<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">EPE</journal-id><journal-title-group><journal-title>Energy and Power Engineering</journal-title></journal-title-group><issn pub-type="epub">1949-243X</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/epe.2017.98028</article-id><article-id pub-id-type="publisher-id">EPE-78187</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Engineering</subject></subj-group></article-categories><title-group><article-title>
 
 
  Modelling Study of Magnetic Field Effect on the Performance of a Silicon Photovoltaic Module
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dioari</surname><given-names>Ulrich Combari</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Issa</surname><given-names>Zerbo</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Martial</surname><given-names>Zoungrana</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Emmanuel</surname><given-names>Wendsongre Ramde</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dieudonné</surname><given-names>Joseph Bathiebo</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff2"><addr-line>Department of Mechanical Engineering, Kwame Nkrumah University of Science and Technology, Kumasi, Ghana</addr-line></aff><aff id="aff1"><addr-line>Laboratory of Thermal and Renewable Energies, Department of Physics, University Ouaga I Prof. Joseph KI-ZERBO, 
Ouagadougou, Burkina Faso</addr-line></aff><pub-date pub-type="epub"><day>04</day><month>08</month><year>2017</year></pub-date><volume>09</volume><issue>08</issue><fpage>419</fpage><lpage>429</lpage><history><date date-type="received"><day>July</day>	<month>8,</month>	<year>2017</year></date><date date-type="rev-recd"><day>Accepted:</day>	<month>August</month>	<year>4,</year>	</date><date date-type="accepted"><day>August</day>	<month>7,</month>	<year>2017</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  Solar Photovoltaic is a very promising solution that can greatly contribute in solving the increasing global energy demand. In both rural and urban areas, photovoltaic modules are in some instances installed close to telecommunication antennas or voltage transformers which generate important magnetic fields in their vicinity. The question is whether or not these magnetic fields affect the performances of the photovoltaic installations. This article presents a modelling study of external magnetic field effect on the electrical parameters of a photovoltaic module. The photocurrent, the photovoltage, the electric power, the series and the shunt resistances of the photovoltaic module, made up of ideal cells, are deduced from those of a silicon solar cell. Then, the I-V and P-V curves are plotted and the theoretical values of the electrical parameters of the photovoltaic module are deduced. The series and shunt resistances of the photovoltaic module are calculated using well known equations and the previous electrical parameters. The results show the negative effect of magnetic field on the performance of a solar photovoltaic module.
 
</p></abstract><kwd-group><kwd>Conversion Efficiency</kwd><kwd> Magnetic Field</kwd><kwd> Modelling Study</kwd><kwd> Photovoltaic Module</kwd><kwd> Series Resistance</kwd><kwd> Shunt Resistance</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Solar Photovoltaic is a very promising solution that can contribute in solving the increasing energy demand. The performance of photovoltaic systems depends on a number of parameters such as ambient temperature, solar irradiance, sunshine duration, relative humidity, atmospheric concentrations of aerosols (harmattan dust particles for example), windspeed, wind chill and direction, rainfall, mode of installation and orientation (rooftop or ground-mounted) etc. [<xref ref-type="bibr" rid="scirp.78187-ref1">1</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref2">2</xref>] .</p><p>The challenge of researchers is twofold: the first challenge is to improve solar cells efficiency through their manufacturing technique and the second challenge is to examine the characteristics of PV modules and the external factors (environmental conditions) that affect them.</p><p>In order to investigate the effect of external factors on PV modules, various researchers have used theoretical methods under different environmental conditions and arrived at different results.