research papers
Soft X-ray diffraction patterns measured by a LiF detector with sub-micrometre resolution and an ultimate dynamic range
aJoint Institute for High Temperatures, Russian Academy of Sciences, Izhorskaya Street 13 Bd 2, Moscow 125412, Russian Federation, bSkobeltsyn Institute of Nuclear Physics, Lomonosov Moscow State University, Leninskie gory, GSP-1, Moscow 119991, Russian Federation, cMoscow Engineering Physics Institute (MEPhI), Kashirskoe shosse 31, Moscow 115409, Russian Federation, dInstitute for Open and Transdisciplinary Research Initiatives, Osaka University, 2-6 Yamadaoka, Suita, Osaka 565-0871, Japan, eRussian Academy of Sciences, Federal Research Centre – Crystallography and Photonics, Leninskii pr-t 59, Moscow 119333, Russian Federation, fDeutsches Elektronen-Synchrotron (DESY), Notkestrasse 85, Hamburg 22607, Germany, gNational Research Tomsk Polytechnic University (TPU), 30 Lenin Avenue, Tomsk 634050, Russian Federation, hAnalytical Chemistry – Biointerfaces, Ruhr University Bochum, Universitatsstrasse 150, Bochum 44780, Germany, iDivision of Synchrotron Radiation Research, Department of Physics, Lund University, Box 118, SE-221 00 Lund, Sweden, and jInstitute of Laser Engineering, Osaka University, 2-6 Yamadaoka, Suita, Osaka 565-0871, Japan
*Correspondence e-mail: spikuz@gmail.com
The unique diagnostic possibilities of X-ray diffraction, small X-ray scattering and phase-contrast imaging techniques applied with high-intensity coherent X-ray synchrotron and X-ray free-electron laser radiation can only be fully realized if a sufficient 7 within the sub-micrometre spatial resolution. At the PETRA III facility, the diffraction pattern created behind a circular aperture with a diameter of 5 µm irradiated by a beam with a photon energy of 500 eV was recorded on a LiF crystal. In the diffraction pattern, the accumulated dose was varied from 1.7 × 105 J cm−3 in the central maximum to 2 × 10−2 J cm−3 in the 16th maximum of diffraction fringes. The period of the last fringe was measured with 0.8 µm width. The PL response of the LiF crystal being used as a detector on the irradiation dose of 500 eV photons was evaluated. For the particular model of laser-scanning confocal microscope Carl Zeiss LSM700, used for the readout of the PL signal, the calibration dependencies on the intensity of photopumping (excitation) radiation (λ = 488 nm) and the gain have been obtained.
and/or spatial resolution of the detector is available. In this work, it is demonstrated that the use of lithium fluoride (LiF) as a (PL) imaging detector allows measuring of an X-ray diffraction image with a of ∼10Keywords: diffraction patterns; LiF detectors; color centers.
1. Introduction
Various diagnostic techniques based on X-ray radiation such as coherent X-ray diffractive imaging, ptychographic coherent diffractive imaging and small-angle X-ray scattering are broadly used these days for studying matter at the nanometre scale. The advent of next-generation synchrotron sources as well as X-ray free-electron lasers (XFELs) delivering highly coherent and ultrabright radiation opens unique opportunities to study ultrafast processes in matter including various high energy-density physics (HEDP) phenomena. In turn, it imposes additional requirements on X-ray detection systems to be applied in such studies. In particular, the detector should be sustainable to ultraintense X-ray fluxes and strong electromagnetic pulses (EMPs).
One of the most important requirements for a detector in such types of experiment is the simultaneous support of sub-micrometre spatial resolution, a wide
and a large field of view. The use of conventional detectors often cannot satisfy this requirement when recording images at intense X-ray fields.While commonly used CCD cameras may provide a high 4) and tremendous sensitivity where almost every single photon can be detected in a real-time acquisition mode, these detectors are quite fragile to overexposure and unsustainable to EMPs, and their use in HEDP experiments is often restricted.
