2013
DOI: 10.1364/oe.21.017340
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X-ray phase contrast imaging and noise evaluation using a single phase grating interferometer

Abstract: In this paper we present some quantitative measurements of X-ray phase contrast images and noise evaluation obtained with a recent grating based X-ray phase contrast interferometer. This device is built using a single phase grating and a large broadband X-ray source. It was calibrated using a reference sample and finally used to perform measurements of a biological fossil: a mosquito trapped in amber. As phase images, noise was evaluated from the measured interferograms.

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Cited by 33 publications
(33 citation statements)
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“…Similar setups have been used to measure the wavefront of synchrotron radiation [17] and to perform imaging [18,19]. In this work we emphasize optimization for high performance of the sensor on a single-shot basis with an unattenuated full FEL beam, and its applications to systematic studies of FEL beam characteristics at different locations along the beam path.…”
Section: Introductionmentioning
confidence: 99%
“…Similar setups have been used to measure the wavefront of synchrotron radiation [17] and to perform imaging [18,19]. In this work we emphasize optimization for high performance of the sensor on a single-shot basis with an unattenuated full FEL beam, and its applications to systematic studies of FEL beam characteristics at different locations along the beam path.…”
Section: Introductionmentioning
confidence: 99%
“…This reflects that the monochromatic fringe phase shift generated by a sample is inversely proportional to the square of photon energy, providing the photon energy is away from the absorption edges of the sample elements. Under polychromatic X-ray illumination, one may retrieve the polychromatic fringe phase shift φ m,Poly (x, y) from the fringe pattern by using either the phase stepping method or the Fourier analysis method [4,[13][14][15][16][17]. We realized that, regardless of the method used, the retrieved polychromatic fringe phase shift φ m,Poly (x, y) is given by…”
Section: Methodsmentioning
confidence: 99%
“…The reduced grating-to-detector distance R 2 /M g (with M g = 1) was set to the 1 st and 3 rd Talbot distances at the design energy. The polychromatic fringe phase shifts φ 2,Poly (x, y) was retrieved from the simulated fringe pattern by using the Fourier analysis method, as reported in [13,14,16,17]. Based on the simulated φ 2,Poly (x, y) data, we determine the monochromatic fringe shift φ Figure 4 plots the simulation results for a π-grating interferometer setup, in which the grating design energy E D was set to 18 keV and the grating-detector distance was set to the 1 st fractional Talbot distance, i.e., R 2 /M g = p 2 1 /8λ D , where λ D is the X-ray wavelength at the design energy.…”
Section: For π-Grating Interferometersmentioning
confidence: 99%
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