However, the diffracted intensity of the superlattice reflections is weaker than that of the γ′-Fe4N formed on pure Fe.
However, the reflections are weak or are not observed if objects are transparent, black, or mirror planes.
As expected, the satellite reflections are weaker than adjacent substructure reflections.
This also means that when the modeled reflection paths are weak, the MVUE could perform surprisingly as poor as the case where the paths are strong.
The total reflection component of a radar wave dominates on calm water, and therefore the backscatter is weak.
Indeed, reflection artifacts may be weak or even absent and thus not detectable by eye when consolidation is small or far from pleural line.
For 6,6′ -BZ, a weak reflection is observed at q of 1.8 Å–1 in its GIXD image, also suggesting the presence of π π interactions.
The two strongest reflections of the intermediate phase are marked by arrows and an additional weaker reflection is circled with a dashed line.
In general, the property is referred to as (arithmetic) put-call symmetry at K [4], which is weaker than the reflection principle that ensures put-call symmetry for any K.
A comparison of the cases of fixed and fluctuating charge on the dust grains reveals that the solitons of higher amplitudes evolve in the plasma having dust charge fluctuations, but the weaker soliton reflection is realized under this situation.
