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THE SOLAR CELL LASER SCANNER Emmett L. Miller, Shy-Shiun Chern and Alex Shumka Jet Propulsion Laboratory, California Institute of Technology INTRODUCTION As part of the Low Cost Solar Array Program a t Jet Propulsion Laboratory, failure analyses have been performed on over 300 photovoltaic modules from thirty different manufacturers and five coun- tries. Because of the volume of work and the var- iety of module types encountered, it has been nec- essary to develop non-destructive techniques to rapidly locate the failure sites. This paper will present design details and results obtained with one instrument developed specifically for this purpose, the Solar Cell Laser Scanner (SCLS). The effects of applying a bias current to the modules will also be discussed, based upon experimental observations and computer generated predictions. THE INSTRUMENT Preliminary results obtained with a prototype SCLS were presented earlier(1). The present in- strument is a completely new design, incorporating significantly improved resolution, scanning and display capabilities. The instrument is shown i n Figure 1, and a block diagram of the principal components is shown in Figure 2. It utilizes a focused, ten milliwatt helium-neon laser beam, raster-scanned over the solar module by galvanom- eter-driven mirrors. Optical components are mounted on a 3' x 4' optical table (Figure 3), pro- viding a stable platform with ample space for addi- tion of auxiliary apparatus. Standard, commercial- l y available components were used wherever possible, to minimize costs and development time. This ap- proach resulted in a system which is not as compact or portable as an integrated design, but which al- lows great flexibility for future modifications. An "inverted1' geometry was chosen to provide a target position located as close as possible to the scanning mirrors (Module Position A in Figure 2). For scanning an entire module, a 45' mirror directs the beam onto module position B. The optical system consists of an aperture an& variable attenuator, a The research described in this paper was carried out at the Jet Propulsion Laboratory, California Insti- tute of Technology, and was sponsored by the Depart- ment of Energy through an agreement with NASA. FIGURE 1. The Solar Cell Laser Scanner. FIGURE 2. Block Diagram of the Solar Cell Laser Scanner. Proceedings of the 15th IEEE Photovoltaic Specialists Conference Orlando, FL, May 11-15, 1981, pp. 1126-1133

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Page 1: THE SOLAR CELL LASER SCANNER Jet Propulsion Laboratory, California Institute of … › adv_tech › photovol › 2016ENG › Solar... · 2016-12-19 · THE SOLAR CELL LASER SCANNER

THE SOLAR CELL LASER SCANNER

Emmett L. Mi l l e r , Shy-Shiun Chern and Alex Shumka

J e t Propulsion Laboratory, Ca l i fo rn ia I n s t i t u t e of Technology

INTRODUCTION

A s p a r t of t h e Low Cost Solar Array Program a t J e t Propulsion Laboratory, f a i l u r e analyses have been performed on over 300 photovol ta ic modules from t h i r t y d i f f e r e n t manufacturers and f i v e coun- t r i e s . Because of t h e volume of work and the var- i e t y of module types encountered, it has been nec- e s sa ry t o develop non-destructive techniques t o r ap id ly l o c a t e the f a i l u r e s i t e s . This paper w i l l p resent design d e t a i l s and r e s u l t s obtained wi th one instrument developed s p e c i f i c a l l y f o r t h i s purpose, t he Solar Ce l l Laser Scanner (SCLS). The e f f e c t s of applying a b i a s cu r ren t t o t h e modules w i l l a l s o be d iscussed, based upon experimental observat ions and computer generated predic t ions .

THE INSTRUMENT

Preliminary r e s u l t s obtained wi th a prototype SCLS were presented e a r l i e r ( 1 ) . The present in- strument is a completely new design, incorpora t ing s i g n i f i c a n t l y improved r e so lu t ion , scanning and d i sp lay c a p a b i l i t i e s . The instrument is shown i n Figure 1, and a block diagram of the p r i n c i p a l components i s shown in Figure 2. It u t i l i z e s a focused, t e n m i l l i w a t t helium-neon l a s e r beam, raster-scanned over t h e s o l a r module by galvanom- eter-driven mirrors. Op t i ca l components a r e mounted on a 3' x 4' o p t i c a l t a b l e (Figure 3 ) , pro- viding a s t a b l e platform wi th ample space f o r addi- t i o n of a u x i l i a r y apparatus. Standard, commercial- l y a v a i l a b l e components were used wherever poss ib l e , t o minimize c o s t s and development time. This ap- proach r e s u l t e d in a system which is n o t a s compact o r po r t ab le a s an in t eg ra t ed design, but which a l - lows grea t f l e x i b i l i t y f o r f u t u r e modifications.