(up to 1 × 10The issue can be mitigated with the application of analog detectors such as image plates (IPs), scintillator screens or X-ray films, though they are less convenient for real-time data acquisition. However, they provide a limited spatial resolution (not better than 25 µm for IPs and 4 to 5 µm for X-ray films) and their 5 for a single exposure.
does not exceed 10A relatively new and promising X-ray detector is lithium fluoride (LiF) in the form of bulk crystal and thin film, which has demonstrated its performance as a 2D and 3D imaging tool in a wide range of applications including X-ray microradiographs of small biological objects in the water-window spectral range (energy range between the absorption edges of carbon and oxygen at 284 eV and 532 eV) (Baldacchini et al., 2003); visualization and characterization of focused X-ray beams (Faenov et al., 2009; Pikuz et al., 2015; Bonfigli et al., 2016); coherent X-ray beam metrology by diffraction method (Ruiz-Lopez et al., 2017); X-ray radiography with a large aspect ratio field-of-view/spatial resolution; and, in particular, in the interests of HEDP (Faenov et al., 2018), phase-contrast imaging and quality control of nano-thickness foils (Faenov et al., 2010; Pikuz et al., 2018) and space-resolved dosimetry (Kurobori & Matoba, 2014).
The principle of the operation with the LiF detector is shown in Fig. 1. When a photon with energy exceeding 14 eV propagates in the medium, the absorbed energy moves electrons from the to the of the crystal. Free electrons occupy anion vacancies in crystal cells and create so-called F color centers (CCs). During the relaxation process, primary F centers aggregate to more complex CC structures containing several excited centers. Among various aggregates of CCs, only F2 and F3+ have practical importance for imaging applications. They are metastable and have almost overlapping broad absorption bands at ∼450 nm [see Fig. 1(c)]. This means that they can be simultaneously excited by a single pumping wavelength. Moreover, they mainly contribute to visible luminescence in two well-separated broad emission bands in the green (F3+) and in the red (F2) spectral ranges [see Fig. 1(c)]. It is essential that CCs are stable at room temperature, so the hidden image formed within the LiF volume is kept for many years almost without decay. In comparison, the lifetime of stored CCs in IPs is of a few hours and the corresponding readout process must be carried out immediately after the exposure. Note that these centers can also be generated by protons (Piccinini et al., 2017; Montereali et al., 2018), neutrons (Faenov et al., 2015), electrons (Almaviva et al., 2007), and γ and X-ray photons (Kurobori et al., 2014; Voitovich et al., 2013).
To finalize the X-ray detection procedure (Fig. 1), the distribution of CCs can be conveniently observed by a fluorescent optical microscope. For recounting of the microscope (PL) signal into the accumulated dose in the crystal, one should know the microscope apparatus functions [see the red rectangle in Fig. 1(d)] as well as the dependence of the CCs number on the absorbed dose [the green rectangle in Fig. 1(d)]. In this article, we follow from the microscope signal to the real accumulated dose of the LiF crystal.
The LiF detector does not require any electronic circuits and therefore is not sensitive to electromagnetic noise, which can be an issue for the use of CCD cameras. The disadvantage of the LiF detector is in its inability to display the image in real time, at least with existing microscope readout systems, until a special fiber-connected fluorescent microscope head can be built. The total time to obtain an image using this detector is comparable with the readout time for the IPs. A typical scan of the image (512 × 512 pixels) takes tens of seconds, depending on the scanning conditions. However, when the experimental setup employs a vacuum vessel, the most time-consuming readout stage is the venting and opening of the vacuum chamber which may cost ∼1 h of operation.
Characterization of the metrological properties of the LiF crystals such as sensitivity, et al., 2015; Grum-Grzhimailo et al., 2017; Bonfigli et al., 2019), while the data in a soft spectral range were previously measured only by using a laser-plasma source (Baldacchini et al., 2005), and there are no data on the dependence of LiF PL response to narrow-bandwidth quasi-monochromatic radiation. The main aim of the present work is in the precise characterization of the response function, sensitivity threshold and of the LiF detector in the vicinity of the water-window band. The performance of the LiF detector is demonstrated by the measurement of soft-X-ray diffraction patterns with sub-micrometre resolution and the ultimate dynamic range.
and the spatial resolution is an important prerequisite when using it as an X-ray detector. There have been several studies of such functions for hard X-rays (Pikuz2. Experimental method
The experiment was performed at the soft X-ray beamline P04 of the third-generation synchrotron source PETRA III at DESY, Hamburg, Germany (Viefhaus et al., 2013). An APPLE-II type helical undulator of length 5 m with 72 magnetic periods was tuned to deliver photons at an energy of 500 eV (Rose et al., 2015). The X-ray beam was focused by the two-mirror system in vertical and horizontal directions. The measurements were carried out in the holographic Roentgen scattering (HORST) vacuum chamber (Rose et al., 2018).
