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Energy and the New Reality, Volume 2: C-Free Energy Supply Chapter 2: Solar Energy L. D. Danny Harvey [email protected] This material is intended for use in lectures, presentations and as handouts to students, and is provided in Powerpoint format so as to allow customization for the individual needs of course instructors. Permission of the author and publisher is required for any other usage. Please see www.earthscan.co.uk for contact details. Publisher: Earthscan, UK Homepage: www.earthscan.co.uk/?tabid=101808

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Energy and the New Reality, Volume 2: C-Free Energy Supply Chapter 2: Solar Energy L. D. Danny Harvey [email protected]. Publisher: Earthscan, UK Homepage: www.earthscan.co.uk/?tabid=101808. - PowerPoint PPT Presentation

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Page 1: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Energy and the New Reality, Volume 2:

C-Free Energy Supply

Chapter 2: Solar Energy

L. D. Danny [email protected]

This material is intended for use in lectures, presentations and as handouts to students, and is provided in Powerpoint format so as to allow customization for the individual needs of course instructors. Permission of the author and publisher is required for any other usage. Please see www.earthscan.co.uk for contact details.

Publisher: Earthscan, UKHomepage: www.earthscan.co.uk/?tabid=101808

Page 2: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Framework• Solar flux density on a plane perpendicular to the sun’s rays at

the mean Earth-Sun distance, Qs, is 1370 W/m2

• The intercepted solar radiation flux (Qs x πRe2) is about 11000

times the 2005 world primary power demand of 15.3 TW• About 0.8% of the world’s desert area (or 80,700 km2) covered

with 10% efficient modules would be all that is required to generate the total world electricity consumption in 2005 of about 18000 TWh

• However, cumulative installation of PV panels to date is only 25 km2

• The solution is to directly use solar energy where-ever possible (for passive heating and ventilation, for thermal-driven cooling, and for daylighting), and to use solar electricity only where electricity really is needed.

Page 3: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

This chapter discusses:

• Photovoltaic generation of electricity• Solar-thermal generation of electricity• Solar thermal energy for space heating and for

hot water• Solar thermal energy for air conditioning• Industrial uses of solar thermal energy• Direct uses of solar energy for desalination, in

agriculture and for cooking

Page 4: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Chapter 4 (Buildings) of Volume 1 discusses passive (as opposed to active) uses of solar energy, with the building itself serving as a collector of solar energy. These passive uses are

• Passive heating• Passive ventilation• Daylighting

Page 5: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Chapter 11 (Community-Integrated Energy systems with Renewable Energy) of this volume

discusses seasonal underground storage of solar thermal energy for space heating and for domestic

hot water

Page 6: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.1a Stereographic sun path diagram

Source: Computed using The Solar Tool developed by Square One Research, available through Ecotech (ecotech.com)

Page 7: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.1b Stereographic sun path diagram

Source: Computed using The Solar Tool developed by Square One Research, available through Ecotech (ecotech.com)

Page 8: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.1c Stereographic sun path diagram

Source: Computed using The Solar Tool developed by Square One Research, available through Ecotech (ecotech.com)

Page 9: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.1d Stereographic sun path diagram

Source: Computed using The Solar Tool developed by Square One Research, available through Ecotech (ecotech.com)

Page 10: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.2a Solar irradiance, daily variation, clear sky

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Figure 2.2b Solar irradiance, daily variation , clear sky

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Figure 2.2c Solar irradiance, daily variation, clear sky

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Figure 2.2g Solar irradiance, daily variation, clear sky

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Page 14: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.2h Solar irradiance, daily variation, clear sky

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Page 15: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.2i Solar irradiance, daily variation, clear sky

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Page 16: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Observations on the diurnal variations (Fig 2.2):

• On June 21

- the further north, the longer the day and the less intense the noon peak

- the differences in irradiance on a panel tilted at the latitude angle are smaller than on a horizontal panel

- there is almost no difference in the irradiance on a sun-tracking PV panel within 5 hours of solar noon, but irradiance is less at other times at high latitudes because of the greater pathlength through the atmosphere (so more radiation is absorbed by the atmosphere)

• On Dec 21

-- the further north, the shorter the day

– differences are much greater, and sun tracking does not help much at high latitude (because even when pointed at the sun, the pathlength through the atmosphere is large)

Page 17: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.3a Solar irradiance, annual variation, clear sky

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Figure 2.3b Solar irradiance, annual variation, clear sky

Page 19: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.3c Solar irradiance, annual variation, clear sky

Page 20: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Observations on seasonal variation of diurnal average irradiance on a PV panel (Fig 2.3)

• If the panel has a fixed tilt equal to the latitude of the site, the result is greater irradiance in winter and less in summer compared to a horizontal panel

• 1-axis tracking, whereby the tilt is adjusted each day to equal the latitude minus solar declination, gives greater irradiance all year compared to fixed tilt

• 2-axis tracking is substantially better than 1-axis tracking

Page 21: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.4a Solar irradiance on windows in June, clear sky

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Page 22: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.4b Solar irradiance on windows in December, clear sky

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Page 23: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.5 Annual average solar irradiance (W/m2) at ground level on a horizontal surface

Source: Henderson-Sellers and Robinson (1986, Contemporary Climatology, Longman, Harlow, U.K)

Page 24: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Supplemental Figure: Solar irradiance on a horizontal surface, kWh/m2/yr

Source: Prepared from data file obtained from the NASA Surface Meteorology and Solar Energy website, power.larc.nasa.gov

500 700 900 1100 1300 1500 1700 1900 2100 2300 2500

Page 25: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Supplemental Figure: Solar irradiance on a surface tilted toward the equator at an angle equal to the latitude angle, kWh/m2/yr

500 700 900 1100 1300 1500 1700 1900 2100 2300 2500

Source: Prepared from data file obtained from the NASA Surface Meteorology and Solar Energy website, power.larc.nasa.gov

