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A formula for the power in partially failed PV fields
G. Ambrosone, S. Catalanotti, U. Coscia, G. Troise
To cite this version:
G. Ambrosone, S. Catalanotti, U. Coscia, G. Troise. A formula for the power in partially failed PV fields. Revue de Physique Appliquée, Société française de physique / EDP, 1983, 18 (10), pp.645-649.
�10.1051/rphysap:019830018010064500�. �jpa-00245126�
A formula for the power in partially failed PV fields
G.
Ambrosone,
S.Catalanotti,
U. Coscia and G. TroiseIstituto di Fisica, Facoltà di Ingegneria, Università di Napoli, Piazzale Tecchio, Napoli, Italy (Reçu le 10 février 1983, révisé le 30 juin, accepté le 7 juillet 1983)
Résumé. 2014 Dans cet article nous présentons des formules analytiques donnant les courbes de puissance en fonction
de cellules endommagées pour quelques configurations. Les configurations analysées sont simples (au maximum
elles sont constituées par quatre niveaux de connexion) car les premiers niveaux sont les plus responsables de la perte en puissance.
Abstract. 2014 In this paper we present analytical formulae which give the curves of power as a function of failed cells, for some configurations. The configurations analysed are simple (maximum four connection levels) because
the first levels are the more responsible for the power decrease.
Classification
Physics Abstracts
86.30J
Introduction.
In
previous
papers[1, 2]
we have studied the decrease of the powersupplied by
aphotovoltaic
field with failed cells. In the first of these papers[1]
aproba-
bilistic
approach
has beenused;
itgives
exactanaly-
tical formulae which are difficult to use for
large
fields.In the second paper
[2]
the sameproblem
has beentreated with a statistical
approach;
in this case wehave
shown,
for severalconfigurations
of thefield,
the power decrease as a function of the failure number.
Both these methods
require long
computer cal- culations and therefore cannot be used for fieldconfigu-
ration
optimizations.
In this paper we want to overcome this obstacle
by introducing
ananalytical expression
for the power decrease as a function of the failure number and of the parameters of the field. Thisexpression
canbe
easily
used tostudy
theoptimal configuration taking
into account variousproblems
such as thefailure one, the connection costs, and so on.
Our
analytical
formula for the powerfunction,
inspite
of thesimplifications made,
issensibly
accurate.
In this paper our
hypotheses
on the cell characte- ristics and on the failures are not described asthey
were
widely
discussed in reference 1. Weonly study
ideal cells with fill factor
equal
to one and thefailures, mutually
exclusive andstatistically independent,
pro- duce a circuitopening
inside the failed cell.In the first section we
briefly
discuss the formalism and the powercomputation
used in thepaper.
Inthe second section we present an
analytical expression
for the power as a function of the failure number in PS fields. In section 3 we
expand
this formula tomore
complex
fields.Finally,
in section4,
we present asimple appli-
cation of our
formulae,
to determine theoptimal configuration
of aphotovoltaic
field.1. The power calculation.
This section is devoted to define some
quantities
and togive
some more details about ourproblem.
Let us consider T
cells;
thesymbol
s, pi ... sn pn represents, in this paper, a field in which S 1 cellsare series connected to constitute a group; pi groups
are connected in
parallel ; s2 sub-arrays
s 1 p, are connected inseries,
etc.Finally
p~sub-arrays
sl pi S2 ... SIt are connected in
parallel.
Obviously
we can writeThe current
1(0) supplied by
the intact field iswhere
/1
is the currentproduced by
asingle
cell.If there are R failed
cells,
the currentproduced by
the field will beproportional
to(1 - R +)
whereArticle published online by EDP Sciences and available at http://dx.doi.org/10.1051/rphysap:019830018010064500
646
R + is the number of ways in which the current cannot
flow. The fractional current will
be,
thereforeNow we can consider fields connected to a power
tracker,
to a storage cell or to a resistive load. In the last case the power will beproportional
to the square of the current whereas in the first two cases the power will beproportional
to the current. We can concludethat the ratio :
will represent the fractional power for fields connected to a power tracker or to a storage cell or the square root of the fractional power for fields connected to
a resistive load. If we are
mainly
interested in theslope
of the power curves, we can treat the ratioas the fractional power; it is obvious
that,
if the load isresistive,
the valuesgiven by
our formulae mustbe
squared.
