Intro to Solar Energy UCSD Many slides courtesy of Prof. Tom Murphy Lecture 9 Spring 2008 UCSD 2 1 Intro to Solar Energy Spring 2008 UCSD UCSD above the atmosphere at ground level O2 H2O Atmospheric absorption H2O H2O,CO2 H2O, CO2 much room for improvement/growth, but going backwards! 3 Lecture 9 4 2 Intro to Solar Energy Spring 2008 UCSD UCSD 5 Lecture 9 6 3 Intro to Solar Energy Spring 2008 UCSD UCSD 7 Lecture 9 8 4 Intro to Solar Energy Spring 2008 UCSD UCSD 9 Lecture 9 10 5 Intro to Solar Energy Spring 2008 UCSD UCSD ranges in W/m2: < 138 138–162 162–185 185–208 208–231 > 231 11 Lecture 9 divide by 24 hr to get average kW/m2 12 6 Intro to Solar Energy Spring 2008 UCSD UCSD 13 Lecture 9 14 7 Intro to Solar Energy Spring 2008 UCSD UCSD 15 Lecture 9 Solar Land Area Requirements 6 Boxes at 3.3 TW Each 16 8 Intro to Solar Energy Spring 2008 UCSD UCSD 17 Lecture 9 18 9 Intro to Solar Energy Spring 2008 UCSD UCSD 19 Lecture 9 10 Intro to Solar Energy Spring 2008 UCSD UCSD Question Question How was the midterm? Green houses get hotter than the outside air because A. About right B. Too hard C. Too long D. Too short or too easy E. I won't know until I get my score! A. Glass is transparent to IR allowing the heat energy in B. Glass is transparent to visible light but opaque to IR C. The glass prevents wind from carrying away the heated air D. Glass amplifies the solar energy E. Both B. and C. 21 Lecture 9 22 11 Intro to Solar Energy Spring 2008 UCSD UCSD Question Does the Sun provide enough energy to meet all current human needs? A. Yes B. Eventually yes, but current technology is not available C. Maybe yes, if humans can reduce their need for energy D. No, current human use is more than the Sun provides E. It is not clear at the present time 23 Lecture 9 24 12 Intro to Solar Energy Spring 2008 UCSD UCSD 25 Lecture 9 26 13 Intro to Solar Energy Spring 2008 UCSD UCSD 27 Lecture 9 28 14 Intro to Solar Energy Spring 2008 UCSD UCSD 29 Lecture 9 30 15 Intro to Solar Energy Spring 2008 UCSD UCSD 31 Lecture 9 32 16 Intro to Solar Energy Spring 2008 UCSD UCSD 33 Lecture 9 34 17 Intro to Solar Energy Spring 2008 UCSD UCSD 35 Lecture 9 36 18 Intro to Solar Energy Spring 2008 UCSD UCSD 37 Lecture 9 38 19 Intro to Solar Energy Spring 2008 UCSD UCSD 39 Lecture 9 Power Tower in Barstow, CA 40 20 Intro to Solar Energy Spring 2008 UCSD UCSD 41 Lecture 9 42 21 Intro to Solar Energy Spring 2008 UCSD UCSD 43 Lecture 9 44 22 Intro to Solar Energy Spring 2008 UCSD UCSD 45 Lecture 9 46 23 Intro to Solar Energy Spring 2008 UCSD UCSD photon of light electric field n-type silicon electric field n-type silicon p-type silicon p-type silicon 47 Lecture 9 liberated electron 48 24 Intro to Solar Energy Spring 2008 UCSD UCSD current flow external load 49 Lecture 9 50 25 Intro to Solar Energy Spring 2008 UCSD UCSD 0.58 +0.58 +0.58 +0.58 +0.58 +0.58 3.5 volts 51 Lecture 9 52 26 Intro to Solar Energy Spring 2008 UCSD UCSD 53 Lecture 9 54 27 Intro to Solar Energy Spring 2008 UCSD UCSD 55 Lecture 9 56 28 Intro to Solar Energy Spring 2008 UCSD UCSD Question The energy from the Sun is 100% used in which of the following? A. Silicon photovoltaic solar cells B. Photosynthesis C. Passive solar space heating D. Flat plate solar thermal water heating E. Non of the above 57 Lecture 9 58 29 Intro to Solar Energy Spring 2008 UCSD UCSD Question In planning a rooftop solar system, how many watts per square meter should you use? A. About 1386 W/m2 B. About 1/2 of 1386 W/m2 C. About 500 W/m2 D. About 171 W/m2 E. None of the above flat arrangement 59 Lecture 9 tilted arrangement 60 30 Intro to Solar Energy Spring 2008 UCSD UCSD 61 Lecture 9 62 31 Intro to Solar Energy Spring 2008 UCSD UCSD based on clear, sunny days overall winner Lecture 9 better in summer good in winter 2nd place 63 64 32 Intro to Solar Energy Spring 2008 UCSD 65 Lecture 9 33