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The model illustrates the solar spectrum distributions under the Fresnel lens.
Simulation results provided a wide spectrum of combinations of net fluxes and energy spectrum distributions.
In SHM, long-term sensing information is split into pieces according to time and spectrum distributions.
The result of this study provides the information of illumination patterns under a circular lens, which will help to match up various spectrum distributions to their suitable solar applications.
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Figure 3 Sensed spectrum distribution.
Figure 8 Clutter power spectrum distribution at CUT.
In contrast, the power output of p-Si is not sensitive to spectrum distribution.
Figure 7 Energy spectrum distribution of the bound conformations for HSA (A) and BSA (C).
This work focused on the influence of energy spectrum distribution on drop breakage in turbulent flows.
The results show that the power output of a-Si PV module mainly depends on spectrum distribution.
This calls for an adaptive dynamic strategy to be introduced by an SP for efficient spectrum distribution.
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