An "inverted1' geometry was chosen t o provide a t a r g e t pos i t i on located a s c l o s e a s poss ib l e t o t h e scanning mi r ro r s (Module Pos i t i on A i n Figure 2) . For scanning an e n t i r e module, a 45' mirror d i r e c t s t h e beam onto module p o s i t i o n B. The o p t i c a l system c o n s i s t s of an ape r tu re an& v a r i a b l e a t t enua to r , a

The research described i n t h i s paper was c a r r i e d out a t t h e J e t Propulsion Laboratory, Ca l i fo rn ia I n s t i - t u t e of Technology, and was sponsored by t h e Depart- ment of Energy through an agreement wi th NASA.

FIGURE 1. The Solar C e l l Laser Scanner.

FIGURE 2. Block Diagram of t h e Solar C e l l Laser Scanner.

Proceedings of the 15th IEEE Photovoltaic Specialists ConferenceOrlando, FL, May 11-15, 1981, pp. 1126-1133

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FIGURE 3. P r inc ipa l o p t i c a l components. L = Laser; S = Shut ter and Aperture; A = Variable Attenuator; E = Beam Expander and S p a t i a l F i l t e r ; F = Focusing Lens; M = Galvanometer Driven Mirrors.

bulb-operated s h u t t e r , and a 9X beam expander and s p a t i a l f i l t e r . Focusing is accomplished by posi- t ion ing t h e output l e n s of t h e beam expander, using a separa te rack-and-pinion mount. The approximate diameter of t h e focused spot is determined by focusing dis tance, D, t h e foca l length of the e x i t l ens , F, and the pinhole diameter, d , where F=80mm and d = 25 um:

D - F Spot Diameter = -

F d*

Thus, f o r the two module pos i t ions , t h e predic ted spot s i z e is:

Pos i t ion A D = 210 mm Size = 3.04 mm (1.57 mil )

Pos i t ion B D = 1730 mm Size = 0.52 mm (20.5 mil)

The scanning system c o n s i s t s of two orthogonally mounted galvanometers with pos i t ion sensors, pro- v id ing feedback t o t h e galvanometer c o n t r o l l e r s and pos i t ion s i g n a i s t o t h e d i sp lay system. The gal- vanometers a r e dr iven by standard e l e c t r i c a l func- t i o n generators with a t r i a n g l e waveform. The beam p o s i t i o n i s monitored on an osci l loscope, whfch a l s o serves t o d i sp lay t h e photocurrent s i g n a l am- p l i tude . I n addi t ion, t h e module under t e s t may be observed continuously on a closed c i r c u i t TV sys- t e m , which a i d s i n posi t ioning t h e beam on a par- t i c u l a r area.

