The American Standard Safety Standard for Non-medical X-ray and Sealed Gamma-Ray Sources. Part IThe American Standard Safety Standard for Non-medical X-ray and Sealed Gamma-Ray Sources. PartI. General Z54.1-1963. National Bureau of Standards Handbook 93. Available from the Superintendent of Documents, Government Printing Office, Washington, D. C. 20402, 1963. Price 30 cents.

Radiology ◽  
1964 ◽  
Vol 82 (6) ◽  
pp. 1076-1076
1963 ◽  
Vol 7 ◽  
pp. 584-589
Author(s):  
M. C. Farquhar ◽  
M. M. English

AbstractA method is presented for the quantitative determination of thorium in monazite by fluorescent X-ray speetrometry. Strontium is used as an internal standard, and sample preparation consists of mechanically blending the finelyground (325-mesh) sample with reagent grade strontium carbonate. The prepared sample blend is packed into a sample cup and irradiated at 50 kV and 27 mA. A lithium fluoride analyzing crystal is used, and the intensity of the Th Lα1 and Sr Kα peaks are scaled. Intensities are corrected fov background. Calibration is achieved with a single sample of monazite of known thorium content. National Bureau of Standards monazite sample number 2601 (9.65% ThO2) was used in this work. The standard monazite is blended with strontium carbonate, irradiated, and scaled under the same conditions as the sample. The thorium content of the sample is then calculated by the equation: %ThO2 = (R sample) (%ThO2 standard)/R standard, where R = Thcounts/sec/Srcounts/sec. Replicate results agreed within 0.2% ThO2 on six samples of monazite which contained from 4.4% to 6.8% ThO2. Independent results by a second laboratory show no significant difference in precision.The method was used to determine the thorium content gf several rare-earth materials which contained approximately 0.5% to 1.0% TriOs. The results agree closely with values obtained by gamma-ray spectrometry.


1987 ◽  
Vol 48 (C9) ◽  
pp. C9-367-C9-370
Author(s):  
C. B. COLLINS ◽  
F. DAVANLOO ◽  
T. S. BOWEN ◽  
J. J. COOGAN
Keyword(s):  

2003 ◽  
Vol 8 (5-6) ◽  
pp. 60-64
Author(s):  
A.I. Arkhangelsky ◽  
◽  
Yu.D. Kotov ◽  
P.Yu. Chistiakov ◽  
◽  
...  

1998 ◽  
Vol 502 (1) ◽  
pp. 428-436 ◽  
Author(s):  
Igor V. Moskalenko ◽  
Werner Collmar ◽  
Volker Schonfelder

1996 ◽  
Vol 165 ◽  
pp. 313-319
Author(s):  
Mark H. Finger ◽  
Robert B. Wilson ◽  
B. Alan Harmon ◽  
William S. Paciesas

A “giant” outburst of A 0535+262, a transient X-ray binary pulsar, was observed in 1994 February and March with the Burst and Transient Source Experiment (BATSE) onboard the Compton Gamma-Ray Observatory. During the outburst power spectra of the hard X-ray flux contained a QPO-like component with a FWHM of approximately 50% of its center frequency. Over the course of the outburst the center frequency rose smoothly from 35 mHz to 70 mHz and then fell to below 40 mHz. We compare this QPO frequency with the neutron star spin-up rate, and discuss the observed correlation in terms of the beat frequency and Keplerian frequency QPO models in conjunction with the Ghosh-Lamb accretion torque model.


2021 ◽  
Vol 366 (4) ◽  
Author(s):  
Zhi-Ying Liu ◽  
Fu-Wen Zhang ◽  
Si-Yuan Zhu

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