Optimization of Nanosecond Fission Ion Chambers for Reactor Physics Applications

1975 ◽  
Vol 22 (1) ◽  
pp. 686-690 ◽  
Author(s):  
N. W. Hill ◽  
J. T. Mihalczo ◽  
J. W. Allent ◽  
M. M. Chiles
Keyword(s):  
2021 ◽  
pp. 101-112
Author(s):  
Wei Shen ◽  
Benjamin Rouben

The power referred to most frequently in reactor physics is neutron power. Neutron power is essentially the fission rate multiplied by the average prompt energy released and recovered per fission (see Section 2.1.2). It is also called “prompt” power, as it appears very quickly following fission. We cannot measure neutron power directly, but we do monitor the neutron flux with ion chambers located outside the calandria and in-core flux detectors. These neutronic signals are calibrated to the thermal-power measurement which allows neutron power to be derived.


2017 ◽  
Author(s):  
Chad L. Pope ◽  
◽  
Edward S Lum ◽  
Ryan Stewart ◽  
Bilguun Byambadorj ◽  
...  

2016 ◽  
Vol 2 ◽  
pp. 14 ◽  
Author(s):  
Benjamin A. Lindley ◽  
Dan Kotlyar ◽  
Geoffrey T. Parks ◽  
John N. Lillington ◽  
Bojan Petrovic
Keyword(s):  

2007 ◽  
Vol 30 (1) ◽  
pp. 25-32 ◽  
Author(s):  
R. A. Kinhikar ◽  
R. Upreti ◽  
S. Sharma ◽  
C. M. Tambe ◽  
D. D. Deshpande

Author(s):  
Ze-guang Li ◽  
Kan Wang ◽  
Gang-lin Yu

In the reactor design and analysis, there is often a need to calculate the effects caused by perturbations of temperature, components and even structure of reactors on reactivity. And in sensitivity studies, uncertainty analysis of target quantities and unclear data adjustment, perturbation calculations are also widely used. To meet the need of different types of reactors (complex, multidimensional systems), Monte Carlo perturbation methods have been developed. In this paper, several kinds of perturbation methods are investigated. Specially, differential operator sampling method and correlated tracking method are discussed in details. MCNP’s perturbation calculation capability is discussed by calculating certain problems, from which some conclusions are obtained on the capabilities of the differential operator sampling method used in the perturbation calculation model of MCNP. Also, a code using correlated tracking method has been developed to solve certain problems with cross-section changes, and the results generated by this code agree with the results generated by straightforward Monte Carlo techniques.


1968 ◽  
Vol 46 (10) ◽  
pp. S611-S613 ◽  
Author(s):  
K. Nagashima ◽  
H. Ueno ◽  
S. Mori ◽  
S. Sagisaka

The sidereal time variation is analyzed using data for the ion chambers at Cheltenham and Christchurch for the period 1938–58 and for the meson and neutron components during the IGY. All the results derived from these three kinds of data support the existence of a two-way sidereal anisotropy, suggested by Jacklyn, which has two maxima of the cosmic-ray intensity in the directions of 8 h and 20 h S.T. (sidereal time).


2011 ◽  
Vol 174 (2) ◽  
pp. 196-213 ◽  
Author(s):  
Mark D. DeHart ◽  
Stephen M. Bowman
Keyword(s):  

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