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Our problem is, roughly speaking, to estimate the reflection channel (boldsymbol h_{1}^{ k)}), sometimes called the main reflection channel, because the reflectivity and velocity are directly related with the amplitude and phase of (boldsymbol h_{1}^{ k)}) as shown in (3)–(6).
In Set A, in order to make the analysis simple and clear, we assume that the main reflection channel (boldsymbol h_{1}^{ k)}) consists of two steps of reflectivity ("high" and "low") and only the interference from Radar-2 exists.
(B) Nonetheless, it is not reasonable to consider the MF output as a good approximation to the main reflection channel.
The intensity of diffuse scattering, arising due to static displacements of atoms, increases when approaching to the main reflection.
The main reflection peak of the XRD pattern at 2θ = 43° can be attributed to (200) plane.
e Estimate |y av |2 of the squared amplitude (left |boldsymbol h_{1}^{ k)}right |^{2}) of the main reflection channel.
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For the SnS2@CoS2 rGO composite, the main reflections are well ascribed to the characteristic peaks of SnS2 and CoS2.
In addition detailed flipcharts recorded the main reflections during the group discussions.
The final fit to the diffraction data is excellent for the main reflections (Table 1 ▶).
In the last step the restraints were released, resulting in a good fit to the main reflections with R obs = 0.0412.
All additional weaker satellite reflections were indexed with the q vector (0, β, 0) (de Wolff, 1974 ▶) using the closest main reflection along b * as reference.
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