Page 26: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Supplemental Figure: Ratio of annual irradiance on a surface tilted at the latitude angle to the annual irradiance on a horizontal surface

0.98 1.00 1.05 1.10 1.15 1.20 1.25

Source: Prepared from data files obtained from the NASA Surface Meteorology and Solar Energy website, power.larc.nasa.gov

Page 27: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Two broad ways of making electricity from solar energy:

• Photovoltaic (PV)

• Solar thermal

Page 28: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

PV Electricity

• Electromagnetic radiation (including light) comes in packets called photons, each with energy hv, where h=Plank’s constant and v is the frequency of the radiation

• Electrons in an atom exist in different energy levels

• A photon can bump an electron to a higher energy level if the energy of the photon exceeds the difference in energy from one level to the next

Page 29: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

PV electricity (continued)

• When a solid forms, two outer energy bands are formed, often separated by a gap

• The lower energy band is called the valence band, the upper the conduction band

• In a conductor, electrons occur in both bands and they overlap

• In an insulator, the valence band is filled and the conduction band is empty, and the two bands do not overlap

• In a semi-conductor, electrons occur in both bands and there is a small gap between the bands

Page 30: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

PV electricity (continued)

• Silicon is a semi-conductor with a valence of 4 (4 electrons in the outer shell)

• Two semiconductor layers are used – one layer (called the n-type layer) is doped with atoms have an valence of 5 (the extra electron is not taken up in the crystal lattice and so it free to move), and the other layer (called the p-type layer) is doped with atoms having a valence of 3, so there are empty electron sites (called holes)

• The juxtaposition of the n- and p layers is called a p-n junction.

Page 31: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.6 Steps in the generation of electricity in a photovoltaic cell

Source: US EIA (2007, Solar Explained, Photovoltaics and Electricity)

Page 32: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.7 Layout of a silicon solar cell

Source: Boyle (2004, Renewable Energy, Power for a Sustainable Future, 65-104, Oxford University Press, Oxford)

Page 33: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Components of a PV system

• Module – consists of many cells wired together• Support structure• Inverter – converts DC module output to AC

power at the right voltage and frequency for transfer to the grid

• Concentrating mirrors or lens for concentrating PV systems

Page 34: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Types of PV cells

• Single-crystalline• Multi-crystalline• Thin-film amorphous silicon• Thin-film compound semiconductors• Thin-film multi-crystalline• Nano-crystalline dye-sensitized cells• Plastic cells

Page 35: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Thin-film compound semiconductors

• Cadmium telluride (CdTe)

• Copper-indium-diselenide (CuInSe2, CIS)

• Copper-indium-gallium-diselenide (CIGS)• Gallium arsenide (GaAs)

Page 36: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Table 2.3 Best efficiencies achieved as of 2009

U n co n ce n tr a ted S u n lig h t C o n ce n tr a te d S u n lig h t Te ch n o lo g y C e ll M o d u le C e ll C o n ce n tr a tio n F a cto r

S in g le- ju n ctio n s ilic o n se m ic o n d u cto r c- S i 2 5 .0 2 2 .9 2 7 .6 9 2 m -S i 2 0 .4 1 5 .5 a - S i 9 .5 t h in- film S i 1 6 .7 8 .2

S in g le -ju n ctio n co m p o u n d sem ico n d u cto rs C d Te 1 6 .7 1 0 .9 C IG S 1 9 .4 1 3 .5 2 1 .8 1 4 In P 2 2 .1 th in - film G a A s 2 6 .1 2 8 .8 2 3 2 m -G a A s 1 8 .4

M u lti- ju n c tio n se m ic o n d u cto rs a - S i/µ c - S i 11 .7 a - S i/a- S iG e/a -S iG e 1 0 .4 th in - film G a A s/C IS 2 5 .8 G a In P /G a A s 3 0 .3 G a In P /G a A s/G e 3 2 .0 4 0 .7 2 4 0 G a In P /G a In A s/G e 4 1 .1 4 5 4

P h o to c h e m ic a l a n d O rg a n ic D y e-sen s itized 1 0 .4 O rg a n ic 5 .2

Page 37: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.8 Trend in efficiency of PV cells and modules

Source: Extended from IEA (2003, Renewables for Power Generation, Status and Prospects, International Energy Agency, Paris)

Page 38: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.9. Structure of the

GaInP/GaInAs/Gemulti-junction

Cell

Source: Kinsey et al (2009, Progress in Photovoltaics: Research and Applications 16, 503-508)

Page 39: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.10 Organic Semiconductors

Source: Rand et al (2007, Progress in Photovoltaics: Research and Applications 15, 659–676)

Page 40: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.11 Dye-sensitized Solar Cell

Source: McConnell (2002, Renewable and Sustainable Energy Reviews 6, 271–295, http://www.sciencedirect.com/science/journal/13640321)

Page 41: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Factors affecting module efficiency

• Solar irradiance – efficiency peaks at around 500 W/m2 for non-concentrating cells

• Temperature – efficiency decreases with increasing temperature, more so for c-Si and CIGS, less for a-Si and CdTe

• Dust – can reduce output by 3-6% in desert areas

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Figure 2.12a Module efficiency vs solar irradiance, theoretical calculations

Source: Topic et al (2007, Progress in Photovoltaics: Research and Applications 15, 19–26)

Page 43: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.12b Module efficiency vs solar irradiance, measurements

Source: Mondol et al (2007, Progress in Photovoltaics: Research and Applications 15, 353–368)

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System efficiency is the product of

• Module efficiency• Inverter efficiency• MPP-tracking efficiency

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Figure 2.13a Inverter & MPP Efficiency, calculated

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Figure 2.13b Inverter & MPP Efficiency, measured

Source: Mondol et al (2007, Progress in Photovoltaics: Research and Applications 15, 353–368)