</p><p>Nema et al. [<xref ref-type="bibr" rid="scirp.78187-ref3">3</xref>] and Asghar et al. [<xref ref-type="bibr" rid="scirp.78187-ref4">4</xref>] both proposed Matlab/simulink models of PV cells and simulated the effects of temperature and solar irradiation on the electrical performances of PV modules. The PV cells were modelled with the single exponential equation and Simulink was used to simulate the performance of the PV cells/modules under varying solar irradiation and temperature. The authors concluded that the open circuit voltage decreases linearly with an increase in the cell temperature but increases logarithmically with an increase in solar radiation. The short-circuit current on the other hand was said to be a linear function of the solar irradiation. It increases with an increase in solar irradiation as well as an increase in temperature. In a similar vein, Skoplaki et al. [<xref ref-type="bibr" rid="scirp.78187-ref5">5</xref>] studied the effects of temperature on both the electrical efficiency and power output of PV modules. They concluded that the electrical efficiency and the power output of a PV module decrease linearly with an increasing operating temperature. Alsayid et al. [<xref ref-type="bibr" rid="scirp.78187-ref6">6</xref>] and Boukebbous et al. [<xref ref-type="bibr" rid="scirp.78187-ref7">7</xref>] , with a Matlab/simulink model, also simulated the impact of partial shading on the performance of PV modules. The simulation results showed that, under partially shaded conditions, the maximum power produced by PV modules decreases. Besides these studies, Siddiqui et al. [<xref ref-type="bibr" rid="scirp.78187-ref8">8</xref>] used one year data to develop empirical correlations between the efficiency of solar photovoltaic modules and ambient temperature as well as wind speed. The correlated equations can predict with good accuracy the efficiency of a PV module with respect to ambient temperature and wind speed for a particular location. Besides these climatic and seasonal parameters, other researchers proposed studying the modelling of the effect of magnetic field on the properties of solar cells. Madougou et al. [<xref ref-type="bibr" rid="scirp.78187-ref9">9</xref>] showed that, for each illumination mode of the bifacial solar cell, the photocurrent density decreases with the magnetic field while the photovoltage increases with the magnetic field for front side and simultaneous front and back side illumination. At last, the authors concluded that the I-V characteristics of the bifacial silicon solar cell decrease with the magnetic field. Zerbo et al. [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] showed that the maximum electric power and the conversion efficiency of a bifacial solar cell decrease with the increase of magnetic field while the fill factor and the load resistance at the maximum power point increase. In a similar vein, Zoungrana et al. [<xref ref-type="bibr" rid="scirp.78187-ref12">12</xref>] studied a silicon solar cell under an intense light concentration and obtain the same results as Zerbo et al. [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] .</p><p>The aim of this work is to investigate the deterioration effect of magnetic field on the performance of a photovoltaic module. This is done by simulation, on a PV module made up of ideal solar cells, by finding the electrical parameters such as the current and voltage at maximum power point, the short-circuit-current, the open circuit voltage, the maximum electric power, the fill factor, the conversion efficiency and the charge resistance at the maximum power point using simultaneously the I-V and P-V characteristics. Then, the series and shunt resistances of the photovoltaic module are calculated using equations developed by some researchers and the electrical parameters mentioned previously.</p></sec><sec id="s2"><title>2. Theoretical Background</title><p>The PV module is made up of one branch of 36 mono-facial cells connected in series. The synoptic scheme of the photovoltaic module is given in <xref ref-type="fig" rid="fig1">Figure 1</xref>.</p><p>To investigate the effect of the external magnetic field on the electrical parameters of the PV module, we applied a variable external magnetic field, parallel to the surface of the n-p junction of the 36 mono-facial cells, as shown for a silicon solar cell in previous works [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] .