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This PDF file contains the front matter associated with SPIE Proceedings Volume 8141, including the Title Page, Copyright Information, Table of Contents, Introduction, and the Conference Committee listing.
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Christian G. Schroer, Susanne Hönig, Andy Goldschmidt, Robert Hoppe, Jens Patommel, Dirk Samberg, Andreas Schropp, Frank Seiboth, Sandra Stephan, et al.
Modern hard x-ray scanning microscopes generate x-ray beams with lateral sizes well below 100 nm. Characterizing
these beams in terms of shape and size by conventional techniques is tedious, requires highly accurate
test objects and stages, and yields only incomplete information. Since recently, we use a ptychographic scanning
coherent diffraction imaging technique in order to characterize hard x-ray nano beams in x-ray scanning microscopes,
obtaining a detailed quantitative picture of the complex wave field in the nano focus and allowing one
to reconstruct the exit wave field behind the nano-focusing optic, giving detailed insight into its aberrations.
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We present a method for the propagation of partially coherent radiation using coherent mode decomposition and
wavefront propagation. The radiation field is decomposed into a sum of independent coherent modes. Each mode
is then propagated separately using conventional wavefront propagation techniques. The summation of these
modes in the plane of observation gives the coherence properties of the propagated radiation. As an example,
we analyze propagation of partially coherent radiation transmitted through a single circular aperture.
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Partially-coherent wavefront propagation calculations have proven to be feasible and very beneficial in the design of
beamlines for 3rd and 4th generation Synchrotron Radiation (SR) sources. These types of calculations use the framework
of classical electrodynamics for the description, on the same accuracy level, of the emission by relativistic electrons
moving in magnetic fields of accelerators, and the propagation of the emitted radiation wavefronts through beamline
optical elements. This enables accurate prediction of performance characteristics for beamlines exploiting high SR
brightness and/or high spectral flux. Detailed analysis of radiation degree of coherence, offered by the partially-coherent
wavefront propagation method, is of paramount importance for modern storage-ring based SR sources, which, thanks to
extremely small sub-nanometer-level electron beam emittances, produce substantial portions of coherent flux in X-ray
spectral range. We describe the general approach to partially-coherent SR wavefront propagation simulations and present
examples of such simulations performed using "Synchrotron Radiation Workshop" (SRW) code for the parameters of
hard X-ray undulator based beamlines at the National Synchrotron Light Source II (NSLS-II), Brookhaven National
Laboratory. These examples illustrate general characteristics of partially-coherent undulator radiation beams in low-emittance
SR sources, and demonstrate advantages of applying high-accuracy physical-optics simulations to the
optimization and performance prediction of X-ray optical beamlines in these new sources.
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Advances at SR sources in the generation of nanofocused beams with a high degree of transverse coherence call
for effective techniques to simulate the propagation of partially coherent X-ray beams through complex optical
systems in order to characterize how coherence properties such as the mutual coherence function (MCF) are
propagated to the exit plane. Here we present an approach based on Monte Carlo sampling of the Green
function. A Gauss-Shell Stochastic Source with arbitrary spatial coherence is synthesized by means of the
Gaussian copula statistical tool. The Green function is obtained by sampling Huygens-Fresnel waves with
Monte Carlo methods and is used to propagate each source realization to the detector plane. The sampling is
implemented with a modified Monte Carlo ray tracing scheme where the optical path of each generated ray is
stored. Such information is then used in the summation of the generated rays at the observation plane to account
for coherence properties. This approach is used to simulate simple models of propagation in free space and with
reflective and refractive optics.
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This paper presents the outcome of ray tracing simulations for different optical schemes to be setup at the
European X-ray Free Electron Laser facility (XFEL.EU), Germany: one- or two- channel (cut) crystal X-ray
monochromators (K-Mono; using spontaneous radiation) are planned and designed mainly for photon beam
based alignment, which is gap tuning of the undulator segments and phase tuning of the phase shifters during
commissioning and maintenance of the undulators. The coherent SASE (Self Amplified Spontaneous Emission)
radiation will be monitored pulse-resolved by single-shot spectrometers of which two types are investigated: i) a
three element spectrometer, design proposed by Yabashi et al., which consists of a curved focusing mirror,
followed by a flat analyzer crystal and a 2D-detector.ii) a two element spectrometer based on a reflection zone
plate that reflects and focuses in one step, and a 2D-detector (currently under development).
