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UNIT - II
Solar Energy
Environmental Impacts of Solar Power
• The sun provides a tremendous resource for generating clean and
sustainable electricity without toxic pollution or global warming
emissions.
• The potential environmental impacts associated with solar
power — land use and habitat loss, water use, and the use of
hazardous materials in manufacturing — can vary greatly depending
on the technology, which includes two broad categories:
photovoltaic (PV) solar cells or concentrating solar thermal plants
(CSP).
• The scale of the system — ranging from small, distributed rooftop
PV arrays to large utility-scale PV and CSP projects — also plays a
significant role in the level of environmental impact.
Land Use
• Depending on their location, larger utility-scale solar facilities can
raise concerns about land degradation and habitat loss. Total land
area requirements varies depending on the technology, the
topography of the site, and the intensity of the solar resource.
Estimates for utility-scale PV systems range from 3.5 to 10 acres per
megawatt, while estimates for CSP facilities are between 4 and 16.5
acres per megawatt.
• Unlike wind facilities, there is less opportunity for solar projects to
share land with agricultural uses. However, land impacts from
utility-scale solar systems can be minimized by siting them at lower-
quality locations such as brownfields, abandoned mining land, or
existing transportation and transmission corridors [1, 2]. Smaller
scale solar PV arrays, which can be built on homes or commercial
buildings, also have minimal land use impact.
Water Use
• Solar PV cells do not use water for generating electricity. However, as in all
manufacturing processes, some water is used to manufacture solar PV
components.
• Concentrating solar thermal plants (CSP), like all thermal electric plants,
require water for cooling. Water use depends on the plant design, plant
location, and the type of cooling system.
• CSP plants that use wet-recirculating technology with cooling towers
withdraw between 600 and 650 gallons of water per megawatt-hour of
electricity produced. CSP plants with once-through cooling technology
have higher levels of water withdrawal, but lower total water consumption
(because water is not lost as steam). Dry-cooling technology can reduce
water use at CSP plants by approximately 90 percent.
• However, the tradeoffs to these water savings are higher costs and lower
efficiencies. In addition, dry-cooling technology is significantly less
effective at temperatures above 100 degrees Fahrenheit.
Hazardous Materials
• The PV cell manufacturing process includes a number of hazardous materials, most
of which are used to clean and purify the semiconductor surface. These chemicals,
similar to those used in the general semiconductor industry, include hydrochloric
acid, sulfuric acid, nitric acid, hydrogen fluoride, 1,1,1-trichloroethane, and
acetone. The amount and type of chemicals used depends on the type of cell, the
amount of cleaning that is needed, and the size of silicon wafer.
• Workers also face risks associated with inhaling silicon dust. Thus, PV
manufactures must follow U.S. laws to ensure that workers are not harmed by
exposure to these chemicals and that manufacturing waste products are disposed
of properly.
• Thin-film PV cells contain a number of more toxic materials than those used in
traditional silicon photovoltaic cells, including gallium arsenide, copper-indium-
gallium-diselenide, and cadmium-telluride[5]. If not handled and disposed of
properly, these materials could pose serious environmental or public health
threats. However, manufacturers have a strong financial incentive to ensure that
these highly valuable and often rare materials are recycled rather than thrown
away.
Life-Cycle Global Warming Emissions
• While there are no global warming emissions associated
with generating electricity from solar energy, there are
emissions associated with other stages of the solar life-
cycle, including manufacturing, materials transportation,
installation, maintenance, and decommissioning and
dismantlement. Most estimates of life-cycle emissions for
photovoltaic systems are between 0.07 and 0.18 pounds of
carbon dioxide equivalent per kilowatt-hour.
• Most estimates for concentrating solar power range from
0.08 to 0.2 pounds of carbon dioxide equivalent per
kilowatt-hour. In both cases, this is far less than the lifecycle
emission rates for natural gas (0.6-2 lbs of CO2E/kWh) and
coal (1.4-3.6 lbs of CO2E/kWh) .
Measurement of Sunshine Duration
Sunshine duration is the length of time that the ground
surface is irradiated by direct solar radiation (i.e., sunlight
reaching the earth's surface directly from the sun).
