Energy Absorption and Integral Dose in X-Ray and Radium Therapy: A Review

Radiology ◽  
1946 ◽  
Vol 47 (3) ◽  
pp. 263-278 ◽  
Author(s):  
C. W. Wilson
1997 ◽  
Vol 82 (6) ◽  
pp. 2742-2753 ◽  
Author(s):  
T. H. V. T. Dias ◽  
J. M. F. dos Santos ◽  
P. J. B. M. Rachinhas ◽  
F. P. Santos ◽  
C. A. N. Conde ◽  
...  

Radiology ◽  
1925 ◽  
Vol 4 (5) ◽  
pp. 384-389
Author(s):  
R. R. Wahl
Keyword(s):  
X Ray ◽  

2018 ◽  
Vol 185 (1) ◽  
pp. 27-33
Author(s):  
Katharina Bairlein ◽  
Oliver Hupe

Abstract In Report No. 90 of the International Commission on Radiation Units and Measurements (ICRU), new mass energy-absorption coefficients are listed which are based on renormalized Scofield photoeffect cross-sections. The mass energy-absorption coefficients are the basis for the conversion coefficients from air kerma to the operational quantities listed in ISO 4037-3. Although ICRU does not give a recommendation if these new mass energy-absorption coefficients should be applied instead of the values used so far, an examination of the possible consequences for radiation protection quantities is necessary. We calculated the conversion coefficients for the X-ray qualities specified in ISO 4037-1 with the new mass energy-absorption coefficients and with the mass energy-absorption coefficients used so far to determine the deviations. Our calculations show that the change of the conversion coefficients due to the new values from ICRU Report No. 90 is negligible.


1915 ◽  
Vol 19 (12) ◽  
pp. 445-445
Author(s):  
Robert Knox
Keyword(s):  
X Ray ◽  

1987 ◽  
Vol 93 ◽  
pp. 281-292
Author(s):  
W. Pietsch ◽  
W. Voges ◽  
E. Kendziorra ◽  
M. Pakull

AbstractThe 805 sec pulsing X-ray source H2252−035 has been observed for 7 h on September 14/15 and on September 17, 1983 in X-rays with the low energy telescope and the medium energy detectors of EXOSAT. While below 2 keV the semiamplitude of the 805 s pulses is ~ 100% in the 2.3–7.9 keV band it is only ~ 40%. X-ray dips that are more pronounced in low energies occur simultaneously with the orbital minimum of the optical light curve. The medium energy spectra during dips with respect to the non dip spectrum can be explained by just enhanced cold gas absorption of an additional absorbing column of 2 1022 cm−2. Model spectra for the 805 s minimum have to include a strong iron emission line at 6.55 keV with an equivalent width of 3 keV in addition to a reduced continuum intensity (radiating area) and enhanced low energy absorption.


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