As mentioned above, knowledge of both the response function and the (a). Both the diode and the LiF crystal were mounted on a single motorized scanning stage with nanometre precision. A simple translation motion was therefore sufficient in order to choose to send the synchrotron radiation to either the diode or the LiF crystal. First, the integral incident on the LiF detector position was measured by a diode as ∼109 photons per second. The diode was calibrated with a monochromatic source of known intensity prior to the experiment. The area of the beam was limited to a slit gap with a size of 100 µm. The diffraction pattern was recorded at a distance of 1 m from the slit. The whole image of the pattern was measured by the LiF detector in a field of view of 2 mm and with an exposure time of 180 s. Additionally, the 2D intensity profile was measured by scanning the photodiode through the center of the diffraction pattern in horizontal and vertical directions. The field of view of the photodiode was limited by a pinhole of size 1.5 µm.
of the LiF detector is important for a successful application. In the first phase of the experiment, we investigated the response function of LiF crystal to soft X-ray radiation. For this, the diffraction pattern behind a slit was captured by a LiF crystal and then it was compared with data from a calibrated photodiode. A sketch of the experimental setup is shown in Fig. 2In the second step of the experiment, a series of measurements using the slit and the pinhole were conducted to identify the (b)]. The intensity distribution of the synchrotron beam was measured at sequences of planes. For that purpose, the LiF crystal was moved along the Z axis in the range 1 to 12 mm (an axis along the beam propagation direction).
of the crystal and to demonstrate the imaging capability of LiF [see Fig. 2After the experiments, the LiF crystals were analyzed by a confocal laser-scanning microscope (model Carl Zeiss LSM700). The PL signal from the irradiated crystal was recorded by a 16-bit photomultiplier (PMT). The PL intensity was controlled by the PMT voltage (parameter gain) and the level of excitation radiation (the LSM laser power). The calibration parameters were obtained as a function of the intensity of photopumping (excitation) radiation (λ = 488 nm) and the gain for the particular model of laser-scanning confocal microscope. A detailed description of the calibration procedure is presented in the Appendix A.
It is known that only F2 and F3+ CCs are metastable and emit in the visible range [see Fig. 1(b)], i.e. giving the contribution to the LSM signal. There is no general way to evaluate the dose quantitatively as a function of emitting CCs number. However, we were able to excite mainly F2 type of CCs via the 488 nm pumping laser, where the F3+ signal is almost suppressed [see Fig. 1(b)].
3. Response of the LiF detector as a function of the X-ray dose
To define the PL response of the LiF detector, we used the diffraction pattern obtained in the first experiment [see Fig. 2(a)]. Fig. 3(a) shows a PL image of the diffraction pattern recorded on the LiF detector. Because of the high spatial resolution and the large field of view of the LiF detector, the diffraction pattern with a large number of well resolved fringes is clearly seen. The fringes in the horizontal direction are numerous and stem from a small slit size while the fringes in the vertical direction are few as a result of a widely opened vertical slit.
The spatial distribution of the beam obtained using a diode and a LiF crystal (along the same part of the diffraction pattern as had been scanned by the photodiode) is presented in Figs. 3(b) and 3(c) (black and red lines) in the horizontal and vertical directions, respectively. It can be seen that the obtained data differ considerably for the detectors. Since the LSM signal depends on the concentration of the F2 and F3+ CCs, we can conclude that the response of the LiF detector on the accumulated dose is nonlinear.
These days, the physics of CCs generation is not completely clear in relation to the dose/fluence of the 2, F3+), the F centers should be accumulated. The formation of single centers can be described by a semi-empirical function (Baldacchini et al., 2005),
but it is known that the mechanism of formation of F centers is statistical. In order to obtain metastable states which emit in the visible range (such as Fwhere f(D, P) is the CC concentration (1 cm−3), k is the coefficient indicating the F-type CCs density, D is the X-ray dose (J cm−3), P is the dose rate and Ps is the X-ray power threshold.
