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Hindawi Publishing CorporationInternational Journal of PhotoenergyVolume 2013, Article ID 925280, 9 pageshttp://dx.doi.org/10.1155/2013/925280
Research ArticleEffect of Temperature and Humidity on the DegradationRate of Multicrystalline Silicon Photovoltaic Module
N. C. Park,1 W. W. Oh,2 and D. H. Kim2
1 Components & Materials Physics Research Center, Korea Electronic Technology Institute, No. 68 Yaptap-dong, Bundang-gu,Seongnam-si, Gyeonggi-do 463-816, Republic of Korea
2Department of Materials Science and Engineering, Korea University, Anam-dong, Seongbuk-gu, Seoul 136-701, Republic of Korea
Correspondence should be addressed to N. C. Park; [email protected] and D. H. Kim; [email protected]
Received 2 October 2013; Accepted 14 November 2013
Academic Editor: Dionissios Mantzavinos
Copyright ยฉ 2013 N. C. Park et al. This is an open access article distributed under the Creative Commons Attribution License,which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
In a PV module, the relative humidity (rh) of a front encapsulant is different from that of a backside encapsulant (rhback). In thisstudy, the effective humidity (rheff ) in a PV module was investigated to study the effects of moisture variation on the degradationrate (๐
๐ท). rheff represents uniform humidity in a PV module when it is exposed to certain damp heat conditions. Five types of
accelerated tests were conducted to derive the relation between rheff and rhback. rheff showed a linear relationship with rhback atconstant temperature. Two types of models, namely, Eyring and Peck models, were used for predicting the ๐
๐ทof PV modules,
and their results were compared.The ๐ ๐ทof PVmodules was thermally activated at 0.49 eV. Furthermore, the temperature and rheff
history of PVmodules over one year were determined at two locations:Miami (FL, USA) and Phoenix (AZ, USA).The accumulated๐ ๐ทvalues based on the temperature and rheff of the modules were calculated by summing the hourly degradation amounts over
the time history.
1. Introduction
Moisture can diffuse into photovoltaic (PV)modules throughtheir breathable back sheets or their ethylene vinyl acetate(EVA) sheets [1]. When in service in hot and humid climates,PV modules experience changes in the moisture content, theoverall history of which is correlated with the degradation ofthe module performance [1]. If moisture begins to penetratethe polymer and reaches the solar cell, it can weaken theinterfacial adhesive bonds, resulting in delamination [2] andincreased numbers of ingress paths, loss of passivation [3],and corrosion of solder joints [4, 5]. Of these possibilities, theoccurrence of corrosion has one of the highest frequenciesin outdoor-exposed PV modules [6]. Significant losses inPV module performance are caused by the corrosion ofthe cell, that is, the SiNx antireflection coating, or thecorrosion of metallic materials, that is, solder bonds andAg fingers [7, 8]. Corrosion is defined as the destructivechemical or electrochemical reaction of a metal with its
environment. The moisture from the environment may leadto electrochemical reactions that can result in corrosion.For the electrochemical reaction of metals with their envi-ronment, an aqueous, ion-conduction enabling environmentis necessary; moreover, at high temperatures, gas-metalreactions are possible [9]. The International ElectrotechnicalCommission (IEC) 61215 test defines a damp heat (DH)test in 10.13. The DH test is conducted for determining theeffect of long-term penetration of humidity on materials.Therefore, many researchers have studied the reliability ofPV modules on the basis of IEC 61215. Laronde et al. [10]have employed DH testing to study the degradation of PVmodules subjected to corrosion. Peike et al. [11] have reportedthat grid corrosion or reduced conductivity between theemitter and grid is the most likely cause of DH-induceddegradation. They have also shown that high temperaturesaccelerate water vapor permeation into the module and thesubsequent degradation reactions. Furthermore, it has beenreported that loss of adhesion strength is exacerbated by
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2 International Journal of Photoenergy
exposure to high humidity environments [2] and facilitatesthe delamination of EVA from the cell [3], which results ingrid corrosion [12]. Therefore, in order to understand theeffect of grid corrosion on the degradation of PV modules,one needs to comprehend how the surrounding environmentaffects the module temperature (๐
๐) and moisture content of
themodule. Kempe [1] has suggested that analytical equationscan be used to determine timescales formoisture ingress withbreathable back sheets. Koehl et al. [13] have showed thatthe maximum moisture concentration in front of a cell wasnot reached after 1,000 h under DH conditions at 85โC and85% rh because of the long path to the back sheet. They havealso documented that the humidity in front of the cell is notdirectly influenced by ambient fluctuations in actual weatherconditions.