We canconclude,
with thisexception,
that the fractional power is
The power
depends
on the failuredistribution,
so we must determine the mean value of the fractional power, over all the
possible distributions,
to obtain the mean fractional power(m.f.p.)
If we introduce the cell failure ratio
(c.f.r.)
we obtain
In a
previous
paper[2]
we have shown that PSfields have a
regular
behaviourand,
moreover, that(concerning
the failureproblem)
PS fields and themore
complex
ones(for
instanceSPS, PSP, SPSP)
are very similar. In this paper we will use these results to obtain an
analytical expression
for the power.We do not treat SP
fields;
weonly
recall that forSP fields it is
possible
to find the exactformula,
which can beeasily simplified by using
theproba-
bilistic
techniques.
2.
Analytical
form of them.f.p.
in PS fields.From the considerations of section
1,
we start to determine theanalytical
form of them.f,p.
for a PSfield. In this case the
m.f.p.
isgiven by
where R + is the maximum number of failed cells among the s
parallels.
Let us consider a P
field,
made up of pparallel
connected cells. The fractional power, when R failures occur, will be
For a P field we can write
i.e. the fractional power is
independent
of thespecific
distribution of the failures in the field.
Let us
consider,
now, a P2 field(i.e.
a field built up withonly
twoparallels).
The c.f.r. xp and xp2 whichsupply
the samem.f.p.
are relatedby
Moreover,
as it was stated in reference2,
values of c.f.r. xp, xp2l ..., Xp2.’ whichgive
the samem.f.p.
for
P, P2,
..., P2" fields mustobey
thefollowing
relations :
Consequently
We will assume
that,
for any sthen
To determine the function h we have calculated the values of the ratios
for fixed values of power wp,
with p
as parameter.These ratios are function of the power wp ; as
we can write
we can represent the ratios as a function of the failure
number Rp
= pxp.In
figure
1 the ratios areplotted
as a function ofRp
for four valuesof p (p
=3, 10, 20, 50)
and several values of s. As we can see, all thepoints
can be con-sidered as
belonging
to asingle
curve, whenRp
p.For
Rp ^~
p the curves aredependent
onthe p
value.In
equation
1 the function hdepends
on two para- meters w and p ;by
a semitheoreticalapproach
it ispossible
to deduce that these parameters are relatedso that the function h
depends only
on theparameter
p( 1 - w).
Fig. 1. - The ratios
Xp)Xp(2::.)
as a function of p. xp for several values of p and s. The curve represents the fit (withthe corrective exponential term) specified in the text.
Let us consider a P2 field. For a fixed value of R, the
possible
values of willcorrespond
tospecific
values of failed cellspertaining
to each ofthe
parallels.
Let us indicateby
R + thehigher
andby
R - the lower of these twovalues;
we will writewhere d represents the fluctuation of the failures
occurring
in twoparallels.
Thecorresponding
valueof the
fractional
power will beand furthermore
where
The mean value
(over
all thepossible
distributions of R failures in the P2field)
of thefluctuations, d,
will
depend,
of course, on R and p. Now we remarkthat,
if the failure number R is much lower than 2 p, the(R
+l)-th
failure can occur with identical pro-bability
in each of the twoparallels, independently
of the failures
already
occurred in eachparallel.
Therefore we can write
We
emphasize
that this formula is validonly
forR2p.
By using
thishypothesis, equation
2 becomesFor
physical
reasons the functionG(R)
must beinvertible and therefore we can write
Finally
we obtainbut
xp
= xp and thereforeWith this
analysis
we have obtained the same for- mula as inequation
1. Here thedependence
on p and xp isspecified
as adependence
on p. xp.Now we can use the results shown in reference 2 to
give
theexplicit
form of the functionh(p. xp).
