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TRANSCRIPT
Microstructural Studies on Fire-Through Front
Contact Metallization of Si Solar Cells
Suhaila Sepeai, M.Y.Sulaiman, Saleem H.Zaidi, Kamaruzzaman Sopian Solar Energy Research Institute (SERI)
Universiti Kebangsaan Malaysia (UKM)
43600 UKM Bangi, Selangor, Malaysia
Email: [email protected]/ [email protected]
Abstract- Screen-printed Silver/Argentum (Ag) metallization is
used in the photovoltaic industry for the front-side emitter
contacts of crystalline silicon solar cells owing to its cost-
effectiveness and high throughput. In order to obtain a better
understanding for the formation of Ag paste and silicon (Si)
interface, the firing treatment was studied. The microstructure
properties of the fire-through Ag metal contacts formed on
pyramid textured silicon wafers are investigated. The best firing
temperature is 800!"#$%&'#()#*+,)#-%.-/%�*1&(2,#(񔔗#()8#
efficiency of 13.67%. The Scanning Electron Microscopy (SEM)
characterization of Ag shows that as the temperature further
increased, the particles of Ag fuse together and the decrease of the
Ag thin film thickness indicates that n+ layer has been formed.
I. INTRODUCTION
Front contact formation is critical for achieving high
efficiency solar cells. Requirements for a good front contact are
uniform, low resistance and have an ohmic contact with high
shunt resistance. Such a contact will produce a high open-
circuit voltage (Voc) and high fill factor (FF) [1]. Fire-through
metallization is the most common method for forming front
contact on screen-printed silicon solar cells. Screen printing
technique typically used in industrial metallization due to its
cost-effectiveness, rapid and simple production, compared to
the photolithography and buried-contact techniques which is
time-consuming and expensive [2]. The applied metallization
technique determines the shadowing and series resistance
losses, determines the emitter diffusion profile and surface
doping concentration[3].
An aspect of considerable importance is the issue of metal
contacts on the n-side of the silicon solar cell. Argentum (Ag)
and aluminium (Al) pastes typically use for the front and back
contacts, respectively. Requirements for a good paste are low
resistivity, good printability and good adhesion. It allows a
good contact formation on shallow homogeneous emitters [4].
Low resistivity ohmic contact also desirable to prevent current
losses and contribute in the increase of efficiency [5]. In solar
cell manufacturing, the contact firing is usually done in
infrared (IR) heated conveyor belt furnaces. Rapid firing at a
high temperature is done to avoid the degradation of the
electrical quality of the Ag metal contact [6].
In this research, we have investigated the microstructure of
the front-side contact/solar cell emitter interface fired at
temperatures of 650 to 800!C. It shows that the metal contacts
could be fired at a higher temperature in air ambient which
facilitates the formation of low resistance ohmic contacts
between the silver metal and n+ silicon surface. This process is
very simple and has advantage of making fire-through ohmic
contacts on shallower emitters.
II. EXPERIMENTAL
Solar cell devices with a basic structure which is consist of
p-type silicon (Si) wafer, n-type semiconductor, sandwiches by
Argentum (Ag) and Aluminium (Al) as a front and back
contact was fabricated. The structure is shown in Figure 1. The
<100> Si wafer substrate was used. The Si wafer was initially
cleaned by dipping into solution of hydrofluoric acid (HF) and
nitric acid (HNO3) in a ratio of 1:100 for 10 minutes. After
rinsing with deionized water, it was then dipped into HF and
water (H2O) in a ratio of 1:50 for 1 minute. The wafer was then
immersed in 10% potassium hydroxide (KOH) at a temperature
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cleaned in HF:H2O. The wafer should be hydrophobic when
tested with water to indicate that it was finally cleaned.
The texturing process was undertaken after the cleaning
procedure. The wafers were textured using a solution of KOH,
iso-propil alcohol (IPA) and H2O in the ratio of 1:5:125. After
the texturing process, the wafers were subjected to the n-type
diffusion procedure. The heavily doped n+ region was formed
on the Si wafer surface by phosphorous diffusion at 900°C for
RSM2011 Proc., 2011, Kota Kinabalu, Malaysia
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30 minutes using phosphorous oxychloride (POCl3) as the
diffusion source. The edges of Si wafers were then etched by
Xenon Difluoride (XeF2).
The wafers were then ready for the metallization process.
The Ag and Al pastes were screen-printed on both of Si wafers
forming the front and back contacts, respectively. After oven
drying at 100°C for 15 min, the solar cells were fired in a rapid
thermal annealing (RTA) furnace. The firing temperature was
varied in the range of 650&'#.!#=%%&'1##>8/#"+,+08/<#0!5:(#?/550#
were analyzed using light Current-Voltage (LIV) Measurement
System. The cross section images of solar cells and grain size
images of Ag paste have been characterized by Scanning
Electron Microscope with a magnification of 1000.
