The present invention relates to a thin-film solar cell module.
In recent years, thin-film photoelectric conversion devices formed in accordance with a plasma CVD method using gases as materials have been receiving attention. Examples of such thin-film photoelectric conversion devices include silicon-based thin-film photoelectric conversion devices made of silicon-based thin-films and thin-film photoelectric conversion devices made of CIS (CuInSe2) compounds and CIGS (Cu(In, Ga)Se2) compounds, and the development of these has been accelerated and the quantity of their production has been increased. These photoelectric conversion devices are greatly characterized in that semiconductor layers or metal electrode films are layered on an inexpensive substrate having a large area using a plasma CVD apparatus, a sputtering apparatus and other film forming apparatuses, and then separated and connected through laser patterning or the like so as to provide a potential that photoelectric conversion devices having high performance can be fabricated at a low cost.
In addition, a thin-film solar cell module 210 in
Patent Document 1: Japanese Unexamined Patent Application Publication No. 2001-68713
Thin-film solar cell modules have such problems that a relatively thin photoelectric conversion layer makes it easy for a leak current to flow through solar cells, and the leak current lowers the output of the thin-film solar cell module.
The present invention is provided in view of this situation and provides a thin-film solar cell module where a leak current can only slightly lower the output of the thin-film solar cell module.
The thin-film solar cell module according to the present invention has: a substrate; and a cell module having three or more cell strings, each of which has a constant width, wherein each cell string has a plurality of solar cells having the same width as the cell string and connected in series, the above-described cell strings have the same length as the above-described solar cells connected in series and are provided on the above-described substrate in parallel connection so as to be aligned in the direction perpendicular to the direction in which the above-described solar cells are connected in series, the above-described solar cells respectively have a front surface electrode, a photoelectric conversion layer and a rear surface electrode layered in this order, each cell string has contact lines having the same width as the cell string and electrically connecting the front surface electrode of a first solar cell to the rear surface electrode of a second solar cell, the first and second solar cells being included in the cell string and adjacent to each other, and the cell strings at both ends in the three or more cell strings have a width narrower than the other cell string.
The present inventors had conducted diligent research and found that the closer the cell string is to an end of the thin-film solar cell module, the easier it is for a leak current to occur in a solar cell included in the cell string. Though the reason for this is not clear, the following reason is a possibility. When the photoelectric conversion layer in a thin-film solar cell module is formed in a plasma CVD apparatus or a sputtering apparatus, for example, the closer a point is to an end of the substrate, the more difficult it is for the material for forming the photoelectric conversion layer to be supplied to the point, and therefore, in some cases, the photoelectric conversion layer 253 is thinner as it is closer to an end of the substrate 201, as shown in
In the case where a large leak current occurs in the location C in
In the thin-film solar cell module according to the present invention, the width of the cell string close to an end of the thin-film solar cell module where it is easy for a leak current to occur is smaller than the width of the other cell strings. Alternatively, the width of the cell strings at both ends is in a certain range. Therefore, the area of the light receiving surface of the cell strings at ends where it is easy for a leak current to occur can be smaller than the area of the light receiving surface of other cell strings. The output of the cell strings is proportional to the area of its light receiving surface, and therefore, in the thin-film solar cell module according to the present invention, the output of the cell strings at the ends where it is easy for a leak current to occur can be smaller than that of the other cell strings. Accordingly, in the thin-film solar cell module according to the present invention, in the case where a large leak current occurs in a cell string close to an end of the thin-film solar cell module, though the output of the cell string at the end of which the output is smaller than the other cell strings may lower, the output of the other larger output cell strings does not lower, and therefore the reduction in the output of the thin-film solar cell module can be small due to the effects of the leak current.
In addition, the thin-film solar cell module according to the present invention has a substrate; and a cell module having three or more cell strings, each of which has a constant width, wherein each cell string has a plurality of solar cells having the same width as the cell string and connected in series, the above-described cell strings have the same length as the above-described solar cells connected in series and are provided on the above-described substrate in parallel connection so as to be aligned in the direction perpendicular to the direction in which the above-described solar cells are connected in series, the above-described solar cells respectively have a front surface electrode, a photoelectric conversion layer and a rear surface electrode layered in this order, each cell string has contact lines having the same width as the cell string and electrically connecting the front surface electrode of a first solar cell to the rear surface electrode of a second solar cells, the first and second solar cells being included in the cell string and adjacent to each other, and the cell strings at both ends in the three or more cell strings have a width of 5 mm or more and 255 mm or less, or a width of 0.36% or more and 18% or less of the sum of the widths of all the cell strings included in the above-described cell module.
In the thin-film solar cell module according to the present invention, cell strings can be formed in portions where it is easy for a leak current to occur, and therefore the output in the portions where it is difficult for a leak current to occur can be prevented from lowering. As a result, the reduction in the output of the thin-film solar cell module can be small due to the effects of the leak current.
In addition, the thin-film solar cell module according to the present invention has: a substrate; and a cell module having three or more cell strings, each of which has a constant width, wherein each cell string has a plurality of solar cells having the same width as the cell string and connected in series, the above-described cell strings have the same length as the above-described solar cells connected in series and are provided on the above-described substrate in parallel connection so as to be aligned in the direction perpendicular to the direction in which the above-described solar cells are connected in series, the above-described solar cells respectively have a front surface electrode, a photoelectric conversion layer and a rear surface electrode layered in this order, each cell string has contact lines having the same width as the cell string and electrically connecting the front surface electrode of a first solar cell to the rear surface electrode of a second solar cell, the first and second solar cells being included in the cell string and adjacent to each other, and the cell string at the center in the three or more cell strings has a width greater than that of the other cell strings.
In the thin-film solar cell module according to the present invention, the cell string at the center where it is difficult for a leak current to occur can have a width greater than that of the other cell strings. In this area, it is particularly difficult for a leak current to occur, and therefore a cell string having a large output can be fabricated. When the width of the cell string at the center is great, the number of division lines for electrical separation can be reduced, and therefore the loss in the light receiving area and the number of steps can be reduced.
a) is a schematic cross sectional diagram along chain line S-T in
b) is a schematic cross sectional diagram showing an enlargement of the portion B surrounded by a dotted line in
a) is a schematic plan diagram showing the portion A surrounded by a dotted line in
b) is a diagram showing the cross sectional area of a contact line;
a) to 4(c) are diagrams for illustrating a term “connection in parallel in a bidirectional manner;”
a) and 13(b) are schematic cross sectional diagrams for illustrating a cause of a leak current.
In the following, one embodiment of the present invention is described in reference to the drawings. The structures shown in the drawings and in the following description are illustrative, and the scope of the present invention is not limited to these structures.
Here, the thin-film solar cell modules shown in
The thin-film solar cell module 1 according to the present embodiment has: a substrate 2; and a cell module la including three or more cell strings 21, each of which has a constant width, wherein each cell string 21 has a plurality of solar cells 27 having the same width as the cell string 21 and connected in series, the cell strings 21 have the same length as the solar cells 27 connected in series and are provided on the substrate 2 in parallel connection so as to be aligned in the direction perpendicular to the direction in which the solar cells 27 are connected in series, the solar cells 27 respectively has a front surface electrode 3, a photoelectric conversion layer (5, 7, 9) and a rear surface electrode 11 layered in this order, each cell string 21 has contact lines 17 having the same width as the cell string 27 and electrically connecting the front surface electrode 3 of a first solar cell 27 to the rear surface electrode 11 of a second solar cell 27, the first and second solar cells 27 being included in the cell string 21 and adjacent to each other, and the cell strings 27 at both ends are characterized by having a width narrower than the other cell strings 27.
In the following, each of the constitutional elements of the thin-film solar cell module 1 according to the present invention is described.
The substrate 2 is not particularly limited, but in the case of a superstrate type structure, for example, substrates having light transmitting properties, such as glass substrates having a resistance to heat in the plasma CVD film forming process, and resin substrates, such as of polyimide, can be used. In the case of a substrate structure, there are no particular limitations for the substrate.
The size of the substrate 2 is not particularly limited as long as a cell module 1a can be formed.
There are no particular limitations in the cell module 1a as long as it includes three or more cell strings 21 that respectively have a constant width L and are provided on the substrate 2 as to be aligned in the direction perpendicular to the direction in which the solar cells 27 are connected in series. In addition, a plurality of cell modules la may be formed on the same substrate.