</p><sec id="s2_1"><title>2.1. Effect of Magnetic Field on I-V Characteristics</title><p>For a monocrystalline photovoltaic module, which is made up of N<sub>p</sub> parallel branches with each branch involving N<sub>s</sub> cells in series, the photocurrent can be expressed by Equation (1).</p><disp-formula id="scirp.78187-formula202"><label>(1)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x2.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x3.png" xlink:type="simple"/></inline-formula>is the photocurrent density of a silicon solar cell under magnetic field [<xref ref-type="bibr" rid="scirp.78187-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref12">12</xref>] .</p><p>In the same way, the voltage of the photovoltaic module depends on the number of cells Ns connected in series. This is expressed by Equation (2).</p><disp-formula id="scirp.78187-formula203"><label>(2)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x4.png"  xlink:type="simple"/></disp-formula><p><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x5.png" xlink:type="simple"/></inline-formula>is the photovoltage of a silicon solar cell under magnetic field [<xref ref-type="bibr" rid="scirp.78187-ref9">9</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref12">12</xref>] .</p><p>It appears in the expressions of I and V that they depend on junction dynamic velocity, Sf [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] . The variations of this parameter (junction dynamic velocity) lead to the values of I and V.</p><p><xref ref-type="fig" rid="fig2">Figure 2</xref> presents the I-V characteristic curves of the photovoltaic module for different values of the magnetic field’s intensity.</p><fig id="fig1"  position="float"><label><xref ref-type="fig" rid="fig1">Figure 1</xref></label><caption><title> Synoptic scheme of photovoltaic module</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-6202051x6.png"/></fig><fig id="fig2"  position="float"><label><xref ref-type="fig" rid="fig2">Figure 2</xref></label><caption><title> Photocurrent-photovoltage characteristic versus intensity of magnetic field (L = 0.02 cm; H = 0.03 cm; D = 35 cm<sup>2</sup>/s; μ<sub>n</sub> = 1350 cm<sup>2</sup>/V∙s, N<sub>p</sub> = 1, N<sub>S</sub> = 36, S = 7.5 cm<sup>2</sup>)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-6202051x7.png"/></fig><p>I-V curves of the photovoltaic module have the same shape than those of a silicon solar cell [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] . It can be noted that, for an increasing intensity of the magnetic field, the short-circuit current decreases considerably while the open circuit voltage increases slightly. Furthermore, it can be observed that as the intensity of the magnetic field increases, the maximum power point is shifted towards higher values of the photovoltage and lower values of the photocurrent. This situation corresponds to a displacement of the operating point of the photovoltaic module and subsequently an increase of the charge resistance at the maximum power point [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] .</p></sec><sec id="s2_2"><title>2.2. Effect of Magnetic Field on P-V Characteristics</title><p>The electric power delivered by the monocrystalline solar photovoltaic module to an external circuit is expressed by Equation (3):</p><disp-formula id="scirp.78187-formula204"><label>(3)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x8.png"  xlink:type="simple"/></disp-formula><p>The electric power delivered by the solar photovoltaic module to an external circuit depends also on the junction dynamic velocity Sf. While taking the junction dynamic velocity as a variable, <xref ref-type="fig" rid="fig3">Figure 3</xref> is a plot of the photovoltaic module P-V characteristic curves for different values of the intensity of the magnetic field.</p><p>The P-V characteristic curves of the photovoltaic module have also the same shape than those of a silicon solar cell [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] . From the various curves in <xref ref-type="fig" rid="fig3">Figure 3</xref>, it can be observed that firstly, at any specified intensity of the magnetic field, the electric power increases with the photovoltage, reaches a peak and then decreases with increasing photovoltage; secondly, at any given photovoltage, the electric power decreases as the intensity of the magnetic field increases; thirdly, as the intensity of the magnetic field increases, the curves shifts to the right,</p><fig id="fig3"  position="float"><label><xref