As mentioned above, PV modules are degraded by ambi-ent temperature and humidity; moreover, these factors canaccelerate the degradation.This degradation is mainly causedby corrosion [4, 5, 7, 8, 10, 11]. It can be assumed that thetemperature of a PV module is uniform; however, moistureconcentration in a PV module is not uniform.Therefore, it isdifficult to predict moisture-induced degradation.
Therefore, in this study, effective humidity (rheff ) in aPV module was investigated to study the effect of moisturevariation in a PV module. rheff represents uniform humidityin a PVmodule when it is exposed to certain DH conditions.This paper documents the relation of rheff with ambienttemperature and humidity. Moreover, the resultant moduledegradation rate (๐
๐ท) for various rheff values is also reported
in this paper. These data allow the prediction of real-worldthermal- andmoisture-induced๐
๐ทvalues of PVmodules and
enable the computation of acceleration factor (AF) for theDHtest.
2. Experiments
Six-inchmulticrystalline Si (m-Si) solar cells were used in thisstudy.The typical characteristics of the cells at a light intensityof 1 sun were approximately as follows: open-circuit voltage(๐oc), 0.60V; short-circuit current density (๐ฝsc), 33.9mA/cm
2;fill factor (FF), 0.72; and conversion efficiency, 16.8%.
A copper ribbon wire, which was plated with62Sn36Pb2Ag solder, was used for cell interconnection.The dimensions of the ribbon wire were 0.15mm ร 1.5mm.The samples were divided into two groups on the basisof lamination conditions. Type 1 was arranged with EVA,cell, and EVA. Type 2 was laminated with low-iron glass ofarea 180mm ร 180mm and thickness 3.2mm, an EVA ofthickness 0.35mm, a cell, an EVA, and a TPT back sheet ofthickness 0.35mm, as shown in Figures 1(a), 1(b), and 1(c).The solar cells were laminated with EVA by heating themup to 150โC for 12min. After encapsulation, the sampleswere divided into five groups and exposed to acceleratedstresses, as shown in Table 1. Five kinds of test conditionswere selected: 85โC, 85% rh (8585), 65โC, 85% rh (6585),and 45โC, 85% rh (4585) for temperature acceleration and65โC, 75% rh (6575), and 65โC, 65% rh (6565) for humidity
Table 1: Test conditions for accelerated tests.
Number Temperature(โC)Relative
humidity (%)Sample size
(EA)1 85 85 102 65 85 103 45 85 104 65 75 105 65 65 10
acceleration. A total of five cases, each with ten samples, weretested. DH conditions were obtained in an environmentalchamber (Hygros340C, ACS Co., Massa Martaba, Italy).
The electrical performance of each sample was measuredevery 200 h using a solar simulation system (K202 Lab200,Mac Science, Seoul, South Korea). The standard test condi-tions were (a) irradiance: 1000W/m2, (b) cell temperature:25โC, and (c) spectral distribution of irradiance: AM 1.5G(IEC 60904-3).
Accelerated tests (ATs) were conducted for 4,500 h for8585, 6585, and 4585 and for 3,200 h for 6575 and 6565. Themaximum power of all samples decreased by over 5% afterthe ATs. Using the results, the average ๐
๐ทfor each condition
was calculated.
