Thermo-Fluid Ch 8

Authors and Acknowledgements

  • John Andrews and Nick Jelley (2017).
  • Lecture 13: Photovoltaics by Ramesh K. Agarwal, Washington University in St. Louis. Contact: rka@wustl.edu

Textbook Reference

  • Andrews & Jelley: Energy Science, 3rd Edition
  • Photovoltaic Effect: An Introduction to Solar Cells

References

  • The Physics of Solar Cells by Jenny Nelson, Imperial College Press, 2003.
  • Solar Cells by Marin A. Green, The University of New South Wales, 1998.
  • Silicon Solar Cells by Martin A. Green, The University of New South Wales, 1995.

Solar Energy Potential

  • Theoretical energy available:
    • 1.76 × 10^5 TW striking the Earth
  • Practical energy harnessing potential:
    • 600 TW (considering 2% of Earth’s surface area)
  • Conversion Efficiency:
    • Approximately 10%
  • Electricity Generation Potential:
    • Approximately 60 TW
  • Estimated Global Demand in 2050:
    • Between 30-35 TW

Land Area Required for Solar Energy

  • Distribution of Energy Generation in Various Regions:

    • Europe
    • North America
    • Asia and Russia
    • South America
    • Africa
    • Australia and Oceania
  • Example Calculation:

    • 6 Boxes at 4.2 TW each = 25 TW (Source: EB, Inc. 1998)

Solar Land Area Requirement in the U.S.

  • Geographical Spread:
    • Various states detailed with approximate land area requirements for solar energy setup based on land-use efficiency.

Photovoltaic Energy Conversion Technologies

  • First Generation (I):
    • Crystalline PV
  • Second Generation (II):
    • Thin Film PV
  • Third Generation (III):
    • Based on nanotechnology, utilizing collections of atoms from semiconducting materials.
    • Films with nano-crystalline structures and nanostructured conducting polymers designed to absorb a vast portion of the solar spectrum.
    • Expected high efficiency and low cost from PV cells made from thinly stacked plastic sheets.

Role of Photo-Electrochemistry in Solar Cells

  • Converging area between solar cell technology and battery or fuel cell technology.
  • Plays a significant role in the development of organic solar cells.

Photovoltaic Efficiency Over Time

  • Power Conversion Efficiency (%):
    • Crystalline Si, Amorphous Si, Nano TiO₂, CIS/CIGS, CdTe from 1950-2000 shown over several decades graphically.

Cost Trends in Photovoltaics

  • Cost of Electricity Generated by Photovoltaics:
    • Levelized cost of electricity (COE) trends in cents/kWh from 1980 to 2020.

The Solar Spectrum

  • Definition:
    • Corresponds to the spectrum of a black body at 5800 K.
  • Impact of Atmosphere:
    • Sunlight intensity reduced from 1.36 kW/m² (AM0) to 1.0 kW/m² (AM1.5).
    • AM1.5 considers that sunlight's effective path through the atmosphere is approximately 1.5 times the height of the standard atmosphere.
    • Corresponds to sunlight at an angle of 48 degrees to the vertical.
  • Absorption of Wavelengths:
    • Water vapor, CO2, and CH4 mostly absorb in the infrared region, corresponding to photon energies below 1.7 eV.
    • Visible light energy ranges from ~ 3 eV (400 nm) to ~ 1.7 eV (700 nm).

Incident Solar Radiation Data

  • Total Incident Power from the Sun:
    • Approximately 150,000 TW.
  • Comparison with Global Power Consumption (2022):
    • Approximately 23 TWth.
  • Average Solar Flux on Earth:
    • ~ 1 kW/m² with attenuation from 1.37 kW/m² to 1.0 kW/m² due to the atmosphere.
  • Silicon Photovoltaic (PV) Cells:
    • ~20% conversion efficiency observed.
    • Installed capacity and growth statistics from 2015 to 2021:
    • 2015: 242 GWh, 2021: 950 GWh.
  • Cost Competitiveness:
    • PV systems becoming competitive or cheaper than fossil fuel generation in various sunny regions.

