The calculated spectra of reflection and external quantum efficiency (EQE) match well with the experimental results in a full-wavelength range.
At frequencies where noise levels are sufficiently low, spectra of reflection coefficients show four distinct sets of characteristics: a flat spectrum, a spectrum with a significant spectral hole at approximately 1 or 3 Hz, a spectrum with a strong peak at approximately 2 or 3 Hz, and a spectrum containing both a sharp peak and a significant hole.
Our modeling results suggest that holes and peaks in the spectra of reflection coefficients can be qualitatively explained by a sinusoidal or spike-like topography at the ICB, with wavelengths and heights ~1 1.5 km, whereas a liquid or solid layer overlying the ICB does not reproduce any of the observed spectral features.
Using a positional map in this study was very useful in delineating the full spectrum of the reflections regarding partner notification for HIV within and across groups of counsellors.
Reflection spectrum of ITO shows the minimum reflection of 0.4% at 523 nm while reflection spectrum of TiO2 shows the minimum reflection of 3.5% at 601 nm within the 400- to 1,000-nm 1,000-nm
For all the CNT materials used, the spectra of the reflection loss versus frequency showed the presence of two minima.
The spectra of the reflection and transmission loss in a tilt angle range useful for fiber sidetap filter design is presented for the first time.
Figure 2 The spectra of optical reflection for nanowire arrays measured at different temperatures of 4.2, 70, 150, 200, and 297 K as indicated.
Featureless high-resolution spectra of the reflection grating spectrometer aboard XMM-Newton suggest the presence of a hydrogen atmosphere, as previously indicated by Chandra results.
The spectra of specular reflection of p- and s-polarized light were measured at near-normal incidence of light (approximately 10°) on GaAs surface over the range of GaAs fundamental photosensitivity (0.4 to 0.9 μm).