In 2003, WMO defined sunshine duration as the period during
which direct solar irradiance exceeds a threshold value of
120 watts per square meter (W/m2).
This value is equivalent to the level of solar irradiance shortly
after sunrise or shortly before sunset in cloud-free
conditions. It was determined by comparing the sunshine
duration recorded using a Campbell-Stokes sunshine
recorder with the actual direct solar irradiance.
Campbell-Stokes Sunshine Recorders
Principles and Structure :
A Campbell-Stokes sunshine recorder
concentrates sunlight through a glass sphere
onto a recording card placed at its focal point.
The length of the burn trace left on the card
represents the sunshine duration.
Reading of Recording Paper
To obtain uniform results for observation of sunshine duration with a
Campbell-Stokes sunshine recorder, the following points should be noted when
reading records:
(a) If the burn trace is distinct and rounded at the ends, subtract half of the
curvature radius of the trace’s ends from the trace length at both ends.
Usually, this is equivalent to subtracting 0.1 hours from the length of each
burn trace.
(b) If the burn trace has a circular form, take the radius as its length. If there
are multiple circular burns, count two or three as a sunshine duration of 0.1
hours, and four, five or six as 0.2 hours. Count sunshine duration this way in
increments of 0.1 hours.
(c) If the burn trace is narrow, or if the recording card is only slightly discolored,
measure its entire length.
(d) If a distinct burn trace diminishes in width by a third or more, subtract 0.1
hours from the entire length for each place of diminishing width. However, the
subtraction should not exceed half the total length of the burn trace.
Jordan Sunshine Recorders
• A Jordan sunshine recorder lets in sunlight
through a small hole in a cylinder or a semi-
cylinder onto photosensitized paper set inside
the cylinder on which traces are recorded.
One common type has two hollow semi-cylinders arranged back to
back with their flat surfaces facing east and west. Each flat surface
has a small hole in it. The Jordan sunshine recorder used by JMA is
the same in principle, but consists of a hollow cylinder with two
hole.
The instrument has its cylinders inclined to the relevant latitude and
their axes set in the meridional direction. Photosensitized paper
with a time scale printed on it is set in the cylinders in close contact
with the inner surface. When direct solar radiation enters through
the hole, the paper records the movement of the sun as a line.
Sunshine duration is ascertained by measuring the length of time
the paper was exposed to sunlight.
Measurement of Solar Radiation
Radiometers
A radiometer absorbs solar radiation at its sensor, transforms it into heat and
measures the resulting amount of heat to ascertain the level of solar radiation.
Methods of measuring heat include taking out heat flux as a temperature change
(using a water flow pyrheliometer, a silver-disk pyrheliometer or a bimetallic
pyranograph) or as a thermoelectromotive force (using a thermoelectric
pyrheliometer or a thermoelectric pyranometer). In current operation, types using a
thermopile are generally used.
The radiometers used for ordinary observation are pyrheliometers and pyranometers
that measure direct solar radiation and global solar radiation, respectively, and these
instruments are described in this section. For details of other radiometers such as
measuring instruments for diffuse sky radiation and net radiation, refer to ”Guide to
Meteorological Instruments and Observation Methods” and “Compendium of Lecture
Notes on Meteorological Instruments for Training Class III and Class IV Meteorological
Personnel” published by WMO.
Pyrheliometers
• A pyrheliometer is used to measure direct
solar radiation from the sun and its marginal
periphery.
• To measure direct solar radiation correctly, its
receiving surface must be arranged to be
normal to the solar direction. For this reason,
the instrument is usually mounted on a sun-
tracking device called an equatorial mount.
ANGSTROM ELECTRICAL COMPENSATION PYRHELIOMETER
SILVER-DISK PYRHELIOMETER
THERMOELECTRIC PYRHELIOMETER
Pyranometers
A pyranometer is used to measure global
solar radiation falling on a horizontal surface. Its
sensor has a horizontal radiation-sensing surface
that absorbs solar radiation energy from the
whole sky (i.e. a solid angle of 2π sr) and
transforms this energy into heat. Global solar
radiation can be ascertained by measuring this
heat energy. Most pyranometers in general use
are now the thermopile type, although bimetallic
pyranometers are occasionally found.
