2016
DOI: 10.1117/12.2232382
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Practical beam transport for PFI

Abstract: The Planet Formation Imager (PFI) is a future kilometric-baseline infrared interferometer to image the complex physical processes of planet formation. Technologies that could be used to transport starlight to a central beamcombining laboratory in PFI include free-space propagation in air or vacuum, and optical fibres. This paper addresses the design and cost issues associated with free-space propagation in vacuum pipes. The signal losses due to diffraction over long differential paths are evaluated, and concep… Show more

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Cited by 2 publications
(3 citation statements)
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“…After the 2014 SPIE meeting where the PFI project was introduced, a Science Working Group (SWG; headed by Stefan Kraus) and a Technical Working Group (TWG; headed first by David Buscher, and now Michael Ireland) were formed involving around one hundred astronomers around the world. Based on the early top-level science requirements first outlined in 2014, the 2016 SPIE meeting in Edinburgh saw even more contributions which explored technical solutions to achieve these science goals [17,14,12,16,19,3,21]. For instance, a mid-infrared wavelength range was chosen over mm-wave or near-infrared to access the most diverse aspects of planet formation in the "warm dust" zone.…”
Section: Technical Description Of the Pfi Arraymentioning
confidence: 99%
“…After the 2014 SPIE meeting where the PFI project was introduced, a Science Working Group (SWG; headed by Stefan Kraus) and a Technical Working Group (TWG; headed first by David Buscher, and now Michael Ireland) were formed involving around one hundred astronomers around the world. Based on the early top-level science requirements first outlined in 2014, the 2016 SPIE meeting in Edinburgh saw even more contributions which explored technical solutions to achieve these science goals [17,14,12,16,19,3,21]. For instance, a mid-infrared wavelength range was chosen over mm-wave or near-infrared to access the most diverse aspects of planet formation in the "warm dust" zone.…”
Section: Technical Description Of the Pfi Arraymentioning
confidence: 99%
“…The PFI SWG and TWG have published a large number of articles in SPIE, outlining both the science case 2, 5 and possible technical implementations of PFI. 1,3,4,[6][7][8][9][10] This year there are about 13 contributions directly related to PFI: In addition to this work, the PFI TWG will write at least one paper in the planned Science White Book to define a baseline PFI architecture to reference in the science chapters.…”
Section: Introductionmentioning
confidence: 99%
“…Various scientific and technology aspects of PFI have been explored already in a series of papers first at the 2014 SPIE [1][2][3] and then at the 2016 SPIE. [4][5][6][7][8][9][10] More information on the PFI Project can be found at the project website http: //planetformationimager.org.…”
Section: Introductionmentioning
confidence: 99%