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932 ENERGY COLLECTED AND DELIVERED BY PV MODULES<br />

20.5.3.4 Daily irradiation<br />

The most accurate way of calculating G dm (β, α) from G dm (0) is, first, to calculate the<br />

hourly horizontal irradiation components G hm (0), D hm (0) and B hm (0); second, to transpose<br />

them to the inclined surface G hm (β, α), D hm (β, α) and B hm (β, α); and, finally, to integrate<br />

during the day.<br />

Such a procedure, summarised in Figure 20.16, allows us to account for the<br />

anisotropic properties of diffuse radiation, and leads to good results whatever the<br />

orientation of the inclined surface. However, it is laborious to apply and a computer<br />

must be used. It is interesting to mention that, for the case of surfaces tilted to the equator<br />

(α = 0), frequently encountered in photovoltaic applications, if the diffuse radiation is<br />

taken to be isotropic, the following expression may be applied<br />

G d (β, 0) = B d (0) × RB + D d (0) 1 + cos β<br />

2<br />

+ ρG d (0) 1 − cos β<br />

2<br />

(20.39)<br />

where the factor RB represents the ratio between the daily direct irradiations on an inclined<br />

surface and on an horizontal surface, and may be approximated by setting it equal to the<br />

corresponding ratio between daily extraterrestrial irradiations on similar surfaces. Hence,<br />

RB is given as follows:<br />

RB =<br />

ω SS<br />

π<br />

180 [sign(φ)]sinδ sin(|φ|−β) + cos δ cos(|φ|−β)sin ω SS<br />

π<br />

ω S<br />

180 sin δ sin φ + cos δ cos φ sin ω S<br />

(20.40)<br />

where ω SS is the sunrise angle on the inclined surface, which is given by<br />

ω SS = max[ω S , − arccos(−[sign(φ)]tanδ tan(abs(φ) − β))] (20.41)<br />

It is interesting to observe that for the equinox days, δ = 0 ⇒ ω S = ω SS and<br />

equation (20.40) becomes RB = cos[abs(φ) − β]/ cos φ.<br />

Example: Estimate the average daily irradiation in January at Changchun–China<br />

(φ = 43.8 ◦ ) over a fixed surface facing south and tilted at an angle β = 50 ◦ with respect<br />

to the horizontal, knowing that the mean value of the global horizontal irradiation is<br />

G dm (0) = 1861 Wh/m 2 and the ground reflection ρ = 0.2. The solution is as follows:<br />

January ⇒ d n = 17; δ =−20.92 ◦<br />

φ = 43.8 ◦ ⇒ ω S =−68.50 and B 0d (0) = 3586 Wh/m 2 ⇒ K Tm = 0.519<br />

⇒ F Dm = 0.414<br />

D dm (0) = 770 Wh/m 2 ; B dm (0) = 1091 Wh/m 2<br />

arccos(− tan δ tan(φ − β)) =−92.38 ◦ ⇒ ω SS =−68.5 ◦ ⇒ RB = 2.741

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