* Catalog Data Sheet, Or ie l Corporation

The e a r l i e r r e s u l t s were obtained by d i r e c t imaging of t h e photocurrent on a standard osc i l lo - scope. This has now been replaced by an image s to r - age system, which permits the photocurrent image t o be s tored a t the slow galvanometer scan r a t e and then displayed f o r extended per iods on a high reso- l u t i o n TV monitor. The scan converter/image s to r - age u n i t r ece ives i ts beam pos i t ion s i g n a l s from t h e mirror pos i t ion s igna l s through t h e scan con t ro l u n i t developed in-house. This scan con t ro l u n i t in- corporates a s i n g l e con t ro l which serves t o vary t h e magnification of t h e image by a t tenuat ing the def lec- t i o n s igna l s fed t o t h e galvanometer con t ro l l e r s , and simultaneously amplifying t h e mirror pos i t ion s igna l outputs an equivalent amount. Thus, t h e beam pos i t ion s igna l s fed t o the image s torage u n i t always have the same amplitude, independent of the s i z e of t h e a rea scanned. This scanned a rea can be posit ioned anywhere on a 3' x 4' a rea (Module posi- t i o n B). A sweep s igna l invers ion switch i s pro- vided f o r use wi th t h e 45' mirror t o r e t a i n co r rec t image re la t ionsh ips . The most c r i t i c a l p a r t of t h e d i sp lay system is the s igna l ampl i f ier . This must not only amplify t h e small photocurrent generated by t h e l a s e r , but permit app l i ca t ion of a consider- ab ly l a r g e r dc b i a s cu r ren t through t h e module. The ampl i f i e r developed a t JPL is e s s e n t i a l l y a current- to-voltage converter with v a r i a b l e o f f s e t t o ad jus t f o r the dc vol tage r e s u l t i n g from app l i ca t ion of a dc forward b i a s cu r ren t t o t h e module. A highly s t ab le , ex te rna l dc cu r ren t source i s u t i l i z e d t o supply t h i s b ias . The output ga in ,po la r i ty and o f f s e t a r e con t ro l l ab le , and d i g i t a l panel meters a r e provided f o r se tup and monitoring purposes.

P r a c t i c a l Limitations

Ear l ig r , t h e minimum o p t i c a l path length and re- s u l t a n t spot s i z e were discussed. Actual r e so lu t ion is l imi ted by a number of o ther f a c t o r s including:

1. Sca t t e r ing from'dust i n the atmosphere and on the var ious o p t i c a l surfaces .

2. Imperfections i n t h e o p t i c a l components.

3. The textured g l a s s supers t r a t e used on many modules.

4. Ref lect ions wi thin the modules.

5. Defocusing v s scan angle.

6. *Resolution of t h e image s to rage and d i sp lay system.

7. Scanning speedltime-constant e f f e c t s .

8. E l e c t r i c a l no i se and spurious pickup.

9 . Signal d r i f t when using b i a s current .

Other than per iodic cleaning, l i t t l e can be done about t h e f i r s t four f ac to r s . Defocusing versus scan angle is a l imi t ing f a c t o r when scan- ning a reas g rea te r than about 50mm diameter a t pos i t ion A, o r 60 cm diameter a t pos i t ion B. A t t h e extreme d e f l e c t i o n angle of f12.5' mirror

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angle , t h e defocused spot s i z e would be about 2 m , compared wi th t h e center l i n e spot s i z e of 0.05 - 0.5 mrn. When higher r e so lu t ion is required, i t i s necessary t o l i m i t t h e d e f l e c t i o n angle and inc rease t h e image magnification on t h e TV screen. The image s torage/scan converter system and t h e TV mon- i t o r a r e high reso lu t ion u n i t s , each capable of over 1000 l i n e s r e so lu t ion . A t un i ty magnification, t h i s corresponds t o an image r e s o l u t i o n of about 0.25mm. The s tored image can be enlarged wi th the zoom con- t r o l up t o 36X to take advantage of t h i s c a p a b i l i t y . A TV r a t e of 1225 l ines / f rame is u t i l i z e d , r a t h e r than t h e standard 525 l i n e s , t o f u r t h e r improve t h e displayed image.

Scanning speedlt ime constant e f f e c t s a r e q u i t e no t i ceab le on modules from c e r t a i n manufacturers, e s p e c i a l l y those using l a r g e a rea c e l l s with high shunt r e s i s t a n c e . These e f f e c t s can be p a r t i a l l y av@femE $j i gpplging a b i a s cu r ren t t o t h e panel; however, t h e operator may be forced t o use a much slower scan speed than normal. This is more of an operat ing l i m i t a t i o n than a reso lu t ion l i m i t a t i o n , so long a s t h e operator monitors t h e s igna l wave- form and a d j u s t s these parameters t o e l iminate time constant e f f e c t s ( i .e . , overshoot and undershoot when t h e beam crosses me ta l l i za t ion s t r i p s ) .