Equation (1) shows that the response function of the crystal is not linear with respect to the absorbed dose. Statistical accumulation of single centers is needed for the accumulation of more complex defects in the (F2 and F3+). If we assume that these events are independent, then the response function of the LiF crystal can be approximated as a power law. This allows us to obtain a quantitative dose distribution based on the number of observable F3+ CCs as
where D is the deposed dose, B represents a coefficient (representing together the probability of CC creation by 500 eV photons and the emissivity of the F3+ CCs fluorescence), n is the power index and f(F3+) is the F3+ centers concentration (cm−3),
where ILSM700 is the gray value (counts of the microscope) and Fscan is the microscope function.
In the work of Bonfigli et al. (2010), LiF crystals were irradiated by soft X-rays emitted by a laser-plasma source in the energy range from 0.05 to 2 keV (maximum intensity for 1 keV). The same dependence [equation (2)] was used for the fitting of the experimental points. It was found that n = 2.2 for X-ray fluxes up to 120 µJ cm−2, which corresponds to the accumulated dose of 1.2 kJ cm−3 in LiF [see equation (2)] for F3+-type CCs.
Applying the response function [in the form of equation (2)] with a variable exponent n to the beam profile data obtained using the LiF crystal [Figs. 3(b) and 3(c), red lines], we found the best fitting exponent value of n = 2.2 at which the diode and the crystal data are in good agreement. Fig. 3(d) shows the dependence of the standard deviation on the exponent n between the diode and LiF data in our experiment. As one can see, the best correlation between the diode and LiF data is observed at n = 2.2 [see Figs. 3(b) and 3(c), blue and black lines] that corresponds to the minimum deviation in Fig. 3(d). Finally, equations (2) and (3) can be rewritten in the form
Thus, we found that, for the monochromatic radiation with an energy of 500 eV, the response function of the LiF detector coincides with that obtained for polychromatic laser-plasma radiation [in the work of Bonfigli et al. (2010)] within a similar range of absorbed dose.
4. Evaluation of LiF detector dynamic range
Conventional X-ray detectors such as CCDs, IPs, radiochromic films and diodes typically provide a 5 in a single exposure. Here we specify the of a detector as the ratio of the saturation (or damage) threshold to the minimum signal being recognized over the noise level of the same detector. In the following, we evaluate the of the LiF detector. To do this, a pinhole was put at a distance of 12 mm upstream of the crystal for the observation of diffraction patterns in the far zone [see Fig. 2(b)]. The exposure time of the crystal was 100 min for the accumulation of the maximum dose on the detector.
of not more than ∼10It is evident that if we try to determine the 4 for LSM700). However, we were able to vary the parameters of the microscope such as the gain of the PMT and the laser power to increase or decrease the signal value, and then combine both readouts to build a joint wide-range image. The corresponding apparatus functions linking the PL signal measured at different PMT gain and laser power to an actual accumulated dose were obtained for the LSM700 microscope in the frame of this work and are given in Appendix A. Thus, we can extend the of the entire recording system (readout system + LiF crystal) to the of the LiF detector. The technique becomes possible because the LiF detector can be read out many times. At first look, it may be expected that the excitation of CCs during the first readout decreases the total signal for future readings, but it is found that the signal decreases less than 0.1% after every scan. This allows a low signal to be observed as well as an extremely high one by varying the scanning parameters. On the contrary, such an approach is impossible for CCDs and IPs because the signal is wiped out after the first scan.
in one frame it is limited by the of the readout system (this value is 6 × 10Using this technique, the full intensity distribution of the X-ray beam passing the 5 µm pinhole was observed and is given in Fig. 4. If we consider the frame (a) obtained at gain = 360, one can only observe the central part of the beam, while the diffraction rings are not visible. Then, with the increase of the gain to 740, the central part of the image becomes saturated while the number of visible fringes increases [see Fig. 4(b), green frame].
It should be emphasized that we did not see the expected form (circle) of the signal behind the pinhole on the detector. This fact can be associated with instability of the beam in time (for long exposures).
