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The LCLS beam provides revolutionary capabilities for studying the transient behavior of matter in extreme conditions. The particular strength of the Matter in Extreme Conditions instrument is that it combines the unique LCLS beam with high-power optical laser beams, and a suite of dedicated diagnostics tailored for this field of science. In this p...

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... In a typical experiment, the optical beam either drives a shock wave through a target or heats it to a high temperature. The shocked or heated region is then probed with the X-rays. Since the targets are typically destroyed by the optical laser beam on each shot, many targets can be mounted and positioned in the interaction region without venting the chamber. A motorized alignment stage, with six degrees of freedom, allows for a total area of 150 mm  25 mm to mount targets. The optical and X-ray beam are aligned and overlapped on a Ce:YAG scintillator target at the interaction point. The fluorescence signal created by the optical or X-ray laser beam can be imaged with long-distance microscopes, with a resolution of 18 m m, and overlap is achieved by steering the optical beam with a motorized focusing lens. In Fig. 2 a schematic of the MEC beamline including the most important devices and their location is shown. Table 1 summarizes the specifications of the X-ray beamline, the optical laser and details of the hutch. Compared with the other hutches at LCLS, MEC distinguishes itself by virtue of its two relatively high power and high energy optical laser systems. 2.2.1. Nd:glass laser system . The front-end of the Nd:glass laser system at MEC consists of a CW cavity operating at 1054 nm. The beam is subsequently sent through an electro- optical modulator and molded to the required pulse length and shape. The modulator has a rise time of 200 ps, and intrinsic time jitter with respect to its input trigger of 20 ps. Pulse lengths from 2 ns up to 200 ns are possible. The pulse is subsequently split into two arms, further amplified, and finally frequency-doubled to 527 nm. The maximum beam energy per arm is 25 J for pulses that are 25 ns or longer. For shorter pulses, the beams are intensity-limited to approximately 1 J ns À 1 , although this is dependent on the pulse shape. The repetition rate is determined by the cool-down time of the large-diameter glass amplifiers, which is approximately 7 min. The unfocused beam size is 40 mm. The beams are typically focused with 250 mm focal-length singlet lenses and hybrid phase plates for focal spots of 100 m m, 150 m m, 250 m m and 500 m m. Alternatively, users can bring their own focusing solution. The Ti:sapphire laser at MEC has a front-end oscillator that is phase-locked to the RF of the LCLS linac to assure timing synchronization with the X-ray pulses, resulting in an arrival time jitter between the X-rays and the optical beam of approximately 150 fs RMS. The oscillator output is stretched to 150 ps and amplified in a regenerative amplifier. The output of this regenerative amplifier is compressed and sent through a cross-polarized-wave generator (XPW) to enhance the contrast and reduce the pre-pulse on the laser. The cleaned pulse is re-stretched and amplified to a final energy of 1.5 J, with a repetition rate of 5 Hz. Adaptive optics ( i.e. a deformable mirror) are installed after the final amplifier to remove any wavefront aberrations that are present. The beam is compressed in vacuum to 50 fs and sent to the chamber with a beam diameter of 50 mm and an energy of 1 J. Alternatively, the beam can be sent to a final amplifier that uses the arms of the MEC glass laser as a pump, increasing the energy to 7 J after compression, with a beam diameter of 85 mm. Cool-down time of the glass pump limits the repetition rate to one shot every seven minutes in this operation mode. More detailed information about the laser, and the way it is used and synchronized with the LCLS X-ray beam, is given by Minitti et al. (2015). The ability to focus the LCLS beam down to sub-micro- meter spots, and its coherent nature, allow for imaging applications with unprecedented spatial and temporal resolution. MEC has taken advantage of this capability to make phase-contrast images of shock waves going through a solid (Schropp et al. , 2012). For this experiment, the LCLS beam was focused with another set of Be lenses placed inside the MEC target chamber that is not part of the standard MEC beamline. The lens set has a focal length of 170 mm and focuses to a spot of nominally 85 nm (FWHM). The characterization of this spot, which is the illumination source of the phase-contrast imaging (PCI) experiment, is highly important for a quanti- tative analysis of PCI data. This step was performed using scanning coherent X-ray microscopy (often also denoted from the interaction by ptychography) (Rodenburg & Faul- diagnostics, kner, 2004; Thibault et al. , 2009; Maiden the arrival time & Rodenburg, 2009; Schropp et al. , lenses, M1 2010, 2013 a , b ). The technique is based beam, WIN is a of the MEC target on the scanning of a nano-structured of the undulator. sample through a spatially confined and coherent X-ray beam. The measurement of the far-field diffraction patterns at each scan position allows for the reconstruction of the transmission function of the sample as well as the focused LCLS beam. In Fig. 3 the results of such a ptychographic experiment are summarized. The focus size was determined to have a central spot of approximately 100 nm (FWHM). After