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We present a new software project aimed at development of a novel and unique software environment, suited and
capable of solving a wide set of X-ray FEL optics problems. The complex of programs is based upon libraries of the
Synchrotron Radiation Workshop (SRW) package. The software can be used by XFEL experimental groups for
developing scientific instruments, planning experiments and processing experimental data. Specific examples of
applications of FEL wavefront propagation simulations are presented: modeling of edge radiation at the soft X-ray FEL
facility FLASH and of the wavefront propagation through grazing incidence optics of the hard X-ray beamlines of the
European XFEL. Possible ways for parallelization of calculations are also discussed.
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A software system has been developed for high-performance Computed Tomography (CT) reconstruction, simulation
and other X-ray image processing tasks utilizing remote computer clusters optionally equipped with multiple Graphics
Processing Units (GPUs). The system has a streamlined Graphical User Interface for interaction with the cluster. Apart
from extensive functionality related to X-ray CT in plane-wave and cone-beam forms, the software includes multiple
functions for X-ray phase retrieval and simulation of phase-contrast imaging (propagation-based, analyzer crystal based
and Talbot interferometry). Other features include several methods for image deconvolution, simulation of various
phase-contrast microscopy modes (Zernike, Schlieren, Nomarski, dark-field, interferometry, etc.) and a large number of
conventional image processing operations (such as FFT, algebraic and geometrical transformations, pixel value
manipulations, simulated image noise, various filters, etc.). The architectural design of the system is described, as well as
the two-level parallelization of the most computationally-intensive modules utilizing both the multiple CPU cores and
multiple GPUs available in a local PC or a remote computer cluster. Finally, some results about the current system
performance are presented. This system can potentially serve as a basis for a flexible toolbox for X-ray image analysis
and simulation, that can efficiently utilize modern multi-processor hardware for advanced scientific computations.
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Penetration, micro-resolution, and scattering were the keywords of x-ray analyses in the 20th century. Over the last 15
years, a great class of coherent imaging techniques has emerged as new tools, allowing for low-dose imaging of biological
specimen on the nanoscale.
Apart from experimental and technical challenges, a better understanding of partially coherent beam propagation is the
key for exploiting the new methods' full performance. We present a simulation framework to calculate the mutual intensity
and the degree of spatial coherence of typical x-ray focusing and filtering devices used at 3rd generation synchrotron
radiation sources.
We propose the following modeling scheme: A set of independent point-sources yield independent basic fields, which
are superposed in a stochastic manner; by taking the ensemble average, both partially coherent intensity and degree of
coherence can be obtained from the mutual intensity. By including real structure effects, like height deviations of focusing
mirrors, and vibration of optical components, advanced predictions of x-ray beams can be made. This knowledge is
expected to improve reconstruction results from coherent imaging experiments.
Coherence simulations of focusing mirrors are presented and validated with analytical results as well as with experimental
tests. Coherence filtering by use of x-ray waveguides is shown numerically. We also present first simulations for
partially coherent focusing by compound refractive lenses.
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Polycapillary optics consist of hundreds of thousands of tiny hollow tubes that utilize total external reflection to redirect
x-rays incident at grazing angles. These optics have been developed for various applications, from beam filtering to x-ray
collimating or focusing. A fully three-dimensional Monte-Carlo-based ray-tracing simulation of polycapillary optics
has been developed to model a variety of optics geometries. Good agreement to experimental data was found with a
small number of fitting parameters.
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The software package PHASE includes routines for the propagation of coherent light within the stationary phase
approximation (SPA). The code is based on a nonlinear analytic transformation of electric field arrays across
longitudinally extended optical elements in normal and grazing-incidence geometries. Recently, the representation of the
optical elements (OEs) has been extended to 8th-order polynomials in the OE-coordinates. Strongly curved mirror
surfaces can be treated and systematic fabrication errors can be modeled up to 8th order. Each element is represented by
an individual matrix and the combination of several elements is accomplished by simple matrix multiplications. The
SPA-method can be interpreted as a thick lens approximation, whereas the Fourier Optics algorithm deals with thin
lenses. Both methods have advantages and disadvantages. Recently, the PHASE package has been extended to Fourier
Optics methods. The appropriate propagator or even a combination of different propagators can be selected from the
same interface, which is running under IDL. This permits a one-by-one comparison of both methods via the same
interface, which helps to evaluate the advantages and limitations of both methods.
