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Figure 4 shows the expected defocusing loss in units of dB, −10 log L, as a function of the ray closest distance r0 for D = 1, 2, and 5 RV.
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The optical trapping forces on the microsphere in the ray optics regime were measured as a function of the trap depth.
For the angular dependence analysis, whole, uniform, and non-uniform output currents were calculated as a function of the irradiation angle for an 241Am gamma-ray source.
Figure 6 presents theoretical X-ray transmission in the geometry ϕ = θ = 45° through a thickness of 1, 5, 10, 50 and 100 μm of different pure pigments as a function of the energy of X-ray photons.
The γ-rays attenuation-coefficients were measured as a function of the percentage of lead oxides for several γ-ray energies using point sources [241Am, 133Ba, 137Cs, and 60Co].
Fig. 3 Count rate of cosmic-ray muons as a function of the distance (X) of the hitting point from the PMT.
The impact of dislocations on the SiGe crystal quality is analysed by comparing the width of X-ray diffraction peaks as a function of the heterostructure size.
Here, s = 4πsin/λ is the momentum transfer as a function of the scattering angle 2θ and λ is the X-ray wavelength.
The behavior of the 1/f and white noise terms is studied as a function of the main device parameters before and after exposure to 10 keV X-rays and 60Co γ-rays.
In figure 4 the evolution of the diffracted intensity as a function of the incidence angle is presented (the evolution of the X-ray diffracted intensity as a function of the incidence angle is essentially the same for [29]).
By X-ray diffraction measurements phase formation was determined as a function of the ion-to-atom arrival ratio.
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