Page 47: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.14 Current-voltage combinations (MPP) giving the maximum power production for different

solar irradiances on the module

Source: Hastings and Mørck (2000, Solar Air Systems: A Design Handbook. James & James, London)

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Figure 2.15 MPP-tracking efficiency

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The net effect of all the losses is represented by the performance ratio: the ratio of actual kWh of generated AC electricity to kWh of DC electricity produced by the module

Recent values have averaged around 75-80%

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Building-Integrated PV (BiPV)

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Figure 2.16 PV mounted onto a sloping roof

Source: Prasad and Snow (2005, Designing with Solar Power: A Sourcebook for Building Integrated Photovoltaics, Earthscan/James & James, London)

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Figure 2.17 PV integrated into a sloping roof

Source: Omer et al (2003, Renewable Energy 28, 1387-1399, http://www.sciencedirect.com/science/journal/09601481)

Page 53: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.18a BiPV on single-family house in Finland

Source: Hestnes (1999, Solar Energy 67, 181–187, http://www.sciencedirect.com/science/journal/0038092X)

Page 54: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.18b BiPV on a single-family house in Maine

Source: Hestnes (1999, Solar Energy 67, 181–187, http://www.sciencedirect.com/science/journal/0038092X)

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Supplemental figure: BiPV on multi-unit housing somewhere in Europe

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Figure 2.19 PV modules (attached to insulation) on a horizontal flat roof

Source: www.powerlight.com

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Figure 2.21 BiPV (opaque elements) on the Condé Nast building in New York

Source: Eiffert and Kiss (2000, Building-Integrated Photovoltaic Designs for Commercial and Institutional Structures: A Sourcebook for Architects, National Renewable Energy Laboratory, Golden, Colorado)

Page 58: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.22 PV modules servings as shading louvres onthe Netherlands Energy Research Foundation building

Source: Photographs by Marcel von Kerckhoven, BEAR Architecten (www.bear.nl)

Page 59: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Supplemental figure PV modules as vertical shading louvres on the SBIC East head office building in Tokyo

Source: Shinkenchiku-Sha and www.oja-services.nl/iea-pvps/cases jpn_02.htm

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Figure 2.23 PV modules providing partial shading in the atrium of the Brundtland Centre (Denmark, left)

and Kowa Elementary School (Tokyo, right)

Source: Shinkenchiku-Sha Source: Henrik Sorensen, Esbensen Consulting

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Supplemental figure: Amersfoort project, The Netherlands

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Table 2.4: Potential electricity production from BiPV

Potential BiPVArea (km2)

Potential SolarElectricity (TWh/yr)

Source: Gutschner and Task 7 Members (2001, Potential for Building-Integrated Photovoltaics, www.iea-pvps.org)

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Parking lots in the US:

• Area of 1.9 million ha (19000 km2, or 137.8 km x 137.8 km)

• PV covering all parking lots at 180 W/m2 and 15% efficiency would generate

~ 4500 TWh/yr• Total US electricity demand is

~ 4200 TWh/yr

Page 64: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Concentrating PV

• More sunlight on the expensive solar cell (by up to a factor of 500), using less expensive mirrors or lens

• Cell efficiencies are greater under concentrated sunlight, compounding the benefit of greater solar irradiance

• Works only with direct irradiance (not diffuse)• Requires 1- or 2-axis sun tracking• Passive or active heat removal required

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Figure 2.24 Concentrating PV using a Fresnel lens

Source: www.ENTECHSolar.com

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Figure 2.25 Entech concentrating PV

Source: www.ENTECHSolar.com

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Figure 2.26 Amonix concentrating PV

Source: www.amonix.com

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Figure 2.27 Flatcon point focus concentrating PV

Source: Peharz and Dimroth (2005, Progress in Photovoltaics: Research and Applications 13, 627–634)

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Figure 2.28b Growth in installed PV power, 2004-2014

Source: EPIA Market Update reports and IEA-PVPS Trends reports

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Figure 2.28a Growth in annual PV production

Source: EPIA Market Update reports and IEA-PVPS Trends reports

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Source: G. Masson, 2012. PV Market Status, A New Ecosystem for Electric Utilities

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Cost of PV electricity

• Module cost per kW peak output

= (module cost per m2 )/ (ηm Ip)

where Ip is the assumed maximum irradiance (1000 W/m2) and η m is the module efficiency (sunlight to DC). This cost is cost per peak kW of DC electricity output.

• Electricity cost ($/kWh) =

(CRF+INS)*(1+ID)*CapCost/(8760 * CF * ηbos) where CRF and INS are the cost recovery and insurance

factors, ID is an indirect factor, CapCost is the total capital cost ($/kWp-DC), CF = Ia/Ip ,ηbos is the balance-of system efficiency, and Ia is the mean annual irradiance

Page 73: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Component and installed costs (as of 2010)

• Modules: ~ $400/m2, or $4000/kW-DC if the efficiency is 10%

• Inverters: ~ $300-600/kW-DC (less for larger systems)

• Total installed cost: ~ $6000-9000/kW-AC

Page 74: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Costs of alternative cladding materials:

• Stainless steel: ~ $250-350/m2

• Glass-wall systems: ~ $500-750/m2

• Rough stone: ~ ≥ $750/m2

• Polished stone: ~ $2000-2500/m2

Page 75: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Projection of future costs

• Extrapolation using the progress ratio concept• Engineering-based bottom-up analysis

(Recall from the wind chapter: The progress ratio is the factorby which the cost is multiplied for each successive doubling in cumulative global production. It gives a good fit to thechange in cost over time for a very wide range of technologies,although of course the progress ratio value varies fromtechnology to technology, but is usually 0.8-0.9)

Page 76: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Figure 2.29 Price of Photovoltaic Module

1

10

100

0.1 1 10 100 1000 10000

Cumulative global PV module shipments in MWp

Pri

ce

of

PV

mo

du

les

(U

S$

/Wp)

Source: van Sark et al (2008, Progress in Photovoltaics: Research and Applications 16, 441-453)

Page 77: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

Results of bottom-up analyses:

• A “bottom-up analysis” involves an item-by-item consideration of everything that affects cost, and how each could change over time or with economies of scale.