Fig. 5 shows the dose profile of the X-ray radiation restored along the dashed white line in Fig. 4, which was found by using the previously obtained equation (4) for the response function of LiF. It is seen that 16 diffraction fringes are clearly distinguishable. The last ring has a dose of 2 × 10−2 J cm−3, while the maximum dose is 1.7 × 105 J cm−3. Thus, we can conclude that the LiF detector allows one to build up a single exposure X-ray image with a of not less than 107. The absorbed dose in the last visible diffraction ring corresponds to the sensitivity threshold of the LiF crystal. This value is four to five orders more than for a CCD; however, the advantage of LiF is the possibility to use it in high-intensity fields.
It should also be emphasized that the LiF −3, the high dose rate delivered by XFEL pulses may already cause the ablation of the detector surface at a few kJ cm−3 per femtosecond pulse. In our experiments, the dose rate did not exceed 30 J cm−3 per synchrotron pulse. It is worth noting that the maximum dose for the damage to LiF crystal was not accumulated in the experiment. Thus, the potential of the crystal is more significant than what we have registered.
does not depend on the photon energy or accumulated dose, but might be limited in the case of high beam fluxes. While the LiF detector is still operational at enormous accumulated doses over several MJ cm5. Spatial resolution and imaging capability of the crystal
In experiments where the structure of an object should be determined at the nanometre scale, the detector must also have a high spatial resolution. Potentially, a LiF crystal can have a spatial resolution comparable with atomic size. However, practically this value is limited by both the spatial resolution of the readout system and the size of the secondary electron cloud. The latter effect strongly depends on the X-ray energy. The physics of this process are discussed in the work by Grum-Grzhimailo et al. (2017) in detail. As an example, the spatial resolution of the LiF crystal achieved for hard X-ray photons of an XFEL (10.1 keV) was ∼1.2 µm (Pikuz et al., 2015), while for a soft X-ray laser-plasma source the diffraction pattern was obtained with a resolution of 0.05–0.075 µm (Oliva et al., 2008; Ustione et al., 2006) by using scanning near-field optical microscopy.
For our conditions, the radius of the secondary electron cloud is expected to be less than 10 nm for the X-ray beam with 500 eV energy and cannot affect the resolution power. Therefore, in our experiment, the spatial resolution of the LiF detector is limited by the readout system. We scanned the irradiated LiF crystal using the immersion objective with a numerical aperture value of 1.4 and an excitation wavelength of 488 nm that allowed us to achieve a spatial resolution of ∼0.2 µm.
The X-ray beam profiles were obtained in the planes at different distances from the pinhole (see Fig. 6, left column). The spatial distribution of the beam spot with a size of 4 µm was recorded. Fig. 6 shows features in the central region of the beam (for z = 1.3 mm and z = 1.5 mm). Because of the provided spatial resolution of the LiF detector, we could observe inhomogeneities of the spatial distribution of the X-ray beam in various planes. The LiF image profile shows the features in the X-ray beam distribution (∼0.8 µm in size) in Fig. 6(c). This value is greater than can be expected from both the blurring effect by the secondary electron cloud (several nanometres) and the spatial resolution of the LSM700 microscope.
We also simulated the propagation of the X-ray beam through the setup to compare it with the experimental beam distribution. The modeling was performed with a software framework for coherent and partially coherent X-ray wavefront propagation simulations – WavePropaGator (Samoylova et al., 2016), which is a development of the calculation methods implemented in SRW and which is available through open-access code (Chubar et al., 2008). The results of the modeling are presented in Fig. 6 (images in red frames). It can be seen that the spatial distribution of the beam is similar for all z planes. However, the amplitudes and symmetry of the experimental beam profiles differ from the modeling (see Fig. 6, black and red lines on the graphics). The size of the features in the simulated beam profile is the same as for the experimental data [see Fig. 6(c)]. Thus, we expect that for the water-window X-ray range the real spatial resolution of the LiF detector should be better than we were able to demonstrate in particular experimental configurations. Finally, it should be noted that in this article we provide just an example of LiF imaging capabilities and not careful measurements of the spatial resolution limit.
