Beamline BL-07 at Indus-2: a facility for microfabrication research

2013 ◽  
Vol 21 (1) ◽  
pp. 259-263 ◽  
Author(s):  
V. P. Dhamgaye ◽  
G. S. Lodha ◽  
B. Gowri Sankar ◽  
C. Kant
Keyword(s):  
Stainless Steel ◽  
Energy Spectrum ◽  
X Rays ◽  
Spectral Bandwidth ◽  
Modes Of Operation ◽  
X Ray ◽  
Honeycomb Structures ◽  
Stencil Mask ◽  
And Performance

The X-ray lithography beamline on Indus-2 is now operational, with two modes of operation. With a pair of X-ray mirrors it is possible to tune the energy spectrum between 1 and 20 keV with a controlled spectral bandwidth. In its `no optics' mode, hard X-rays up to 40 keV are available. Features and performance of the beamline are presented along with some example structures. Structures fabricated include honeycomb structures in PMMA using a stainless steel stencil mask and a compound refractive X-ray lens using a polyimide–gold mask in SU-8.

scholarly journals Spectral Tomography for 3D Element Detection and Mineral Analysis

Minerals ◽  
2021 ◽  
Vol 11 (6) ◽  
pp. 598
Author(s):  
Jose R. A. Godinho ◽  
Gabriel Westaway-Heaven ◽  
Marijn A. Boone ◽  
Axel D. Renno
Keyword(s):  
Energy Spectrum ◽  
3D Imaging ◽  
X Rays ◽  
3D Images ◽  
Characterization Methods ◽  
X Ray ◽  
Additional Information ◽  
Mineral Phases ◽  
Spectral Computed Tomography

This paper demonstrates the potential of a new 3D imaging technique, Spectral Computed Tomography (sp-CT), to identify heavy elements inside materials, which can be used to classify mineral phases. The method combines the total X-ray transmission measured by a normal polychromatic X-ray detector, and the transmitted X-ray energy spectrum measured by a detector that discriminates between X-rays with energies of about 1.1 keV resolution. An analysis of the energy spectrum allows to identify sudden changes of transmission at K-edge energies that are specific of each element. The additional information about the elements in a phase improves the classification of mineral phases from grey-scale 3D images that would be otherwise difficult due to artefacts or the lack of contrast between phases. The ability to identify the elements inside the minerals that compose ore particles and rocks is crucial to broaden the application of 3D imaging in Earth sciences research and mineral process engineering, which will represent an important complement to traditional 2D imaging mineral characterization methods. In this paper, the first applications of sp-CT to classify mineral phases are showcased and the limitations and further developments are discussed.

A multi-length-scale USAXS/SAXS facility: 10–50 keV small-angle X-ray scattering instrument

2013 ◽  
Vol 46 (5) ◽  
pp. 1508-1512 ◽  
Author(s):  
Byron Freelon ◽  
Kamlesh Suthar ◽  
Jan Ilavsky
Keyword(s):  
Small Angle ◽  
Soft Matter ◽  
High Energy ◽  
X Rays ◽  
X Ray ◽  
X Ray Scattering ◽  
Wide Range ◽  
And Performance ◽  
New Facility ◽  
Ray Scattering

Coupling small-angle X-ray scattering (SAXS) and ultra-small-angle X-ray scattering (USAXS) provides a powerful system of techniques for determining the structural organization of nanostructured materials that exhibit a wide range of characteristic length scales. A new facility that combines high-energy (HE) SAXS and USAXS has been developed at the Advanced Photon Source (APS). The application of X-rays across a range of energies, from 10 to 50 keV, offers opportunities to probe structural behavior at the nano- and microscale. An X-ray setup that can characterize both soft matter or hard matter and high-Zsamples in the solid or solution forms is described. Recent upgrades to the Sector 15ID beamline allow an extension of the X-ray energy range and improved beam intensity. The function and performance of the dedicated USAXS/HE-SAXS ChemMatCARS-APS facility is described.

scholarly journals Design and Performance of the X-ray Polarimeter X-Calibur

2014 ◽  
Vol 03 (02) ◽  
pp. 1440008 ◽  
Author(s):  
M. Beilicke ◽  
F. Kislat ◽  
A. Zajczyk ◽  
Q. Guo ◽  
R. Endsley ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Detection Efficiency ◽  
Grazing Incidence ◽  
High Energy ◽  
X Rays ◽  
Field Orientation ◽  
Synchrotron Source ◽  
X Ray ◽  
And Performance ◽  
Detector Assembly