E l e c t r i c a l no i se pickup has been troublesome, compounded by t h e antenna-like l a r g e su r face a rea of t h e module. Considerable ca re must be paid t o sh ie ld ing and e l iminat ing ground loops. An addi- t i o n a l problem occasional ly encountered is s igna l d r i f t when applying l a r g e r than normal b i a s cur- r e n t s , e spec ia l ly t o modules wi th high shunt r e s i s - tance c e l l s . This is suggestive of a heat ing ef- f e c t , but t h e mechanism has not y e t been conclu- s i v e l y i d e n t i f i e d .

Attempts have been made t o measure t h e a c t u a l r e so lu t ion of t h e instrument by scanning over a sharp edge placed i n f r o n t of a bare photocel l a t var ious working d i s t ances . With t h e instrument i n ILS uurual condlclon, ~ . e . , without taking unusual measures t o optimize i t s performance, t h e approxi- mate beam diameter was about 0.5mm a t pos i t ion B , i n agreement wi th the predic ted c a p a b i l i t y of t h e beam expander. A t p o s i t i o n A, t h e measurement i s more d i f f i c u l t t o perform accurate ly , but t h e ap- parent beam diameter was i n t h e range of 0.05 - 0.1 m, somewhat l a r g e r than predic ted.

RESULTS

A t JPL t h e SCLS has been used rou t ine ly on mod- u l e s submitted f o r f a i l u r e ana lys i s . Many of these modu-les had previously been, subj ec ted t o environ- mental t e s t i n g o r extended f i e l d service , and ex- h ib i t ed s i g n i f i c a n t l o s s e s in power output. Cracked c e l l s , f r ac tu red in terconnect ions , delami- nat ion, and va r ious o the r f a i l u r e modes have been encountered. The most common use of t h e SCLS has been t h e rapid loca t ion of cracked o r shorted c e l l s which have a s i g n i f i c a n t e f f e c t on the module out- put. Rela t ively l i t t l e d e t a i l e d , high reso lu t ion study of individual d e f e c t s has been done a s ye t , al though other author,^ have reported on t h e use- fu lness of t h e technique f o r such inves t iga t ions (2-4).

The SCLS images a r e o f t e n q u i t e s t r i k i n g f o r these damaged modules. Figure 4 shows an example where por t ions of c e l l s have been p a r t i a l l y i so- l a t e d from t h e remainder by cracks. The r e s i s t i v e connection ac ross t h e crack a l lows these por t ions t o be imaged a t reduced i n t e n s i t y . Figure 5 shows a l a r g e (2' x 4 ' ) module conta ining 224 ribbon c e l l s , two of which e x h i b i t missing a r e a s because of cracks . Locating cracks on these c e l l s by v i s u a l inspect ion is usua l ly d i f f i c u l t and t ed ious , where- a s the SCLS image c l e a r l y r e v e a l s which c e l l s have s i g n i f i c a n t e l e c t r i c a l degradation. Of course , these modules may have o the r c e l l s wi th l o c a l i z e d d e f e c t s o r cracks which have not a f fec ted t h e i r e l e c t r i c a l c h a r a c t e r i s t i c s appreciably . Such de- f e c t s may.Le revealed a t higher magnif ica t ions . A l l of these module images e x h i b i t s u b s t a n t i a l d i f f e r - ences i n image b r igh tness from c e l l t o c e l l . At zero b i a s cu r ren t , observing t h e s h o r t c i r c u i t cur- r e n t image, t h e r e i s a d i r e c t c o r r e l a t i o n between the b r igh tness of a c e l l and its shunt r e s i s t a n c e . It was noted, however, t h a t t h i s r e l a t i o n s h i p changes wi th a p p l i c a t i o n of forward dc b i a s c u r r e n t . The r e l a t i v e b r igh tness of c e l l s wi th in a module may change t o t h e ex ten t t h a t "dark" c e l l s ( a t zero b ias ) may become b r i g h t , and i n i t i a l l y b r i g h t c e l l s may become da rk under biased condi t ions . A t y p i c a l sequence is shown i n Figure 6. Note t h e complete r e v e r s a l of r e l a t i v e b r igh tness of s e v e r a l c e l l s a s the cu r ren t was increased £om zero t o 48 mA. A t higher b i a s cu r ren t s , t h e ce l l - to -ce l l b r igh tness v a r i a t i o n s tended t o disappear a s t h e o v e r a l l s ig- n a l i n t e n s i t y decreased.

