Gamma ray production cross section from energetic neutron inelastic scattering for methodical improvements in planetary gamma-ray spectroscopy [electronic resource]

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 str...

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Bibliographic Details
Online Access: Online Access
Corporate Author: Los Alamos National Laboratory (Researcher)
Format: Government Document Electronic eBook
Language:English
Published: Washington, D.C. : Oak Ridge, Tenn. : National Aeronautics and Space Administration Announcement ; distributed by the Office of Scientific and Technical Information, U.S. Department of Energy, 1991.
Subjects:

MARC

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245 0 0 |a Gamma ray production cross section from energetic neutron inelastic scattering for methodical improvements in planetary gamma-ray spectroscopy  |h [electronic resource] 
260 |a Washington, D.C. :  |b National Aeronautics and Space Administration Announcement ;  |a Oak Ridge, Tenn. :  |b distributed by the Office of Scientific and Technical Information, U.S. Department of Energy,  |c 1991. 
300 |a Pages: (11 p) :  |b digital, PDF file. 
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500 |a Published through SciTech Connect. 
500 |a 01/01/1991. 
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500 |a " conf-910422--7" 
500 |a "DE92007411" 
500 |a International topical conference on methods and applications of radioanalytical chemistry II (MARC-2), Kona, HI (United States), 21-27 Apr 1991. 
500 |a Drake, D.M.; Reedy, R.C.; Gearhart, R.; Castaneda, C.M.; Englert, P.A.J.; Sanii, B. 
520 3 |a 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. 
536 |b W-7405-ENG-36. 
650 7 |a Iron.  |2 local. 
650 7 |a Neutron Reactions.  |2 local. 
650 7 |a Planets.  |2 local. 
650 7 |a Gamma Spectroscopy.  |2 local. 
650 7 |a Chemical Composition.  |2 local. 
650 7 |a Cross Sections.  |2 local. 
650 7 |a Inelastic Scattering.  |2 local. 
650 7 |a Mev Range 01-10.  |2 local. 
650 7 |a Mev Range 10-100.  |2 local. 
650 7 |a Neutron Spectra.  |2 local. 
650 7 |a Surfaces.  |2 local. 
650 7 |a Baryon Reactions.  |2 local. 
650 7 |a Elements.  |2 local. 
650 7 |a Energy Range.  |2 local. 
650 7 |a Hadron Reactions.  |2 local. 
650 7 |a Metals.  |2 local. 
650 7 |a Mev Range.  |2 local. 
650 7 |a Nuclear Reactions.  |2 local. 
650 7 |a Nucleon Reactions.  |2 local. 
650 7 |a Scattering.  |2 local. 
650 7 |a Spectra.  |2 local. 
650 7 |a Spectroscopy.  |2 local. 
650 7 |a Transition Elements.  |2 local. 
650 7 |a Inorganic, Organic, Physical And Analytical Chemistry.  |2 edbsc. 
650 7 |a Classical And Quantum Mechanics, General Physics.  |2 edbsc. 
650 7 |a Radiation Chemistry, Radiochemistry, And Nuclear Chemistry.  |2 edbsc. 
710 2 |a Los Alamos National Laboratory.  |4 res. 
710 1 |a United States.  |b National Aeronautics and Space Administration.  |4 spn. 
710 1 |a United States.  |b Department of Energy.  |b Office of Scientific and Technical Information.  |4 dst. 
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