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we present the developments of the McXtrace project, a free, open source software package based on Monte
Carlo ray tracing for simulations and optimisation of complete X-ray instruments.
The methodology of building a simulation is presented through an example beamline, namely Beamline 811
at MAX-lab, Lund, Sweden - a beamline dedicated to materials science.
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The X-ray emission of the HU52 Apple2 undulator of the SOLEIL DEIMOS (Dichroism Experimental Installation for
Magneto-Optical Spectroscopy) beamline is analyzed using the Bragg diffraction of a Si(111) crystal at various
undulator gaps in linear horizontal polarization. Measurements are compared with simulations in order to determine
undulator properties. The method allows also to get information on the electron beam.
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The coherent soft x-ray and full polarization control (CSX) beamline at the National Synchrotron Light Source -
II (NSLS-II) will deliver 1013 coherent photons per second in the energy range of 0.2-2 keV with a resolving power
of 2000. The source, a dual elliptically polarizing undulator (EPU), and beamline optics should be optimized to
deliver the highest possible coherent flux in a 10-30 μm spot for use in coherent scattering experiments. Using
the computer code Synchrotron Radiation Workshop (SRW), we simulate the photon source and focusing optics
in order to investigate the conditions which provide the highest usable coherent intensity on the sample. In
particular, we find that an intermediate phasing magnet is needed to correct for the relative phase between the
two EPUs and that the optimum phase setting produces a spectrum in which the desired wavelength is slightly
red-shifted thus requiring a larger aperture than originally anticipated. This setting is distinct from that which
produces an on-axis spectrum similar to a single long undulator. Furthermore, partial coherence calculations,
utilizing a multiple electron approach, indicate that a high degree of spatial coherence is still obtained at the
sample location when such an aperture is used. The aperture size which maximizes the signal-to-noise ratio
of a double-slit experiment is explored. This combination of high coherence and intensity is ideally suited for
x-ray ptychography experiments which reconstruct the scattering density from micro-diffraction patterns. This
technique is briefly reviewed and the effects on the image quality of proximity to the beamline focus are explored.
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Ultra-low emittance third-generation synchrotron radiation sources such as the NSLS-II offer excellent opportunities for
the development of experimental techniques exploiting x-ray coherence. Coherent light scattered by a heterogeneous
sample produces a speckle pattern characteristic for the specific arrangement of the scatterers. This may vary over time,
and the resultant intensity fluctuations can be measured and analyzed to provide information about the sample dynamics.
X-ray photon correlation spectroscopy (XPCS) extends the capability of dynamic light scattering to opaque and turbid
samples and extends the measurements of time evolution to nanometer length scales. As a consequence XPCS became
crucial in the study of dynamics in systems including, but not being limited to, colloids, polymers, complex fluids,
surfaces and interfaces, phase ordering alloys, etc. In this paper we present the conceptual optical design and the
theoretical performance of the Coherent Hard X-ray (CHX) beamline at NSLS-II, dedicated to XPCS and other coherent
scattering techniques. For the optical design of this beamline, there is a tradeoff between the coherence needed to
distinguish individual speckles and the phase acceptance (high intensity) required to measure fast dynamics with an
adequate signal-to-noise level. As XPCS is a "photon hungry" technique, the beamline optimization requires maximizing
the signal-to-noise ratio of the measured intensity-intensity autocorrelation function. The degree of coherence, as
measured by a two-slit (Young) experiment, is used to characterize the speckle pattern visibilities. The beamline
optimization strategy consists of maximization of the on-sample intensity while keeping the degree of coherence within
the 0.1-0.5 range. The resulted design deviates substantially from an ad-hoc modification of a hard x-ray beamline for
XPCS measurements. The CHX beamline will permit studies of complex systems and measurements of bulk dynamics
down to the microsecond time scales. In general, the 10-fold increase in brightness of the NSLS-II, compared to other
sources, will allow for measurements of dynamics on time-scales that are two orders of magnitude faster than what is
currently possible. We also conclude that the common approximations used in evaluating the transverse coherence
length would not be sufficiently accurate for the calculation of the coherent properties of an undulator-based beamline,
and a thorough beamline optimization at a low-emittance source such as the NSLS-II requires a realistic wave-front
propagation analysis.