MODULE EFFECTS ON IMAGE BRIGHTNESS

Unlike t h e more common s o l a r module measurements, SCLS generated photocurrent i s obtained from only a

FIGURE 4. SCLS image of a 23" x 23" module containing 42 3" diameter c e l l s . Arrows i n d i c a t e cracked c e l l s .

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very small spot i l luminated a t very high i n t e n s i t y , perhaps 10-50 suns. Character izat ion of t h e re- sponse of a cell and a module t o t h i s type of s t i m - u l u s is e s s e n t i a l f o r understanding t h e e f f e c t of c e l l parameters and d e f e c t s on t h e output. The f o l - lowing d i scuss ion considers v a r i a t i o n s of s e r i e s and shunt r e s i s t a n c e and diode s a t u r a t i o n cur ren t , which a r e shown t o have a s i g n i f i c a n t e f f e c t on t h e SCLS image b r igh tness of individual c e l l s i n a mod- ule . E f f e c t s of c e l l shee t r e s i s t a n c e on t h e images of s i n g l e c e l l s have been inves t iga ted by o the rs , and a r e not discussed here ( 2 , 4 ) .

I n Figure 7, a standard equivalent c i r c u i t f o r a c e l l is modified t o separa te t h e c e l l i n t o i l lumi- nated and non-illuminated por t ions . This c e l l is connected i n s e r i e s wi th o the rs t o form a module. Becai~se only a small por t ion of t h e c e l l is i l lumi- nated at any time, it may be assumed t h a t t t e shunt r e s i s t a n c e of the non-illuminated region, R s H ~ , is almost equal t o t h a t of the e n t i r e c e l l , RSHX. Also, f o r slow scanning speeds, junction capacitance ef- f e c t s may be neglected. I n Figure 7 , i t i s assumed t h a t t h i s s e r i e s s t r i n g of c e l l s a r e connected t o a current-to-voltage converter having zero input impe- dance, and no ex te rna l cur ren t b i a s is appl ied. Typi- c a l shunt r e s i s t a n c e s a r e i n the range oil-500ohms, and photocurrents from the l a s e r a r e a few m i l l i - amperes o r l e s s . Under these condi t ions , t o a f i r s t approximation, diode e f f e c t s may be neglected and t h e equivalent c i r c u i t becomes a simple resis- tance network. Consequently, t h e output c u r r e n t becomes d i r e c t l y proport ional t o the shunt r e s i s - tance of t h e c e l l being i l luminated.

Bias Current E f f e c t s

The output c h a r a c t e r i s t i c s a r e q u i t e d i f f e r e n t when an e x t e r n a l dc b i a s cur ren t i s appl ied t o t h e module. Referring t o Figure 8 , when a b i a s cur ren t , IB is applied from a constant cur ren t generator , vo l t age source, EB, is adjusted t o o f f s e t the module terminal dc vol tage, VB, r e s u l t i n g f r o m t h e b i a s cur- r en t . Thus, the net dc vol tage a t t h e current-to-

FIGURE 5. SCLS image of a 2 ' x 4 ' module containing 224 ribbon c e l l s . Arrows i n d i c a t e cracked c e l l s .

vo l t age converter inpu t s is zero. Under these con- d i t i o n s , IL = -IB and IS = 0. When a spot is i l l u - minated on a cell, t h e module current , IL, is com- posed of t h e b i a s cur ren t p lus an add i t iona l term, t h e photocurrent, flowing in t h e opposi te d i rec t ion . ~ h u s , IL = IS -IB, o r IS = IL + IB. This is t h e s ig - n a l cu r ren t which is amplified and imaged.