Here, in the present invention, the lengthwise direction is the direction in which solar cells 27 are connected in series and the crosswise direction is the direction in which the cell strings 21 are aligned. In
The method according to which cell strings 21 are connected in parallel is not particularly limited, but they may be connected in parallel through common electrodes 23 that are connected to both ends of each cell string 21, for example. In addition, the common electrodes 23 include first common electrodes and second common electrodes, and the first common electrodes and the second common electrodes electrically connect the cell strings so that a current generated in the cell strings can flow into each other of the cell strings. In addition, the first common electrodes and the second common electrodes can be provided so that the two electrodes of the cell strings can be electrically connected to each other.
Here, the width of the cell strings 21 in the present invention is the length of the cell strings in the crosswise direction, and the width of the cell strings 21 is the length L of the cell strings 21 in the direction in which the cell strings 21 are aligned, for example, as in
Though the size of the cell module 1a is not particularly limited, the width in the direction perpendicular to the direction in which the solar cells 27 are connected in series is 500 mm or more and 3000 mm or less (a value in a range between any of the two from among 500 mm, 600 mm, 700 mm, 800 mm, 900 mm, 1000 mm, 1200 mm, 1400 mm, 1600 mm, 1800 mm, 2000 mm, 2200 mm, 2400 mm, 2600 mm, 2800 mm and 3000 mm), for example. This is because it becomes easy for a leak current to flow through the cell strings 21 at both ends when the cell module 1a is a certain size.
In addition, “connection in parallel in a bidirectional manner” in the present invention means such a state that a current generated in one cell string 21 can flow into the other cell string 21 and vice versa.
The cell module 1a can provide an output of 90 W or more and 385 W or less under such conditions that the light source is a xenon lamp, irradiance is 100 mW/cm2, AM (air mass) is 1.5, and the temperature is 25° C. As a result, this invention can be applied to a thin-film solar cell module 1 having a large photovoltaic power where a solar cell 27 or a contact line 17 is easily damaged due to a hot spot phenomenon. In many cases, reduction in the output due to a leak current becomes a problem in thin-film solar cell modules having an output in such a range.
Here, AM represents an effect of absorption and scattering of solar light in the air on the wavelength distribution of the intensity of solar light. This is AM 0 in outer space and AM 1 on the surface of the Earth in the case where the light enters vertically to the surface of the Earth. The solar light with AM at 1.5, which is one condition for the output of the solar cell, means that the light has passed through the air layer 1.5 times longer than that of AM 1.
In addition, the output of the cell module la can be 50 W, 60 W, 70 W, 80 W, 90 W, 100 W, 110 W, 120 W, 130 W, 140 W, 150 W, 160 W, 170 W, 180 W, 190 W, 200 W, 210 W, 220 W, 230 W, 240 W, 250 W, 260 W, 270 W, 280 W, 290 W, 300 W, 310 W, 320 W, 330 W, 340 W, 350 W, 360 W, 370 W, 380 W or 385 W, for example. The output of the cell module la may be any one of these numerical values or less, or may be in a range between any two.
Each cell string 21 have a plurality of solar cells 27 having the same wide as the cell string 21 and connected in the series in the lengthwise direction, and have a constant width. In addition, each cell string 21 has two electrodes, one of which is electrically connected to a first common electrode and the other is electrically connected to a second common electrode. The two electrodes may be provided adjacent to the solar cells 27 at the ends of a plurality of solar cells 27 connected in series in the lengthwise direction. In addition, the two electrodes may be same as the front surface electrode or the rear surface electrode of the solar cells 27 at the ends. In addition, three or more cell strings 21, of which the length in the lengthwise direction is the same and each of which has a constant width, are provided on a substrate 2 so as to be aligned in the crosswise direction. The number of cell strings 21 may be 3, 4, 5, 6, 8, 10, 12, 14, 16, 18, 20, 22, 24, 26, 28 or 30, for example. In addition, the number may be in a range between any two of the numbers of cell strings 21 shown here. The number of cell strings 21 may be 3 or more and 20 or less. As a result, the light receiving area of the cell strings 21 at the ends can be sufficiently smaller than the light receiving area of the other cell strings 21, and thus the reduction in the output of the thin-film solar cell module 1 can be smaller due to a leak current.
Here, the cell strings 21 at the end in the present invention are cell strings 21 having another cell string 21 only on one side from among the cell strings 21 aligned in the crosswise direction. In
The width L′ of the cell strings 21 at the two ends from among the three or more cell strings 21 is smaller than the width L of the other cell strings 21. As a result, the area of the light receiving surface of the cell strings 21 at the two end is smaller than that of the other cell strings 21, and the output is also smaller than that of the other cell strings 21. As a result, even in the case where a large leak current is generated in the cell strings 21 at the two ends, reduction in the output of the thin film solar cell module 1 can be small.
In addition, the form of the cell strings 21 is not particularly limited as long as the length in the lengthwise direction is the same and the width is constant in the crosswise direction, but they are practically rectangular (or square) and are aligned in the crosswise direction.
For example, rectangular cell strings 21 can be provided and aligned in the crosswise direction, as shown in
The cell strings 21 at the two ends from among the above-described three or more cell strings 21 may have a width of 5 mm or more and 255 mm or less. As a result of the below described experiment, it has been found that a leak current is easily generated in the solar cells 27 within 255 mm from an end of the cell module, and therefore when the width is 255 mm or less, the output of the cell strings inside the point 255 mm from an end where it is difficult for a leak current to be generated can be prevented from lowering. Preferably, the cell strings 21 at the two ends have a width of 5 mm or more and 155 mm or less. This is because the probability of a leak current being generated is high in this range. More preferably, the cell strings 21 at the two ends may have a width of 5 mm or more and 55 mm or less. This is because the probability of a leak current being generated is particularly high in this range.
In addition, the cell strings 21 at the two ends from among the above-described three or more cell strings 21 may have a width of 0.36% or more and 18% or less of the sum of the widths of all the cell strings 21 included in the cell module 1a. As a result, the output of the cell strings inside the point 18% of the width from an end where it is difficult for a leak current to be generated can be prevented from lowering. Preferably, the cell strings 21 at the two ends have a width 0.36% or more and 11% or less. This is because the probability of a leak current being generated is high in this range. More preferably, the cell strings 21 at the two ends have a width 0.36% or more and 4% or less. This is because the probability of a leak current being generated is particularly high in this range.
In addition, the cell module 1a includes five or more cell strings 21, and the sum of the widths of the two cell strings 21 from at least the cell string at either end from among the above-described five or more cell strings may be 11 mm or more and 255 mm or less, or 0.71% or more and 18% or less of the sum of the widths of all the cell strings 21 included in the cell module 1a. In the thin-film solar cell module 1 shown in
In addition, the cell module 1a may include seven or more cell strings 21, and the sum of the widths of the three cell strings 21 from at least either end of the above-described seven or more cell strings 21 may be 17 mm or more and 255 mm or less, or 1.07% or more and 18% or less of the sum of the widths of all the cell strings included in the cell module 1a. In the thin-film solar cell module 1 shown in
In addition, the output of each cell string 21 can be made 30 W or less under such conditions that the light source is a xenon lamp, the irradiance is 100 mW/cm2, AM is 1.5, and the temperature is 25° C. As a result, even in the case where one or a few solar cells 27 included in the cell string 21 are in a shade, the solar cells 27 can be prevented from being damaged due to a hot spot phenomenon (this was clarified from the below described experiment). The smaller the output of the cell string 21 is, the more the output can be prevented from lowering due to a hot spot phenomenon. When the output is small, however, the light receiving area is small and the probability of the entire cell string 21 being in a shade becomes high, thus making the probability of a contact line 17 being damaged high.
Here, the light receiving area and the output are in a proportional relationship. Here, as for a hot spot phenomenon, in the case where some solar cells included in a cell string do not receive any solar light, the photovoltaic power in the other solar cells causes insulation breakdown in the solar cells that do not receive any solar light (which work as a diode having rectification of a current in the direction opposite to that generated by the photovoltaic power), and thus heat is generated locally. This heat is considered to melt a metal included in the solar cells, and thus causes damage to the solar cell, such as film peeling.