3. ๐ ๐ท
Prediction Models andEffective Humidity
๐ ๐ทdata can be postulated with an empirical kinetic model
by assuming that the rate of degradation is proportional tothe concentration of water in PV modules, and that the rateconstant has Arrhenius temperature dependence.
Escobar and Meeker [14] has proposed two degradationmodels: variations of Eyring and Peckmodels, which are usedfor operating conditions when temperature and humidity arethe accelerated stresses in a test. The degradation rate basedon the Eyring model (๐
๐ท,Eyring) is given by
๐ ๐ท,Eyring = ๐ด exp(
โ๐ธ๐
๐๐โ๐
rh) , (1)
where ๐ธ๐is the thermal activation energy of the degradation
process (eV), ๐ is the Boltzmann constant (8.62ร10โ5 eV/K),๐ is the temperature (โK), and rh is the relative humidity (%).๐ด and ๐ are two constants dependent on the failure mode. ๐
๐ท
(%/h) is the inverse of the mean time to failure (MTTF) ata given condition. In order to obtain ๐
๐ท, we determined the
time to 5% reduction in the initial maximum power (๐max)at all samples. The life distributions were determined withALTA 7 software. Using the results, theMTTFwas calculated.
The other degradation model based on the Peck model(๐ ๐ท,Peck) is expressed as follows:
๐ ๐ท,Peck = ๐ต exp (
โ๐ธ๐
๐๐) โ (rh)๐, (2)
where ๐ต and ๐ are two constants dependent on the failuremode.
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International Journal of Photoenergy 3
Cell
EVA
(a)
(b) (c)
Cell
EVA
Back sheet
Glass
Figure 1: Test samples for DH tests: (a) PV module with EVA/cell/EVA structure (Type 1), (b) PV module with glass/EVA/cell/EVA/backsheet structure (Type 2).
0.7
0.8
0.9
1.0
0 1000 2000 3000 4000Time (h)
Type 1: EVA/cell/EVA
Aver
age n
orm
aliz
edP
max
85โC, 85% rh 65โC, 85% rh45โC, 85% rh 65โC, 75% rh65โC, 65% rh
Figure 2: Average normalized ๐max of Type 1 as a function of time.
In order to obtain๐ด,๐ธ๐in (1) and๐ต, ๐ in (2), the equations
can be represented on a logarithmic scale by a straight line,using the following equations:
ln (๐ ๐ท,Eyring) = ln (๐ด) โ (
๐ธ๐
๐๐) โ (๐
rh) ,
ln (๐ ๐ท,Peck) = ln (๐ต) โ (
๐ธ๐
๐๐) + ๐ ln (rh) .
(3)
A plot of the left-hand side of (3) versus 1/๐ (โK) gives anArrhenius plot with a slope ๐ธ
๐/๐ and an intercept ln(๐
0).
ln(๐ ๐ท) versus 1/๐ (โK) gives an Arrhenius plot with a
slope ๐ธ๐/๐ and intercepts ln(๐ด) and ln(๐ต).
The rh in PV modules depends on their ambient cli-mate, material (encapsulant, back sheet) properties, and theoperation conditions. If all information is available, moistureconcentration in the backside encapsulant can be calculated
using the diffusionmodel [1]. However, the moisture concen-tration in the front encapsulant is different from that at theback of the cell because of the long path from the back sheet[13]. In a 85โC, 85% rh test, the maximum moisture contentin the backside encapsulant was reached quickly; however,the maximum moisture content of the front encapsulantwas not reached even after 1,000 h of exposure time [13].Therefore, rheff of a PV module was considered to determinethe uniform moisture content in the module.
In order to derive the effect of uniform humidity in a PVmodule on its degradation, PVmodules with a EVA/cell/EVAstructure (Type 1) were used as shown in Figure 1(a). This isbecause the cell and EVA layer structure allow water vaporto permeate the surface of the cell within minutes during theDH test [15].