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Convenience and cost often lead to synchrotron beamlines where the final bendable Kirkpatrick-Baez focusing pair must
relay the final image to different samples at different image distances e.g., [Proc. FEL2009, 246-249 (2009)] either for
different experimental chambers, or diagnostics. We present an initial analytical approach, starting from, and extending
the work of Howells et al. [OE 39(10), 2748-62 (2000)] to analyze the trade-offs between choice of mirror, bending
couples and the given, shaped sagittal width of the optic. Both experimentally and in simulation, we have found that
after an appropriate re-bending, sagittally shaped optics can perform with high quality at significantly different incidence
angles and conjugate distances. We present one successful demonstration from the ALS Optical Metrology Beamline
5.3.1, and review some new closed form analytical solutions with a view towards understanding our results.
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The Sub-micron Resolution X-ray spectroscopy (SRX) beamline will benefit from the ultralow emittance of the National
Synchrotron Light Source II to address a wide variety of scientific applications studying heterogeneous systems at the
sub-micrometer scale. This work focuses on the KB branch (ΔE: 4.65-28 keV). Its main optical components include a
horizontally focusing mirror forming an adjustable secondary source, a horizontally deflecting monochromator and two
sets of Kirkpatrick-Baez mirrors as focusing optics of two distinct inline stations for operations requiring either high flux
or high resolution. In the first approach, the beamline layout was optimized with ray-tracing calculations involving
Shadowvui computer codes. As a result, the location and characteristics of optics were specified for achieving either the
most intense or the smallest monochromatic beam possible on the target (1013 ph/s or 1012 ph/s respectively in a 500 nm
or 65 nm focal spot). At the nanoprobe station, the diffraction limited focusing of X-rays is governed by the beam
coherence. Hence, a classical geometric approach is not anymore adapted. To get reliable estimates of the Nanoprobe
performances, a wavefront propagation study was performed using Synchrotron Radiation Workshop (SRW) code. At
7.2 keV, calculations show an intense (1012 ph/s) 67 nm wide diffraction limited spot achieved with actual metrological
data of mirrors.
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The ray-tracing is power-full technique for the design and the prediction of the performances of an X-Ray optics. When
working with traditional monolithic shells, the possible design is quite constrained once fixed the focal length, the
dimensions of the module and the field of view: simulations are used to determine the effective area and optical
performances of realized mandrels and shells, taking into account for example profile errors or roundness measurements.
Instead, when the optics are segmented into two separate reflective surface, integration errors with respect to position
and rotation of the plates play an important role and may be also used to recover intrinsic plate errors. Moreover when
the mirror segments are produced by replica, it is possible to optimize the design of a module to be cost effective. In this
paper we present the design of a prototype module for the International X-ray Observatory (IXO) resulting from a
proprietary ray tracing code. The module will be composed by 20 plate pairs all made with the same integration forming
mandrel. The degradation of optical performances of the prototype are expected to be limited to few arc seconds.
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Numerical simulation of the performance of new beamlines and those under upgrade requires sophisticated and reliable
information about the expected surface slope and height distributions of planned x-ray optics before they are fabricated.
Obtaining such information should be based on the metrology data measured from existing mirrors that are made by the
same vendor and technology, but, generally, with different sizes, slope and height rms variations. In this work, we
demonstrate a method for highly reliable forecasting of the expected surface slope distributions of the prospective x-ray
optics. The method is based on an autoregressive moving average (ARMA) modeling of the slope measurements with a
limited number of parameters. With the found parameters of the ARMA model, the surface slope profile of an optic with
the newly desired specification can reliably be forecast. We demonstrate the high accuracy of this type of forecasting by
comparing the power spectral density distributions of the measured and forecast slope profiles.