In addition, the cell strings 21 can be connected to each other in parallel in a bidirectional manner, and the cell strings 21 at the two ends from among the aligned cell strings 21 can satisfy that (P−Ps)/Sc is 10.7 (kW/cm2) or less when the output of the above-described cell modules is P (W), the output of the cell strings is Ps (W), and the cross sectional area of the contact lines included in the cell strings is Sc (cm2) under such conditions that the light source is a xenon lamp, irradiance is 100 mW/cm2, AM is 1.5, and the temperature is 25° C. As a result, even in the case where the entirety of at least one of the cell strings 21 at the two ends included in the cell module 1a is in a shade, the contact lines 17 in this cell string 21 can be prevented from being damaged (this is clarified from the below described experiment). Here, even in the case where the cell strings 21 at the two ends do not satisfy the above-described conditions, sometimes the contact lines 17 can be prevented from being damaged. Though the reason for this is not clear, the probability of a leak current flowing through the cell string 21 at an end is high, and therefore the current is not concentrated on the contact lines but is dispersed. Thus, the power consumed in the contact lines 17 is considered to be small.
Here, these contact lines 17 are considered damaged as follows. In the case where the majority of only one or a few cell strings included in the thin-film solar cell module is in a shade, the photovoltaic power of this cell string lowers. As a result, the photovoltaic power caused by the other light receiving cell strings makes a current flow through the cell string in a shade in the direction opposite to the current that flows when the cell string receives light. This current may damage a contact line for connecting solar cells in series included in the cell string. This is considered to be because the density of the power applied to the cell string in the shade due to the photovoltaic power of the light receiving cell strings becomes the greatest in the contact lines. As a result of such damage, the output of this cell string lowers, and thus the output of the thin-film solar cell module is considered to lower.
In the case where a single cell string 21 is in a shade, the power generated in all the other cell strings 21 is applied to the cell string 21 in a shade. The value of the power applied to the cell string 21 in a shade is (the power P of the cell modules 1a)−(the power Ps of the cell string 21 in a shade). The smaller the value of Ps of the cell string 21 is, the greater the value (P−Ps) is, and therefore when the output Ps of each cell string 21 is lowered by increasing the number of parallel divisions for the cell strings, the power applied to the cell string 21 in a shade increases.
In addition, the cell strings 21 other than the cell strings 21 at the two ends may have the density of the power applied to contact lines (P−Ps)/Sc be 10.7 (kW/cm2) or less when the output of said cell module 1a is P (W), the output of the cell strings 21 is Ps (W), and the area of the cross section of the contact lines 17 included in the cell strings 21 is Sc (cm2) under such conditions that the light source is a xenon lamp, the irradiance is 100 mW/cm2, AM is 1.5, and the temperature is 25° C. As a result, the contact lines 17 can be prevented from being damaged even in the case where any cell string 21 in the cell module la is in a shade.
In addition, the cell strings 21 may have the density of the power applied to contact lines (P−Ps)/Sc be 10.7 (kW/cm2) or less when the output of said cell module la is P (W), the output of the cell strings 21 is Ps (W), and the area of the cross section of the contact lines 17 included in the cell strings 21 is Sc (cm2) under such conditions that the light source is a xenon lamp, the irradiance is 100 mW/cm2, AM is 1.5, and the temperature is 25° C. As a result, the contact lines 17 can be prevented from being damaged even in the case where any cell string 21 in the cell module la is in a shade.
In addition, the cell string 21 at the center may have a width greater than that of the other cell strings 21. As a result, the output of the cell string in a portion where it is difficult for a leak current to be generated is large. In addition, when the width of the cell string at the center is great, the number of division lines for electrical division can be reduced, and therefore loss of the light receiving area and the number of steps can be reduced. Here, the cell string 21 at the center in this invention refers to one cell string at the center in the case where there is an odd number of cell strings and either of the two cell strings 21 at the center in the case where there is an even number of cell strings.
The width Lb of the cell string 21 at the center in
In addition, the cell string 21 at the center may have a width of 670 mm or less or 50% or less of the sum of the widths of all cell strings 21 included in the cell module 1a. In this range, it is particularly difficult for a leak current to flow, and therefore the effect of a leak current is small and the cell string has a large output. The width Lb of the cell string 21 at the center in
Solar cells 27 are respectively provided with a front surface electrode 3, a photoelectric conversion layer (5, 7, 9) and a rear surface electrode 11 layered in this order. In addition, the solar cells 27 included in a cell string 21 have the same width as the cell string 21 and are connected in series in the lengthwise direction through contact lines 17, which electrically connect the front surface electrode 3 of one solar cell 27 to the rear surface electrode 11 of the adjacent solar cell 27 and have the same width as the cell string 21.
Though the form of the solar cells 27 is not particularly limited, it is practically rectangular or square. For example, a plurality of rectangular solar cells 27 can be connected in series in the direction Y, as in
In the case where the thin-film solar cell module I is of a superstrate type, a front surface electrode 3, a photoelectric conversion layer (5, 7, 9) and a rear surface electrode 11 are provided and layered on a substrate 2 in this order. In the case where the thin-film solar cell module 1 is of a substrate type, a rear surface electrode 11, a photoelectric conversion layer (5, 7, 9) and a front surface electrode 3 are provided and layered on a substrate 2 in this order.
The front surface electrode 3 is made of a conductive material and has light transmitting properties. The front surface electrode 3 is made of a metal oxide, such as SnO2, ITO or ZnO, and SnO2, ITO or the like, which include Sn, are preferable.
There are no particular limitations in the photoelectric conversion layer as long as it has an n type semiconductor layer and a p type semiconductor layer so as to perform photoelectric conversion. The photoelectric conversion layer may have a pn junction made of an n type semiconductor layer and a p type semiconductor layer or a pin junction made of an n type semiconductor layer, an i type semiconductor layer and a p type semiconductor layer. In addition, the photoelectric conversion layer may have a plurality of pin junctions or pn junctions. A first photoelectric conversion layer 5, a second photoelectric conversion layer 7 and a third photoelectric conversion layer 9 may be provided, for example, as in
Though a case where the i type semiconductor layers in the first photoelectric conversion layer 5 and the second photoelectric conversion layer 7 are respectively amorphous layers and the i type semiconductor layer in the third photoelectric conversion layer 9 is a microcrystalline layer is cited as an example, the following descriptions can basically be applied for thin-film solar cell modules having other structures, for example, thin-film solar cell modules having such a structure that all of the i type semiconductor layers in the first to third photoelectric conversion layers are all amorphous layers or all crystal layers, thin-film solar cell modules having such a structure that the i type semiconductor layer in the first photoelectric conversion layer is an amorphous layer, and the i type semiconductor layers in the second and third photoelectric conversion layers are both microcrystalline layers, thin-film solar cell modules having such a structure as to omit either or both of photoelectric conversion the second photoelectric conversion layer and the third photoelectric conversion layer, and thin-film solar cell modules having such a structure as to be provided with another photoelectric conversion layer on the downstream side of the third photoelectric conversion layer.
In addition, though a case is cited as an example where a p type semiconductor layer, an i type semiconductor layer and an n type semiconductor layer are aligned in this order in the pin junction in each photoelectric conversion layer, the following description can basically be applied to the case where an n type semiconductor layer, an i type semiconductor layer and a p type semiconductor layer are aligned in this order in the pin junction in each photoelectric conversion layer.
The first photoelectric conversion layer 5 is provided with a p type semiconductor layer 5a, a buffer layer 5b made of an i type amorphous layer, an i type amorphous layer 5c and an n type semiconductor layer 5d layered in this order. The second photoelectric conversion layer 7 is provided with a p type semiconductor layer 7a, a buffer layer 7b made of an i type amorphous layer, an i type amorphous layer 7c and an n type semiconductor layer 7d layered in this order. The third photoelectric conversion layer 9 is provided with a p type semiconductor layer 9a, an i type microcrystalline layer 9b and an n type semiconductor layer 9c layered in this order. The buffer layers 5b and 7b can be left out. The p type semiconductor layers are doped with p type impurity atoms, such as of boron or aluminum, and the n type semiconductor layers are doped with n type impurity atoms, such as phosphorous. The i type semiconductor layers may be completely non-doped semiconductor layers or weak p type or weak n type semiconductor layers with a microscopic amount of impurities and having sufficient photoelectric conversion functions. In the present specification, semiconductor layers means amorphous or microcrystalline semiconductor layers, and amorphous layers and microcrystalline layers mean amorphous and microcrystalline semiconductor layers, respectively.