ref-type="fig" rid="fig3">Figure 3</xref></label><caption><title> Electric power-photovoltage characteristic versus intensity of magnetic field (L = 0.02 cm; H = 0.03 cm; D = 35 cm<sup>2</sup>/s; μ<sub>n</sub> = 1350 cm<sup>2</sup>/V∙s, N<sub>p</sub> = 1, N<sub>S</sub> = 36, S = 7.5 cm<sup>2</sup>)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-6202051x9.png"/></fig><p>compelling the peak electric power to occur at higher photovoltage. This results in an increase of the charge resistance at the maximum power point and that corresponds to a displacement of the photovoltaic module’s operating point [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] .</p></sec><sec id="s2_3"><title>2.3. Effect of Magnetic Field on the Series Resistance</title><p>The series resistance is caused by the movement of electrons through the emitter and the base of a solar cell, the contact resistance between the metal contact and the silicon and the resistance of metal grids at the front and the rear of the solar cell [<xref ref-type="bibr" rid="scirp.78187-ref13">13</xref>] .</p><p>We extrapolate the equation of the series resistance of a silicon solar cell [<xref ref-type="bibr" rid="scirp.78187-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref15">15</xref>] to a PV module. Consequently, the expression of the series resistance of a PV module is given by Equation (4a):</p><disp-formula id="scirp.78187-formula205"><label>(4a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x10.png"  xlink:type="simple"/></disp-formula><p>Taking into account Equation (1) and Equation (2), Equation (4a) becomes:</p><disp-formula id="scirp.78187-formula206"><label>(4b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x11.png"  xlink:type="simple"/></disp-formula><p>We consider a PV module made up of n sets of N<sub>p</sub> parallel branches connected in series. Each branch consists of N<sub>s</sub> cells connected in series. The Equation (4b) becomes:</p><disp-formula id="scirp.78187-formula207"><label>(4c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x12.png"  xlink:type="simple"/></disp-formula><p>The series resistance of a PV module can be written according to the series resistance of each solar cell of the PV module.</p><disp-formula id="scirp.78187-formula208"><label>(4d)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x13.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x14.png" xlink:type="simple"/></inline-formula> which is the series resistance of a solar cell.</p><p>The curve of the series resistance versus magnetic field intensity is plotted in <xref ref-type="fig" rid="fig4">Figure 4</xref>.</p><p>The curve in <xref ref-type="fig" rid="fig4">Figure 4</xref> shows that the series resistance increases with the magnetic field. The increase of the series resistance leads to a decrease of the current provided by PV module to an external load.</p></sec><sec id="s2_4"><title>2.4. Effect of Magnetic Field on the Shunt Resistance</title><p>The shunt resistance is due to manufacturing defects and also lightly by poor solarcell design. It corresponds to an alternate current path for the photocurrent [<xref ref-type="bibr" rid="scirp.78187-ref13">13</xref>] . In the Shockley five-parameter model of a solar cell, a shunt resistance represents the leakage current along the edges of the solar cell [<xref ref-type="bibr" rid="scirp.78187-ref16">16</xref>] . The shunt resistance is indicative of good or bad quality of a solar cell because when it is large, the leakage current through the solar cell is low and vice versa [<xref ref-type="bibr" rid="scirp.78187-ref15">15</xref>] .</p><p>We extrapolate also the equation of the shunt resistance of a silicon solar cell [<xref ref-type="bibr" rid="scirp.78187-ref13">13</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref14">14</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref15">15</xref>] to a PV module. Thus, the expression of the shunt resistance of a PV module is given by Equation (5a):</p><disp-formula id="scirp.78187-formula209"><label>(5a)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x15.png"  xlink:type="simple"/></disp-formula><p>For a PV module made up of n sets of N<sub>p</sub> parallel branches connected in series, in which each branch consists of N<sub>s</sub> cells connected in series, the Equation (5a) becomes:</p><disp-formula id="scirp.78187-formula210"><label>(5b)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x16.png"  