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Systematic error and instrumental drift are the major limiting factors of sub-microradian slope metrology with state-of-the-art x-ray optics. Significant suppression of the errors can be achieved by using an optimal measurement strategy
suggested in [Rev. Sci. Instrum. 80, 115101 (2009)]. Here, we report on development of an automated, kinematic,
rotational system that provides fully controlled flipping, tilting, and shifting of a surface under test. The system is to be
integrated into the Advanced Light Source long trace profiler, LTP-II, allowing for complete realization of the
advantages of the optimal measurement strategy method. We describe in detail the system's specification, design
operational control and data acquisition. The performance of the system is demonstrated via the results of high precision
measurements with a number of super-polished mirrors.
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This paper present the advance in X-ray optics performances prediction achieved by means of a advantageous synergy
between the TraceIT ray-tracing code, capable to take into account the mirror shells shape error, and an opportune
mirror shells 3D metrology. The trend for future X-ray missions is to make use of optical modules working in grazing
incidence whose mirror shells are characterized by large diameters and small thickness. The floppiness of these mirrors
induces noticeable shape errors and a consequent degradation of the optical quality. It is hence crucial to have a
simulation tool capable to evaluate these errors impact on the mirror optical quality at the focal plane and, of course, a
metrological machine capable to characterize the shell 3D shape. The synergy between these two contributions,
accurate 3D mirror shells metrology and TraceIT ray-tracing, offers us the possibility to simulate the quality of an
optical surface within an uncertainty of 1 arcsec. This work shows the TraceIT code structure and its advantages, a
brief description of the adopted metrological machine and an example of their synergised applications: the evaluation
of the optical quality of a prototypal mirror shell and an estimation of the committed in this evaluation caused by the
metrological error.
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Ray tracing simulations are often performed for an ideal situation of perfect alignment, but it is usually necessary to
move optical components for various reasons. The mounts that hold these components can be complicated and modeling
their motion is vital to understanding how they affect the performance of the system. This paper examines the behaviour
of a six-strut kinematic mount using MapleSim to investigate and understand precisely how a mirror pole moves with its
mount and quantify any cross-coupled motion that may occur during actuator adjustments. This positional information
can be used to mitigate errors, improve ray tracing results, and assist in alignment.
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Theoretical analysis of high-energy-resolution x-ray optics, such as backscattering and four-bounce monochromators
and analyzers, has been carried out using computer modeling within the framework of the dynamical theory of x-ray
diffraction. This analysis identifies several important techniques for the precise alignment and determination of the
energy and bandwidth of the monochromators. The destructive contribution of multiple-wave diffraction to the scattering
intensity of x-ray backscattering optics has also been analyzed in details. An important method has been identified which
allows this destructive contribution to be avoided.
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A point-to-point x-ray focusing of a spherical wave by means of cylindrically bent crystal in symmetric Bragg back
diffraction geometry was investigated theoretically and simulated numerically. To separate the focal plane from an
incident x-ray beam, a thin flat crystal was introduced into the setup. The effect of flat crystal diffraction on the
focusing performance of the double crystal setup is discussed. It is shown that the aberration free focusing can be
achieved with aspherical surface shape of the strongly bent crystal. A correction term for the surface displacement
function free from spherical aberrations is derived. Thorough numerical simulations demonstrated agreement with
the theoretical analysis and excellent focusing performance of 2.4 nm. Theoretically, the demonstrated result can be
further improved almost by an order of magnitude.
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At XFEL sources, coherent and time-resolved experiments will strongly depend on the properties of the incoming
radiation passed through beamline optical elements to experimental stations. We investigate analytically and make
numerical modeling of SASE pulse propagation through optical transport systems of hard X-ray FEL beamlines. The
results on evolution of SASE XFEL pulses and its statistical properties during propagation through a double crystal
monochromator in Bragg and Laue diffraction geometry are presented.
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Recent advances in x-ray detection technology and diagnostic design have dramatically improved the ability
of using x-ray imaging and spectroscopic diagnostics to accurately measure important parameters in magnetically
confined and laser produced fusion plasmas. With these advancements, the detailed characterization
of the diagnostic system properties has become ever more important. We present an overview of current
and future x-ray diagnostic requirements for fusion plasmas and describe, in particular, diagnostic systems
employing spherically bent crystals to resolving characteristic x-ray lines from trace impurities with energies
in the range 1-20keV. The requirements and challenges for the simulation of existing and planned diagnostic
installations and are discussed.
