fazio, H. A. MacEwen, & M. Lystrup (Eds.), Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave (Vol. 10698). [106984K] SPIE. https://doi.org/10.1117/12.2312185

The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD. / Imada, Hiroaki; Dotani, Tadayasu; Hasebe, Takashi; Hazumi, Masashi; Inatani, Junji; Ishino, Hirokazu; Kashima, Shingo; Katayama, Nobuhiko; Kimura, Kimihiro; Matsumura, Tomotake; Nagata, Ryo; Sekimoto, Yutaro; Sugai, Hajime; Suzuki, Aritoki; Utsunomiya, Shin.

Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. ed. / Giovanni G. Fazio; Howard A. MacEwen; Makenzie Lystrup. Vol. 10698 SPIE, 2018. 106984K.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Imada, H, Dotani, T, Hasebe, T, Hazumi, M, Inatani, J, Ishino, H, Kashima, S, Katayama, N, Kimura, K, Matsumura, T, Nagata, R, Sekimoto, Y, Sugai, H, Suzuki, A & Utsunomiya, S 2018, The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD. in GG Fazio, HA MacEwen & M Lystrup (eds), Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. vol. 10698, 106984K, SPIE, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave, Austin, United States, 6/10/18. https://doi.org/10.1117/12.2312185
Imada H, Dotani T, Hasebe T, Hazumi M, Inatani J, Ishino H et al. The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD. In Fazio GG, MacEwen HA, Lystrup M, editors, Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. Vol. 10698. SPIE. 2018. 106984K https://doi.org/10.1117/12.2312185
Imada, Hiroaki ; Dotani, Tadayasu ; Hasebe, Takashi ; Hazumi, Masashi ; Inatani, Junji ; Ishino, Hirokazu ; Kashima, Shingo ; Katayama, Nobuhiko ; Kimura, Kimihiro ; Matsumura, Tomotake ; Nagata, Ryo ; Sekimoto, Yutaro ; Sugai, Hajime ; Suzuki, Aritoki ; Utsunomiya, Shin. / The optical design and physical optics analysis of a cross-Dragonian telescope for LiteBIRD. Space Telescopes and Instrumentation 2018: Optical, Infrared, and Millimeter Wave. editor / Giovanni G. Fazio ; Howard A. MacEwen ; Makenzie Lystrup. Vol. 10698 SPIE, 2018.
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abstract = "The Lite satellite for the studies of B-mode polarization and Inflation from the cosmic microwave background (CMB) Radiation Detection (LiteBIRD) is a next generation CMB satellite dedicated to probing the inflationary universe. It has two telescopes, Low Frequency Telescope (LFT) and High Frequency Telescope (HFT) to cover wide observational bands from 34 GHz to 448 GHz. In this presentation, we report the optical design and characterization of the LFT. We have used the CODE-V to obtain the LFT optical design based on a cross- Dragonian telescope. It is an image-space telecentric system with an F number of 3.5 and 20 x 10 degrees2 field of view. The main, near and far side lobes at far-field have been calculated by using a combination of HFSS and GRASP 10. It is revealed that the LFT telescope has good main lobe properties to satisfy the requirements. On the other hand, the side lobes are affected by the stray light that stems from the triple reflection and the direct path from feed. In order to avoid the stray light, the way to block these paths is now under study.",
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