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It might instead be due to scattering in a preferred direction, as a result of asymmetric turbulence in the gas surrounding the black hole.
Pham et al. (2009), analyzing rotational motion within the P coda, discussed on the fact that no torsional motion can be observed within a homogeneous media and that the observed torsion may be due to scattering within the crust.
This could be due to scattering of light in the coating, in the direction of the detector.
However, there is a substantial degree of periodicity, and the enhancement would also be due to scattering of light from the embedded SiO2 mask.
This may be due to scattering near the source region, as discussed in previous studies that determined magnitudes from SP data (e.g., (Schweitzer and Kværna 1999; Takemura et al. 2015).
The broad-band increase in absorption in this area could be due to scattering by silver nanoparticles and DOPA oxidation.
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The data are corrected for background contributions, and this feature does not appear in the data for the base samples, so it is assumed that this feature is due to scattering from the amorphous binding material present in the simulants.
Within the plateau area approximately (57 59)%, (59 63)%, (52 63)% and (58 61)% of this fraction was due to scattered and reabsorbed radiation for the LSO, GSO, YAP and LuAP scintillators, respectively.
As hypothesized in [30], this effect could be due to scatter correction.
It is assumed to be due to scatter radiation producing electrons in the amplifying circuit of the electrometer.
The long absorption tail (between 400 800 nm) in the case of cubic sphalerite ZnS (Zn:S = 1 3) was due to scattering by the crystals [19].
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