The materials of the semiconductor layers for forming the photoelectric conversion layers are not particularly limited, and examples are silicon-based semiconductors, CIS (CuInSe2) compound semiconductors and CIGS (Cu(In, Ga)Se2) compound semiconductors. In the following, a case where the semiconductor layers are made of silicon-based semiconductors is cited as an example. Silicon-based semiconductors means amorphous or microcrystalline silicon or semiconductors where carbon, germanium or another impurity is added to amorphous or microcrystalline silicon (silicon carbide, silicon germanium and the like). In addition, microcrystalline silicon means silicon in a mixed state of crystal silicon having a crystal grains with a small diameter (approximately several tens to several thousands of angstrom) and amorphous silicon. Microcrystalline silicon is formed in the case where a crystal silicon thin film is fabricated at a low temperature in a non-equilibrium process, such as a plasma CVD method, for example.
The rear surface electrode 11 is made of a conductive material. The structure and the material of the rear surface electrode 11 are not particularly limited, but in an example, the rear surface electrode 11 has a multilayer structure of a transparent conductive film and a metal film. The transparent conductive film is made of SnO2, ITO, ZnO or the like. The metal film is made of a metal, such as silver or aluminum. The transparent conductive film and the metal film are formed in accordance with a method, such as CVD, sputtering or vapor deposition.
Contact lines 17 electrically connect the front surface electrode 3 of one solar cell 27 to the rear surface electrode 11 of an adjacent solar cell that is included in the same cell string 21. As shown in
In addition, in the case where one cell string 21 included in the cell module 1a is in a shade and the photovoltaic power of the other cell strings 21 makes a current flow through the cell string 21 in a shade, the current mainly flows through the front surface electrode 3, the contact line 17 and the rear surface electrode 27 included in the cell string 21, and in many cases, the cross sectional area of the contact line 17 is the smallest from among the cross sectional areas of the conductors, and therefore the density of the power applied to the contact line 17 is the greatest.
In addition, the contact line 17 has a cross sectional area. Sc of L×W, where W may be 40 μm to 200 μm and L may be 5 cm to 50 cm. As a result, the light receiving area of the solar cells 27 is secured, and in addition, the cross sectional area of the contact lines 17 is sufficiently large. The width W of one side of the cross section of the contact lines 17 is 20 μm to 300 μm, for example, and it is preferable for it to be 40 μm to 200 μm. When the width W of a side of the cross section of the contact lines 17 is small, the area Sc is small, which makes the density of the power applied to the contact lines (P−Ps)/Sc large. When the width W of a side of the cross section of the contact lines 17 is large, the effective power generating area is small. Thus, when the width W of a side of the cross section of the contact lines 17 is 40 μm to 200 μm, the density of the power applied to the contact lines (P−Ps)/Sc is not too large and a wide effective power generating area can be secured. The width W of one side of the cross section of the contact lines 17 is concretely 20 μm, 30 μm, 40 μm, 50 μm, 60 μm, 70 μm, 80 μm, 90 μm, 100 μm, 110 μm, 120 μm, 130 μm, 140 μm, 150 μm, 160 μm, 170 μm, 180 μm, 190 μm, 200 μm, 210 μm, 220 μm, 230 μm, 240 μm, 250 μm, 260 μm, 270 μm, 280 μm, 290 μm or 300 μm. The width W of one side of the cross section of the contact lines 17 may be in a range between any two of the numerical values shown here.
Next, a plasma CVD apparatus for forming a semiconductor layer included in the above-described thin-film solar cell module will be described by use of
The structure illustrated in
As shown in
More specifically, the plasma CVD apparatus shown in
The power supply section 108 is connected to one end of a power introducing line 106a. The other end of the power introducing line 106a is connected to the impedance matching circuit 105. One end of a power introducing line 106b is connected to the impedance matching circuit 105, and the other end of the power introducing line 106b is connected to the cathode electrode 102. The power supply section 108 may output either of a CW (continuous waveform) alternating current output or a pulse-modulated (on/off control) alternating current output, or may be one capable of switching these outputs to output.
The frequency of the alternating electric power outputted from the power supply section 108 is generally 13.56 MHz, but it is not limited thereto, and frequencies of several kHz to VHF band and a microwave band may be used.
On the other hand, the anode electrode 103 is electrically grounded, and a substrate 107 is located on the anode electrode 103. The substrate 107 is, for example, the substrate 2 on which the front surface electrode 3 is formed. The substrate 107 may be placed on the cathode electrode 102, but it is generally placed on the anode electrode 103 in order to reduce degradation of film quality due to ion damage in plasma.
The gas intake section 110 is provided in the film forming chamber 101. A gas 118 such as a dilution gas, a material gas, and a doping gas is introduced from the gas intake section 110. Examples of the dilution gas include a gas including a hydrogen gas. Examples of the material gas include a silane base gas, a methane gas, a germane gas, and the like. Examples of the doping gas include a doping gas of a p-type impurity such as a diborane gas, and a doping gas of an n-type impurity such as a phosphine gas.
Further, the gas exhaust section 116 and a pressure control valve 117 are connected in series to the film forming chamber 101, and the gas pressure in the film forming chamber 101 is kept approximately constant. It is desirable that the gas pressure is measured at a position away from the gas intake section 110 and a gas exhaust outlet 119 in the film forming chamber, because measurement of the gas pressure at a position close to the gas intake section 110 and the gas exhaust outlet 119 causes errors somewhat. By supplying electric power to the cathode electrode 102 under this condition, it is possible to generate plasma between the cathode electrode 102 and the anode electrode 103 to decompose the gas 118, and to form the semiconductor layer on the substrate 107.
The gas exhaust section 116 may be one capable of evacuating the film forming chamber 101 to reduce the gas pressure in the film forming chamber 101 to a high vacuum of approximately 1.0×10−4 Pa, but it may be one having an ability for evacuating gases in the film forming chamber 101 to a pressure of approximately 0.1 Pa in view of simplification of an apparatus, cost reduction, and an increase in throughput. The volume of the film forming chamber 101 has been getting larger as the size of the substrate of the semiconductor device grows. When such a film forming chamber 101 is highly evacuated to a vacuum, a high-performance gas exhaust section 116 is required, and therefore it is not desirable from the viewpoint of simplification of an apparatus and cost reduction, and it is more desirable to use a simple gas exhaust section 116 for a low vacuum.
Examples of the simple gas exhaust section 116 for a low vacuum include a rotary pump, a mechanical booster pump, a sorption pump, and the like, and it is preferable to use these pumps alone or in combination of two or more kinds thereof.
The film forming chamber 101 of the plasma CVD apparatus used in this embodiment can be sized in approximately 1 m3, for example. As a typical gas exhaust section 116, a mechanical booster pump and a rotary pump connected in series can be used.
Next, a method for producing the thin-film solar cell module according to an embodiment of the present invention will be described by use of
Hereinafter, the method will be described taking, as an example, the case of forming the semiconductor layer by use of a plasma CVD apparatus of a single chamber type having one film forming chamber as shown in
In the production method of this embodiment, the first photoelectric conversion layer 5, the second photoelectric conversion layer 7, and the third photoelectric conversion layer 9 are formed in the same film forming chamber. To form the photoelectric conversion layers in the same film forming chamber means that the first, second, and third photoelectric conversion layers 5, 7, 9 are formed by use of the same electrode or different electrodes in the same film forming chamber, and it is desirable that the first, second, and third photoelectric conversion layers 5, 7, 9 are formed by use of the same electrode in the same film forming chamber. Further, it is desirable from the viewpoint of improving production efficiency that the first, second, and third photoelectric conversion layers 5, 7, 9 are successively formed without being released to the air on the way. Furthermore, it is desirable from the viewpoint of improving production efficiency that substrate temperatures during the formation of the first, second, and third photoelectric conversion layers 5, 7, 9, are the same.
Hereinafter, a method for producing the thin-film solar cell module 1 will be described in detail. The method to be described below is exemplification, and the thin-film solar cell module 1 may be produced by a method other than the method to be described below.
