scholarly journals High spatial resolution inorganic scintillator detector for high‐energy X‐ray beam at small field irradiation

2020 ◽  
Vol 47 (3) ◽  
pp. 1364-1371
Author(s):  
Sree Bash Chandra Debnath ◽  
Carole Fauquet ◽  
Agnes Tallet ◽  
Anthony Goncalves ◽  
Sébastien Lavandier ◽  
...  

2013 ◽  
Vol 425 (6) ◽  
pp. 062012
Author(s):  
Robin M Baur ◽  
Mark W Tate ◽  
Darren S Dale ◽  
Sol M Gruner


2012 ◽  
Vol 706-709 ◽  
pp. 1661-1666
Author(s):  
Abdelilah Benmarouane ◽  
Pierre Millet ◽  
Thomas Buslaps ◽  
Alain Lodini ◽  
Veijo Honkimäki

The aim of the present study was to study the interface implant-bone by synchrotron radiation, the implant has two faces the first one coated with hydroxyapatite and the second uncoated. In orthopaedic surgery, Titanium (Ti-Al-4V) implants are currently coated with hydroxyapatite (HAp), Ca10(PO4)6(OH)2, in order to obtain a stable and functional direct connection between the bone and the implant. At the implant-bone interface, the new bone reconstituted after two months of implantation must have the same properties like the natural bone in order to accept the implant. Therefore we studied the texture of the reconstituted bone crystals at the interface applying non destructive x-ray diffraction. The required high spatial resolution was achieved utilizing high-energy synchrotron radiation on ID15 at ESRF in Grenoble, France.



2014 ◽  
Vol 86 (21) ◽  
pp. 10892-10899 ◽  
Author(s):  
Francesco Paolo Romano ◽  
Claudia Caliri ◽  
Luigi Cosentino ◽  
Santo Gammino ◽  
Lorenzo Giuntini ◽  
...  


1971 ◽  
Vol 41 ◽  
pp. 134-134
Author(s):  
Albert G. Opp ◽  
Nancy G. Roman

High energy astrophysical observations supported by the National Aeronautics and Space Administration will be conducted primarily from the Small Astronomy Satellites (SAS) and the High Energy Astronomy Observatories (HEAO). At the present time, three Small Astronomy Satellites have been approved for flight. The first (SAS A) will carry a set of collimated proportional counters to conduct a high sensitivity, high spatial resolution, all sky survey for X-ray sources, to search for temporal variations in the source intensity, and to measure the spectral distribution of sources in the energy range 1 to 20 keV. The spacecraft will carry two collimator systems of 1 by 10 deg and 10 by 10 deg fullwidth. The proportional counters are gas-filled beryllium window tubes. SAS A is planned for launch in late 1970.



2013 ◽  
Vol 86 ◽  
pp. 60-65 ◽  
Author(s):  
F.P. Romano ◽  
C. Altana ◽  
L. Cosentino ◽  
L. Celona ◽  
S. Gammino ◽  
...  


2012 ◽  
Vol 111 (8) ◽  
pp. 084904 ◽  
Author(s):  
Amrinder S. Gill ◽  
Zhong Zhou ◽  
Ulrich Lienert ◽  
Jonathan Almer ◽  
David F. Lahrman ◽  
...  


2015 ◽  
Vol 22 (4) ◽  
pp. 043114 ◽  
Author(s):  
C. M. Huntington ◽  
H.-S. Park ◽  
B. R. Maddox ◽  
M. A. Barrios ◽  
R. Benedetti ◽  
...  




2003 ◽  
Vol 104 ◽  
pp. 247-250
Author(s):  
T. Bigault ◽  
E. Ziegler ◽  
Ch. Morawe ◽  
W. Ludwig ◽  
R. Soufli


Radiology ◽  
2015 ◽  
Vol 275 (1) ◽  
pp. 310-310 ◽  
Author(s):  
Richard M. Morris ◽  
Lang Yang ◽  
Miguel A. Martín-Fernández ◽  
Jose M. Pozo ◽  
Alejandro F. Frangi ◽  
...  


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