It would be poss ib le t o apply t h e same simplify- ing a s s y p t i o n s made earlier regarding Figure 7, i. e. , R S H ~ ss R s H ~ , and c a l c u l a t e t h e s i g n a l cur ren t of Figure 8 by applying t h e standard equation f o r diode cur ren t a s a funct ion of c e l l voltage. How- ever, s i n c e a computer w i l l be used t o provide numer- i c a l so lu t ions , it is not necessary t o make t h a t approximation. I n Appendix A, t h e following equa- t i o n is derived which r e l a t e s t h e s i g n a l cur ren t t o the parameters of t h e spot being i l luminated, the c e l l on which t h a t spot is located, and t h e remainder of t h e module:

CX is a constant , dependent upon the c h a r a c t e r i s t i c s of t h e spot being i l luminated, i . e . , rSX and rSHX. Fy i s a funct ion of t h e s lopes of t h e I-V curves ( i . e . , the dynamic impedances) of the c e l l being scanned and the remainder of the module a t the se lec ted b i a s cur ren t . ZM i s the e f f e c t i v e dc impedance of t h e remainder of the module a t t h e se lec ted b i a s cur ren t .

Computer Generated Resul ts

An 1108 EXEC 8 computing system was u t i l i z e d t o solve equation (1) f o r se lec ted s o l a r c e l l and module parameters, following an i t e r a t i v e proce- dure. The r e s u l t s presented i n t h i s paper a r e based ,upon the assumptions l i s t e d i n Appendix B. Various curves of Is vs VB were p lo t t ed f o r t h e following cases:

1. The c e l l being scanned contains loca l i zed inhomogeneities, represented by values of r~ and rsHX which d i f f e r from the nominal vafues .

2. The c e l l being scanned has t o t a l s e r i e s and/ o r shunt r e s i s t a n c e s which d i f f e r from t h e nominal values .

The computer simulation r e s u l t s a r e shown i n Figures 9 and 10. A reference curve f o r a c e l l hav- ing nominal parameters was included on each f igure . It should be r e a l i z e d t h a t these curves represen t a f i r s t order simulation. The computer program- tends t o average the dynamic impedances, ZM and Zy, between t h e i r values with and without i l luminat ion. This is, i n e f f e c t , an assumption of low c a r r i e r

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A B C

a) No Bias Current

A B C

-

FIGURE 6. Cell-to-cell br ightness changes with b i a s cur ren t .

i n j e c t i o n l eve l . The r e s u l t a n t curves a r e not in- tended t o represent any p a r t i c u l a r type of d e f e c t , but t o suggest t h e general trend of t h e i r e f f e c t s .

Figure 9 shows t h e e f f e c t s of loca l ized in- homogeneities, i . e . , where t h e parameters of t h e spot being il luminated a r e abnormal, but a l l c e l l s i n the module have t h e same nominal parameters. A s expected, higher s e r i e s r e s i s t a n c e o r diode current r e s u l t i n lower output. However, a region of lower than nominal shunt res i s tance , which would appear dark a t zero o r low b i a s cur ren t , may become br igh te r than surrounding regions a t b i a s cur ren t s over some crossover point , a s shown i n Figure 9b. ,Also, t h e d i f fe rence i n s igna l l e v e l , and there- f o r e t h e image con t ras t between regions of d i f f e r - ing parameters v a r i e s with t h e b i a s cur ren t l e v e l .

Figure 10 shows t h e dramatic e f f e c t of b i a s cur- r e n t on t h e ce l l - to -ce l l br ightness , when t h e c e l l being scanned has lower than nominal shunt r e s i s - tance. In agreement with t h e experimental r e s u l t s shown i n Figure 6, such a c e l l would appear dark a t low b i a s currents , but increase i n br ightness t o a much higher l e v e l a t some higher current l e v e l . Based upon these and other computer simulations, t h e following conclusions can be reached :

Images of c e l l s wi th low shunt r e s i s t a n c e w i l l i nc rease i n b r igh tness with appl ica- t i o n of b ias c u r r e n t , while normal c e l l images decrease i n br ightness . A cross- over point may be reached, such t h a t t h e ce l l - to -ce l l b r igh tness r a t i o s a r e reversed.

Similar bcightness changes could occur on loca l ized inhomogeneities.

Proper s e l e c t i o n of b i a s c u r r e n t l e v e l can improve t h e c o n t r a s t and d e t e c t a b i l i t y of loca l ized inhomogeneities.