Fig. 1 The structure of basic Si solar cell device
III. RESULT AND DISCUSSION
Figure 2 shows the current-voltage (I-V) curve of basic Si solar cell. Based on the figure, it can be seen that the voltage or
open circuit voltage (Voc) increased with the increasing of
firing temperature. In typical result, the Voc value for the device
fired at 650, 730, 750 and 800°C are 0.468, 0.468, 0.480 and
0.492 V, respectively (Table 1). It is important to note here
that, despite the increase in the Voc as the temperature
increases, it also causes an increase in the short circuit current
(Isc), fill factor (FF), shunt resistance (Rsh) and efficiency. The
efficiency for the device fired at 650, 730, 750 and 800°C are
5.25, 5.69, 8.25 and 10.49, respectively. The inconsistent value
of ISC is due to the leakage current. When shunt resistance is low, the diode acts more like a resistive element. Thus, the
behavior becomes similar to that of a photoconductor.
It can be simply understood that, to increase the Voc, the
optimization of the interface characteristic and the carrier
mobility of the device are required. We have carried out the
firing treatment on the device, to achieve enhancement in
efficiency. We found that the performance of the device can be
substantially improved, reflecting the enhancement of the
carrier mobility in the device.
Fig. 2. I-V curve of solar cell with a variation on firing temperature, x = 650 –
880 °C
TABLE 1
SUMMARIZED RESULT FROM I-V CURVE WITH A VARIATION OF FIRING
TEMPERATURE
Temperature Voc Isc FF Rsh Eff
(%)
650 0.468 0.08523 0.41458 0.75 5.25
730 0.468 0.09241 0.48171 0.78 5.69
750 0.480 0.10970 0.49360 0.80 8.25
800 0.492 0.10805 0.62195 0.83 10.49
This assumption strongly confirmed by the Ag grain size
images of un-fired cell, fired at 650°C and 742°C (Figure 3-5).
SEM has characterized these images. The grain size of Ag
before firing process is 416.44 nm. There is an increase in the
particle size because the adjoining particles fuse together. As
the temperature is increased, many Ag particles agglomerate
and fuse together into bunches. At the peak temperature, some of the agglomerates close to the surface react with Si to form
n+ layer. The n+ layer provides the tunnel for electron. The
electron can move easily to the electrode and this enhances the
open circuit voltage (Voc).
Fig. 3. The grain size of Argentum paste before firing process.
RSM2011 Proc., 2011, Kota Kinabalu, Malaysia
365
Fig. 4. The grain size of Argentum paste for a firing temperature at 650°C
Fig. 5. The grain size of Argentum paste for a firing temperature at 742°C
There are other reasons for the increasing of the Voc of the
solar cells, for instance the thickness of the thin film that
closely related to the carrier diffusivity in the device. Figure 6
shows the cross section images of solar cells before firing
process. It is clearly shown that the Ag particles have not fuse
yet and the thin film of Ag is on the pyramid textured Si wafer.
Figure 7 and 8 shows cross section images of firing
temperature at 650 and 742°C, respectively. The thickness of
cell fired at 650°C is 16.72 µm, while the thickness of cell fired
at 742°C is 14.74 µm. From these figures, it is clearly shown
that the Ag paste diffuse in the n-type Si layer after firing process. This is proved that n+ layer has been form.
Fig. 6. The cross-section images of solar cell before firing process
Fig. 7. The cross-section images of solar cell for a firing temperature at 650°C
Fig. 8. The cross-section images of solar cell for a firing temperature at 742°C
Although the solar cell devices have been successfully obtained, however, their efficiency was still low, namely
10.49%. Since our assumption that the improvement of the
solar cells performance upon firing might be caused by the
change in the interface characteristic and carrier mobility, we
investigate the effect of Silicon Nitride (SiN) as anti-reflecting
coating in order to improve the efficiency. We study the optical
property, which is the reflectivity of the device. From the result
shows in Figure 9, it was found that the textured wafer still
have a high reflectivity in a range of visible light, 400 – 700
nm. It is indicates that the light is not fully absorb by the
textured wafer. Hence, fewer electrons generated and it leads to a low efficiency. The reflectivity is better after we applied SiN,
which is below 0.1. We then applied SiN to all the devices. The
result shows in Table 2, that the Voc, Isc, FF and efficiency were
improved. The highest efficiency obtained is 13.67%.
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366
Fig. 9. Reflectance of the planar, textured and textured with a SiN thin film on
Si wafer.
TABLE 2
SUMMARIZED RESULT FROM I-V CURVE WITH A VARIATION OF FIRING
TEMPERATURE
Temperature After SiN deposition
(°C) Voc Isc FF Eff.
(%)
650 0.468 0.081395 0.49877 6.03
730 0.504 0.12664 0.58529 11.86
750 0.492 0.14837 0.53305 12.35
800 0.504 0.13577 0.62937 13.67
IV. CONCLUSION
The best firing temperature of crystalline silicon solar cell have
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open circuit voltage at 0.5042V and efficiency of 13.67%. The
choice of this parameter will be used for future advanced solar
cell fabrication. It is hoped that it may lead to an increase in the
contact adhesion. The result of Scanning Electron Microscope
proved the formation of the n+ layer, which is, provides the
tunnel for the electron. Further research on higher firing
temperature and its effect on contact adhesion and thickness
will be reported out in the future.
ACKNOWLEDGEMENT
This work has been carried out with the support of the
Malaysia Ministry of Science, Technology and Innovation
(MOSTI) under the TechnoFund and Fundamental Research
Grant Scheme.
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