Paper
19 July 2016 Optical design and verification of a 4mm receiver for the 20m telescope at Onsala Space Observatory
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Abstract
The work of this research is the design, analysis and verification of the optical performance of a 4mmreceiver channel for the 20 m telescope at Onsala Space Observatory, Onsala, Sweden. The 4 mm (75 GHz) receiver is a newly proposed channel designed to be installed parallel to the existing 3 mm (100 GHz) channel targeting new science at that longer wavelength. Gaussian beam mode analysis is used to produce the fundamental optical design of the system. The design is then analysed more accurately with the physical optics approximation. We report on the comparison of simulation and measurement and verification of the system design.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
George W. Walker, Eimante Kalinauskaite, Darragh N. McCarthy, Neil A. Trappe, Anthony Murphy, Leif Helldner, Miroslav G. Pantaleev, and Jonas Flygare "Optical design and verification of a 4mm receiver for the 20m telescope at Onsala Space Observatory", Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 99142V (19 July 2016); https://doi.org/10.1117/12.2232576
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Cited by 2 scholarly publications.
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KEYWORDS
Mirrors

Receivers

Receivers

Gaussian beams

Optical design

Optical design

Space telescopes

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