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94 THE PHYSICS OF THE SOLAR CELL<br />

Table 3.2 Si solar cell model<br />

parameters<br />

Parameter<br />

Value<br />

A 100 cm 2<br />

W N 0.35 µm<br />

N D 1 × 10 20 cm −3<br />

D p<br />

1.5 cm 2 /V-s<br />

S F,eff 3 × 10 4 cm/s<br />

τ p 1 µs<br />

L p 12 µm<br />

W P 300 µm<br />

N A 1 × 10 15 cm −3<br />

35 cm 2 /V-s<br />

D n<br />

S BSF<br />

100 cm/s<br />

τ n 350 µs<br />

L n 1100 µm<br />

power point is found by solving<br />

∂P<br />

∂V ∣ = ∂(IV)<br />

V =VMP<br />

∂V ∣ =<br />

V =VMP<br />

[<br />

I + V ∂I ]∣ ∣∣∣V<br />

= 0 (3.132)<br />

∂V =VMP<br />

for V = V MP . The current at the maximum power point, I MP , is then found by evaluating<br />

equation (3.130) at V = V MP .<br />

The rectangle-defined V OC and I SC provides a convenient means for characterizing<br />

the maximum power point. The fill factor, FF, is a measure of the squareness of the I –V<br />

characteristic and is always less than one. It is the ratio of the areas of the two rectangles<br />

shown in Figure 3.16 or<br />

FF =<br />

An empirical expression for the fill factor is [15]<br />

P MP<br />

V OC I SC<br />

= V MPI MP<br />

V OC I SC<br />

(3.133)<br />

FF =<br />

V OC − kT q ln[qV OC/kT + 0.72]<br />

. (3.134)<br />

V OC + kT /q<br />

Arguably, the most important figure of merit for a solar cell is its power conversion<br />

efficiency, η, which is defined as<br />

η = P MP<br />

P in<br />

= FFV OCI SC<br />

P in<br />

(3.135)<br />

The incident power, P in , is determined by the properties of the light spectrum incident<br />

upon the solar cell. Further information regarding experimental determination of these<br />

parameters appears in Chapter 16.

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