First, the front surface electrode 3 is formed on the substrate 2. For example, they may be formed by a method such as a CVD method, a sputtering method, and a vapor deposition method.
Next, the front surface electrode division line 13 dividing the front surface electrode 3 is formed in a crosswise direction. For example, the front surface electrode division line 13 extending in an X direction in
Next, the first photoelectric conversion layer 5 is formed on the obtained substrate. As described above, since the first photoelectric conversion layer 5 has the p-type semiconductor layer 5a, the buffer layer 5b, the i-type amorphous layer 5c, and the n-type semiconductor layer 5d, the respective semiconductor layers are formed in order.
A gas replacement step of replacing the inside of the film forming chamber 101 with a replacement gas is performed to reduce the concentration of impurities in the film forming chamber 101 before the formation of the p-type semiconductor layer 5a (that is, before the formation of the first photoelectric conversion layer 5) and before the formation of the i-type amorphous layer 5c. Since the impurities introduced in the preceding step or the impurities immixed from the outside when a substrate is carried into the film forming chamber 101 remain in the film forming chamber 101, quality of the semiconductor layer is deteriorated if the semiconductor layer takes in the impurities. Therefore, the concentration of the impurities in the film forming chamber 101 is reduced in advance. The gas replacement step is also performed before the formation of the p-type semiconductor layer 7a (that is, before the formation of the second photoelectric conversion layer 7), before the formation of the i-type amorphous layer 7c, before the formation of the p-type semiconductor layer 9a (that is, before the formation of the third photoelectric conversion layer 9), and before the formation of the i-type microcrystalline layer 9b. Here, each gas replacement step may be performed under the same condition, or under different conditions.
In addition, when the plasma CVD apparatus of a multi-chamber type is used, the concentration of the impurities in the film forming chamber can be reduced by changing the film forming chamber in place of performing the gas replacement step. In general, the p-type semiconductor layer 5a and the buffer layer 5b are formed in a first film forming chamber, the i-type amorphous layer 5c is formed in a second film forming chamber, and the n-type semiconductor layer 5d is formed in a third film forming chamber. Further, the p-type semiconductor layer 7a, the buffer layer 7b, and the p-type semiconductor layer 9a are formed in the first film forming chamber, the i-type amorphous layer 7c and the i-type microcrystalline layer 9b are formed in the second film forming chamber, and the n-type semiconductor layer 7d and the n-type semiconductor layer 9c are formed in the third film forming chamber. The p-type amorphous layer and the buffer layer may be formed in different film forming chambers.
Hereinafter, a step of forming the first photoelectric conversion layer 5 will be described in detail.
The substrate 2 on which the front surface electrode 3 is formed is installed in the film forming chamber 101, and thereafter the gas replacement step of replacing the inside of the film forming chamber 101 with a replacement gas is performed. This gas replacement step is performed to reduce the concentration of the impurities which are immixed from the outside of the film forming chamber 101 in carrying a substrate to be provided with a semiconductor layer into the film forming chamber 101. Further, when the thin-film solar cell module is produced repeatedly, the first to third photoelectric conversion layers are formed repeatedly, and therefore the n-type semiconductor layer 9c of the third photoelectric conversion layer 9, previously formed, is deposited on an inner wall, an electrode, and the like in the film forming chamber 101. Therefore, it will be a problem that impurities released from the n-type semiconductor layer 9c of the third photoelectric conversion layer 9, particularly impurities that determine a conductive type of the n-type semiconductor layer 9c of the third photoelectric conversion layer 9, are immixed in the p-type semiconductor layer 5a of the first photoelectric conversion layer 5. Accordingly, the gas replacement step is performed before the formation of the p-type semiconductor layer 5a to reduce the amount of n-type impurities to be immixed in the p-type semiconductor layer 5a.
Thereby, a semiconductor layer of good quality can be formed as the p-type semiconductor layer 5a of the first photoelectric conversion layer 5. Here, since the p-type semiconductor layer 5a generally includes p-type conductive impurities in a concentration of approximately 1×1020 cm−3, satisfactory photoelectric conversion characteristics are attained if the concentration of the immixed n-type conductive impurities is approximately 1×1018 cm−3 or less, which is 2 digits less than the concentration of the p-type conductive impurities.
The gas replacement step can be performed through an operation cycle in which, for example, a hydrogen gas is introduced into the film forming chamber 101 as a replacement gas (step of introducing a replacement gas), the introduction of the hydrogen gas is stopped when the internal pressure of the film forming chamber 101 reaches a predetermined pressure (for example, approximately 100 Pa to 1000 Pa), and the hydrogen gas is evacuated until the internal pressure of the film forming chamber 101 reaches a predetermined pressure (for example, approximately 1 Pa to 10 Pa) (evacuation step). This cycle may be repeated more than once.
The period of time required to perform the above-mentioned one cycle can be several seconds to several tens of seconds. Specifically, the step of introducing a replacement gas can be performed over 1 to 5 seconds, and the evacuation step can be performed over 30 to 60 seconds. Even when the steps are performed in such a short period of time, the concentration of the impurities in the film forming chamber can be reduced by repeating this cycle more than once. Therefore, the method for producing the thin-film solar cell module according to this embodiment is also practical when it is applied to mass production devices.
In this embodiment, it is preferable that an internal pressure of the film forming chamber 101 after introducing a replacement gas and an internal pressure after evacuating the replacement gas are set in advance. In the step of introducing a replacement gas, the evacuation from the film forming chamber 101 is stopped, and when the internal pressure of the film forming chamber 101 reaches above the internal pressure after introducing the replacement gas, the introduction of the replacement gas is stopped to terminate the step of introducing a replacement gas. In the evacuation step, the introduction of the replacement gas is stopped, and when the internal pressure of the film forming chamber 101 reaches below the internal pressure after evacuating the replacement gas, the evacuation is stopped to terminate the evacuation step.
By increasing the number of repetitions of the cycle, or by decreasing the ratio (M/m) of a pressure M after evacuating the replacement gas to a pressure m after introducing the replacement gas, the concentration of the impurities existing in the film forming chamber 101 can be more reduced.
Further, in this embodiment, the present invention is described taking, as an example, the case where a hydrogen gas is used as a replacement gas, but in another embodiment, any gas usable for formation of an i-type layer, such as a silane gas, may be used as a replacement gas. The gas usable for the formation of the i-type layer are also usable for the formation of any of the p-type, i-type, and n-type semiconductor layers. Accordingly, it is preferable to use a gas used for the formation of the i-type layer as a replacement gas, because in this case, no impurity from this gas is immixed in the semiconductor layer.
Further, in another embodiment, an inert gas or the like, which does not have an effect on film quality of the semiconductor layer may be used as a replacement gas. In particular, a gas having a large atomic weight is apt to remain in the film forming chamber 101 after the evacuation of the inside of the film forming chamber 101 and is suitable for a replacement gas. Examples of the inert gas include an argon gas, a neon gas, a xenon gas, and the like.
Further, the replacement gas may be a mixture gas of any one or more of gases usable for the formation of the i-type layer and one or more inert gases.
3-3-2. Step of Forming p-Type Semiconductor Layer
Next, the p-type semiconductor layer 5a is formed. Hereinafter, a step of forming the p-type semiconductor layer 5a will be described.
First, the inside of the film forming chamber 101 can be evacuated to a pressure of 0.001 Pa and the substrate temperature can be set at a temperature of 200° C. or lower. Thereafter, the p-type semiconductor layer 5a is formed. A mixture gas is introduced into the film forming chamber 101 and the internal pressure of the film forming chamber 101 is kept approximately constant by a pressure control valve 117 provided in an exhaust system. The internal pressure of the film forming chamber 101 is in a range of for example, 200 Pa to 3600 Pa. As the mixture gas to be introduced into the film forming chamber 101, for example, a gas including a silane gas, a hydrogen gas, and a diborane gas can be used. Further, the mixture gas can include a gas (for example, methane gas) containing carbon atoms in order to reduce the amount of light absorption. The flow rate of the hydrogen gas can be 5 times or more and 300 times or less larger than that of the silane gas, and it is preferably approximately 5 times to 30 times in the case of forming a p-type amorphous layer, and 30 times to 300 times in the case of forming a p-type microcrystalline layer.