Solar Radiation Characteristics

  • Radiation Types:
    • Direct and Diffuse radiation percentages affected by clarity of sky (Average yearly: 30%).
  • Variability with Geography:
    • Total radiation ranges from 2300 kWh/m² in tropics to ~800 kWh/m² in arctic regions.
    • Intensity on cloudy versus sunny days noted (10% near arctic vs. 50% in tropics).
  • Insolation Definition:
    • Average energy hitting earth daily (kWh/m²/day); varies by latitude and seasonal changes.

Overview of Solar Cells

  • Definition of Solar Cell:
    • Fundamental unit in photovoltaic systems, converting solar radiation to electric current. Typically made from semiconductors.
  • Semiconductor Classification:
    • Materials can conduct electricity.
    • Metals: Good conductors.
    • Insulators: Poor conductors.
    • Semiconductors: Intermediate class with moderate conductivity, affected by temperature and impurities.

Example Calculations in Solar Energy

  • Example 8.1:
    • Calculation for energy incident on a solar cell given intensity 200 W/m² and an area of 0.1 m².
    • Calculation of Incident Power (P):
    • P=IimesA=200imes0.1=20extW=0.02extkWP = I imes A = 200 imes 0.1 = 20 ext{ W} = 0.02 ext{ kW}
    • Calculation of Incident Energy (E):
    • E=Pimest=0.02extkWimes24exth=0.48extkWhE = P imes t = 0.02 ext{ kW} imes 24 ext{ h} = 0.48 ext{ kWh}
    • Also calculated as E=Pimest=20extWimes24imes60imes60s=1.73extMJE = P imes t = 20 ext{ W} imes 24 imes 60 imes 60s = 1.73 ext{ MJ}
  • Variation with Sunlight Angle:
    • If sunlight arrives at an angle of 30°:
    • The incident power is reduced by factor extcos(30°)ext{cos}(30°).
    • New incident energy is E=0.42extkWhextor1.50extMJE = 0.42 ext{ kWh} ext{ or } 1.50 ext{ MJ}

Understanding Photons in Photovoltaics

  • Definition of Photon:
    • Smallest energy unit transferred in atomic processes, specifically a quantum of light.
  • Einstein’s Relation for Photons' Energy (ε):
    • Given by the formula: ext{Energy}
      ightarrow ext{ } ext{ε} = h imes v
    • Where hh = Planck's constant = 6.62 × 10^-34 joule-sec and vv = frequency in cycles/s.
  • Wavelength Calculation:
    • Relationship given by: c=extλimesvc = ext{λ} imes v
    • Where cc = speed of light = 3 × 10^8 m/s and extλext{λ} = wavelength in meters.
  • Energy Quantization:
    • Radiation is in whole multiples of hv (as photons).

Power Relations in Photovoltaic Applications

  • Incident Power Formula:
    P=IimesAP = I imes A
  • Incident Energy Calculation:
    E=PimestE = P imes t
  • Photon Flux Definition:
    • Number of photons crossing a unit area per second. Quantified in PV calculations.
  • Energy of a Photon Record:
    • For a red light wavelength of λ=6000Aλ = 6000A (or 6000 × 10^-10 m).

Example 8.2 Reflection and Photon Flux Calculation

  • Photon Flux Calculation:
    • Light with a wavelength of 510 nm (green) and intensity of 500 W/m² incident on a solar cell.
  • Calculating Photon Energy:
    • The energy of a photon:
      Eextλ=hcλ=1240510=2.43eVE_ ext{λ} = h \frac{c}{λ} = \frac{1240}{510} = 2.43 eV
    • After conversion to Joules:
      Eextλ=2.43imes1.6imes1019=3.89imes1019JE_ ext{λ} = 2.43 imes 1.6 imes 10^{-19} = 3.89 imes 10^{-19} J
  • Photon Flux (F) Derivation:
    • F=IEextλ=5003.89imes1019extphotons/m2/sF = \frac{I}{E_ ext{λ}} = \frac{500}{3.89 imes 10^{-19}} ext{ photons/m²/s}
    • Result: Fhickapprox1.29imes1021extphotonsm2exts1F hickapprox 1.29 imes 10^{21} ext{ photons m}^{-2} ext{s}^{-1}

