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Some of these neutron rich nuclei will produce observational signatures in form of gamma ray lines during their decay.
In future studies, further detailed simulations of the emission and transport of radiation produced by cosmic radiation, including secondary products such as neutrons and gamma rays, are essential to determine the relationship between the chemical abundances and the intensities of gamma ray lines for planetary nuclear spectroscopy.
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Admittedly, comparable analytical facilities could be added to x-ray beam lines, as in the case of energy-dispersive spectroscopy carried out simultaneously with x-ray diffraction [18].
If the leaf position (lp) in the field space is known, a ray line along which irradiation will drop to 50% of the initial irradiation can be defined.
Marker 1 on the film was 30 mm away from the crosshair isocentre and the MLC edge travelled to abut the crosshair central axis ray line for irradiation.
W. Cattaneo, et al., Characterization of a tagged γ-ray beam line at the daΦne beam test facility, Nucl.
Kα X-ray lines were analysed except for lead (Mα lines).
The X-ray lines show considerable broadening, indicating the fine particle nature of the ferrite.
Nevertheless, the intensity of graphene X-ray lines is under possibility for quality Rietveld refinement.
The energy resolution of the system, as obtained with several fluorescence X-ray lines, is described.
The most important γ-ray lines result from the decay chains of 56Ni, 57Ni, and 44Ti.
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