After the internal pressure of the film forming chamber 101 is stabilized, an alternating electric power of several kHz to 80 MHz is inputted to the cathode electrode 102 to generate plasma between the cathode electrode 102 and the anode electrode 103, thereby forming an amorphous or microcrystalline p-type semiconductor layer 5a. The power density per unit area of the cathode electrode 102 is preferably in a range of 0.01 W/cm2 to 0.3 W/cm2 in the case of forming a p-type amorphous layer, and it is preferably in a range of 0.02 W/cm2 to 0.5 W/cm2 in the case of forming a p-type microcrystalline layer.
Thus, the p-type semiconductor layer 5a having a desired thickness is formed, and then input of the alternating electric power is stopped and the film forming chamber 101 is evacuated to a vacuum.
The thickness of the p-type semiconductor layer 5a is preferably 2 nm or more, more preferably 5 nm or more in terms of providing an adequate internal electric field for the i-type amorphous layer 5c. Further, the thickness of the p-type semiconductor layer 5a is preferably 50 nm or less, more preferably 30 nm or less in terms of necessity for suppressing the amount of light absorption on a side of light entrance of an inactive layer.
Next, an i-type amorphous layer is formed as the buffer layer 5b. First, a background pressure in the film forming chamber 101 is evacuated to a vacuum of approximately 0.001 Pa. The substrate temperature can be set at a temperature of 200° C. or lower. Next, a mixture gas is introduced into the film forming chamber 101, and the internal pressure of the film forming chamber 101 is kept approximately constant by the pressure control valve 117. The internal pressure of the film forming chamber 101 is adjusted to be in a range of, for example, 200 Pa to 3000 Pa. As the mixture gas to be introduced into the film forming chamber 101, for example, a gas including a silane gas and a hydrogen gas can be used. Further, the mixture gas can include a gas (for example, methane gas) containing carbon atoms in order to reduce the amount of light absorption. Desirably, the flow rate of a hydrogen gas is approximately several times to several tens of times larger than that of a silane gas.
After the internal pressure of the film forming chamber 101 is stabilized, an alternating electric power of several kHz to 80 MHz is inputted to the cathode electrode 102 to generate plasma between the cathode electrode 102 and the anode electrode 103, thereby forming an i-type amorphous layer as the buffer layer 5b. The power density per unit area of the cathode electrode 102 may be in a range of 0.01 W/cm2 to 0.3 W/cm2.
Thus, the i-type amorphous layer having a desired thickness is formed as the buffer layer 5b, and then input of the alternating electric power is stopped and the inside of the film forming chamber 101 is evacuated to a vacuum.
By forming the i-type amorphous layer as the buffer layer 5b, the concentration of boron atoms in atmosphere in the film forming chamber 101 is reduced to allow reduction of boron atoms to be immixed in the i-type amorphous layer 5c to be formed next.
The thickness of the i-type amorphous layer as the buffer layer 5b is desirably 2 nm or more in order to inhibit diffusion of boron atoms from the p-type semiconductor layer 5a to the i-type amorphous layer 5c. On the other hand, this thickness is desirably as small as possible in order to suppress the amount of light absorption to increase light reaching the i-type amorphous layer 5c. The thickness of the buffer layer 5b is generally adjusted to 50 nm or less.
Next, a gas replacement step is performed in the same manner as in “3-3-1. Gas replacement step”.
The p-type semiconductor layer 5a, formed in the preceding step, is deposited on an inner wall and an electrode in the film forming chamber 101. Therefore, it will be a problem that impurities released from the p-type semiconductor layer 5a, particularly impurities that determine a conductive type of the p-type semiconductor layer 5a are immixed in the i-type amorphous layer 5c, but by performing the gas replacement step before the formation of the i-type amorphous layer 5c, the amount of the above-mentioned impurities to be immixed in the i-type amorphous layer 5c can be reduced. Thereby, a semiconductor layer of good quality can be formed as the i-type amorphous layer 5c.
3-3-5. Step of Forming i-Type Amorphous Layer
Next, the i-type amorphous layer 5c is formed. First, the background pressure in the film forming chamber 101 is evacuated to a vacuum of approximately 0.001 Pa. The substrate temperature can be set at a temperature of 200° C. or lower. Next, a mixture gas is introduced into the film forming chamber 101 and the internal pressure of the film forming chamber 101 is kept approximately constant by the pressure control valve 117. The internal pressure of the film forming chamber 101 is adjusted to be in a range of, for example, 200 Pa to 3000 Pa. As the mixture gas to be introduced into the film forming chamber 101, for example, a gas including a silane gas and a hydrogen gas can be used. The flow rate of the hydrogen gas is preferably approximately several times to several tens of times larger than that of the silane gas, more preferably 5 times or more and 30 times or less. In this case, the i-type amorphous layer 5c of good film quality can be formed.
After the internal pressure of the film forming chamber 101 is stabilized, an alternating electric power of several kHz to 80 MHz is inputted to the cathode electrode 102 to generate plasma between the cathode electrode 102 and the anode electrode 103, thereby forming the i-type amorphous layer 5c. The power density per unit area of the cathode electrode 102 can be in a range of 0.01 W/cm2 to 0.3 W/cm2.
Thus, the i-type amorphous layer 5e having a desired thickness is formed, and then input of the alternating electric power is stopped and the inside of the film forming chamber 101 is evacuated to a vacuum.
The thickness of the i-type amorphous layer 5c is preferably set at 0.05 μm to 0.25 μm in consideration of the amount of light absorption and deterioration of photoelectric conversion characteristics due to light degradation.
3-3-6. Step of Forming n-Type Semiconductor Layer
Next, the n-type semiconductor layer 5d is formed. First, the background pressure in the film forming chamber 101 is evacuated to a vacuum of approximately 0.001 Pa. The substrate temperature can be set at a temperature of 200° C. or lower, for example 150° C. Next, a mixture gas is introduced into the film forming chamber 101 and the internal pressure of the film forming chamber 101 is kept approximately constant by the pressure control valve 117. The internal pressure of the film forming chamber 101 is adjusted to be in a range of, for example, 200 Pa to 3600 Pa. As the mixture gas to be introduced into the film forming chamber 101, a gas including a silane gas, a hydrogen gas, and a phosphine gas can be used. The flow rate of the hydrogen gas can be 5 times or more and 300 times or less larger than that of the silane gas, and it is preferably approximately 5 times to 30 times in the case of forming an n-type amorphous layer, and 30 times to 300 times in the case of forming an n-type microcrystalline layer.
After the internal pressure of the film forming chamber 101 is stabilized, an alternating electric power of several kHz to 80 MHz is inputted to the cathode electrode 102 to generate plasma between the cathode electrode 102 and the anode electrode 103, thereby forming an amorphous or microcrystalline n-type semiconductor layer 5d. The power density per unit area of the cathode electrode 102 is preferably in a range of 0.01 W/cm2 to 0.3 W/cm2 in the case of forming an n-type amorphous layer, and it is preferably in a range of 0.02 W/cm2 to 0.5 W/cm2 in the case of forming an n-type microcrystalline layer.
The thickness of the n-type semiconductor layer 5d is preferably 2 nm or more in order to provide an adequate internal electric field for the i-type amorphous layer 5c. On the other hand, the thickness of the n-type semiconductor layer 5d is preferably as small as possible in order to suppress the amount of light absorption in the n-type semiconductor layer 5d as an inactive layer, and it is generally adjusted to 50 nm or less.
Thus, the first photoelectric conversion layer 5 including the i-type amorphous layer 5c can be formed.
Next, the second photoelectric conversion layer 7 is formed on the obtained substrate. As described above, the second photoelectric conversion layer 7 has the p-type semiconductor layer 7a, the buffer layer 7b, the i-type amorphous layer 7c, and the n-type semiconductor layer 7d, and the respective semiconductor layers are therefore formed in order.
Hereinafter, a step of forming the second photoelectric conversion layer 7 will be described in detail.