xlink:type="simple"/></disp-formula><fig id="fig4"  position="float"><label><xref ref-type="fig" rid="fig4">Figure 4</xref></label><caption><title> Series resistance versus magnetic field intensity (D = 35 cm<sup>2</sup>∙s<sup>−1</sup>; μ = 1350 cm<sup>2</sup>∙(V∙s)<sup>−1</sup>; L = 0.02 cm; H = 0.03 cm; n = 1; N<sub>p</sub> = 1; N<sub>s</sub> = 36; S = 7.5 cm<sup>2</sup>; Sf = 1 cm∙s<sup>−1</sup>)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-6202051x17.png"/></fig><p>Thus, the shunt resistance of PV module can be written according to the shunt resistance of a solar cell:</p><disp-formula id="scirp.78187-formula211"><label>(5c)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x18.png"  xlink:type="simple"/></disp-formula><p>with <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x19.png" xlink:type="simple"/></inline-formula> which is the shunt resistance of a solar cell.</p><p>We plot in <xref ref-type="fig" rid="fig5">Figure 5</xref> the curve of the shunt resistance versus magnetic field intensity.</p><p>The curve in <xref ref-type="fig" rid="fig5">Figure 5</xref> shows that the shunt resistance increase with the magnetic field. The increase of the shunt resistance of the photovoltaic module means a decrease of the losses of carriers at the junction of its solar cells.</p></sec></sec><sec id="s3"><title>3. Results and Discussion</title><sec id="s3_1"><title>3.1. Method of Electrical Parameters Determination</title><sec id="s3_1_1"><title>3.1.1. Determination of Electrical Parameters Using I-V/P-V Method</title><p>We present in this section a method to determine the electrical parameters of the photovoltaic module (current and voltage at maximum power point, maximum electric power, fill factor, conversion efficiency and charge resistance at the maximum power point).</p><p>For that, we plot in the same axes system the I-V and P-V curves for a given magnetic field intensity. Using simultaneously the I-V and P-V curves, we determine the values of the maximum electric power P<sub>m</sub>, the voltage and current at the maximum power point<inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x20.png" xlink:type="simple"/></inline-formula>, the short-circuit current I<sub>sc</sub> and the open circuit voltage V<sub>oc</sub> according to the magnetic field intensity [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] [<xref ref-type="bibr" rid="scirp.78187-ref17">17</xref>] .</p><p>The fill factor (FF) of the photovoltaic module is then calculated using Equation (6):</p><disp-formula id="scirp.78187-formula212"><label>(6)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x21.png"  xlink:type="simple"/></disp-formula><fig id="fig5"  position="float"><label><xref ref-type="fig" rid="fig5">Figure 5</xref></label><caption><title> Shunt resistance versus magnetic field intensity (D = 35 cm<sup>2</sup>∙s<sup>−1</sup>; μ = 1350 cm<sup>2</sup>∙(V∙s)<sup>−1</sup>; L = 0.02 cm; H = 0.03 cm; n = 1; N<sub>p</sub> = 1; N<sub>s</sub> = 36; S = 7.5 cm<sup>2</sup>; Sf = 10<sup>8</sup> cm∙s<sup>−1</sup>)</title></caption><graphic mimetype="image"   position="float"  xlink:type="simple"  xlink:href="http://html.scirp.org/file/2-6202051x22.png"/></fig><p>The determination of the voltage and the current at the maximum power point <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x23.png" xlink:type="simple"/></inline-formula> allows us to calculate the charge resistance at the maximum power point using Ohm’s law:</p><disp-formula id="scirp.78187-formula213"><label>(7)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x24.png"  xlink:type="simple"/></disp-formula><p>The conversion efficiency of the photovoltaic module is calculated using Equation (8):</p><disp-formula id="scirp.78187-formula214"><label>(8)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x25.png"  xlink:type="simple"/></disp-formula><p>P<sub>inc</sub> is the power of the incident light’s flux and P<sub>inc</sub> = 1000 W/m<sup>2</sup> in Air Mass 1, 5 standard conditions. S<sub>mod</sub> is the area of the photovoltaic module that receives the incident light.</p></sec><sec id="s3_1_2"><title>3.1.2. Determination of Series and Shunt Resistances</title><p>The theoretical values of the series and shunt resistances of the PV module are calculated, according to the magnetic field, using Equation (9) and Equation (10) [<xref ref-type="bibr" rid="scirp.78187-ref18">18</xref>] and the values of <xref ref-type="table" rid="table1">Table 1</xref>.