Authors:
C. Castaneda University of California Crocker Nuclear Laboratory 95616 Davis CA (USA)

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R. Gearhart University of California Crocker Nuclear Laboratory 95616 Davis CA (USA)

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B. Sanii University of California Crocker Nuclear Laboratory 95616 Davis CA (USA)

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P. Englert San Jose State University 95192 San Jose CA (USA)

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D. Drake Los Alamos National Laboratory 87545 Los Alamos NM (USA)

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R. Reedy Los Alamos National Laboratory 87545 Los Alamos NM (USA)

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Abstract  

Planetary gamma-ray spectroscopy can be used to chemically analyze the top soil from planets in future planetary missions. The production from inelastic neutron interaction plays an effective role in the determination on the C and H at the surface. The gamma-ray production cross section from the strongest lines excited in the neutron bombardment of Fe have been measured by the use of a time analyzed quasi-mono-energetic neutron beam and a high purity germanium detector. The results from En=6.5, 32, 43, and 65 MeV are presented.

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Journal of Radionalytical and Nuclear Chemistry
Language English
Size A4
Year of
Foundation
1968
Volumes
per Year
1
Issues
per Year
12
Founder Akadémiai Kiadó
Founder's
Address
H-1117 Budapest, Hungary 1516 Budapest, PO Box 245.
Publisher Akadémiai Kiadó
Springer Nature Switzerland AG
Publisher's
Address
H-1117 Budapest, Hungary 1516 Budapest, PO Box 245.
CH-6330 Cham, Switzerland Gewerbestrasse 11.
Responsible
Publisher
Chief Executive Officer, Akadémiai Kiadó
ISSN 0236-5731 (Print)
ISSN 1588-2780 (Online)