CONCLUSIONS

The SCLS has proven t o be an exceedingLy u s e f u l instrument f o r t h e non-destructive evaluat ion and f a i l u r e a n a l y s i s of e n t i r e s o l a r modules, a s we l l a s ind iv idua l c e l l s . It can r a p i d l y d i sc r imina te between d e f e c t s which have an e f f e c t on t h e power output of modules and those which may only be cos- metic. Understanding t h e i n t e r a c t i o n between t h e in tense spot i l luminat ion and t h e module can f u r t h e r increase i ts usefulness , by permit t ing op t i - mum s e l e c t i o n of b i a s conditions.

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FIGURE 8. DC equivalent of a module of N c e l l s with s i n g l e spot i l luminat ion con- nected t o a current-to-voltage converter , C, with a dc o f f s e t vol tage, EB, and a b i a s cur ren t , IB'

The dark equivalent c i r c u i t f o r t h e e n t i r e c e l l .

b- FIGURE 7. DC equivalent of a module of N c e l l s

with s i n g l e spot i l luminat ion, connected t o a current-to-voltage converter with no b i a s cur ren t .

The same il luminated a rea equivalent c i r c u i t a s shown i n Figure 8.

An add i t iona l current generator, IX, i n p a r a l l e l with the above, where IX i s equal t o t h e current which would flow through t h e "il luminated area" a t a c e l l vol tage, VX, i f the l a s e r beam were o f f .

Now, with t h i s subs t i tu t ion , Iy i n Figure 8 becomes t h e t o t a l dark current which would flow through Cel l X a t vol tage VX. This may be calcu- l a ted from t h e standard diode equation. 10, the current flowing from the illuminaSed area, i? now the sum of two currents , IX and IoX, where IoX is t h a t por t ion of t h e generated photocurrents, IoX, which flows out of t h e i l luminated area. Applying t h e standard diode equation, these cur ren t s a re :

where :

I = diode d i f fus ion and recombination D~ and I% cur ren t s

0 = q / k ~ : q = e lec t ron charge; k = Boltzmann1s constant T = temperature, O K

Also :

APPENDIX A

Derivation of Equation (1)

In Figure 8, t h e c e l l being scanned by t h e l a s e r , Ce l l X, is represented by a small i l luminated area , ac t ing a s a cur ren t generator , i n p a r a l l e l with t h e remaining non-illuminated area . The non-illumi- nated remainder a c t s a s a passive diode-res is tor network load. This "load" equivalent c i r c u i t d i f - f e r s from t h a t f o r t h e e n t i r e c e l l only by the ef- f e c t s of t h e "missing" i l luminated area . By adding such an a rea t o t h e non-illuminated c e l l , i t s equiv- a l e n t c i r c u i t may be replaced by t h a t of the e n t i r e c e l l . This added a rea a c t s a s an add i t iona l cur- Define : r e n t load which must be compensated f o r by a paral- l e l current generator , which suppl ies p rec i se ly t h e same amount of cur ren t . Therefore, the representa- t i o n of Ce l l X i n Figure 8 may be replaced by a p a r a l l e l combination of t h r e e elements:

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150 I I I I I I I I I

- 1) STANDARD PARAMETERS

MODULE VOLTAGE, V B

a) Effects of High Diode Current (2) and High Series Resistance (3)

01 I 1 1 I I I I 1 0 10 20, 30 40

MODULE VOLTAGE, V B

150.

b) Effects of Low Shunt Resistance

I I I I I I I I

- 1) STANDARD PARAMETERS -

FIGURE 9. IS vs VB for a 40 cell module, showing effects of localized inhomogeneities at spot being illuminated. Iox = 5 mA.

150- 1 I I I I I I I I 1) STANDARD - PARAMETERS -

120 - 2) DIODE CURRENT

4 = 3 (STANDARD) - a (A

- - 90- 5

- OC w 3 - 0

-

60- - - V) P - -

30- - - -

0 I I I I I I I I I 0 8 16 24 32 40

MODULE VOLTAGE, V B

FIGURE 10. IS vs VB for a 40 cell module, showing effects of non-average parameters on the cell being scanned, IOx = 2 mA.

From the above, it may be shown that:

(5) Let ZM be defined as the effective static impedance of the (N-1) non-illuminated cells. The voltage across the cell being scanned, VX, can then be rep- resented as:

ZM is a function of IL which may be approximated by calculations, based upon average cell parameters for the type of cells in the module.