</p><disp-formula id="scirp.78187-formula215"><label>(9)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x26.png"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.78187-formula216"><label>(10)</label><graphic position="anchor" xlink:href="http://html.scirp.org/file/2-6202051x27.png"  xlink:type="simple"/></disp-formula></sec></sec><sec id="s3_2"><title>3.2. Values of Electrical Parameters of the PV Module</title><sec id="s3_2_1"><title>3.2.1. Electrical Parameters Using I-V/P-V Method</title><p>The PV module is made up of 36 cells connected in series. Each cell has an area of 7.5 cm<sup>2</sup>. Therefore, the PV module area is: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x28.png" xlink:type="simple"/></inline-formula>The power of the incident light received by the PV module is: <inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x28.png" xlink:type="simple"/></inline-formula><inline-formula><inline-graphic xlink:href="http://html.scirp.org/file/2-6202051x29.png" xlink:type="simple"/></inline-formula></p><p>The characteristic values of the PV module under magnetic field are given in <xref ref-type="table" rid="table1">Table 1</xref>.</p><table-wrap id="table1" ><label><xref ref-type="table" rid="table1">Table 1</xref></label><caption><title> Electrical parameters of the PV module under magnetic field</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >B (mT)</th><th align="center" valign="middle" >0</th><th align="center" valign="middle" >10</th><th align="center" valign="middle" >15</th><th align="center" valign="middle" >30<sup> </sup></th><th align="center" valign="middle" >50</th></tr></thead><tr><td align="center" valign="middle" >I<sub>sc</sub> (A)</td><td align="center" valign="middle" >0.23542</td><td align="center" valign="middle" >0.15406</td><td align="center" valign="middle" >0.13881</td><td align="center" valign="middle" >0.11192</td><td align="center" valign="middle" >0.091723</td></tr><tr><td align="center" valign="middle" >V<sub>oc</sub> (V)</td><td align="center" valign="middle" >23.121</td><td align="center" valign="middle" >25.281</td><td align="center" valign="middle" >25.567</td><td align="center" valign="middle" >26.019</td><td align="center" valign="middle" >26.306</td></tr><tr><td align="center" valign="middle" >I<sub>max</sub> (A)</td><td align="center" valign="middle" >0.22426</td><td align="center" valign="middle" >0.14759</td><td align="center" valign="middle" >0.1328</td><td align="center" valign="middle" >0.10739</td><td align="center" valign="middle" >0.08794</td></tr><tr><td align="center" valign="middle" >V<sub>max</sub> (V)</td><td align="center" valign="middle" >20.167</td><td align="center" valign="middle" >22.216</td><td align="center" valign="middle" >22.537</td><td align="center" valign="middle" >22.934</td><td align="center" valign="middle" >23.253</td></tr><tr><td align="center" valign="middle" >P<sub>max</sub> (W)</td><td align="center" valign="middle" >4.5226</td><td align="center" valign="middle" >3.2788</td><td align="center" valign="middle" >2.9929</td><td align="center" valign="middle" >2.4628</td><td align="center" valign="middle" >2.0449</td></tr><tr><td align="center" valign="middle" >R<sub>MPP</sub> (Ω)</td><td align="center" valign="middle" >89.927</td><td align="center" valign="middle" >150.525</td><td align="center" valign="middle" >169.706</td><td align="center" valign="middle" >213.558</td><td align="center" valign="middle" >264.419</td></tr><tr><td align="center" valign="middle" >FF (%)</td><td align="center" valign="middle" >83.088</td><td align="center" valign="middle" >84.184</td><td align="center" valign="middle" >84.332</td><td align="center" valign="middle" >84.573</td><td align="center" valign="middle" >84.75</td></tr><tr><td align="center" valign="middle" >η (%)</td><td align="center" valign="middle" >16.75</td><td align="center" valign="middle" >12.144</td><td align="center" valign="middle" >11.085</td><td align="center" valign="middle" >09.121</td><td align="center" valign="middle" >07.574</td></tr></tbody></table></table-wrap><p>These results show that the current at maximum power point and the short- circuit current decrease considerably while the voltage at maximum power point and the open circuit voltage increases weakly with the increase of the magnetic field intensity. Thus, the intensities of current decrease strongly for a slightly increase of the different voltage when the magnetic field intensity increases. That explains the decrease of the maximum electric power and the conversion efficiency.