A New Technique of X-Ray Diffraction Microscopy of Scanning Type

1967 ◽  
Vol 6 (12) ◽  
pp. 1393-1396
Author(s):  
Seigô Kishino ◽  
Yoshimitsu Sugita ◽  
Kazutake Kohra
1963 ◽  
Vol 7 ◽  
pp. 209-228 ◽  
Author(s):  
Douglas B. Nash

AbstractResults of an experimental X-ray study on 96 synthetic glasses show that the 2θ positions of glass diffraction maxima have an inverse relation to SiO2 concentration in silicate glasses. This relationship is the basis of a new technique for semiquantitative determinations of SiOa in silicate materials by X-ray diffraction methods. Samples to be examined are fused and the resulting glass scanned from 12 to 40° 2θ using CiiKa radiation. The mean 2θ position of the diffraction maximum is a measure of the SiOs content of the glass. Calibration curves for both weight and molecular percent SiO2 vs. 2θ are presented in this report. The technique requires only small, unweighed amounts of sample for analysis ; it is simple, rapid, and utilizes standard diffraction equipment without modification. Its accuracy, at present, allows SiOa determinations to within ±1 to 4% of the actual concentration.


1992 ◽  
Vol 70 (5) ◽  
pp. 319-321
Author(s):  
G. Leclerc ◽  
J. Beerens ◽  
C. Aktik ◽  
L. Paquin ◽  
M. Isai

We report here a new technique for evaporating polycrystalline InSb films, using hydrogen beams as carriers for each elemental source. The films obtained show X-ray diffraction patterns before annealing that are totally exempt from impurity peaks, unlike those other workers have previously reported for evaporated InSb.


1993 ◽  
Vol 49 (s1) ◽  
pp. c10-c10
Author(s):  
G. N. Greaves ◽  
A. J. Dent ◽  
B. R. Dobson ◽  
S. M. Clark ◽  
C. A. Ramsdale ◽  
...  

1995 ◽  
Vol 66 (2) ◽  
pp. 1419-1421 ◽  
Author(s):  
S. Kojima ◽  
Y. Kudo ◽  
S. Kawado ◽  
T. Ishikawa ◽  
T. Matsushita

1993 ◽  
Author(s):  
Robert Austin ◽  
Takahisa Minamitani ◽  
Brian Ramsey
Keyword(s):  
X Ray ◽  

2015 ◽  
Vol 1 (9) ◽  
pp. e1500578 ◽  
Author(s):  
Wynn C. G. Ho ◽  
Cristóbal M. Espinoza ◽  
Danai Antonopoulou ◽  
Nils Andersson

Pulsars are known for their superb timing precision, although glitches can interrupt the regular timing behavior when the stars are young. These glitches are thought to be caused by interactions between normal and superfluid matter in the crust of the star. However, glitching pulsars such as Vela have been shown to require a superfluid reservoir that greatly exceeds that available in the crust. We examine a model in which glitches tap the superfluid in the core. We test a variety of theoretical superfluid models against the most recent glitch data and find that only one model can successfully explain up to 45 years of observational data. We develop a new technique for combining radio and x-ray data to measure pulsar masses, thereby demonstrating how current and future telescopes can probe fundamental physics such as superfluidity near nuclear saturation.


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