As we can see in
figure 1,
the function h appears to be ahyperbola.
Therefore we use the functionThe values" of the
parameters
whichgive
the bestfit for all the
points,
areWe remark that our fit does not
give
agood
agree- ment for values ofRp
near 1,when p
issmall,
i.e.when the first failure causes a great decrease of the power. This
region
can be fittedby adding
an expo- nential term; we obtain a new functionwhere c = 4.129 x
1013
and = 32.058.Once the
explicit
form of the function h isknown,
we can compute the c.f.r. as a function of the
m.f.p.
value. We have
In
figure
2 we compare the power curve calculated with our formula to the exact resultspresented
inreference 2. As
expected,
the agreement is verygood
for
high
values of them.f.p.,
for any p and s. Theerror increases when the
m.f.p.
decreasesbecause,
in this case,
Rp ~
p and, aspreviously
said, our formulae arejustified only
if p.648
Fig. 2. - Power curves for several couples p, s. The full line curves represent the m.f.p. computed in reference 2;
the dashed line curves represent the fit presented in the
text.
3. The
analytical
form of them.f.p.
for morecomplex
fields.
In this section we want to
give
theanalytical
formulaof the
m.f.p.
for fields whose behaviour can beeasily
deduced from that of PS fields. As shown in reference 2 these fields are the
PSP,
the SPS and the SPSP field.3 .1 PSP FIELDS.
- By using simple
considerations(see
Ref.2)
for a pl Sl p2 fields we can writeif when
Consequently
we obtainif
or
for
In this case the current decrease caused
by
thefirst failure is
generally low,
therefore in theexplicit
formula of the function h the corrective
exponential
term is not needed.
3.2 SPS FIELDS. - In reference 2 we showed that in a
s1 PI S2 field the first series is not
relevant,
i.e. wecan write
if
This relation allows us to write
if
or
3 . 3 SPSP FIELDS. - The formula
previously
writtencan be used also for s, pl S2 P2 fields because the
m.f.p.
isindependent
on the lastparallel
connectionvalue p2.
In this case we write
for
or
for
4.
Application example.
To show the
utility
of our formulae for them.f.p.
we can
study a PS
field.Let us suppose that we
repair
the fieldonly
whenthe fractional power
supplied by
the field decreases below 0.8.We want to determine the maintenance cost as a
function of the number p of
parallel
connected cells.We suppose the cells to have a mean life r. Then the c.f.r. as a function of time t is
The time interval between two maintenance opera- tions will be
Let us suppose, now, that the maintenance cost
depends
on two parameterswhere a is a constant value.
b is the substitution cost of the failed cells.
The annual cost of maintenance will be
and therefore
and
finally
For a numerical evaluation we put
bsp
= 300 aand therefore we
obtain,
for ps = 100000,
the dataplotted
infigure
3.The
optimal
valueof p
can,then,
be obtainedconsidering
also the other aspects of theproblem,
such as connections cost and
safety problems.
Asthese informations are out of the interest of this paper, we do not treat them.
5. Conclusions.
We have
developed
ananalytical
method that allows toevaluate,
in aquite satisfactory
way, power curves ofcomplex
fields as a function of the number of failed cells. Theexpressions
we have obtained areFig. 3. - The equivalent maintenance cost cl as a function of parallel number p, for PS fields.
valid when the number of failed cells is low. This
corresponds
tohigh
values of fractional power, which is the situation ofpractical
interest.Our results enable us to say that the first connection levels are the more
responsible
for the power decrease and thereforethey
must beoptimized
with greatcare.
References
[1] AMBROSONE, G. et al., Failure problem in photovoltaic fields : probabilistic approach (submitted for publi-
cation in Revue Phys. Appl.).
[2] AMBROSONE, G. et al., A statistical solution for the failure problem in large photovoltaic fields (sub-
mitted for publication in Revue Phys. Appl.).