• Projected near-term (2015) module costs of $1/Wp for both c-Si and a-Si, installed costs of $3/Wp or less with 1 GWp/yr manufacturing facilities

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What actually happened?

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Trend in average PV module costs in the US

Source: Clean Energy Canada (2015)

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Installed cost of residential PV systems in Germany and the US (and the common module+inverter cost)

Source: Seel et al. (2014, Energy Policy 69:216-226)

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Cost of electricity from systems installed at the end of 2012 in Los Angeles, in Los Angeles if they had German costs, and in German

cities (which have much less solar radiation). Electricity costs with Los Angeles solar radiation and German installed-costs would be about 8

cents/kWh without any subsidy.

Source: Seel et al. (2014, Energy Policy 69:216-226)

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Costs of signing up a residential PV customer in the US and Germany

Source: Seel et al. (2014, Energy Policy 69:216-226)

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Person-hours spend installing a PV system in the USA and Germany (left) and in doing various paperwork (right)

Source: Seel et al. (2014, Energy Policy 69:216-226)

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Figure 2.30 Triple-junction a-Si on laminated roofing

Source: Hegedus (2006, Progress in Photovoltaics: Research and Applications 14, 393–411)

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Resource constraints on thin-film PV

• CIGS will be limited by the indium supply• CdTe will be limited by the tellurium supply• The constraints involve both the absolute supply

of In or Te, and the rate at which it can be supplied

• In and Te are supplied as a byproduct of mining copper, zinc, and bauxite

Page 87: Publisher: Earthscan, UK Homepage:  earthscan.co.uk/?tabid=101808

In the absence of concentrating PV,

• CdTe, CIGS, and a-Si:Ge together are unlikely to be able to provide more than 1 TW peak power (compared to 4.3 TW global electricity generating capacity and 15.3 TW average global primary power demand in 2005)

• Dye-sensitized cells (which require ruthenium) could provide 6 TWp

• Near 100% recycling of rare elements would be required for long-term sustainability

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Solar Thermal Generation of Electricity

• Mirrors are used to concentrate sunlight either onto a line focus or a point focus

• Steam is generated, and then used in a steam turbine

• In some cases, concentrated solar energy heats a storage medium (such as molten salt), so electricity can be generated 24 hours per day using stored heat at night

• Best in desert or semi-desert regions, as only direct-beam solar radiation can be used

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The radiation available for use by concentrating solar thermal power (CSTP) systems is referred to as the ‘direct normal’ radiation – the annual value is the irradiance on a surface that is always at 90o to the sun’s rays

As only the direct beam radiation can be used, the peak irradiance that can be used by CSTP is typically about 850 W/m2, compared to 1000 W/m2 for PV systems

Thus, peak power capacity for CSTP is given assuming a direct beam irradiance of 850 W/m2 rather than 1000 W/m2

The annual capacity factor is equal to the annual average direct normal irradiance (in W/m2) divided by 850 W/m2 (in the same way that the annual capacity factor for PV is given by the annual average irradiance on the module divided by 1000 W/m2)

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Supplemental Figure: Annual direct normal irradiance, kWh/m2/yr

500 700 900 1100 1300 1500 1700 1900 2100 2300 2500

Source: Prepared from data files obtained from the NASA Surface Meteorology and Solar Energy website, power.larc.nasa.gov

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Supplemental Figure: Ratio of annual direct normal irradiance to annual total irradiance on a horizontal surface

0.6 0.8 0.9 1.0 1.1 1.2 1.3 1.4

Source: Prepared from data files obtained from the NASA Surface Meteorology and Solar Energy website, power.larc.nasa.gov

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Types of Solar Thermal Systems:

• Parabolic trough• Parabolic dish (Stirling engine)• Central tower

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Figure 2.34a Parabolic trough schematic

Source: Greenpeace (2005, Wind Force 12: A Blueprint to Achieve 12% of the World’s Electricity from Wind Power by 2020, Global Wind Energy Council, www.gwec.org)

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Figure 2.34b Central receiver schematic

Source: Greenpeace (2005, Wind Force 12: A Blueprint to Achieve 12% of the World’s Electricity from Wind Power by 2020, Global Wind Energy Council, www.gwec.org)

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Figure 2.34c Parabolic dish schematic

Source: Greenpeace (2005, Wind Force 12: A Blueprint to Achieve 12% of the World’s Electricity from Wind Power by 2020, Global Wind Energy Council, www.gwec.org)

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Figure 2.35a Parabolic Trough Thermal Electricity, Kramer Junction, California

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Figure 2.35b Parabolic Trough Thermal Electricity, Kramer Junction, California

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Figure 2.35c Close-up of parabolic trough

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Growth in global CSTP capacity, 2006-2014

Source: Compiled from various REN21 Update reports

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Distribution of CSTP capacity at the end of 2014

Source: REN21 2015 Update

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The latest parabolic trough systems either

• Directly heat the water that will be used in the steam turbine, or

• Directly heat water that in turn is circulated through a hot tank of molten salts (40% K-nitrate and 60% Na-nitrate), with the molten salts storing heat and in turn heating the steam that is used in a steam turbine, as illustrated in the following diagram

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Figure 2.36 AndaSol-1 Schematic

Source : Translated from Aringhoff (2002, Proyectos Andasol, Plantas Termosolares de 50 MW’, Presentation at the IEA Solar Paces 62nd Exco Meetings Host Country Day )

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Molten salt storage tanks at Andasol-1, Spain

Source: Garvin Heath (2009, LCA of Parabolic Trough CSP….), www.nrel.gov/docs/fy09osti/46875.pdf

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With thermal storage,

• Electricity can be generated 24 hours per day• The capacity factor (average output over peak

output) can reach 85%

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Figure 2.37 Parabolic trough capacity factor

