Solar Energy
1. History of Solar Energy
Ancient Uses:
Sun-oriented building designs (e.g., passive heating).
Magnifying glasses for fire-starting (Greece, Rome, China).
Modern Era:
1954: First photovoltaic (PV) cell invented (4% efficiency).
1958: PV used in space programs.
1979: Carter installed solar panels on the White House.
1990s: Germany’s "1000 Roof Program" (subsidies + grid sales).
2. How Solar Energy Works
Two Main Categories:
Solar Heating:
Passive: Building design (window orientation, thermal mass).
Active: Pumps/fans to transfer heat (e.g., flat plate collectors).
Solar Electricity:
Photovoltaic (PV):
Sunlight → Electrons → Electricity via semiconductors (e.g., silicon).
Band Gap: Silicon’s 1.14 eV limits efficiency (~20% currently, 33% theoretical max).
Concentrated Solar Power (CSP) (Photothermal):
Mirrors focus sunlight to heat fluid → steam → turbine → electricity.
Pros: Thermal storage for nighttime use.
Cons: Low efficiency (~4%), needs large land area.
3. Solar Industry Basics
Key Components:
PV panels (rooftop/utility-scale), inverters, batteries for storage.
Grid Integration:
Net metering (sell excess power back to grid).
Growth Drivers:
R&D (efficiency improvements), subsidies, economies of scale.
4. Advantages of Solar Energy
Clean: No CO₂ emissions or noise.
Renewable: Abundant sunlight globally.
Versatile: Scales from small (rooftops) to large (farms).
5. Disadvantages & Challenges
Intermittency: No sun at night/cloudy days (needs storage/grid mix).
Efficiency Limits:
Silicon PV: ~20% efficiency (33% theoretical cap).
CSP: ~4% efficiency.
Environmental Impacts:
Manufacturing: Energy-intensive, toxic chemicals (e.g., cadmium).
Land use: Large footprints for utility-scale projects.
6. Key Concepts & Equations
Band Gap (Silicon): 1.14 eV → Limits photon absorption efficiency.
Theoretical Efficiency: 33% for single-junction PV cells (Shockley-Queisser limit).