</p><p>Conversely, we have observed an increase of the fill factor and the charge resistance at the maximum power point. But, for a given charge resistance, the increase of magnetic field induced a decrease of the maximum electric power and the conversion efficiency, and therefore the magnetic field causes a deterioration of the performance of the PV module.</p><p>These results are in agreement with the theoretical ones of a silicon solar cell [<xref ref-type="bibr" rid="scirp.78187-ref11">11</xref>] .</p></sec><sec id="s3_2_2"><title>3.2.2. Values of Series and Shunt Resistance</title><p>The values of the series and shunt resistances of the PV module under magnetic field are given in <xref ref-type="table" rid="table2">Table 2</xref>.</p><p>These results confirm that the values of the series and shunt resistances of the PV module increase when the magnetic field intensity increases. The increase of the value of the shunt resistance of the photovoltaic module means a decrease of the losses of carriers at the junction of its solar cells while the increase of the value of the series resistance means a decrease of the current provided by the photovoltaic module to the external load.</p><p>The increase of the series and shunt resistances and the decrease of the current provided by the photovoltaic module to the external load show that the photovoltaic module has a resistive behavior under magnetic field as a solar cell [<xref ref-type="bibr" rid="scirp.78187-ref10">10</xref>] . This resistive behavior under the magnetic field is the magnetoresistance.</p></sec></sec></sec><sec id="s4"><title>4. Conclusions</title><p>A theoretical study of magnetic field effects on the electrical parameters of silicon photovoltaic module is presented.</p><p>The maximum electric power, the voltage at the maximum power point, the current at the maximum power point, the short-circuit current and the open circuit voltage are determined by means of the theoretical I-V and P-V characteristics. Then we calculated the fill factor (FF) of the photovoltaic module, the conversion efficiency and the charge resistance at the maximum power point using Ohm’s law.</p><table-wrap id="table2" ><label><xref ref-type="table" rid="table2">Table 2</xref></label><caption><title> Series and shunt resistance of the PV module under magnetic field</title></caption><table><tbody><thead><tr><th align="center" valign="middle" >B (mT)</th><th align="center" valign="middle" >0</th><th align="center" valign="middle" >10</th><th align="center" valign="middle" >15</th><th align="center" valign="middle" >30<sup> </sup></th><th align="center" valign="middle" >50</th></tr></thead><tr><td align="center" valign="middle" >R<sub>S</sub> (Ω)</td><td align="center" valign="middle" >8.285</td><td align="center" valign="middle" >13.573</td><td align="center" valign="middle" >14.481</td><td align="center" valign="middle" >18.92</td><td align="center" valign="middle" >22.379</td></tr><tr><td align="center" valign="middle" >R<sub>Sh</sub> (Ω)</td><td align="center" valign="middle" >1807</td><td align="center" valign="middle" >3434</td><td align="center" valign="middle" >3750</td><td align="center" valign="middle" >5063</td><td align="center" valign="middle" >6147</td></tr></tbody></table></table-wrap><p>The numerical data are evidence of a decrease in the maximum electric power and the conversion efficiency with the increase of magnetic field intensity while the fill factor and the resistance at the maximum power point increase. The increase of the values of the series and shunt resistance of the photovoltaic module under magnetic field puts resistive behavior called magnetoresistance in evidence.</p><p>As in the case of a silicon solar cell, the magnetic field causes a deterioration of the performance of a photovoltaic module.</p></sec><sec id="s5"><title>Acknowledgements</title><p>The authors are grateful to International Science Program (ISP) for supporting their research group (energy and environment) and allowing them to conduct this work.</p></sec><sec id="s6"><title>Cite this paper</title><p>Combari, D.U., Zerbo, I., Zoungrana, M., Ramde, E.W. and Bathiebo, D.J. (2017) Modelling Study of Magnetic Field Effect on the Performance of a Silicon Photovoltaic Module. 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