Semiconductor Properties and Band Structure

  • Overview of Semiconductors:
    • Common materials include silicon, gallium arsenide, germanium, and more.
  • band Gap Concept:
    • Energy difference between valence band and conduction band measured in electron volts (eV).
    • Photovoltaic materials only capture photons with energy >= band gap.
    • Example: Silicon is transparent to photons < 1.1 eV due to its band gap.

Doping of Semiconductors

  • Doping Process:
    • Impurities introduce charge carriers, creating n-type (excess electrons) and p-type (excess holes) semiconductors.
  • p-n Junction Formation:
    • The junction between p-type and n-type forms the basis of photovoltaic solar cells.

p-n Junction Diode Characteristics

  • Diode Operation Principle:
    • When illuminated, a net current flows connecting p-type and n-type regions.
    • Solar cell functionality demonstrated by circuit behavior under light impact.

Electrical Behavior of p-n Junctions

  • Current-Voltage (I-V) Dynamics in Diodes:
    • A diode's asymmetric response contrasts with resistors, showing exponential I-V behavior rather than linear.
    • Forward and Reverse bias explained:
    • Forward bias: Allows current flow when the applied voltage exceeds the barrier (0.7 V for silicon).
    • Reverse bias: Increases depletion zone width, thus impeding current.

Performance Calculations in Solar Cells

  • Open Circuit Voltage (Voc) Explanation:
    • Voltage developed when no current is drawn, analogous to battery e.m.f.
  • Short Circuit Current (Isc):
    • Current when terminals shorted together reflects maximum current output.

Characteristics of a Photocell

  • Photocell Current Calculation Example:
    • Relations for reverse light-induced (IL) and photocell current (IC) derived using equations involving the saturation current (IS) and current density (Jsc).
  • Power Generation from Photocell:
    • Power generated expressed as:
      Pc=ICimesVP_c = IC imes V

Efficiency of Photovoltaic Cells

  • Example Efficiency Calculation:
    • For a photocell with given saturation and short circuit current.
  • Evaluation of maximum power output and fill factor obtained through operational formulas.
    • Typical figures illustrated for efficiency outcomes in varied operational conditions.

Summary on Solar Cell Modules

  • Series Connection for Voltage Generation:
    • PV cells connected in series form modules, typically 28-36 in a series to yield 12 V DC.
  • Blocking Diodes:
    • Employed to prevent power loss from failing cells.

Production Overview of Solar Cells

  • Commercial Solar Cell Types:
    • Silicon cells vs. thin film cells.
    • Market shares and trends, including cost reductions through scaling.

Global Trends in Solar Energy

  • Expansion of Capacity:
    • Growth from 41 GWp in 2010 to 950 GWp in 2022, with average capacity factors across regions noted.
  • Projected Potential by 2050:
    • Estimated 2000 - 5000 GWe potential for solar energy generation, especially in developing and hot countries.
  • Environmental Impact:
    • Low CO2 emissions associated with solar energy generation noted.

Key Points in Solar Energy Utilization

  • Resource Availability and Use:
    • Solar energy resource ability is vastly underutilized.
  • Conversion Efficiencies:
    • Increasing possible efficiencies with technology advancements (perovskites).
  • Cost Trends and Production Capacities:
    • Significant drops in electricity generation costs achieving grid parity in sunny regions.
  • Future Prospects for Solar Energy:
    • Potential to exceed 40% contribution of global electricity needs by 2050 and necessitating optimized deployment strategies for variability concerns.