1969
DOI: 10.1016/0020-0891(69)90012-8
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A small lamellar grating interferometer for the very far-infrared

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Cited by 29 publications
(3 citation statements)
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“…Figure 1 shows the schematic setup of the interferometer, and figure 2 is a photograph of the instrument. Two 90 • off-axis parabolic mirrors guide the THz beams and no other optical guiding elements, such as light pipes [8,9,11] or flat mirrors [5][6][7], are needed. The source under test is positioned at the focus of the input parabolic mirror.…”
Section: Instrument Configurationmentioning
confidence: 99%
See 1 more Smart Citation
“…Figure 1 shows the schematic setup of the interferometer, and figure 2 is a photograph of the instrument. Two 90 • off-axis parabolic mirrors guide the THz beams and no other optical guiding elements, such as light pipes [8,9,11] or flat mirrors [5][6][7], are needed. The source under test is positioned at the focus of the input parabolic mirror.…”
Section: Instrument Configurationmentioning
confidence: 99%
“…Without a beam splitter, there is no power reflected back into the source under test. Different types of far-infrared interferometers using lamellar mirrors [5][6][7] were reported previously and their basic theory of operation was covered in [8][9][10]. These instruments were designed for FIR transmission spectroscopy and employed black-body sources or, in one case, synchrotron radiation [11] described here uses a greatly simplified configuration and was designed specifically for source characterization and operation at room temperature.…”
Section: Introductionmentioning
confidence: 99%
“…For a long time the working horse for XUV pump-XUV probe experiments was a double-mirror split-and-delay unit [11][12][13] which impedes phase-resolved measurements due to the nature of its wavefront splitting (see [14][15][16] and Section 2). However, recent successful adaptations of ideas originally invented for far-infrared interferometry [17][18][19][20] to UV [21] and XUV [22] frequencies open new opportunities for phase-resolved (interferometric) experiments at short wavelength FELs with a typical spectral bandwidth of 1%.…”
Section: Introductionmentioning
confidence: 99%