0.0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

0 2 4 6 8 10 12 14 16 18 20

An

nu

al C

aq

pa

cit

y F

ac

tor

Thermal Energy Storage (Hours)

1.0

1.5

2.0

2.5

3.0

3.5

4.0

5.0

Solar Field Size(Solar Multiple)

Source : Price et al (2007, Proceedings of Energy Sustainability 2007, 27-30 June, Long Beach, California)

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Table 2.14 Characteristics of existing and possible future parabolic-trough systems

Source: EC (2007, Concentrating Solar Power, from Research to Implementation, www.solarpaces.org) and Solúcar

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Figure 2.38 Integrated Solar Combined-Cycle (ISCC) powerplant

Source: Greenpeace (2005, Wind Force 12: A Blueprint to Achieve 12% of the World’s Electricity from Wind Power by 2020, Global Wind Energy Council, www.gwec.org)

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Figure 2.39 Parabolic dish/Stirling engine for generation of electricity

Source: US CSP (2002) Status of Major Project Opportunities, presentation at the 2002 Berlin Solar Paces CSP Conference

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Figure 2.40 Stirling Receiver

Source: Mancini et al (2003, Journal of Solar Energy Engineering 125, 135–151)

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Figure 2.41 Energy flow in 4 different parabolic dish/Stirling engine systems

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Figure 2.42 Central tower solar thermal powerplant in California

Source: US CSP (2002) Status of Major Project Opportunities, presentation at the 2002 Berlin Solar Paces CSP Conference

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Figure 2.43 Solar Thermal Seasonal variation in the production of solar-thermal electricity in Egypt, Spain, and Germany

0

20

40

60

80

100

120

Mo

nth

ly E

lec

tric

ity Y

ield

(%

)

El Kharga

Madrid

Freiburg

Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec

Source: GAC (2006, Trans-Mediterranean Interconnection for Concentrating Solar Power, Final Report, www.dlr.de/tt/trans-csp )

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US DOE target for cost of CSTP established in 2010 for 2020 as part of the “SunShot” programme

Source: http://energy.gov/eere/sunshot/downloads/2014-sunshot-initiative-concentrating-solar-power-subprogram-overview

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US CSTP projects online in 2013-2014

Source: http://energy.gov/eere/sunshot/downloads/2014-sunshot-initiative-concentrating-solar-power-subprogram-overview

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Progress toward 2020 cost goals

Source: http://energy.gov/eere/sunshot/downloads/2014-sunshot-initiative-concentrating-solar-power-subprogram-overview

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Pilot projects in China

• 2 central tower projects, July 2013 start,

-a 1-MW powerplant, $5900/kW cap cost, $0.40/kWh, -___electricity cost

-a 50-MW powerplant, $3000/kW , $0.19/kWh• 1 parabolic trough project, 50 MW at $4620/kW,

$0.27/kWh• 1 parabolic dish project, 1 MW at $6505/kW, $0.43/kWh• Costs expected to fall in half by 2020

Source: Zhu et al. (2015, Energy 89:65-74)

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Figure 2.44 Projected cost of heliostats (accounting at present for half the cost of central-tower systems) vs production rate (starting from present

costs and production)

0

50

100

150

200

250

300

100 1000 10000 100000

Pri

ce

(U

SD

/m2)

Production Rate (units/yr)

Source: IEA (2003, Renewables for Power Generation, Status and Prospects, International Energy Agency, Paris)

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Overall projections for CSTP (applicable to all 3 types)

• $2000-3000/kW capital cost

• 5-8 cents/kWh electricity cost

• 25% capacity factor without thermal storage

• 13-15% overall conversion efficiency, sunlight on collectors to AC electricity output

• Saudi Arabia had been planning to install 5 GW of CSTP (roughly doubling current global capacity), which would have driven costs down, but this is on hold due to the self-induced collapse of oil prices (and hence, in the country’s oil revenue)

• Planned projects in Tunisia and Egypt are also on hold because of unrest in the region

• Spain has pulled back for budgetary reasons

• For now, its seems that the US and China will be driving the costs down through learning-by-doing

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Solar Thermal Energy For Heating and for Domestic Hot

Water

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Figure 2.45 Types of collectors for heating and domestic hot water

Source: Everett (2004, Renewable Energy, Power for a Sustainable Future, 17-64, Oxford University Press, Oxford)

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Figure 2.46 Installation of flat-plate solar thermal collectors

Source: www.socool-inc.com

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Figure 2.47a Integration of solar thermal collectors into the building facade

Source: Sonnenkraft, Austria

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Figure 2.47b Integration of solar thermal collectors into the building roof

Source: Sonnenkraft, Austria

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Supplemental figure: Evacuated-tube solar thermal collectors

Source: Posters from the AIRCONTEC Trade Fair, Germany, April 2002, available from www.iea-shc-task25.org

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Supplemental figure: Evacuated-tube solar thermal collectors

Source: Posters from the AIRCONTEC Trade Fair, Germany, April 2002, available from www.iea-shc-task25.org

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Figure 2.48 Integrated passive evacuated-tube collector and storage tank in China

Source: Morrison et al (2004, Solar Energy 76, 135-140, http://www.sciencedirect.com/science/journal/0038092X)

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Figure 2.49 Compound parabolic-trough solar-thermal collector by Solargenix

Source: Gee et al (2003, 2003 International Solar Energy Conference, Kohala Coast, Hawaii, USA, 15-18 March 2003, 295-300)

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Efficiency of solar thermal collectors:

• This is the ratio of heat energy supplied to solar energy incident on the collector

• Heat is lost as the collector heats up• Thus, the key to high efficiency is to supply lots

of heat at a relatively low temperature, through a combination of low inlet water temperature and high flow rate

• To do this, the end use applications must be able to make use of heat at relatively low temperature

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For space heating, this requires being able to use heat as it is generated in a radiant floor heating system, which in turn requires high thermal mass exposed to the inside (so that the building does not overheat) and a high-performance envelope (so that the building stays warm after sunset without having to store solar heat in a hot water tank)

For domestic hot water, this requires use of a thermally-stratified hot-water tank, with cold water from the bottom of the tank fed to the solar collector and hot water for use drawn from the top of the collector

Phase-change materials (which store heat without a further increase in temperature) can also be used. Materials with melting points around 60-70oC would be ideal for domestic hot water applications.

