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720 MEASUREMENT AND CHARACTERIZATION<br />

(E 2 = E 1 ) and assuming no series resistance (R s = 0), the value of K that best translates<br />

the I –V characteristics for temperature is determined.<br />

Translation equations for I SC , V OC ,V max ,andI max as a function of E tot ,T c , absolute<br />

air mass (AM a ), and angle of incidence (AOI) based on multiple regression analysis of<br />

field data have been proposed by King [63]:<br />

I SC (E, T c ,AM a , AOI ) = (E/E 0 )f 1 (AM a )f 2 (AOI )[I SC0 + α ISC (T c − T o )] (16.6)<br />

E e = I SC (E, T c = T 0 ,AM a , AOI )/I SC0 (16.7)<br />

I mp (E e ,T c ) = C 0 + E ec [C 1 + α Imp (T c − T 0 )] (16.8)<br />

V OC (E e , i) = V OC0 + C 2 ln(E e ) + β VOC (T c − T 0 ) (16.9)<br />

V mp (E e ,T c ) = V mp0 + C 3 ln(E e ) + C 4 [ln(E e )] 2 + β Vmp (T c − T 0 ) (16.10)<br />

I SC0 = I SC (E = E 0 ,T c = T 0 ,AM a = 1.5, AOI = 0 ◦ ) (16.11)<br />

V OC0 = V OC (E e = 1,T c = T 0 ) (16.12)<br />

V mp0 = V mp (E e = 1,T c = T 0 ) (16.13)<br />

f 2 =<br />

E 0<br />

I SC (AM a = 1.5,T c = T 0 ) − E diff<br />

I SC0<br />

, (16.14)<br />

E dir cos(θ)<br />

where E is the plane-of-array solar irradiance, E e is the effective irradiance in units of<br />

suns, E 0 is the one-sun irradiance of 1000 Wm −2 , E diff is the diffuse irradiance in the<br />

plane of the module, E dir is the direct-normal irradiance, and AOI is the solar angle<br />

of incidence on the module; T c is the temperature of the cells inside the module, T 0<br />

is the module reference temperature, and α ISC , α Imp , β VOC ,andβ Vmp are the temperature<br />

coefficients of I SC , I mp , V OC ,andV mp , respectively. These temperature coefficients are in<br />

absolute units so they will vary with the size of the PV device, the number of devices<br />

in series, or the number of devices in parallel. The pressure-corrected relative optical air<br />

mass AM a can be written as [64]<br />

AM a = P P 0<br />

[cos(θ) + 0.50572(96.07995 ◦ − θ) −1.6364 ] −1 , (16.15)<br />

where P is the barometric pressure, P 0 is the pressure at sea level, and θ is the angle<br />

between the sun and zenith in degrees. The function f 1 (AM a ) is empirically obtained<br />

from the temperature- and irradiance-corrected I SC versus air mass and assumes that the<br />

only spectral dependence is the zenith angle. Data are collected over a range of irradiances,<br />

incident angles, air masses, and temperatures and a multiple regression analysis is<br />

applied. These translation equations have been compared with simple linear translation<br />

equations derived from simulator-based measurements for several modules using outdoor<br />

data [49]. These translation equations give similar results to equation (16.3) when temperature,<br />

maximum-power tracking, and spectral issues are considered [48]. Other translation<br />

equations for current and voltage are possible [16, 65].

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