6. Summary
An experiment for the calibration of an X-ray lithium fluoride detector was performed at the P04 beamline at PETRA III. As a result, the metrological properties of the LiF crystal were retrieved. In particular, the LiF detector response function was determined for the X-ray deposed dose up to ∼14 kJ cm−3. This function is well described by a power-law dependence (power index n = 2.2). Using this dependence, we demonstrated a of LiF of up to 107 for our experimental conditions. Also, the threshold for the CCs creation was estimated as 2 × 10−2 J cm−3. This value corresponds to the dose in the last visible diffraction fringes for the experiment with pinhole diffraction.
It was also demonstrated that the sub-micrometre imaging capability of the X-ray beam distribution is achieved. LiF images showed the features in the X-ray beam distribution (∼0.8 µm in size) that correspond to the theoretical calculations. These data make it possible to extend the use of LiF as a detector for the diagnostic and characterizing of X-ray beams in extreme-intensity experiments on the study of nanoscale objects.
APPENDIX A
In addition, we also present the microscope calibration functions because there is no such data for the Carl Zeiss LSM700 provided by the vendor. In particular, we found the dependence of microscope counts ILSM700 (PMT signal) on the PMT gain and pumping laser power. For this, we scanned the test plate with different microscope parameters.
Fig. 7(a) shows the dependence of the PMT signal ILSM700 on the laser power (keeping PMT gain parameter G = constant). It is well approximated by a linear dependence with a factor of 0.01 with respect to the reference point at laser power = 100%, where the signal was normalized to 1,
where ILSM700(Plas, G = const) is the PMT signal with the arbitrary value Plas (counts per pixel in the microscope data), Alas is an approximation coefficient of the laser, Plas is the laser-power value and ILSM700(Plas = 100%, G = const) is the PMT signal with Plas = 100%.
Fig. 7(b) shows the dependence of the signal value on the PMT gain. It is well approximated by an exponential dependence with an exponent factor of t = 88 with respect to the reference point at G = 360, where the signal was normalized to 1. So the PMT signal can be presented as
where ILSM700(G, Plas = const) is the PMT signal with arbitrary value gain G (counts of the microscope), AG is an approximation coefficent of the PMT gain, t is an exponent factor and ILSM700(G = 360, Plas = const) is the F3+ centers concentration (cm−3).
If we vary both the PMT gain and laser power parameters, the total PMT signal ILSM700 is
Or, using equations (5) and (6),
Thus, equation (4) in the main section of this article for the absorbed dose D in LiF can be represented in the form
which helps to establish a cross-correspondence in the data measured at different microscope settings.
Using the reference point at Plas = 100% and G = 360 and by comparison with calibrated X-ray photodiode data as shown in Fig. 3, the parameter B representing together the probability of CC creation by 500 eV photons and the emissivity of the F3+ CCs fluorescence has been found to be 3.7 × 10−7. Finally, the absolute dose D value distribution can be revealed for any LSM parameters providing cross-calibration for the data taken with different laser pumping power and PMT gain,
Footnotes
‡Now at: Division of Biology and Chemistry, Laboratory for Biomolecular Research, Paul Scherrer Institute, 5232 Villigen, Switzerland.
Funding information
The following funding is acknowledged: Ministry of Science and Higher Education of the Russian Federation (in the frame of Photon Science Experiment Program and the State assignment No. 01201357846 to JIHT RAS); Foundation for the Advancement of Theoretical Physics and Mathematics `BASIS' (grant No. 18-2-6-67-1 to S. Makarov); Helmholtz Associations Initiative and Networking Fund (Grant No. HRSF-0002 to M. Rose, S. Lazarev, I. Zaluzhnyy and I. Vartanyants); German Federal Ministry of Education and Research (BMBF) (Grant No. 05K19PC2 to A. Rosenhahn); Competitiveness Enhancement Program of National Research Tomsk Polytechnic University.