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Figure 2.50 Efficiency of solar thermal collectors

0.0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1.0

0 0.04 0.08 0.12

Eff

icie

nc

y

(Ti-Ta)/I

Single-glazed

Double-glazed

Evacuated-tube

5-cm Encapsulated TIM

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Costs in Europe

• Solar-air collectors, 200-400 euros/m2

• Flat-plate or CPC collectors, 200-500 euros/m2

• Evacuated-tube collectors, 450-1200 euros/m2

Storage system costs are extra

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Table 2.17 Illustrative costs of solar thermal energy

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Table 2.16: Countries with 1 million m2 or more of solar thermal collectors in 2007.

Source: Weiss et al (2009, Solar Heat Worldwide, www.iea-shc.org)

W ater C o llec to rs A ir C o lle c to rs C o u n try U n g laz ed G laz ed E v a cu a te d U n g laz ed G laz ed

To ta l

To ta l A d d e d in

2 0 0 7 A u stra lia 4 0 7 0 1 6 6 0 2 3 5 7 5 3 7 8 2 A u stria 6 0 8 2 9 5 0 4 3 3 6 0 1 2 9 0 B raz il 9 7 3 5 8 7 0 .3 5 3 6 8 5 5 7 3 C h in a 1 0 ,4 0 0 1 0 3 ,7 4 0 11 4 ,1 4 0 2 1 ,1 4 0 F ran c e + T er r 1 0 5 1 4 1 7 3 3 1 5 5 4 3 2 3 G e rm an y 7 5 0 7 7 8 4 8 6 4 9 3 9 8 9 7 0 G reec e 3 5 6 6 6 .8 3 5 7 3 2 8 3 In d ia 2 1 5 0 1 7 2 1 6 7 2 5 7 Is rae l 2 4 4 9 3 6 4 9 6 1 7 2 Ita ly 2 6 8 7 4 1 0 3 1 0 0 2 2 4 9 Jap a n 6 8 2 5 1 2 7 4 3 4 1 3 7 3 9 9 1 8 3 S p a in 3 11 6 4 4 6 1 2 1 3 2 6 5 S w itz er la n d 2 1 2 4 3 3 2 5 8 3 8 1 5 0 9 7 8 Taiw a n 11 3 7 11 8 1 2 5 5 1 3 5 Tu rk ey 1 0 ,1 5 0 1 0 ,1 5 0 7 0 0 U S A 2 7 ,6 3 9 1 8 9 8 5 7 8 0 .0 9 2 3 0 3 0 ,3 4 6 1 2 7 6 To ta l 3 5 ,8 2 0 6 6 ,2 7 2 1 0 5 ,8 8 5 1 4 0 9 2 8 2 2 0 9 ,6 6 9 2 8 ,4 4 0 To ta l C a p a city (G W t h)

2 5 .1 4 6 .4 7 4 .1 0 .9 9 0 .1 2 1 4 6 .8 1 9 .8

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Figure 2.51 Growth in the worldwide area of solar thermal collectors

The thermal power capacity at the end of 2013 was 373 GW

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Figure 2.52a Top ten countries in terms of total solar thermal collector area, end of 2007

0 20 40 60 80 100 120

China

US

Turkey

Germany

Japan

Australia

Israel

Brazil

Austria

India

Collector Area (millions m2)

Evacuated tube

Glazed

Unglazed

Air

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Figure 2.52b Top ten countries in terms of solar thermal collector area per capita, end of 2007

0 100 200 300 400 500 600 700

Cyprus

Israel

Austria

Greece

Barbados

Australia

Jordon

Turkey

Germany

US

China

Collector Area (m2 per 1000 inhabitants)

Evacuated-tube + Glazed

Unglazed

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System-level interactions with solar domestic hot water

• Normally, some back-up hot water heating system is needed with solar thermal systems

• When solar thermal energy is used, the back-up system on average runs at lower efficiency than if it is the sole source of hot water (efficiency can drop from 85% to 45% if solar provides 80% of the required hot water)

• Thus, the net savings in energy is less than the fraction of the hot-water load met with solar energy (when 80% of the load is met with solar, the savings could be 80% of that, or 64%)

• If the backup system is a modulating condensing heater, there will not be an efficiency loss at part load

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Solar Thermal Energy For Air Conditioning and

Dehumidification

• Absorption chillers• Solid desiccant systems• Liquid desiccant systems

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From Chapter 4 of Volume 1: Desiccant cooling systems require heat in order to regenerate the desiccant. The

desiccant dehumidifies the supply air, making it sufficient dry that cooling of the supply air through evaporation of

water is feasible with producing air that is too humid

D

C

E F G H

AB

EvaporativeCooler

HeatExchanger

DesiccantWheel

HeatInpu t

Optional EvaporativeCoole r

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Temperature-mixing ratio trajectories with desiccant dehumidification and evaporative cooling

0

2

4

6

8

10

12

14

16

18

20

22

24

26

28

30

0 5 10 15 20 25 30 35 40 45 50 55 60 65 70 75 80 85 90 95 10 0

Dry Bulb Temperature (oC)

H 60 40 20

A

B

D

F

10

C

6 3

E G

H'

Mix

ing

Ra

tio

(g

ram

s m

ois

ture

per

kil

og

ram

dry

air

)

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The effectiveness of any cooling system is represented by its Coefficient of Performance (COP), which is the ratio of cooling provided to energy input

