October 11,2013 ECEN 2060 Lecture 21 Fall 2013 Homework Problems\ Chapter 5 problems Solar Spectrum Power Spectrum Planck’s Law Total energy Radiated Stefan-Boltzmann Law Suns Spectrum for T= 5800 ECEN2060 2 Cost of Solar Cells ECEN2060 3 Types and Efficiencies of Some Solar Cells ECEN2060 4 The Useable Solar Spectrum ECEN2060 5 Two dimensional view ECEN2060 6 Energy Level Diagram ECEN2060 7 ECEN2060 8 Photon Activation Requirement for creating an electron hole Pair is hν> Eg h ECEN2060 9 Holes or the Absence of an Electron in the Conduction Band ECEN2060 10 Start Lecture 22 ECEN2060 11 Cut-off Wavelengths The issue is that you can not use the long wavelength solar energy and the short wavelengths lose the energy above the band-gap to heat. ECEN2060 12 Solar Spectrum ECEN2060 13 P-N Junctions ECEN2060 14 ECEN2060 15 P-N Junction Diodes. ECEN2060 16 ECEN2060 17 P-N Junction Diode ECEN2060 18 P-N Junction Diode. ECEN2060 19 Equivalent Circuits ECEN2060 20 Inverted Diode Curve ECEN2060 21 Example For A=100 cm ECEN2060 2 I sc 40ma / cm 2 I o 10 12 A / cm 2 22 Equivalent Circuit For Shading ECEN2060 23 A more complete Equivalent Circuit ECEN2060 24 Effect of ECEN2060 25 Series Resistance Contact resistance, resistance in diode outside of the junction region ECEN2060 26 Series Resistance Added in ECEN2060 27 Equivalent Circuit ECEN2060 28 Total Equivalent Circuit. ECEN2060 29 Combinations to Get to Useful Size ECEN2060 30 Examples ECEN2060 31 Modules to Arrays 1 Voltages for cells add in series 2 Currents for each cell add in parallel ECEN2060 32 Currents add in Parallel ECEN2060 33 Two by Three Arrays ECEN2060 34 Output Power ECEN2060 35 Maximum Power ECEN2060 36 Examples Under Standard Test Conditions ECEN2060 37 Effects of Changes in Temperature ECEN2060 38 Shading ECEN2060 39 Impact of Shading ECEN2060 40 Effects of Shading ECEN2060 41 ECEN2060 42 Bypass Diode Reduces Voltage Across Shaded Cell ECEN2060 43