Next, a gas replacement step is performed in the same manner as in “3-3-1. Gas replacement step”. By performing this gas replacement step, it is possible to reduce the amount of impurities released from the n-type semiconductor layer deposited on an inner wall and an electrode in the film forming chamber 101 during the formation of the n-type semiconductor layer 5d, particularly impurities that determine a conductive type of the n-type semiconductor layer 5d to be immixed in the p-type semiconductor layer 7a. Thereby, a semiconductor layer of good quality can be formed as the p-type semiconductor layer 7a. Here, since the p-type semiconductor layer 7a includes p-type conductive impurities in a concentration of approximately 1×1020 cm−3, satisfactory photoelectric conversion characteristics are attained if the concentration of immixed n-type conductive impurities is approximately 1×1018 cm−3 or less, which is 2 digits less than the concentration of the p-type conductive impurities.
3-4-2. Step of Forming p-Type Semiconductor Layer
Next, the p-type semiconductor layer 7a is formed. The p-type semiconductor layer 7a can be formed in the same manner as in the formation of the p-type semiconductor layer 5a of the first photoelectric conversion layer 5.
Next, the buffer layer 7b is formed in the same manner as in the formation of the buffer layer 5b of the first photoelectric conversion layer 5.
Next, a gas replacement step is performed in the same manner as in “3-3-1. Gas replacement step”. In this gas replacement step, an effect identical or similar to that in the gas replacement step performed before the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 can be attained.
3-4-5. Step of Forming i-Type Amorphous Layer
Next, the i-type amorphous layer 7c is formed. The thickness of the i-type amorphous layer 7c is preferably set at 0.1 μm to 0.7 μm in consideration of the amount of light absorption and deterioration of the photoelectric conversion characteristics due to light degradation.
Further, it is desirable that the bandgap of the i-type amorphous layer 7c of the second photoelectric conversion layer 7 is narrower than the bandgap of the i-type amorphous layer 5c of the first photoelectric conversion layer 5. This is because, by forming such a bandgap, light of wavelength band that the first photoelectric conversion layer 5 cannot absorb can be absorbed in the second photoelectric conversion layer 7, and incident light can be utilized effectively.
In order to narrow the bandgap of the i-type amorphous layer 7c, the substrate temperature during the film formation can be set at a higher temperature. By increasing the substrate temperature, the concentration of hydrogen atoms contained in the film can be reduced and an i-type amorphous layer 7c having a small bandgap can be formed. That is, it is only necessary to adopt a substrate temperature for the formation of the i-type amorphous layer 7c of the second photoelectric conversion layer 7 higher than the substrate temperature for the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5. Thereby, it is possible to make the concentration of hydrogen atoms in the i-type amorphous layer 5c of the first photoelectric conversion layer 5 higher than the concentration of hydrogen atoms in the i-type amorphous layer 7c of the second photoelectric conversion layer 7 and to produce a stacked thin-film solar cell module in which the bandgap of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 is wider than the bandgap of the i-type amorphous layer 7c of the second photoelectric conversion layer 7.
Further, by decreasing the flow rate ratio of a hydrogen gas to a silane gas of a mixture gas to be introduced into the film forming chamber 101 in the formation of the i-type amorphous layer 7c, the concentration of hydrogen atoms contained in the i-type amorphous layer 7c can be reduced and the i-type amorphous layer 7c having a narrow bandgap can be formed. That is, it is only necessary to adopt a flow rate ratio of the hydrogen gas to the silane gas of the mixture gas in the formation of the i-type amorphous layer 7c of the second photoelectric conversion layer 7 smaller than that in the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5. Thereby, it is possible to make the concentration of hydrogen atoms in the i-type amorphous layer 5c of the first photoelectric conversion layer 5 higher than the concentration of hydrogen atoms in the i-type amorphous layer 7e of the second photoelectric conversion layer 7 and to produce a stacked thin-film solar cell module in which the bandgap of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 is wider than the bandgap of the i-type amorphous layer 7c of the second photoelectric conversion layer 7.
Furthermore, it is also possible to adjust the bandgap of the i-type amorphous layer by selecting either forming the i-type amorphous layer by continuous discharge plasma or forming the i-type amorphous layer by pulse discharge plasma. When the i-type amorphous layer is formed by continuous discharge plasma, the concentration of hydrogen atoms contained into the i-type amorphous layer to be formed can be made higher than that in the case of forming the i-type amorphous layer by pulse discharge plasma.
Accordingly, it is possible to produce a stacked thin-film solar cell module in which the bandgap of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 is wider than the bandgap of the i-type amorphous layer 7c of the second photoelectric conversion layer 7 by switching supply electric power for generating plasma so that the i-type amorphous layer 5c of the first photoelectric conversion layer 5 can be formed by continuous discharge plasma and the i-type amorphous layer 7c of the second photoelectric conversion layer 7 can be formed by pulse discharge plasma.
The setting of the substrate temperatures for the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 and the i-type amorphous layer 7e of the second photoelectric conversion layer 7, the setting of the flow rate ratio of the hydrogen gas to the silane gas, and the setting of the switching between the continuous discharge and the pulse discharge may be done separately, or the respective settings may be used in combination. In particular, when the substrate temperatures for the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 and the i-type amorphous layer 7c of the second photoelectric conversion layer 7 are the same, concurrent use of the setting of the flow rate ratio of the hydrogen gas to the silane gas and the switching between the continuous discharge and the pulse discharge is desirable, because it allows the concentration of hydrogen atoms contained in the i-type amorphous layer to be changed by a large amount.
3-4-6. Step of Forming n-Type Semiconductor Layer
Next, the n-type semiconductor layer 7d is formed. The n-type semiconductor layer 7d can be formed in the same manner as in the formation of the n-type semiconductor layer 5d of the first photoelectric conversion layer 5.
Next, the third photoelectric conversion layer 9 is formed on the obtained substrate. As described above, the third photoelectric conversion layer 9 has the p-type semiconductor layer 9a, the i-type microcrystalline layer 9b, and the n-type semiconductor layer 9c, and the respective semiconductor layers are therefore formed in order.
Hereinafter, a step of forming the third photoelectric conversion layer 9 will be described in detail.
First, a gas replacement step is performed in the same manner as in “3-3-1. Gas replacement step”. This gas replacement step has an effect identical or similar to that in the gas replacement step performed before the formation of the second photoelectric conversion layer 7.
3-5-2. Step of Forming p-Type Semiconductor Layer
Next, the p-type semiconductor layer 9a is formed. The p-type semiconductor layer 9a can be formed in the same manner as in the formation of the p-type semiconductor layer 5a of the first photoelectric conversion layer 5.
Next, a gas replacement step is performed in the same manner as in “3-3-1. Gas replacement step”. This gas replacement step has an effect identical or similar to that in the gas replacement step performed before the formation of the i-type amorphous layer 5c of the first photoelectric conversion layer 5 and the i-type amorphous layer 7c of the second photoelectric conversion layer 7.
3-5-4. Step of Forming i-Type Microcrystalline Layer
Next, the i-type microcrystalline layer 9b is formed. The i-type microcrystalline layer 9b can be formed, for example, under the following formation conditions. The substrate temperature is desirably set at a temperature of 200° C. or lower. The internal pressure of the film forming chamber 101 during the formation of the layer is desirably in a range of 240 Pa to 3600 Pa. Further, the power density per unit area of the cathode electrode 102 is desirably set to be in a range of 0.02 W/cm2 to 0.5 W/cm2.
As a mixture gas to be introduced into the film forming chamber 101, for example, a gas including a silane gas and a hydrogen gas may be used. The flow rate of the hydrogen gas is desirably approximately 30 times to several hundreds of times larger than that of the silane gas, more desirably approximately 30 times to 300 times.
The thickness of the i-type microcrystalline layer 9b is preferably 0.5 μm or more, more preferably 1 μm or more in order to secure an adequate amount of light absorption. On the other hand, the thickness of the i-type microcrystalline layer 9b is preferably 20 μm or less, more preferably 15 μm or less in order to secure good productivity.
Thus, an i-type microcrystalline layer 9b having a good crystallinity, in which the intensity ratio I520/I480) of a peak at 520 nm−1 to a peak at 480 nm−1, measured by Raman spectroscopy, is in a range of 3 to 10 can be formed.
3-5-5. Step of Forming n-Type Semiconductor Layer
Next, the n-type semiconductor layer 9c is formed. The n-type semiconductor layer 9c can be formed in the same manner as in the formation of the n-type semiconductor layer 5d of the first photoelectric conversion layer 5.
