20.10.2018 Views

knjiga solarna energija dobra

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

104 THE PHYSICS OF THE SOLAR CELL<br />

4.0<br />

3.5<br />

R Sh very large<br />

3.0<br />

V/R Sh<br />

R Sh = 2 Ω<br />

2.5<br />

Cell current<br />

[A]<br />

2.0<br />

1.5<br />

R Sh = 0.2 Ω<br />

1.0<br />

0.5<br />

0.0 0.0 0.1 0.2 0.3 0.4 0.5 0.6 0.7<br />

Cell voltage<br />

[V]<br />

Figure 3.23 Effect of shunt resistance on the current–voltage characteristic of a solar cell (R S = 0)<br />

and a plot of I SC versus log[I o e qV OC/A o kT − I SC ] will then permit R S to be extracted<br />

from the slope of this line. Similarly, in the regime where only R Sh is important,<br />

equations (3.151) and (3.152) can be combined to give<br />

V OC<br />

R Sh<br />

= I SC − I o e qV OC/A o kT<br />

(3.154)<br />

and R Sh can be determined from the slope of the line given by plotting V OC versus<br />

[I SC − I o e qV OC/A o kT ]. If the series and shunt resistances are such that there is no regime<br />

where they can be neglected, the parameters can, with patience, be extracted through the<br />

process of trial and error.<br />

3.5.4 Temperature Effects<br />

From equations (3.127) and (3.128), it is apparent that<br />

I o1,n ,I o1,p ∝ n 2 i (3.155)<br />

and from equation (3.129) that<br />

I o2 ∝ n i . (3.156)

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!