In case of Type 1, it can be assumed that the rh in thePV module is uniform. If ๐ธ
๐and constants (๐ด, ๐ต, etc.) are
determined, the degradation rate of Type 1 (๐ ๐ท,Type1) can be
predicted with
๐ ๐ท,Type1,Eyring = ๐ด1 exp(
โ๐ธ๐,Type1
๐๐1
โ๐1
rh1
) ,
๐ ๐ท,Type1,Peck = ๐ต1 exp(
โ๐ธ๐,Type1
๐๐1
) โ (rh1)๐1
.
(4)
However, in case of glass/EVA/cell/EVA/back sheet struc-ture (Type 2), rh is not uniform in the PVmodule.Therefore,it is difficult to fix the rh in the PV module. If ๐
๐ท,Type2 isknown, ๐
๐ท,Type2 is expressed with the right-hand side of (4),and rheff is as follows:
๐ ๐ท,Type2 = ๐ด1 exp(
โ๐ธ๐,Type1
๐๐1
โ๐1
rheff,Eyring) ,
๐ ๐ท,Type2 = ๐ต1 exp(
โ๐ธ๐,Type1
๐๐1
) โ (rheff,Peck)๐1
,
(5)
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4 International Journal of Photoenergy
0
20
40
60
80
100
0 20 40 60 80 100rh of the backside EVA (%)
Eyring model
y = 0.8555x + 0.4114
R2 = 0.9986
rheff
(%)
T = 65โC
(a)
0 20 40 60 80 100
rheff
(%)
0
20
40
60
80rh = 85%
Eyring model
y = โ0.0275x + 73.521
R2 = 0.9973
Module temperature (โC)
(b)
0
20
40
60
80
100
0 20 40 60 80 100rh of the backside EVA (%)
rheff
(%)
T = 65โC
Peck model
y = 0.8552x + 0.1582
R2 = 0.9999
(c)
0 20 40 60 80 100
rheff
(%)
0
20
40
60
80rh = 85%
Module temperature (โC)
Peck model
y = โ0.0300x + 74.4167
R2 = 0.9908
(d)
Figure 3: rheff versus rh for the backside EVA and rheff versus module temperature are plotted for two ๐ ๐ท prediction models: (a) rheff versusrh for the backside EVA at constant temperature for Eyringmodel, (b) rheff versusmodule temperature at constant humidity for Eyringmodel,(c) rheff versus rh for the backside EVA at constant temperature for Peck model, (d) rheff versus module temperature at constant humidity forPeck model.
where ๐ธ๐,Type1 and other parameters (๐ด1, ๐1, ๐ต1, and ๐1) can
be determined by ATs as shown in Table 1. Using (5), rheff isrearranged as follows:
rheff,Eyring =โ๐1
ln (๐ ๐ท,Type2) โ ln๐ด1 + (๐ธ๐,Type1/๐๐1)
, (6)
rheff,Peck = (๐ ๐ท,Type2
๐ต1exp(โ๐ธ
๐,Type1/๐๐1))
1/๐1
. (7)
4. Results
4.1. Results of Accelerated Tests. The changes in averagenormalized ๐max of the modules in Type 1 as a function
of time are plotted in Figure 2. The figure shows that ๐maxdecreases linearly over time.The results correspond well withthose found in earlier studies [6, 16]. Several authors [17, 18]argue that the limited experimental evidence available is notenough to take the linear ๐
๐ทfor granted and suggest that
an exponential degradation rate could be a more suitabletrend as is the case in some optoelectronic devices. However,it should be noted that both trends exhibit very similarevolution during the first 10โ15 years; if similar initial annualdegradation rates are assumed, then the linear degradationrate is a more pessimistic estimate [19].
In order to keep the discussions simple, we will notconsider the exponential degradation rate here.
