The determination of the neutron component of cosmic radiation fields in spacecraft

2003 ◽  
Vol 36 (1-6) ◽  
pp. 439-443 ◽  
Author(s):  
D.T. Bartlett ◽  
L.G. Hager ◽  
R.J. Tanner
2020 ◽  
Vol 188 (3) ◽  
pp. 383-388
Author(s):  
L Oster ◽  
I Eliyahu ◽  
Y S Horowitz ◽  
G Reshes ◽  
A Shapiro ◽  
...  

Abstract The results reported herein demonstrate the potential application of combined optically stimulated luminescence/thermoluminescent (OSL/TL) measurements in neutron-gamma discrimination dosimetry. The advantages of OSL/TL are two-fold: (i) The OSL and TL readout can be carried out on the same sample and (ii) the greater efficiency of OSL to high ionization density radiation due to F 2 and F3 excitation. The gamma/electron calibration coefficients for LiF:Mg, Ti (TLD-600 and TLD-700) were measured using a 90Sr/90Y source calibrated at the SARAF-SSDL nuclear facility. The estimation of the neutron calibration coefficients was carried out by irradiation with broad-spectrum beam of fast neutrons with median energy 5 MeV at the Radiological Research Accelerator Facility (RARAF) of Columbia University. Naturally cooled samples of TLD-600 and TLD-700 were dosed to levels of 29.8 Gy neutrons and 6.1 Gy gammas in air and KERMA calculations employed to transfer the levels of dose to6,7LiF. A figure of merit for fast-neutron/gamma ray discrimination was determined at 10.6 for TLD-700 in the current measurements. The use of combined TLD-600/TLD-700 allowed, as well, the determination of a considerable and somewhat unexpected thermal neutron component of 116 Gy in TLD-600.


1947 ◽  
Vol 71 (7) ◽  
pp. 393-398 ◽  
Author(s):  
M. S. Vallarta ◽  
M. L. Perusquía ◽  
J. de Oyarzábal

2019 ◽  
Vol 52 (5) ◽  
pp. 320-325
Author(s):  
A. A. Lychagin ◽  
L. N. Ulyanenko ◽  
S. N. Koryakin ◽  
M. V. Troshina ◽  
S. E. Ulyanenko

1962 ◽  
Vol 40 (3) ◽  
pp. 348-351 ◽  
Author(s):  
R. P. Bukata ◽  
F. K. Chin ◽  
S. Standil

A large crystal total absorption spectrometer has been used to obtain a value of (−.62 ±.05)% per nib for photons above 7 Mev and (−.86 ±.20)% per nib for photons above 35 Mev. The mathematical method used is described and a simple absorption model of the atmosphere is presented.


1999 ◽  
Vol 86 (4) ◽  
pp. 253-258 ◽  
Author(s):  
W. Heinrich ◽  
S. Roesler ◽  
H. Schraube

Sign in / Sign up

Export Citation Format

Share Document