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Variation of environmental neutron flux with altitude and depth of both water and soil

MISCELLANEOUS

Variation of environmental neutron flux with altitude and depth of both water and soil

K. KOMURA
N.K. AHMED
A.H. EL-KAMEL
A.M.M. YOUSEF
Nuclear Science and TechniquesVol.15, No.4pp.248-256Published in print 01 Aug 2004
23100

Applying the extreme low-level γ-ray spectroscopic analysis the environmental neutron flux is measured using different moderator construction and environment through the reaction 197Au (n, γ) 198Au. The contribution of thermal and resonance neutrons is separated using the cadmium difference technique, while fast neutrons are measured by the paraffin moderator. The results of altitude dependence of the neutron flux are discussed. The thermal neutron flux near the surface of sea water is less than its value at 100 cm over ground near sea water, while the value over the surfaces of fresh water is higher than that near the surface of sea water. Also the thermal neutron flux at 5 cm soil depth increases, then decreases to its original value at 10 cm depth and still constant until 25 cm, then decreases rapidly to reach 27% of its original value at 60 cm depth. The soil compositions, corresponding neutron temperatures and effective absorption cross sections of earth are the most effective factors on the equilibrium region of thermal neutrons in the ground.

Extreme low-level γg-ray spectroscopyEnvironmental neutron fluxGold activation
References
[1] Kodama M, Kawasaki S, Imai T et al.

Anomalous atmospheric attenuation of cosmi-ray-produced neutrons near the earth's surface

, in: U.S Department of Energy, Natural Radiation Environment III, 1980, 2: 882
Baidu ScholarGoogle Scholar
[2] Hewitt J E, Hughes L, McCaslin J B et al. Exposure to cosmic-ray neutrons at commercial jet aircraft altitudes, in: U.S Department of Energy, Natural Radiation Environment III, 1980, 2: 855
[3] Nakamura T, Uwamino Y, Ohkubo T et al. Health Phys, 1987, 53(5): 509
[4] Moraal H, Potgieter M S, Stoker P H et al. J Geophys Res, 1989, 94(A2): 1459
[5] Wordel R, Mouchel D, Altzitzoglou T et al. Nucl Instrum Meth Phys Res, 1996, A369: 557
[6] Chung C, Chen C Y, Kung C H. Appl Radiat Isot, 1997, 49(4): 415
[7] Chen C Y, Chung C. Nucl Instrum Meth Phys Res, 1997, A395: 195
[8] O'Sullivan D, Zhou D, Heinrich W et al. Rad Meas, 31: 579
[9] Heinrich W.

Physics of cosmic radiation fields

, Int conf on cosmic radiation and air crew exposure, Dublin, 1998
Baidu ScholarGoogle Scholar
[10] Reitz G. Rad Prot Dos, 1991, 48: 5
[11] O'Brien K, Sandmeier H A, Hansen G E et al. J Geophys Res, 1978, 83(A1): 114
[12] Yamashita M, Stephenson L D, Patterson H W. J Geophys Res, 1966, 71(16): 3817
[13] Dep L, Elmore D, Lipschutz M et al. Nucl Instrum Meth Phys Res, 1994, B92: 301
[14] Sazonova T E, Zanevsky A V, Kharitonov I A et al. Appl Radiat Isot, 1998, 49(9-11): 1185
[15] Komura K, Yousef A M, Ahmed N K et al.

Measurement of environmental neutrons by activation of gold

, Abstract of the 42nd Symp. of Radiation Research of Japan, Sept. 1-3, 1999, Hiroshima, 1-E-11, 88
Baidu ScholarGoogle Scholar
[16] Emmett M B. The Monte Carlo Radiation Transport Code System, ORNL-4972, 1975
[17] Tommasino L. Radiat Prot Dosim, 1999, 86(4): 297
[18] McAulay I R, Bartlett D T, Dietze G et al.

Exposure of air crew to cosmic radiation, A report of EURADOS working group 11

, European Commission, 1997
Baidu ScholarGoogle Scholar
[19] Chung C, Chen C Y. J Geophys Res, 1997, 102(D25): 29827
[20] Hess W N, Canfield E H, Lingenfelter R E. J Geophys Res, 1961, 66(3): 665
[21] Hajnal F, McLaughlin J E, Weinstein M S et al.

USAEC report HASL-241

, 1971
Baidu ScholarGoogle Scholar
[22] Hewitt J E, Hughes L, Baum J W et al. Health Phys, 1978, 34: 375
[23] Bethe H A, Korff S A, Placzek G. Phys Rev, 1940, 57: 573
[24] Swetnick M J. Phys Rev, 1954, 95: 793
[25] Edge R D. Nucl Phys, 1959, 12: 182
[26] Hendrick L D, Edge R D. Phys Rev, 1966, 145(4): 1023