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International Journal of Photoenergy 5
0.8
0.9
1.0
1.1
0 1000 2000 3000 4000Time (h)
Ave
rage
nor
mal
ized
Pm
ax
Conditions: 65โC, 65% rh
RD,Type2 (%/h) = 0.00079
0.7
0.8
0.9
1.0
1.1
0 1000 2000 3000 4000Time (h)
Ave
rage
nor
mal
ized
Pm
ax
Conditions: 65โC, 75% rh
RD,Type2 (%/h) = 0.00132
0.7
0.8
0.9
1.0
1.1
0 1000 2000 40003000 5000Time (h)
Ave
rage
nor
mal
ized
Pm
ax
Conditions: 45โC, 85% rh
RD,Type2 (%/h) = 0.00087
0.7
0.8
0.9
1.0
1.1
0 1000 2000 40003000 5000Time (h)
Ave
rage
nor
mal
ized
Pm
ax
Conditions: 65โC, 85% rh
RD,Type2 (%/h) = 0.00208
0.7
0.8
0.9
1.0
1.1
0 1000 2000 3000Time (h)
Ave
rage
nor
mal
ized
Pm
ax
Conditions: 85โC, 85% rh
RD,Type2 (%/h) = 0.00611
Figure 4: Average normalized ๐max of Type 2 as a function of time. โป shows the measurement data, dotted line (black) shows the predicteddegradation rate obtained using (1), and straight line (red) shows the predicted degradation rate obtained using (2).
Using AT results of Type 1 samples, the ๐ ๐ทwas deter-
mined for each set of conditions.๐ธ๐is obtained by fitting the ๐
๐ทdata in (1) and (2) for
three values of temperature. ๐ธ๐,Type1 and other constants were
calculated as summarized in Table 2.๐ ๐ท,Type2 of the modules was also determined for each
set of conditions. The ๐ ๐ทvalues (%/h) of 8585, 6585, 4585,
6575, and 6565 were 0.00611, 0.00208, 0.00087, 0.00132, and0.00079, respectively.
In order to derive the relationship between rheff and rhin the backside encapsulant, ๐
๐ท,Type2 in (4) was replacedwith ๐
๐ทvalues. Figure 3 shows a plot of rheff versus rh
in the backside encapsulant at a constant temperature andconstant humidity. In bothmodels, rheff versus rh has a linear
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6 International Journal of Photoenergy
30
50
70
85
298 318 338 358Temperature (K)
rheff
(%)
0โ100100โ200200โ300
(a)
30
50
70
85
298 318 338 358Temperature (K)
rheff
(%)
0โ100100โ200
(b)
Figure 5: AF Contours of module temperature and rheff for two ๐ ๐ท prediction models: (a) Eyring model, (b) Peck model.
Table 2: Activation energy and constants of Type 1 samples forEyring and Peck models.Model ๐ธ
๐๐ด1
๐1
๐ต1
๐1
Eyring 0.49 2.40 ร 106 281.86 โ โ
Peck โ โ 0.0037 3.82
relation at a constant temperature, and rheff decreases linearlywith temperature at constant humidity (inset in Figure 3).Therefore, rheff is expressed as follows:
rheff,Eyring = [(73.521 โ 0.0275 โ ๐)]
โ 0.8555rhback + 0.4114
71.2,
(8)
rheff,Peck = [(74.417 โ 0.0300 โ ๐)]
โ 0.8552rhback + 0.1584
71.9.
(9)
Using rheff values at AT conditions, predicted ๐ ๐ทs,Type2of (5) are plotted as a function of time in Figure 4. It showsthat the predicted๐
๐ท,Type2 is almost identical to themeasureddata.
4.2. Acceleration Factor. AF is defined as the ratio betweenthe ๐
๐ทat a given temperature, rheff and ๐ ๐ท at a reference
temperature, and rheff (in our case 25โC, 50% rh) [20]. AF
is expressed as
AFEyring = exp [โ๐ธ๐,Type1
๐(1
๐0
โ1
๐) + ๐1(1
rh0
โ1
rheff)] ,
AFPeck = exp [โ๐ธ๐,Type1
๐(1
๐0
โ1
๐)](
rh0
rheff)
๐1
,
(10)
where ๐0and rh
0are the reference temperature and reference
humidity, respectively.Figure 5 shows the AF contours on plots of rheff ver-
sus module-temperature data. Estimated AFs for the 8585
condition versus 25โC, 50% rh range from 190ร to 250รfor the Peck and Eyring models, respectively. However, inreal-world operation, a constant temperature and rh are notrealistic. To project field ๐
๐ทat a specific location, it was
characterized by the annual module temperature and rh ofthe backside encapsulant.