this characterization, a sample is placed into the divergent X-ray beam at a distance of 0.2 m behind the focus. Another 3.8 m further downstream an X-ray detector is positioned in order to measure the magnified phase-contrast image of the sample. High-resolution images are obtained with sensitivity to both amplitude and phase of the X-ray transmission function of the sample. As an example, Fig. 4 shows an image of a shock wave generated by the MEC glass laser. The laser is oriented perpendicular to the X-rays and is focused on the edge of a 100 m m-thick aluminium foil. The laser is fired, and a shockwave is created when it hits the foil. After 10 ns, the X-rays arrive and capture a snap-shot of the sample. The front of the shock wave, and regions of compressed matter behind it, can clearly be distinguished with a spatial resolution better than 1 m m. In recent years, a lot of effort has gone into measuring dense matter properties at extreme conditions using X-ray Thomson scattering. The spectral analysis of the elastically and inelas- tically scattered X-rays has provided valuable information about electron density, temperature, ionization state and collective behavior (Glenzer et al. , 1999; Landen et al. , 2001; Gregori et al. , 2003; Lee et al. , 2009; Kritcher et al. , 2008; Ma et al. , 2014). However, experimental constraints due to the broadband uncollimated laser-produced X-ray sources ( i.e. backlighters) have limited the experimental accuracy, which makes distinguishing among competing theoretical models difficult. MEC offers the ability to collect highly accurate data using LCLS, revolutionizing X-ray Thomson scattering as a technique to diagnose dense plasmas. To this aim, MEC developed crystal X-ray scattering spectrometers in a von H ́mos geometry for the accurate measurement of angle-resolved scattered spectra (see Fig. 5). The spectrometer detector position can be manually adjusted to accommodate X-ray energies between 4 keV and 8 keV. Motorization of four degrees of freedom allows us to change the scattering angle in situ from 0 to 90 with 1 resolution. Cylindrically curved crystals of either highly oriented pyrolytic graphite (HOPG) (Zastrau et al. , 2012) or highly annealed pyrolytic graphite (HAPG) (Zastrau et al. , 2013) are used to efficiently record scattered spectra. The larger mosaic spread of HOPG results in roughly twice the collection efficiency compared with HAPG, while the latter improves the spectral resolution from 30 eV to 9 eV. Fig. 5( a ) shows a raw image of the scattered spectrum on an aluminium specimen recorded by the HAPG spectrometer in a forward-scattering geometry. A resolution of 9 eV with seeded LCLS operation at 8 keV clearly distinguishes the plasmon feature down-shifted from the elastic peak by approximately 20 eV. With dynamic shock compression, the shift of the plasmon peak results in a direct measurement of electron density (Fletcher et al. , 2013). The opportunity to use an X-ray free-electron laser for investigating phase transitions of materials subjected to high- pressure shocks was recognized early on (Nagler et al. , 2007). Such high-pressure shocks are routinely generated using high- energy laser systems in facilities around the world. Using diffraction from laser-produced X-rays to probe the changes in the microscopic structure of the material has been used very successfully over the last two decades on single crystals (see Loveridge-Smith et al. , 2001; Kalantar et al. , 2005; Jensen & Gupta, 2008; Murphy et al. , 2010; Suggit et al. , 2012, and references therein). However, the investigation of poly- crystalline materials with laser-produced X-ray sources is limited in applicability due to the divergent nature of these sources and the quality of the data that can be achieved. In contrast, the almost perfect collimation of LCLS in combination with its high photon flux make it an excellent source for such research (Milathianaki et al. , 2013). The combination of LCLS with the laser system that is capable of driving Mbar shocks through solid and co-located diagnostics (such as VISAR, XRTS) provides a unique platform for this research. Diffraction of the sample under test is recorded with CSPAD detectors (MEC has both CSPAD-140k and CSPAD-560k) that have been developed by Cornell University and SLAC (Blaj et al. , 2015). In Fig. 6 we show the diffraction recorded on a CSPAD-140k, from a structured Al foil of thickness 100 m m. Fig. 6( a ) shows the unshocked foil. Fig. 6( b ) shows the diffraction 20 ns after optical beam has impinged on the target, showing the growth of grains along favorable orienta- tions as well as clear evidence of lattice decompression under shock release. The method can be used to investigate phase transitions, compression and strength of materials with ...

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... It arises in contexts ranging from astrophysical objects (24)(25)(26) and planetary interiors (27)(28)(29) to inertial confinement fusion (ICF) targets on the way to ignition (30)(31)(32)(33). Creating WDM conditions requires access to specialized experimental facilities (34)(35)(36)(37)(38) that produce shortlived and nonuniform samples with low repetition rates relative to experiments at ambient conditions. These challenges are compounded by the difficulty of simultaneously characterizing the target's thermodynamic conditions and the projectile's energy loss, as well as systematic errors attendant to measuring aggregate energy losses in lieu of energy loss rates. ...
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