THERMOELECTRIC PYRANOMETERS
The instrument’s radiation-sensing element has basically
the same structure as that of a thermoelectric
pyrheliometer. Another similarity is that the
temperature difference derived between the radiation-
sensing element (the hot junction) and the reflecting
surface (the cold junction) that serves as a temperature
reference point is expressed by a thermopile as an
thermoelectromotive force. In the case of a
pyranometer, methods of ascertaining the temperature
difference are as follows:
THERMOELECTRIC PYRANOMETERS
1) Several pairs of thermocouples are connected in series to
make a thermopile that detects the temperature difference
between the black and white radiation-sensing surfaces
(Figures 7.9 (a) and (c)).
2) The temperature difference between two black radiation-
sensing surfaces with differing areas is detected by a
thermopile.
3) The temperature difference between a radiation-sensing
surface painted solid black and a metallic block with high
heat capacity is detected by a thermopile (Figure 7.9 (b)).
BIMETALLIC PYRANOGRAPH
The radiation-sensing element (in the upper right of the figure) consists of two pairs of
bimetals, one painted black and the other painted white, placed in opposite directions
(face up and face down) and attached to a common metal plate at one end. At the other
end, the white bimetallic strips are fixed to the frame of the pyranograph, and the black
ones are connected to the recorder section via a transmission shaft. The deflection of
the free edge of the black strips is transmitted to the recording pen through a
magnifying system. When the air temperature changes, the black and white strips
attached to the common plate at one end both bend by the same amount but in
opposite directions. As a result, only the temperature difference attributed to solar
radiation is transmitted to the recording pen.
Thermoelectric pyranometers and bimetallic pyranographs are both hermetically sealed
in a glass dome to protect the sensor portion from wind and rain and prevent the
sensor surface temperature from being disturbed by wind. A desiccant is placed in the
dome to prevent condensation from forming on the inner surface. The glass allows the
passage of solar radiation in wavelengths from about 0.3 to 3.0 m – a range that covers
most of the sun's radiation energy. Some models are equipped with a fan to prevent
dust or frost, which greatly affect the amount of light received, from collecting on the
dome’s outer surface. It is necessary to check and clean the glass surface at regular
intervals to ensure that the dome wall constantly allows the passage of solar radiation.
15.PPT_RESS_2021-22_1_SOLAR ENERGY.pptx

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15.PPT_RESS_2021-22_1_SOLAR ENERGY.pptx

  • 2. Environmental Impacts of Solar Power • The sun provides a tremendous resource for generating clean and sustainable electricity without toxic pollution or global warming emissions. • The potential environmental impacts associated with solar power — land use and habitat loss, water use, and the use of hazardous materials in manufacturing — can vary greatly depending on the technology, which includes two broad categories: photovoltaic (PV) solar cells or concentrating solar thermal plants (CSP). • The scale of the system — ranging from small, distributed rooftop PV arrays to large utility-scale PV and CSP projects — also plays a significant role in the level of environmental impact.
  • 3. Land Use • Depending on their location, larger utility-scale solar facilities can raise concerns about land degradation and habitat loss. Total land area requirements varies depending on the technology, the topography of the site, and the intensity of the solar resource. Estimates for utility-scale PV systems range from 3.5 to 10 acres per megawatt, while estimates for CSP facilities are between 4 and 16.5 acres per megawatt. • Unlike wind facilities, there is less opportunity for solar projects to share land with agricultural uses. However, land impacts from utility-scale solar systems can be minimized by siting them at lower- quality locations such as brownfields, abandoned mining land, or existing transportation and transmission corridors [1, 2]. Smaller scale solar PV arrays, which can be built on homes or commercial buildings, also have minimal land use impact.
  • 4. Water Use • Solar PV cells do not use water for generating electricity. However, as in all manufacturing processes, some water is used to manufacture solar PV components. • Concentrating solar thermal plants (CSP), like all thermal electric plants, require water for cooling. Water use depends on the plant design, plant location, and the type of cooling system. • CSP plants that use wet-recirculating technology with cooling towers withdraw between 600 and 650 gallons of water per megawatt-hour of electricity produced. CSP plants with once-through cooling technology have higher levels of water withdrawal, but lower total water consumption (because water is not lost as steam). Dry-cooling technology can reduce water use at CSP plants by approximately 90 percent. • However, the tradeoffs to these water savings are higher costs and lower efficiencies. In addition, dry-cooling technology is significantly less effective at temperatures above 100 degrees Fahrenheit.