5. ๐ ๐ท
in Two Benchmark Climates
Two benchmark climates (BMCs) were selected to quantifythe stress: Miami (FL, USA) and Phoenix (AZ, USA). Themodule-temperature history exposed to the two BMCs wasderived from meteorological data [21]. Meteorological datafor Miami, FL, for 2005 and Phoenix, AZ, for 2002 wereobtained from the National Climatic Data Center.
The rh of the backside encapsulant was calculated usingthe model of moisture ingress [1]. We determined theactivation energy for encapsulant solubility in a previousresearch [22]. ๐ธ
๐for maximum water vapor transmission
rate (WVTRmax) of back sheets was evaluated. The tran-sient WVTR was measured using a WVTR instrument(Permatran-W3/33, Mocon, Minneapolis, MN, USA) at 25โC,37.8โC, and 50โC. Assuming an Arrhenius equation betweenWVTRmax and temperature, WVTRmax can be described by
WVTRmax = ๐ด exp (โ๐ธ๐ค
๐๐) . (11)
Parameters ๐ด and ๐ธ๐คwere obtained from a curve fit of a plot
of of ln(WVTRmax) versus 1/๐๐. The ๐ด and ๐ธ๐ค values are2.703 ร 10
6 g/m2/day and 0.367 eV, respectively.The accumulated ๐
๐ทbased on the module temperature
and rheff can be calculated by summing the hourly degrada-tion amounts over the time history, as given by
โ๐ ๐ท,Type2 โ ๐ก = [๐ด1 exp(
โ๐ธ๐,Type1
๐๐1
โ๐1
rheff,Eyring)] โ ๐ก,
โ๐ ๐ท,Type2 โ ๐ก = [๐ต1 exp(
โ๐ธ๐,Type1
๐๐1
) โ (rheff,Peck)๐1
] โ ๐ก.
(12)
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International Journal of Photoenergy 7
0
20
40
60
80
100
Module temperature
rheff
Tem
pera
ture
(โC)
,rh e
ff(%
)
January February March April May June July August September October November December
0
20
40
60
80
100
Tem
pera
ture
(โC)
,rh e
ff(%
)
0
20
40
60
80
100
Time (2005, Miami, FL)
Module temperature
0
20
40
60
80
100
Module temperature
Time (2002, Phoenix, AZ)
Time (January 1โผ10, 2005)
rheffTe
mpe
ratu
re (โ
C),r
h eff
(%)
January February March April May June July August September October November December
Time (October 1โผ10, 2005)
rheff
Tem
pera
ture
(โC)
,rh e
ff(%
)
Figure 6: Module temperature and rheff over one year in 2 benchmark climates. rheff is determined with (8) for Eyring model.
Thermal and rheff,Eyring history of a PV module over oneyear were calculated at two BMCs as shown in Figure 6.Compared with Miami, the module temperature at Phoenixis shifted more than 10โC higher and the rheff has a relativelylow distribution.
Accumulated ๐ ๐ทin the two BMCs is calculated using
(12), which are based on the module temperature and rheffof Figure 6.