X-ray polarimetry promises to give qualitatively new information about high-energy astrophysical sources, such as binary black hole systems, micro-quasars, active galactic nuclei, neutron stars, and gamma-ray bursts. We designed, built and tested a X-ray polarimeter, X-Calibur, to be used in the focal plane of the balloon-borne InFOCμS grazing incidence X-ray telescope. X-Calibur combines a low-Z scatterer with a Cadmium Zinc Telluride (CZT) detector assembly to measure the polarization of 20–80 keV X-rays making use of the fact that polarized photons scatter preferentially perpendicular to the electric field orientation. X-Calibur achieves a high detection efficiency of ≃80%. The X-Calibur detector assembly is completed, tested, and fully calibrated. The response to a polarized X-ray beam was measured successfully at the Cornell High Energy Synchrotron Source. This paper describes the design, calibration and performance of the X-Calibur polarimeter. In principle, a similar space-borne scattering polarimeter could operate over the broader 2–100 keV energy band.

scholarly journals Simultaneous measurements of X-rays and electrons during a pulsating aurora

1998 ◽  
Vol 16 (2) ◽  
pp. 148-160 ◽  
Author(s):  
N. Østgaard ◽  
J. Stadsnes ◽  
K. Aarsnes ◽  
F. Søraas ◽  
K. Måseide ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Energy Range ◽  
Energetic Particle ◽  
Good Method ◽  
Electron Energy Spectrum ◽  
Electron Precipitation ◽  
X Rays ◽  
X Ray ◽  
Electron Spectra ◽  
Simultaneous Measurements

Abstract. The PULSAUR II rocket was launched from Andøya Rocket Range at 23.43 UT on 9 February 1994 into a pulsating aurora. In this paper we focus on the observations of precipitating electrons and auroral X-rays. By using models it is possible to deduce the electron energy spectrum from X-ray measurements. Comparisons are made between the deduced electron fluxes and the directly measured electron fluxes on the rocket. We found the shape of the observed and the deduced electron spectra to fit very well, with almost identical e-folding energies in the energy range from 10 ke V to ~60–80 ke V. For the integrated fluxes from 10.8 to 250 ke V, we found a discrepancy of 30% . By combining two models, we have found a good method of deducing the electron precipitation from X-ray measurements. The discrepancies between calculations and measurements are in the range of the uncertainties in the measurements.Key words. Ionospheric particle precipitation · Magnetospheric physics · Annual phenomena · Energetic particle

scholarly journals NEEDLE DETECTOR OF X-RAY AND GAMMA RADIATION

2017 ◽  
Vol 7 (1) ◽  
pp. 121-124
Author(s):  
Grzegorz Domański ◽  
Roman Szabatin ◽  
Piotr Brzeski ◽  
Bogumił Konarzewski
Keyword(s):  
Energy Spectrum ◽  
Gamma Radiation ◽  
Gamma Rays ◽  
Proportional Counter ◽  
Incident Radiation ◽  
X Rays ◽  
The Novel ◽  
Direction Parallel ◽  
X Ray ◽  
Gas Detector

The article presents the developed structure of the novel needle proportional gas detector (NPC – Needle Proportional Counter) used for the detection of X-rays and gamma rays. The advantage of the detector is its simple mechanical construction and the possibility of detection of incident radiation in a direction parallel to the needle. The measured energy spectrum of the isotope Fe-55 by means of the developed detector is presented.

scholarly journals Unveiling the Multi-wavelength Phenomenology of Anomalous X-ray Pulsars

2004 ◽  
Vol 218 ◽  
pp. 247-250 ◽  
Author(s):  
GianLuca Israel ◽  
Luigi Stella ◽  
Stefano Covino ◽  
Sergio Campana ◽  
Lorella Angelini ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Broad Band ◽  
Archival Data ◽  
X Rays ◽  
Spectral Variability ◽  
Band Energy ◽  
X Ray ◽  
Pulse Phase ◽  
Multi Wavelength ◽  
Ir Bands

During 2002–2003 the number of IR-identified counterparts to the Anomalous X-ray Pulsars (AXPs) has grown to four (4U 0142+61, IE 2259+586, IE 1048.1−5937 and RXS J170849−400910) out of the six objects (plus two candidates) known in this class. More importantly, some new common characteristics have been identified, such as IR variability, IR flattening in the broad-band energy spectrum, X-ray spectral variability as a function of pulse phase (which are not predicted by the magnetar model), and X-ray bursts (which cannot be explained in terms of standard accretion models). We present the results obtained from an extensive multi-wavelength observational campaign carried out with the NTT and CFHT for the optical/IR bands, and XMM and Chandra (plus BeppoSAX archival data) in X-rays. Based on these results and those reported in the literature, the IR-to-X-ray emission of AXPs is compared.

