Correction and verification of x-ray imaging crystal spectrometer analysis on Wendelstein 7-X through x-ray ray tracing

2021 ◽  
Vol 92 (4) ◽  
pp. 043530
Author(s):  
N. A. Pablant ◽  
A. Langenberg ◽  
J. A. Alonso ◽  
M. Bitter ◽  
S. A. Bozhenkov ◽  
...  
2016 ◽  
Vol 87 (11) ◽  
pp. 11E318 ◽  
Author(s):  
W. Yan ◽  
Z. Y. Chen ◽  
W. Jin ◽  
S. G. Lee ◽  
Y. J. Shi ◽  
...  

2021 ◽  
Vol 54 (2) ◽  
pp. 409-426
Author(s):  
Peng Qi ◽  
Xianbo Shi ◽  
Nazanin Samadi ◽  
Dean Chapman

X-ray Laue-type monochromators are common and essential optical components at many high-power X-ray facilities, e.g. synchrotron facilities. The X-ray optics of bent Laue crystals is a well developed area. An incident X-ray beam penetrating a bent Laue crystal will result in a diffracted beam with different angles and energies. There is a need for a way of organizing the rays that allows one to sort out the energy and spatial properties of the diffracted beam. The present work introduces a new approach for describing the general behaviour of bent Laue crystals from a ray-tracing point of view. This quasi-monochromatic beam approach provides an intuitive view of bent-crystal diffraction and leads to deeper understanding. It explains the energy and spatial properties of common and special cases of bent Laue optics, predicts phenomena that can improve energy-dispersion-related X-ray imaging techniques and provides a theoretical framework that makes ray-tracing simulation easier to realize.


2008 ◽  
Author(s):  
S. G. Lee ◽  
J. G. Bak ◽  
M. G. Bog ◽  
U. W. Nam ◽  
M. K. Moon ◽  
...  

2012 ◽  
Vol 83 (8) ◽  
pp. 083506 ◽  
Author(s):  
N. A. Pablant ◽  
M. Bitter ◽  
L. Delgado-Aparicio ◽  
M. Goto ◽  
K. W. Hill ◽  
...  

The satellite Hinotori was launched in 1981 by the Institute of Space and Astronautical Science of Japan. Two major experiments on board the Hinotori satellite were a hard X-ray imaging telescope with modulation collimators, and a high dispersion soft X-ray crystal spectrometer utilizing the Bragg diffraction of X-rays on quartz crystals. These two instruments have revealed for the first time that solar flares show varying characteristics depending on the environment of flaring regions, and that flares produce plasmas as hot as 3-4 x 10 7 K.


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