The normalized ๐ ๐ท,Eyring and ๐ ๐ท,Peck of the PV module
exposed to two BMCs are plotted over one year in Figure 7(a).The accumulated ๐
๐ท,Peck was 3.0% greater than ๐ ๐ท,Eyring inMiami.The conditions of 8585 are normally used forDH testsas IEC 61215.Therefore, the accumulated ๐
๐ทexposed to 8585
was evaluated and compared to the accumulated ๐ ๐ทin the
Miami. The accumulated ๐ ๐ท,Eyring and ๐ ๐ท,Peck for exposure
to 8585 were about 23.7 and 23.1 times greater than those in
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8 International Journal of Photoenergy
1.00 1.03
0.04 0.07 0.0
0.2
0.4
0.6
0.8
1.0
1.2
1.4
Miami,Eyring
Miami,Peck
Phoenix,Eyring
Phoenix, Peck
Nor
mal
ized
RD
over
one
yea
r
RD prediction model
(a)
23.7
9.5
23.1
9.3
0
5
10
15
20
25
30
8585 6585
Acce
lera
tion
fact
or
Accelerated conditions
EyringPeck
(b)
Figure 7: Normalized ๐ ๐ทexposure to actual weather conditions for 1 year and AF of accelerated conditions: (a) normalized ๐
๐ท,Eyring and๐ ๐ท,Peck for an initially dry module after exposure to two BMCs, (b) AF exposure to 85
โC, 85% rh and 65โC, 85% rh is compared to that atMiami (FL, 2005).
Miami, as shown in Figure 7(b). Koehl et al. [13] have reportedthat AF of 8585 is about 23 for a tropical site (Serpong,Indonesia), 40 for an arid site (Sede Boqer, Israel), and 106 foran alpine site (Zugspitze, Germany) for a degradation processwith an activation energy of 0.416 eV.
In case of 6585, the ๐ ๐ทvalues according to Eyring and
Peckmodels are 9.5 and 9.3 times greater than those inMiami.Therefore, it can be supposed that the Peck model is a slightlyconservative estimation for ๐
๐ทprediction.
6. Conclusions
The objectives of this study were to investigate the relationof ambient temperature and humidity with the rheff of a PVmodule and to use the rheff values to predict the ๐ ๐ท valuesunder actual weather conditions.
The degradation of PV modules is accelerated by tem-perature and humidity [1, 4, 5, 10, 11]. It can be assumedthat the temperature in a PV module is uniform. However,the moisture concentration is not uniform [13]. Therefore,we used a Type 1 module with a EVA/cell/EVA structure foruniform humidity in the module.
Two types of models, namely, Eyring and Peck models,were used for ๐
๐ทprediction, and their results were compared
with each other. Five types of ATs were conducted to deter-mine ๐ธ
๐and humidity dependence. The ๐
๐ทs of PV modules
were thermally activated at 0.49 eV.The moisture content in a PV module is dependent on
material properties such as back sheets and EVA. Therefore,we determined the relation between the rh of the backsideencapsulant and rheff . rh of the backside encapsulant wascalculated using the moisture ingress model. Thermal andrheff history of a PV module over one year were calculated intwo BMCs. For exposure to 8585, the accumulated ๐
๐ท,Eyringand ๐
๐ท,Peck values at Phoenix were, respectively, about 23.7and 23.1 times greater than those at Miami.
Abbreviation:
AF: Acceleration factorAT: Accelerated testsBMC: Benchmark climateDH: Damp heatEVA: Ethylene vinyl acetateFF: Fill factorIEC: International Electrotechnical Commission๐ฝsc: Short-circuit current densityMTTF: Mean time to failurePV: Photovoltaic๐ ๐ท: Degradation rate๐ ๐ท,Eyring: Degradation rate based on the Eyring model๐ ๐ท,Peck: Degradation rate based on the Peck model
rh: Relative humidityrhback: Relative humidity of a backside encapsulantrheff : Effective humidity๐๐: Module temperature๐oc: Open-circuit voltage.
Acknowledgments
This work was supported by the New and Renewable Energyof the Korea Institute of Energy Technology Evaluation andPlanning (KETEP) Grant funded by the Ministry of Trade,Industry and Energy (MOTIE) (no. 2012T100100605). Fur-thermore, this work was supported by the Human ResourcesDevelopment of the Korea Institute of Energy TechnologyEvaluation and Planning (KETEP) Grant funded by theKorea Governments Ministry of Knowledge Economy (no.20104010100640).
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