A Spherically Bent Crystal X-Ray Specteometer with Variable Curvature

1973 ◽  
Vol 17 ◽  
pp. 521-530
Author(s):  
Donald L. Parker
Keyword(s):  
Signal To Noise Ratio ◽  
Three Dimensional ◽  
High Signal ◽  
X Rays ◽  
X Ray ◽  
Bent Crystal ◽  
Variable Curvature ◽  
The Face ◽  
Low Levels ◽  
And Performance

AbstractThe design and performance of a spherically bent crystal x-ray spectrometer with variable curvature are given. A thin crystal with the diffracting planes parallel to the face is mounted on a vacuum chuck consisting of an O-ring in a brass mounting. A controlled partial vacuum is applied behind the crystal to cause spherical deformation of the lattice. Thus, rays from a point source on the focusing circle are diffracted to a line image also on the focusing circle. The differential pressure is automatically varied such that the source-to-crystal and crystal-to-image distances are equal and constant for all Bragg angles and hence the simple θ-2θ motion of a one flat crystal spectrometer is used.The data are accumulated by a scanning proportional counter tube placed behind a vertical slit (perpendicular to the scattering plane) located at the image line. The fixed chord length is 22 cm and the instrument is designed to scan from zero up to 120° 2θ. Crystals are easily interchanged and the automatic vacuum regulator has sufficient flexibility to allow tailoring the spherical bending to crystals of materials of various thicknesses. The resolution is easily adjusted by either the size of the x-ray source or the width of the detector slit. The performance of the spectrometer has been evaluated by characteristic x-rays produced by various samples placed in a demountable x-ray tube. The main advantages of this three-dimensional focusing instrument are the very high signal-to-noise ratio and the very low levels of x-ray flux required.

scholarly journals Single-crystal diamond refractive lens for focusing X-rays in two dimensions

2016 ◽  
Vol 23 (1) ◽  
pp. 163-168 ◽  
Author(s):  
S. Antipov ◽  
S. V. Baryshev ◽  
J. E. Butler ◽  
O. Antipova ◽  
Z. Liu ◽  
...  
Keyword(s):  
Single Crystal ◽  
Fresnel Zone ◽  
Two Dimensions ◽  
X Rays ◽  
Fresnel Zone Plates ◽  
X Ray ◽  
Femtosecond Laser Micromachining ◽  
Single Crystal Diamond ◽  
Refractive Lens ◽  
And Performance

The fabrication and performance evaluation of single-crystal diamond refractive X-ray lenses of which the surfaces are paraboloids of revolution for focusing X-rays in two dimensions simultaneously are reported. The lenses were manufactured using a femtosecond laser micromachining process and tested using X-ray synchrotron radiation. Such lenses were stacked together to form a standard compound refractive lens (CRL). Owing to the superior physical properties of the material, diamond CRLs could become indispensable wavefront-preserving primary focusing optics for X-ray free-electron lasers and the next-generation synchrotron storage rings. They can be used for highly efficient refocusing of the extremely bright X-ray sources for secondary optical schemes with limited aperture such as nanofocusing Fresnel zone plates and multilayer Laue lenses.

Observations of SN 1987A from Ginga

1988 ◽  
Vol 7 (4) ◽  
pp. 479-485
Author(s):  
H. Inoue
Keyword(s):  
Energy Spectrum ◽  
Time Variable ◽  
Soft Component ◽  
X Rays ◽  
Hard Component ◽  
X Ray ◽  
Sn 1987A

AbstractResults of the observations of SN 1987A from Ginga are presented. The first detection of X-rays from the SN 1987A was July, 1987. The energy spectrum is quite unnusual for any of the known classes of X-ray sources, and apparently consists of two seperate components; a soft and a hard component. The soft component is significantly time-variable, and also showed a flarelike increase in January, 1988. Whereas, the intensity of the hard component has remained fairly stationary for more than 300 days. The origins of the two components are also discussed.

scholarly journals Laser Larmor X-ray radiation from low-Z matter

1999 ◽  
Vol 17 (1) ◽  
pp. 45-58 ◽  
Author(s):  
YUTAKA UESHIMA ◽  
YASUAKI KISHIMOTO ◽  
AKIRA SASAKI ◽  
TOSHIKI TAJIMA
Keyword(s):  
Energy Spectrum ◽  
Laser Pulse ◽  
Electromagnetic Fields ◽  
Short Pulse ◽  
Intense Laser ◽  
X Rays ◽  
Bremsstrahlung Radiation ◽  
Pulse Laser Irradiation ◽  
X Ray ◽  
Short Pulse Laser

A relativistically intense short laser pulse can produce a large flux of X rays through the interaction with electrons that are driven by its intense electromagnetic fields. Apart from X rays from the high-Z matter irradiation by an intense laser, two main processes, Larmor and Bremsstrahlung radiation, are among the most significant mechanisms for X-ray emission from short-pulse laser irradiation on low-Z matter in the regime of relativistic intensities. We evaluate the power, energy spectrum, brilliance, polarization, and time structure of these X rays. We suggest a few methods that significantly enhance the power of Larmor X rays. Because of the peakedness in the energy spectrum of Larmor X rays, Larmor X rays have important applications.

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