Why Solar Cells? Finite fossil fuel supply Less environmental damage No radiation risk (meltdown) Sun gives us 32 x1024 joules a year, Cover 0.1% of the Earth’s surface with 10% efficient solar cells with an efficiency of would satisfy our present needs.
Greenhouse Effect Human activities have now reached a scale where they are impacting on the planet's environment and its attractiveness to humans.
Spectrum of light
Atmospheric effects have several impacts on the solar radiation at the Earth's surface. The major effects for photovoltaic applications are: a reduction in the power of the solar radiation due to absorption, scattering and reflection in the atmosphere; a change in the spectral content of the solar radiation due to greater absorption or scattering of some wavelengths; the introduction of a diffuse or indirect component into the solar radiation; and local variations in the atmosphere (such as water vapor, clouds and pollution) which have additional effects on the incident power, spectrum and directionality.
Solar Radiation Power emitted from Sun =3.8×1023 (kw) Power direct to Earth=1.8×1014 (kW) Solar constant=1353 W/m2
Air Mass (AM) AM0 : The standard spectrum outside the Earth's atmosphere. AM 1: Light incident with the angle of 0 degree. AM 1.5: Light incident with the angle of 48 degree.
Standard Solar Spectra
Standard Solar Spectra-cont. The AM1.5 Global spectrum is designed for flat plate modules and has an integrated power of 1000 W/m2 (100 mW/cm2). The AM1.5 Direct (+circumsolar) spectrum is defined for solar concentrator work. It includes the direct beam from the sun plus the circumsolar component in a disk 2.5 degrees around the sun. The direct plus circumsolar spectrum has an integrated power density of 900 W/m2.
Compound semiconductors Elemental semiconductors: Si, Ge Compound semiconductors: GaAs, InP Ternary semiconductors: AlGaAs, HgCdTe Quaternary semiconductors: InGaAsP, InGaAlP
Direct and indirect semiconductor
Commercial Si solar cells
Metal-insulator-conductor
Photoelectric effect
Absorption of Light Eph < EG Photons with energy Eph less than the band gap energy EG interact only weakly with the semiconductor, passing through it as if it were transparent. Eph = EG have just enough energy to create an electron hole pair and are efficiently absorbed. Eph > EG Photons with energy much greater than the band gap are strongly absorbed
N- and P-type Addition of impurities with three valence electrons results in available empty energy state, a hole B, Al, In, Ga (Acceptor impurities)
If energy of inclined light (Ehp) > Energy band of material (EG). Then, emit electron-hole pair (EHP) to produce the electric current.
Solar Cell-structure
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