References
Almaviva, S., Baldacchini, G., Piccinini, M. & Montereali, R. M. (2007). J. Non-Cryst. Solids, 353, 687–691. Web of Science CrossRef CAS Google Scholar
Baldacchini, G., Bollanti, S., Bonfigli, F., Flora, F., Di Lazzaro, P., Lai, A., Marolo, T., Montereali, R. M., Murra, D., Faenov, A., Pikuz, T., Nichelatti, E., Tomassetti, G., Reale, A., Reale, L., Ritucci, A., Limongi, T., Palladino, L., Francucci, M., Martellucci, S. & Petrocelli, G. (2005). Rev. Sci. Instrum. 76, 113104. Web of Science CrossRef Google Scholar
Baldacchini, G., Bonfigli, F., Faenov, A., Flora, F., Montereali, R. M., Pace, A., Pikuz, T. & Reale, L. (2003). J. Nanosci. Nanotech. 3, 483–486. Web of Science CrossRef CAS Google Scholar
Bonfigli, F., Gaudio, P., Lupelli, I., Nichelatti, E., Richetta, M., Vincenti, M. A. & Montereali, R. M. (2010). IOP Conf. Ser. Mater. Sci. Eng. 15, 012025. Google Scholar
Bonfigli, F., Hampai, D., Dabagov, S. B. & Montereali, R. M. (2016). Opt. Mater. 58, 398–405. Web of Science CrossRef CAS Google Scholar
Bonfigli, F., Hartley, N., Inubushi, Yu., Koenig, M., Matsuoka, T., Makarov, S., Montereali, R. M., Nichelatti, E., Ozaki, N., Piccinini, M., Pikuz, S., Pikuz, T., Sagae, D., Vincenti, M. A., Yabashi, M. & Yabuuchi, T. (2019). Proc. SPIE, 11035, 110350N. Google Scholar
Chubar, O., Couprie, M. E., Labat, M., Lambert, G., Polack, F. & Tcherbakoff, O. (2008). Nucl. Instrum. Methods Phys. Res. A, 593, 30–34. Web of Science CrossRef CAS Google Scholar
Faenov, A., Matsubayashi, M., Pikuz, T., Fukuda, Y., Kando, M., Yasuda, R., Iikura, H., Nojima, T., Sakai, T., Shiozawa, M., Kodama, R. & Kato, Y. (2015). High Power Laser Sci. Eng. 3, e27. Web of Science CrossRef Google Scholar
Faenov, A., Pikuz, T., Fucuda, Yu., Kando, M., Kotaki, H., Homma, T., Kawase, K., Scobelev, I., Gasilov, S., Kawachi, T., Daido, H., Tajima, T., Kato, Y. & Bulanov, S. (2010). Jpn J. Appl. Phys. 49, 06GK03. Web of Science CrossRef Google Scholar
Faenov, A. Ya., Kato, Y., Tanaka, M., Pikuz, T. A., Kishimoto, M., Ishino, M., Nishikino, M., Fukuda, Y., Bulanov, S. V. & Kawachi, T. (2009). Opt. Lett. 34, 941–943. Web of Science CrossRef PubMed Google Scholar
Faenov, A. Y., Pikuz, T. A., Mabey, P., Albertazzi, B., Michel, T., Rigon, G., Pikuz, S. A., Buzmakov, A., Makarov, S., Ozaki, N., Matsuoka, T., Katagiri, K., Miyanishi, K., Takahashi, K., Tanaka, K. A., Inubushi, Y., Togashi, T., Yabuuchi, T., Yabashi, M., Casner, A., Kodama, R. & Koenig, M. (2018). Sci. Rep. 8, 16407. Web of Science CrossRef PubMed Google Scholar
Grum-Grzhimailo, A. N., Pikuz, T., Faenov, A., Matsuoka, T., Ozaki, N., Albertazzi, B., Pikuz, S., Inubushi, Yu., Yabashi, M., Tono, K., Yumoto, H., Ohashi, H., Ishikawa, T. & Kodama, R. (2017). Eur. Phys. J. D, 71, 69. Google Scholar
Kurobori, T. & Matoba, A. (2014). Jpn J. Appl. Phys. 53, 02BD14. Web of Science CrossRef Google Scholar
Kurobori, T., Miyamoto, Y., Maruyama, Y., Yamamoto, T. & Sasaki, T. (2014). Nucl. Instrum. Methods Phys. Res. B, 326, 76–80. Web of Science CrossRef CAS Google Scholar