  • 5. Hazardous Materials • The PV cell manufacturing process includes a number of hazardous materials, most of which are used to clean and purify the semiconductor surface. These chemicals, similar to those used in the general semiconductor industry, include hydrochloric acid, sulfuric acid, nitric acid, hydrogen fluoride, 1,1,1-trichloroethane, and acetone. The amount and type of chemicals used depends on the type of cell, the amount of cleaning that is needed, and the size of silicon wafer. • Workers also face risks associated with inhaling silicon dust. Thus, PV manufactures must follow U.S. laws to ensure that workers are not harmed by exposure to these chemicals and that manufacturing waste products are disposed of properly. • Thin-film PV cells contain a number of more toxic materials than those used in traditional silicon photovoltaic cells, including gallium arsenide, copper-indium- gallium-diselenide, and cadmium-telluride[5]. If not handled and disposed of properly, these materials could pose serious environmental or public health threats. However, manufacturers have a strong financial incentive to ensure that these highly valuable and often rare materials are recycled rather than thrown away.
  • 6. Life-Cycle Global Warming Emissions • While there are no global warming emissions associated with generating electricity from solar energy, there are emissions associated with other stages of the solar life- cycle, including manufacturing, materials transportation, installation, maintenance, and decommissioning and dismantlement. Most estimates of life-cycle emissions for photovoltaic systems are between 0.07 and 0.18 pounds of carbon dioxide equivalent per kilowatt-hour. • Most estimates for concentrating solar power range from 0.08 to 0.2 pounds of carbon dioxide equivalent per kilowatt-hour. In both cases, this is far less than the lifecycle emission rates for natural gas (0.6-2 lbs of CO2E/kWh) and coal (1.4-3.6 lbs of CO2E/kWh) .
  • 7. Measurement of Sunshine Duration Sunshine duration is the length of time that the ground surface is irradiated by direct solar radiation (i.e., sunlight reaching the earth's surface directly from the sun). In 2003, WMO defined sunshine duration as the period during which direct solar irradiance exceeds a threshold value of 120 watts per square meter (W/m2). This value is equivalent to the level of solar irradiance shortly after sunrise or shortly before sunset in cloud-free conditions. It was determined by comparing the sunshine duration recorded using a Campbell-Stokes sunshine recorder with the actual direct solar irradiance.
  • 8. Campbell-Stokes Sunshine Recorders Principles and Structure : A Campbell-Stokes sunshine recorder concentrates sunlight through a glass sphere onto a recording card placed at its focal point. The length of the burn trace left on the card represents the sunshine duration.
  • 9.
  • 10. Reading of Recording Paper To obtain uniform results for observation of sunshine duration with a Campbell-Stokes sunshine recorder, the following points should be noted when reading records: (a) If the burn trace is distinct and rounded at the ends, subtract half of the curvature radius of the trace’s ends from the trace length at both ends. Usually, this is equivalent to subtracting 0.1 hours from the length of each burn trace. (b) If the burn trace has a circular form, take the radius as its length. If there are multiple circular burns, count two or three as a sunshine duration of 0.1 hours, and four, five or six as 0.2 hours. Count sunshine duration this way in increments of 0.1 hours. (c) If the burn trace is narrow, or if the recording card is only slightly discolored, measure its entire length. (d) If a distinct burn trace diminishes in width by a third or more, subtract 0.1 hours from the entire length for each place of diminishing width. However, the subtraction should not exceed half the total length of the burn trace.
  • 11. Jordan Sunshine Recorders • A Jordan sunshine recorder lets in sunlight through a small hole in a cylinder or a semi- cylinder onto photosensitized paper set inside the cylinder on which traces are recorded.
  • 12.
