A Monte Carlo Simulation Method for Solar Radiant Energy Density with Peak Stability
A technology of solar radiation and simulation method, applied in the field of solar power generation simulation, can solve the problems of deviation of real situation, unstable peak value of simulation results, reducing the credibility of simulation results, etc., to achieve the effect of reducing RMSE
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[0033] Taking the existing two-way Monte Carlo ray tracing algorithm to simulate the radiant energy density of the receiver surface as an example, the calculation steps are as follows:
[0034] 1. According to the sun incidence model, the direction of the incident light is sampled. The light direction is determined by the elevation angle (set as θ) and the azimuth angle (set as )Sure. For example, when using the Buie sun distribution model, Obey the uniform distribution in the [0,2π] interval, and θ obeys the Buie distribution model, as shown in formula 1 and formula 2 respectively:
[0035]
[0036]
[0037] The calculation method of κ and γ is shown in formula 3,
[0038]
[0039] Among them, χ represents the CSR parameter that controls the distribution of Buie's solar light distribution model when the light is greater than the solar opening angle (4.65mrad).
[0040] 2. Sample the intersection of the incident light with the heliostat surface. A point is rand...
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