Next, the photoelectric conversion layer division line is formed in the first to third photoelectric conversion layers 5, 7, 9 so as to extend in the crosswise direction (in the X direction in
Next, the rear surface electrode 11 is formed on the third photoelectric conversion layer 9. The rear surface electrode 11 has a transparent conductive film and a metal film in this order from a side of the third photoelectric conversion layer 9, and these films are therefore formed in order.
The transparent conductive film is formed of SnO2, ITO, ZnO, or the like. The metal film is formed of a metal such as silver and aluminum. The transparent conductive film and the metal film are formed by a method such as a CVD method, a sputtering method, and a vapor deposition method. The transparent conductive film may be omitted.
When the rear surface electrode 11 is formed, a material of the rear surface electrode 11 gets into the photoelectric conversion layer division line to form the contact line 17.
Next, the rear surface electrode division line 29 extending in the crosswise direction (in the X direction in
The rear surface electrode division line 29 can be formed by scribing the rear surface electrode 11 and the first to third photoelectric conversion layers 5, 7, 9 by use of second higher harmonics of a YAG laser, for example.
Through the steps that have been described so far, the band-shaped cell string 21 having the plurality of cells 27 connected to each other in series is obtained.
Next, alignment dividing lines 25 running in the lengthwise direction (the direction Y in
The Alignment dividing line 25 can be formed by scribing the rear surface electrode 11 and the first to third photoelectric conversion layers 5, 7, 9 by use of second higher harmonics of a YAG laser, for example, and by further scribing the front surface electrode 3 by use of a fundamental wave of a YAG laser.
Next, the common electrode 23 is installed so that the plurality of cell strings 21 are connected to each other in parallel to complete production of the thin-film solar cell module 1 of this embodiment.
As described below, the RB current (current when a voltage of from 5 V to 8 V is applied in the direction opposite to the direction of the current due to the photovoltaic power) was measured while changing the width of the cell strings 21. Here, the greater the RB current is, the easier the leak current flows. In this test, the solar cell through which an RB current of 50 mA or more flowed was used as the standard for the flowing leak current. First, samples having the same structure as the thin-film solar cell module according to the above-described embodiment, which is described in reference to
Next, alignment dividing lines were formed so that the cell strings had widths of the cell strings shown in Table 2 (in this order). The RB current (current when a voltage of 5 V is applied in the opposite direction) and I-V were measured for the solar cells of the fabricated samples. Table 2 shows the width (mm) of the cell strings gained by dividing the fabricated samples in this order, the width (%) of each cell string relative to the sum of the widths of all the cell strings, and the number of solar cells where the RB current included in each cell string is 50 mA or more. In addition,
It can be seen from Table 2 and
Furthermore, as described above, the number of solar cells having an RB current of 50 mA or more is small in a range from 355 mm to 1025 mm, and therefore a leak current is considered to be small. In addition, there was no film peeling even when the power output of the cell string was great in the below described hot spot withstanding test in this range.
The distribution of the film thickness of the first photoelectric conversion layer was also checked.
It can be seen from the film thickness distribution measurement that the film thickness is stable at the center, but the film thickness is lower close to an end.
The reason why the number of solar cells having an RB current of 50 mA or more increases as the location is closer to an end of the cell module is unclear. However, the location where the film thickness of the first photoelectric conversion layer is smaller by approximately 10% and the location where the number of solar cells having an RB current of 50 mA or more increases are the same, and therefore this is one possible reason as to why the number of solar cells having an RB current of 50 mA or more increases as the location is closer to an end of the cell module.
A cell hotspot resistance test was performed by the following method.
First, a large number of samples having the same configuration (except that there is no Alignment dividing line 25 and no common electrode 23) as that of the thin-film solar cell module of the embodiment described above with reference to
Each sample produced was measured for an I-V property and an RB current (a current when a voltage of 5 V to 8 V was applied in a reverse direction; the voltage applied was appropriately varied so that the RB current values shown in Table 4 were obtained).
Next, samples that are different from one another in RB current were selected out of the above-described samples. Each of the selected samples was divided in parallel, thereby obtaining a 5 W to 50 W of output of the cell string 21 being evaluated.
Next, the hotspot resistance test was performed on a cell 27 having the smallest area in the cell string 21 for judgment of acceptance with defining a peeled area of less than 10% as an acceptance line. The hotspot resistance test was performed in accordance with TEC 61646 1st EDITION.
As the peeled area, a surface of the sample was photographed from the side of the substrate 2, the contrast of an obtained image was increased to obtain a monochrome image, and a percentage of the area accounted for by the white part in this image was calculated. Since a part that experienced peel-off of a film usually has a larger luminance, the percentage of the area of the white part obtained in the above-described manner corresponds to the percentage of the area of the part that experienced peel-off of a film (peeled area).
Table 4 shows a result obtained. Table 4 shows the results of the measurement of the area where peeling occurred for 54 types of samples having different outputs of the cell strings 21 or different RB currents. Here, the area where peeling occurred exceeded 10% in the samples indicated by dashes.
Table 4 has revealed that the samples are unlikely to experience peel-off of a film in both the case where the magnitude of the RB current is very small (0.019 mA/cm2) and the case where the magnitude of the RB current is very large (6.44 mA/cm2), and the samples are likely to experience peel-off of a film in the case where the magnitude of the RB current is moderate (0.31 to 2.06 mA/cm2), even if the output from the cell string 21 is the same.
It has been also revealed that the peeled area can be held to 10% or less regardless of the value of the RB current, when the output from the cell string is 30 W or less.
Next, a reverse overcurrent resistance test was performed in the following manner.
First, samples having the same configuration as that of the thin-film solar cell module of the embodiment described above with reference to
Next, the reverse overcurrent resistance test was performed by examining whether or not the contact line 17 was damaged when an overcurrent was applied to the produced samples in a reverse direction (the reverse direction referred to means a direction opposite to a direction in which a current passes when the solar cell is in light, that is, it would be a forward direction in the case where the solar cell not in light is considered a diode).
According to the provisions of IEC 61730, the current to be applied here needs to be 1.35 times the anti-overcurrent specification value, and was set to 5.5 A at 70 V here.
Here, when a current is applied to one cell module under the above-described condition, it is apt to be considered that the current will be divided equally to be applied to each cell string connected in parallel. Actually, however, the current can be concentrated in a particular cell string, because the resistance value varies from string to string. On the assumption that this is the worst case situation, problems must be prevented from occurring even when 70 V×5.5 A=385 W is applied to one cell string. Therefore, a power of 70 V×5.5 A=385 W was applied to one cell string 21 to carry out the test.
Samples of 20 types that are different from one another in length L or width W of the cross-section of the contact line 17 were produced to carry out the test. It was judged by visual observation whether or not the contact line 17 was damaged. The contact line 17 was judged to have been damaged when there was discoloring or peel-off in the rear surface electrode 11 in a half oval shape along the contact line 21. Table 5 shows a result obtained.
Table 5 has revealed that when the width W of the cross-section of the contact line 17 is 20 μm and 40 μm, damage to the contact line 17 can be prevented by setting the length L of the cross-section of the contact line 17 to 18 cm or more and 9 cm or more, respectively. In other words, it has been revealed that the cross-sectional area Sc of the contact line 17 should be 20 μm×18 cm=0.036 cm2 or more, or 40 μm×9 cm=0.036 cm2 or more.
Furthermore, it has been revealed that (power applied to cell string 21)/(area Sc of contact line 17)≅10.7 kW/cm2, because the power applied to the cell string 21 was 385 W, and therefore damage to the contact line 17 can be prevented when the power density applied to the contact line 21 is 10.7 kW/cm2 or less.
Here, the above-described cell strings within 18% from both ends shown in Table 2 have a sufficiently large leak path within cells judging from the results of the RB test, and the current does not concentrate on the contact lines but is dispersed, making the power consumed in the contact line small. In such a case, the contact line can be prevented from being damaged even when the above-described relationship is not met.
Number | Date | Country | Kind |
---|---|---|---|
2009-004012 | Jan 2009 | JP | national |
Filing Document | Filing Date | Country | Kind | 371c Date |
---|---|---|---|---|
PCT/JP10/50007 | 1/4/2010 | WO | 00 | 7/8/2011 |