Montereali, R. M., Ampollini, A., Picardi, L., Ronsivalle, C., Bonfigli, F., Libera, S., Nichelatti, E., Piccinini, M. & Vincenti, M. A. (2018). J. Lumin. 200, 30–34. Web of Science CrossRef CAS Google Scholar
Oliva, C., Ustione, A., Almaviva, S., Baldacchini, G., Bonfigli, F., Flora, F., Lai, A., Montereali, R. M., Faenov, A., Pikuz, T. A., Francucci, M., Gaudio, P., Martellucci, S., Richetta, M., Reale, L. & Cricenti, A. (2008). J. Microsc. 229, 490–495. Web of Science CrossRef PubMed CAS Google Scholar
Piccinini, M., Nichelatti, E., Ampollini, A., Picardi, L., Ronsivalle, C., Bonfigli, F., Libera, S., Vincenti, M. A. & Montereali, R. M. (2017). Europhys. Lett. 117, 37004. Web of Science CrossRef Google Scholar
Pikuz, T. A., Faenov, A., Ozaki, N., Matsuoka, T., Albertazzi, B., Hartley, N. J., Miyanishi, K., Katagiri, K., Matsuyama, S., Yamauchi, K., Habara, H., Inubushi, Y., Togashi, T., Yumoto, H., Ohashi, H., Tange, Y., Yabuuchi, T., Yabashi, M., Grum-Grzhimailo, A., Casner, A., Skobelev, I., Makarov, S., Pikuz, S., Rigon, G., Koenig, M., Tanaka, K. A., Ishikawa, T. & Kodama, R. (2018). Matter Radiat. Extremes, 3, 197–206. Web of Science CrossRef Google Scholar
Pikuz, T., Faenov, A., Matsuoka, T., Matsuyama, S., Yamauchi, K., Ozaki, N., Albertazzi, B., Inubushi, Y., Yabashi, M., Tono, K., Sato, Y., Yumoto, H., Ohashi, H., Pikuz, S., Grum-Grzhimailo, A. N., Nishikino, M., Kawachi, T., Ishikawa, T. & Kodama, R. (2015). Sci. Rep. 5, 17713. Web of Science CrossRef PubMed Google Scholar
Rose, M., Senkbeil, T., von Gundlach, A. R., Stuhr, S., Rumancev, Ch., Dzhigaev, D., Besedin, I., Skopintsev, P., Loetgering, L., Viefhaus, J., Rosenhahn, A. & Vartanyants, I. A. (2018). Opt. Express, 26, 1237–1254. Web of Science CrossRef CAS PubMed Google Scholar
Rose, M., Skopintsev, P., Dzhigaev, D., Gorobtsov, O., Senkbeil, T., von Gundlach, A., Gorniak, T., Shabalin, A., Viefhaus, J., Rosenhahn, A. & Vartanyants, I. (2015). J. Synchrotron Rad. 22, 819–827. Web of Science CrossRef CAS IUCr Journals Google Scholar
Ruiz-Lopez, M., Faenov, A., Pikuz, T., Ozaki, N., Mitrofanov, A., Albertazzi, B., Hartley, N., Matsuoka, T., Ochante, R., Tange, Y., Yabuuchi, T., Habara, T., Tanaka, K. A., Inubushi, Y., Yabashi, M., Nishikino, M., Kawachi, T., Pikuz, S., Ishikawa, T., Kodama, R. & Bleiner, D. (2017). J. Synchrotron Rad. 24, 196–204. Web of Science CrossRef CAS IUCr Journals Google Scholar
Samoylova, L., Buzmakov, A., Chubar, O. & Sinn, H. (2016). J. Appl. Cryst. 49, 1347–1355. Web of Science CrossRef CAS IUCr Journals Google Scholar
Ustione, A., Cricenti, A., Bonfigli, F., Flora, F., Lai, A., Marolo, T., Maria Montereali, R., Baldacchini, G., Faenov, A., Pikuz, T. & Reale, L. (2006). Appl. Phys. Lett. 88, 141107. Web of Science CrossRef Google Scholar
Viefhaus, J., Scholz, F., Deinert, S., Glaser, L., Ilchen, M., Seltmann, J., Walter, P. & Siewert, F. (2013). Nucl. Instrum. Methods Phys. Res. A, 710, 151–154. Web of Science CrossRef CAS Google Scholar
Voitovich, P., Kalinov, V. S., Runets, L. P., Stupak, A. P., Martynovich, F., Montereali, R. M. & Baldacchini, G. (2013). J. Lumin. 143, 207–214. Web of Science CrossRef CAS Google Scholar
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