  • 13. One common type has two hollow semi-cylinders arranged back to back with their flat surfaces facing east and west. Each flat surface has a small hole in it. The Jordan sunshine recorder used by JMA is the same in principle, but consists of a hollow cylinder with two hole. The instrument has its cylinders inclined to the relevant latitude and their axes set in the meridional direction. Photosensitized paper with a time scale printed on it is set in the cylinders in close contact with the inner surface. When direct solar radiation enters through the hole, the paper records the movement of the sun as a line. Sunshine duration is ascertained by measuring the length of time the paper was exposed to sunlight.
  • 14. Measurement of Solar Radiation Radiometers A radiometer absorbs solar radiation at its sensor, transforms it into heat and measures the resulting amount of heat to ascertain the level of solar radiation. Methods of measuring heat include taking out heat flux as a temperature change (using a water flow pyrheliometer, a silver-disk pyrheliometer or a bimetallic pyranograph) or as a thermoelectromotive force (using a thermoelectric pyrheliometer or a thermoelectric pyranometer). In current operation, types using a thermopile are generally used. The radiometers used for ordinary observation are pyrheliometers and pyranometers that measure direct solar radiation and global solar radiation, respectively, and these instruments are described in this section. For details of other radiometers such as measuring instruments for diffuse sky radiation and net radiation, refer to ”Guide to Meteorological Instruments and Observation Methods” and “Compendium of Lecture Notes on Meteorological Instruments for Training Class III and Class IV Meteorological Personnel” published by WMO.
  • 15. Pyrheliometers • A pyrheliometer is used to measure direct solar radiation from the sun and its marginal periphery. • To measure direct solar radiation correctly, its receiving surface must be arranged to be normal to the solar direction. For this reason, the instrument is usually mounted on a sun- tracking device called an equatorial mount.
  • 19. Pyranometers A pyranometer is used to measure global solar radiation falling on a horizontal surface. Its sensor has a horizontal radiation-sensing surface that absorbs solar radiation energy from the whole sky (i.e. a solid angle of 2π sr) and transforms this energy into heat. Global solar radiation can be ascertained by measuring this heat energy. Most pyranometers in general use are now the thermopile type, although bimetallic pyranometers are occasionally found.
  • 20. THERMOELECTRIC PYRANOMETERS The instrument’s radiation-sensing element has basically the same structure as that of a thermoelectric pyrheliometer. Another similarity is that the temperature difference derived between the radiation- sensing element (the hot junction) and the reflecting surface (the cold junction) that serves as a temperature reference point is expressed by a thermopile as an thermoelectromotive force. In the case of a pyranometer, methods of ascertaining the temperature difference are as follows:
  • 21. THERMOELECTRIC PYRANOMETERS 1) Several pairs of thermocouples are connected in series to make a thermopile that detects the temperature difference between the black and white radiation-sensing surfaces (Figures 7.9 (a) and (c)). 2) The temperature difference between two black radiation- sensing surfaces with differing areas is detected by a thermopile. 3) The temperature difference between a radiation-sensing surface painted solid black and a metallic block with high heat capacity is detected by a thermopile (Figure 7.9 (b)).
  • 22.
  • 23. BIMETALLIC PYRANOGRAPH The radiation-sensing element (in the upper right of the figure) consists of two pairs of bimetals, one painted black and the other painted white, placed in opposite directions (face up and face down) and attached to a common metal plate at one end. At the other end, the white bimetallic strips are fixed to the frame of the pyranograph, and the black ones are connected to the recorder section via a transmission shaft. The deflection of the free edge of the black strips is transmitted to the recording pen through a magnifying system. When the air temperature changes, the black and white strips attached to the common plate at one end both bend by the same amount but in opposite directions. As a result, only the temperature difference attributed to solar radiation is transmitted to the recording pen. Thermoelectric pyranometers and bimetallic pyranographs are both hermetically sealed in a glass dome to protect the sensor portion from wind and rain and prevent the sensor surface temperature from being disturbed by wind. A desiccant is placed in the dome to prevent condensation from forming on the inner surface. The glass allows the passage of solar radiation in wavelengths from about 0.3 to 3.0 m – a range that covers most of the sun's radiation energy. Some models are equipped with a fan to prevent dust or frost, which greatly affect the amount of light received, from collecting on the dome’s outer surface. It is necessary to check and clean the glass surface at regular intervals to ensure that the dome wall constantly allows the passage of solar radiation.