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The diffraction of an X-ray wavefront from a slightly distorted crystal can be modeled by the Takagi-Taupin
theory, an extension of the well-known dynamical diffraction theory for perfect crystals. Maxwell's equations
applied to a perturbed periodic medium yield two coupled differential equations in the incident and diffracted
amplitude. These equations are discretized for numerical calculation into the determination of the two amplitudes
on the points of an integration mesh, beginning with the incident amplitudes at the crystal's top surface. The
result is a set of diffracted amplitudes on the top surface (in the Bragg geometry) or the bottom surface (in
the Laue geometry), forming a wavefront that in turn can be propagated through free space using the Fresnel-
Huygens equations. The performance of the Diamond Light Source I20 dispersive spectrometer has here been
simulated using this method. Methods are shown for transforming displacements calculated by finite element
analysis into local lattice distortions, and for efficiently performing 3-D linear interpolations from these onto the
Takagi-Taupin integration mesh, allowing this method to be extended to crystals under thermal load or novel
mechanical bender designs.
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The diffraction profiles (or rocking curves) of sagittally bent Laue crystals are known to be significantly wider
than those of perfect crystals as a result of the lattice distortion introduced by the sagittal bending. The existing
analytical model explains the rocking curve broadening as well as the reflectivity observed. Many theoretical
methods were developed for calculating diffraction profiles of meridionally (in the diffraction plane) bent crystals.
In this work, we extend these methods to accommodate sagittally bent crystals. The total lattice distortion
angle for anisotropic crystals under sagittal bending is adapted into the multi-lamellar approximation using the
rotating crystal method, in which the incident angle changes through each lamella. The Penning-Polder theory
is examined for bent crystals with the uniform strain gradient. In addition, the Takagi-Taupin equations are
solved numerically for sagittally bent Laue crystals. Finally, examples of these simulation results are presented
and the merit of each method is discussed.
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The open source Bmad software library, developed at Cornell University, has proved to be a useful tool for
accelerator simulations owing to its modular, object-oriented design. Bmad has been used to simulate the storage
ring CESR for many years, and to design and analyze the proposed Cornell Energy Recovery Linac. Work is
ongoing to expand Bmad in a number of directions. In particular, the ability to be able to do a combined
simulation of accelerated charged-particle beams and the x-ray beams they create is being developed. Ultimately
a complete framework for simulations from the gun cathode (including space-charge) to x-ray generation, to
x-ray tracking through to the experimental end-stations is envisioned. The flexibility of Bmad is such that
multiple propagation algorithms can be accommodated with the user selecting the appropriate algorithm for each
individual element. To this end, the integration of Bmad with the SHADOW tracking code is in development.
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A computer tool for the evaluation of the absorbed and re-scattered power from optical elements in a synchrotron
beamline has been written using the Monte Carlo package PENELOPE. A precise estimation of this power is
needed to assist in the design of the shielding inside the optical chambers that receive high power, like for the
Upgrade Programme at the ESRF. The results for scattered power calculation are presented for three cases i) a
Glidcop mirror for the SESAME Synchrotron, ii) a silicon crystal in use at the ESRF beamline ID06, and iii) a
Laue crystal for the new monochromator of the ESRF ID17 beamline.
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This work presents the recent developments of xraylib, an ANSI C library designed to provide convenient access
to a large number of X-ray related databases, with a focus on quantitative XRF applications. The discussed
enhancements include improved XRF production cross sections that take into account cascade effects and M-lines,
as well as revised line energies, atomic level widths, Compton broadening profiles etc. A full overview is
presented of the complete API.
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Compound refractive lenses (CRL) are widely used to manipulate synchrotron radiation beams. Accurate
modelling of X-ray beam propagation through individual lenses and through "transfocators" composed of a large
number of CRLs is of high importance, since it allows for comprehensive optimization of X-ray beamline designs
for particular user experiments.
In this work we used the newly developed McXtrace ray-tracing package and the SRW wave-optics code to
simulate the beam propagation of X-ray undulator radiation through such a "transfocator" as implemented at ID-
11 at ESRF. By applying two complementary simulation methods, we were able to obtain comparable results
(e.g. the beam's focused properties) and also to provide a complete description of X-ray beam propagation
through the CRLs and other optical components. However, some discrepancies between the results acquired by
both methods (e.g. broader monochromatization degree obtained with the McXtrace code) brought a meaningful
insight into further development strategies for the McXtrace package.