• For conventional electric cooling systems, the COP ranges from 2.0 (low-end room air conditioners) to 7.0 (in large central systems with cooling towers)

• For absorption chillers, the COP is ~0.6 using 90°C heat and ~ 1.2 using 120°C heat as the energy input

• For solid desiccants, the COP is ~ 0.5 using 80°C heat• For liquid desiccants, the COP is ~ 0.75 using 75°C heat

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System considerations with solar air conditioning with absorption chillers:

• If fossil fuels are used to produce heat for absorption chillers as a backup when there is not adequate solar heat, the inefficiency of the absorption chiller compared to an electric chiller offsets some of the benefit of moving from an electric chiller to an absorption chiller using solar energy part of the time

• The low COP of the absorption chiller compared to an electric chillers means that more heat in total needs to be removed by the cooling tower, so the electricity use by auxiliary equipment (fans, motors, pumps) is larger, and this offsets some of the benefit of switching from electricity to solar heat for the core cooling function

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Figure 2.53 COP vs Driving Temperature for thermally-driven cooling equipment

0.0

0.2

0.4

0.6

0.8

1.0

1.2

1.4

50 70 90 110 130 150 170

CO

P

Driving temperature (oC)

Liquid desiccant

Absorption H2O/LiBr

Absorption

Solid desiccant

Absorption NH3/H2O

Absorption diffusion NH3/H2O

Steam jet

Absorption double-effect

Source: Balaras et al (2007, Renewable and Sustainable Energy Reviews 11, 299–314, http://www.sciencedirect.com/science/journal/13640321)

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Costs

• 1000 to 8000 euros per kW of cooling capacity for solar thermal systems

• 100 euros/kW for large conventional cooling systems

• The cost of solar systems is dominated by the cost of the collectors, so if collector costs come down, or the collectors are used for heating in the winter (so that only part of the collector cost need be ascribed to cooling), then the cooling cost will be smaller

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Solar cogeneration

• Mount a PV module over a solar thermal collector, so that both electricity and useful heat are collected

• By removing heat from the back of the module, the PV electrical efficiency increases

• However, the thermal collection efficiency will not be as large as for a dedicated solar thermal collector, and there might be an extra glazing over the PV panel, which reduces the production of electricity by absorbing some solar radiation

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Figure 2.54 Cost vs solar collector area for solar-thermal air conditioning

0

1000

2000

3000

4000

5000

6000

7000

8000

9000

0.0 2.0 4.0 6.0 8.0 10.0

Init

ial C

os

t (E

uro

s/k

W)

Specific Collector Area (m2/kW)

Absorption

Solid desiccant

Liquid desiccant

Absorption NH3/H2O

Absorption H2O/LiBr

Source: Balaras et al (2007, Renewable and Sustainable Energy Reviews 11, 299–314, http://www.sciencedirect.com/science/journal/13640321)

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Figure 2.55 Cost of saved primary energy versusthe magnitude of the savings

0

5

10

15

20

25

25 30 35 40 45 50 55

Co

st

of

Sa

ved

Pri

ma

ry E

ne

rgy

(eu

roc

en

ts/k

Wh

)

Primary Energy Savings (%)

Absorption, heat backup

Absorption, electric backup

Adsorption, heat backup

Adsorption, electric backup

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Figure 2.56 Proposed hybrid electric-thermal cooling using parabolic solar collectors

Solar input100 kW

Parabolicsolarcollector

80 kWthermal

33.6 kWelectricity

100.8 - 134.4 kWcooling

Electricchiller

COP = 3 - 4

51.8 kWcooling

COP = 1.35

Absorptionchiller38.4 kW

thermal

Waste heat

1.0 - - losses

= 0.48

turbine

collector = 0.8

turbine = 0.42

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Figure 2.57: Cross-section of a PV/T solar collector

Source: Charalambous et al (2007, Applied Thermal Engineering 27, 275–286, http://www.sciencedirect.com/science/journal/13594311)

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Industrial uses of Solar Energy

• Low temperature (60-260oC)

Food processing – often at 80-120oC

Textiles

Some chemical and plastics processes• High temperature (900-2400 K, readily achieved

with solar furnaces) reduction of metal ores

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Other uses of solar energy:

• Desalination of seawater• Fixation of nitrogen• Solar cooling of greenhouses (with desiccants

and evaporation)• Crop drying• Cooking

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Desalination Options:

• Solar electricity to power reverse osmosis desalination (80 MJ solar/m3)

• Solar heat to power multi-stage flash desalination (600 MJ solar/m3)

• Extraction from night air with desiccants, regeneration of desiccant with solar heat

• Condensation from humidified air with cool seawater

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Source: Clery (2011, Science 331, 136)

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Source: Clery (2011, Science 331, 136)

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Dealing with intermittency

• Use rapidly variable fossil backup• Aggregate geographically-dispersed PV arrays• Install energy storage (V2G plug-in hybrid cars

in particular) and develop dispatchable loads• Link diverse renewable energy resources

(especially if the variability of non-solar resources complements the solar variability)

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Figure 2.58a PV Variability

0.0

0.1

0.2

0.3

0.4

0.5

0.6

0.7

0.8

0.9

1.0

0 12 24 36 48 60 72

Time (hours)

P/P

In

stal

led

100 systemsone system

Source: Wiemken et al (2001, Solar Energy 70, 6, 513–518, http://www.sciencedirect.com/science/journal/0038092X)

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Figure 2.58b PV Variability

0.0

0.1

0.2

0.3

0.4

0.5

0 6 12 18 24

Time (hours)

No

rmal

ised

Po

wer

Average of 100 systemsStdev of 1 systemStdev of 100 systems

Source: Wiemken et al (2001, Solar Energy 70, 6, 513–518, http://www.sciencedirect.com/science/journal/0038092X)

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Figure 2.59 Decreasing correlation between output of PV modules with increasing distance between them