Also, by inspection of Figure 8:

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It should be r e c a l l e d t h a t VB is being held cons tan t because of t h e fixed o f f s e t vo l t age , EB, and t h e low input impedance of the current-to-voltage conver ter . Therefore, when t h e l a s e r i l lumina tes a spo t , IL decreases by an amount IS, r e s u l t i n g i n a drop i n t h e vo l t age a c r o s s t h e (N-1) non-illuminated c e l l s , AV. Iy must inc rease from its i n i t i a l value , IB, by some amount, A I y , such t h a t t h e corresponding in- c r e a s e i n t h e v o l t a g e drop a c r o s s c e l l X, AV, com- pensates f o r t h e reduced voltage-drop ac ross t h e o the r c e l l s of t h e module. Let Zy and ZM be defined a s t h e dynamic impedance of t h e c e l l X, and t h a t of t h e r e s t of t h e s t r i n g , r e spec t ive ly . AIy can then be given by:

Define:

Is Fy = ~g. i . e . , Py = r a t i o of t h e output s i g n a l (9)

c u r r e n t t o t h e photocurrent in jec ted ac ross c e l l X. Applying equat ions (7) and (8), (9) becomes:

Fy can t h e r e f o r e b e ca lcu la ted from t h e character- i s t i c s of c e l l X and t h e remaining non-illuminated c e l l s , by ass ign ing appropr ia t e va lues f o r t h e i r d iode c u r r e n t s , s e r i e s and shunt r e s i s t a n c e s , f o r s e l e c t e d c u r r e n t l e v e l s , IB.

F i n a l l y , t h e d e s i r e d equat ion ( I ) , i s der ived by s u b s t i t u t i n g (6) and (9) i n t o (5).

APPENDIX B

Assumed cond i t ions f o r computer-generated curves of Figures 9 and 10.

1. Module c o n s i s t s of a s e r i e s s t r i n g of f o r t y c e l l s , each having a diameter of 25 mm.

2. Module i s a t room temperature; the re fo re : f? = 39.

3 . Laser generated photocurrent : I = 2 mA and 5 mA. Ox

4. Nominal c e l l parameters assumed f o r a l l 39 non-illuminated c e l l s :

-10 J = 0.7 x 1 0 amperes Px

J?x = 0.54 x amperes

R = 0.09 ohms sx

5. Laser spot s i z e = 1 mm. Therefore, t h e fac- t o r used t o c a l c u l a t e rSX and r S ~ X i s 625,

from t h e r a t i o of t h e spot s i z e t o t h e c e l l a r e a .

REFERENCES

1. E.L. Mi l l e r , A. Shumka, and M. Gauthier, "A Laser Scanner f o r Solar C e l l Evaluation and F a i l u r e Analysis", Proceedings of t h e Advanced Techniques i n F a i l u r e Analysis Symposium (IEEE), pp 16-24, (1978).

2. K. Lehovec and A. Fedotowsky, "Scanning Light Spot Analysis of Faul ty Solar Cells", Sol id S t a t e E lec t ron ics 23, pp 365-576 (1980).

3. D.A. Yates and R.O. Be l l , "Defect Analysis of Ribbon Solar C e l l s Using A Laser Scanner1', Pro- ceedings of t h e 14 th IEEE Photovol ta ic Special- is ts Conference, pp 1402-1403 (1980).

4. D.E. Sawyer, "A Technique f o r Using an Opt ica l Scanner t o Reveal Solar C e l l Defects", Proceed- ings of t h e 13 th IEEE Photovol ta ic S p e c i a l i s t s Conference, pp 1249-1250 (1978).

ACKNOWLEDGEMENTS

The authors would l i k e t o express t h e i r appreci- a t i o n t o Sid Johnson and Tam Nguyen (JPL) f p r pro- v id ing many of t h e SCLS photographs used i n t h i s r e p o r t . They would a l s o l i k e t o thank Bruce Hancock (now a t the Univers i ty of Ca l i fo rn ia a t Santa Barbara) f o r h i s work i n t h e development of t h e s i g n a l ampl i f i e r , and Harold Becker f o r t h e des ign and development of t h e camera used t o photo- graph the TV monitor.