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ADDITIONAL TOPICS 101<br />

and the internal spectral response as<br />

SR int =<br />

I SC (λ)<br />

qA(1 − s)(1 − r(λ))f (λ)(e −α(λ)W opt<br />

− 1) , (3.147)<br />

where W opt is the optical thickness of the solar cell (technically, also a function of<br />

wavelength). Experimentally, the external spectral response is measured. The internal<br />

spectral response is determined from it along with the knowledge of the grid shadowing,<br />

reflectance, and optical thickness. W opt can be greater than the cell thickness if lighttrapping<br />

methods are used. Such methods include textured surfaces [20] and back-surface<br />

reflectors [21] and are discussed in Chapter 8. The short-circuit current can be written in<br />

terms of the external spectral response as<br />

∫<br />

I SC = SR ext (λ)f (λ) dλ. (3.148)<br />

λ<br />

The internal spectral response gives an indication of which sources of recombination are<br />

affecting the cell performance. This is demonstrated in Figure 3.20 where the internal<br />

spectral response of the silicon solar cell described by the parameters of Table 3.2 is<br />

shown. Also shown is the spectral response when S F,eff = 100 cm/s (a passivated front<br />

surface) and the spectral response when S BSF = 1 × 10 7 cm/s (in effect, no BSF). The<br />

short wavelength response improves dramatically when the front surface is passivated<br />

1.0<br />

S F, eff = 100 cm/s<br />

SR for solar cell<br />

of Table 3.2<br />

0.8<br />

Internal spectral response<br />

0.6<br />

0.4<br />

S BSF = 10 7 cm/s<br />

0.2<br />

0.0 0.2 0.4 0.6 0.8 1.0 1.2<br />

Wavelength<br />

[µm]<br />

Figure 3.20 Internal spectral response of the silicon solar cell defined in Table 3.2

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