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We developed the third version of SHADOW, a ray tracing software widely used to design optical system in the synchrotron world. SHADOW3 is written in Fortran 2003 and follows the new computer engineering standards. The users can always execute the program in the traditional file oriented approach. Moreover, advanced users can create personalized scripts, macros and executables using the new Application Programming Interface SHADOW3-API. It also allows binding of SHADOW3 with several popular programming languages
such as C, C++, python and IDL. We describe the SHADOW3 API structure, and illustrate its use with some examples.
We analyze the possibilities of running SHADOW3 in parallel machines under different environments. A
version using the Open Message Parsing Interface has been implemented. A SHADOW3 postprocessor has been
accelerated with the use Graphics Processing Units. This will open new possibilities to extend the already very
popular ray tracing tool to applications simulating 2D and 3D experiments (like imaging, tomography)
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Optical design of hard x-ray beamlines can be accurately performed through ray tracing simulation technique. We
describe here the way and the tools we use at SOLEIL to develop hard x-ray beamlines such as PSICHÉ, which is a
wiggler beamline performing diffraction and tomography experiments from 20 to 50 keV. This beamline is made of two
focusing stages, one with a long vertical focusing mirror together with a sagittal focusing crystal monochromator to gain
a spot of 100x50 μm and the other one applying a set of graded multilayer KB mirrors to reach 10x10 μm spot. Ray
tracing simulations are performed with SpotX, which provides optical properties of the beamline taking into account
thermal load on optics, surface polishing defects from the profilometer measurements.
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The design of a synchrotron beamline is supported by various software simulation packages containing source
simulation, characterization of X-ray optics, ray-tracing simulation and others separately. Beamline designers and
operators often require instantly data of the beam parameter, which is only feasible with a unified and more user-friendly
software package. The new developed toolkit is a first step in that direction.
Photon flux, bandwidth, beam size and beam divergence are the chosen parameters used for the beamline design and
optimization. A tool was developed, which allows scanning these parameters by changing any input parameter, for
example the photon energy, the vertical mirror position or the horizontal slit size. A tabular input allows scanning with
arbitrary parameters or even different file names (e.g. filter material, surface profile).
We present two methods of calculating power density profiles on the optical components, one by ray-tracing and the
other by transmission calculation using the DABAX library. The second method only considers flat optics, but is a
good approximation and faster than the method based on ray-tracing.
The validation of the developed tools is shown by a comparison of the simulated beam parameters and the measured
ones, which was performed at the Crystallography Beamline (MX2) recently turned into operation at the Brazilian
Synchrotron Light Source (LNLS). We report also the capability of the parameterized scanning method for the alignment
of the optics during the commissioning phase of the beamlines.
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XOP v2.4 consists of a collection of computer programs for calculation of radiation characteristics of X-ray sources and
their interaction with matter. Many of the programs calculate radiation from undulators and wigglers, but others, such as
X-ray tube codes, are also available. The computation of the index of refraction and attenuation coefficients of optical
elements using user-selectable databases containing optical constants is an important part of the package for calculation
of beam propagation. Coupled computations are thus feasible where the output from one program serves as the input to
another program. Recent developments including enhancements to existing programs are described.
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We present the conceptual design of a dispersive X-ray Absorption Fine Structure (XAFS) beamline for MIRRORCLE,
a new compact laboratory X-ray source. This machine accelerates electrons up to 1,4,6 or 20MeV
(depending upon the model) in a ring and produces X-rays when the electrons collide onto a thin target. The
radiation emitted has a white spectrum due to both synchrotron and bremsstrahlung emission. A substantial
part of the electrons are recovered after collisions, and the emitted light has high flux, wide energy spectrum
and a large angular dispersion.
We have opted for a simple beamline design using a collimator, slits, a curved crystal, the sample environment
and a CCD. The beamline parameters (position of the mirror, ray of curvature, slit aperture, reflecting angle, etc.)
have been optimized by defining and improving a figure of merit. This optimization allows for room constraints
(distances among elements), mechanical constraints (minimum curvature radii available) and optical constraints.
Further ray tracing simulations using SHADOW3 have been performed to check all the theoretical results, refine
the final parameters, quantitative flux calculations and for simulating the image on the CCD camera.
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