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When the bent absorption bands cross the straight bands, mode splitting happens, causing the broad enhancement bump with multiple peaks.
If the periodicity of the PME pattern decreases, the multiple peaks disappear while only the broad enhancement bump remains.
On the positive-y side, a faint but broad enhancement extends from (0, 1.5) to (-3, 5) RO upstream.
That is exactly the origin of the broad enhancement peak observed at wavelengths shorter than 600 nm.
Feedburner CEO Dick Costolo emailed Richard MacManus and me on Monday to give us a preview of what he calls "broad enhancement to our stats" that are being released later this morning.
For both devices, it is the excitations of diverse propagating SPP modes at the bottom of PMEs that cause the broad enhancement bump at the short wavelength range superimposed with multiple tiny peaks.
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The spectrum of each component (Figure 4b) shows a broad band enhancement in the 20- to 50-mHz frequency range.
This means that on a statistical basis, increase geomagnetic activity levels are associated with a broad band enhancement in the Pc 5 amplitude.
More broad density enhancements and flow channels (>~500 km) occur during southward Bz.
Moreover, a combination of Pd NPs and NRs decorated on the BiVO4 electrodes leads to a broad-band enhancement across visible-NIR region.
Recently, absorber MNPs are also employed in the quantum dot solar cells to trap solar radiation in the form of localized SPRs, which lead to a broad spectral photocurrent enhancement [15].
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