0.0

0.2

0.4

0.6

0.8

1.0

0 100 200 300 400 500 600 700

Distance (km)

r ij

Source: Wiemken et al (2001, Solar Energy 70, 6, 513–518, http://www.sciencedirect.com/science/journal/0038092X)

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Concluding Comments

• The solar energy resource is enormous but diffuse, so large land areas would be involved in capturing it

• Many of our energy needs involve low-temperature heat (for space heating and hot water, and for some industrial processes), and so do not require the intermediary of expensive solar electricity

• Thus, the first strategy in using solar energy should be to design buildings to make passive use of solar energy – for heating, ventilation, and cooling (which occurs when passive ventilation brings in outside air that is cooler than the temperature that the building would reach on its own)

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Concluding Comments (continued)

• Two strategies for generating electricity for solar energy are photovoltaic (PV) and solar-thermal

• PV electricity can be done centrally or on site as building-integrated PV (BiPV)

• BiPV alone could provide 15-60% of total electricity needs in various countries

• Solar thermal electricity can be generated 24 hours per day but requires direct-beam solar radiation – so it is best in desert or semi-arid regions

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Concluding Comments (continued)

• PV cells can use conventional materials (silicon) or various toxic (As, Cd) or rare (Ge, In, Te, Ru, Se) elements, with those using rare elements being most efficient (up to 30%, vs 10-15% for crystalline silicon-based cells and 6-8% for amorphous silicon)

• Limits on the availability of the rare materials represent real constraints on how much electricity could be supplied with these cells

• The limit can be increased by a factor of 100 or so using concentrating PV cells, and would no longer be an issue.

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Table 2.21: Summary of methods to produce electricity from solar energy

C o sts E ffic ie n c y A d v a n ta g e D isa d v a n ta g e P V

C r y sta llin e s ilic o n (s in g le , p o ly )

3 0 -4 0 ce n ts /k W h in b est lo ca tio n s , 9 -1 3 cen ts /k W h fo r b e st p ro ject io n

1 0 -1 5 % m o d u le s , 2 0 % ev e n tu a lly

S ilica is a b u n d a n t, h ig h er e f fic ie n c y th a n a m o r p h o u s

M a ter ia l in p u ts , g rea te r em b o d ied en er g y

T h in f ilm a m o r p h o u s s ilic o n

5 -6 % m o d u les , 1 0 % h o p ed fo r

C a n g o o n a n y th in g , su ited to co n tin u o u s p ro d u c tio n

L o w e ff ic ien cy

M u lti-ju n ctio n th in film s u s in g v a r io u s r a re su b sta n ce s (e .g . C IS , C d Te )

H ig h e st c o st

2 5 -3 3 % ce lls, 4 1 % u n d e r co n ce n tra ted su n lig h

H ig h e f fic ien cy

U se s to x ic o r ra re e le m en ts , h ig h co st

N a n o cr y sta llin e d y e ce lls

1 0 % ce ll a t 2 5 °C

E ffic ie n c y in c re a ses w ith te m p er a tu re , ca n b e tr a n sp a ren t to v is ib le ra d ia tio n

R e q u ire s r a re ru th en iu m

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Table 2.21: Summary of methods to produce electricity from solar energy

C o sts E ffic ien cy A d v a n ta g e D isa d v a n ta g e C o n ce n tra tin g P V

cr y sta llin e S i 2 8 % @ 9 2 su n s

C IG S 2 2 % @ 1 4 su n s th in -film G a A s 2 9 % @ 2 3 2

su n s G a In P /G a A s/G e 4 1 % @ 4 5 4

su n s

P o te n tia lly lo w e r co st, s tretch es ra re e le m en ts

M o re co m p lica ted , req u ires d irect b ea m so la r ra d ia tio n

Q u a n tu m d o t C o n ce n tra te s d irec t a n d d if fu se ra d ia tio n w ith o u t tr a ck in g

S till u n d er d ev e lo p m e n t

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Table 2.21: Summary of methods to produce electricity from solar energy

C o sts E ffic ie n c y A d v a n ta g e D isa d v a n ta g e T h e rm a l

P a r a b o lic tro u g h

1 2 -2 0 ce n ts /k W h n o w, 5 -1 0 cen ts k W h fu tu re

1 5 -2 0 % , 4 2 -4 8 % C F w ith 6 -h o u r s to ra g e

L a rg e sca le , lo ts o f d e m o p ro jects , so m e s to r a g e

T h e rm a l s to r a g e m o re d if ficu lt th a n fo r o th e r th er m a l m e th o d s

P a r a b o lic d ish

1 0 -1 4 0 0 0 € /k W , ev e n tu a lly $ 2 -3 0 0 0 /k W (8 -2 4 ce n ts /k W h )

2 0 -2 8 %

S u ita b le fo r iso la te d v illa g e s , lo w in fra str u c tu re co sts , q u ick s ta r t

E x p e n siv e a t p re sen t, lim ited h e a t s to r a g e a b ility

C e n tra l rec e iv e r

1 8 -3 2 ce n ts /k W h to d a y

1 0 -1 5 %

M o st a m en a b le to 2 4-h o u r e le ctr ic ity

E a c h m irro r m u st in d iv id u a lly tr a ck th e su n

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Concluding comments (continued)

• PV electricity is currently expensive (~ 20-25 cents/kWh in sunny locations, 45-60 cents/kWh in midlatitude locations) but will likely fall in price by a factor of 2 or more during the next decade

• This would make BiPV highly competitive with peak electricity, which can cost 15-30 cents/kWh (retail price)

• Parabolic-trough concentrating solar-thermal electricity is already in the 12-20 cents/kWh range and could drop to as low as 5 cents/kWh

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Other active uses of solar energy

• Solar air conditioning• Medium-temperature (60-260oC) industrial heat• High-temperature (1000-2500oC) industrial heat• Solar fixation of nitrogen• Crop drying• Cooking