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Energy in Green Building:
The Carbon Imperative and
     the Ruby Slippers


         Dr. Alexandra “Sascha” von Meier
Professor, Dept. of Environmental Studies & Planning
              Sonoma State University
              www.sonoma.edu/ensp
Natural carbon cycle
               ≈ 50 GtC/y


                                               CO2 emissions
                                               ≈ 7 GtC/y




1 GtC/y = 1 billion tons of carbon per year,
which may be bound in CO2 or other compounds
CO2 removal from
atmosphere ≈ 3 GtC/y

        CO2 emissions
        ≈ 7 GtC/y
7   800




          3
Burning fossil fuel means combustion of hydrocarbons:



 CXHY +            O2 → CO2 + H2O
hydrocarbon + oxygen → carbon dioxide + water

where the proportions of CO2 and H2O depend on X and Y
GISS analysis of global surface temperature; 2008 point is 11-month mean.
                                              Source: Jim Hansen, 2008
Five Stages of Receiving
Catastrophic News

Denial
Anger
Bargaining
Depression
Acceptance
Source: Arctic Council and International Arctic Science Committee, www.acia.uaf.edu
Slide: John Holdren
Climate stabilization (at 450 ppm CO2) requires global emissions to peak by 2015
and to fall to ~80% below 2000 levels by 2050


                                                                           Slide: Jim Williams
     Source: Intergovernmental Panel on Climate Change, Climate Change 2007: Synthesis Report
California’s Big Step Forward:
                                                                           Assembly Bill 32
                                         600          Historical
                                                      Emissions
                                                      Inventory                                 2008 Estimate
                                         500

                                                                                                                             2020 Goal under AB32
            Million metric tonnes CO2e




                                         400          Electricity


                                         300
                                                Transportation

                                         200

                                                                                                                                                  2050 Target (EO 03-05)
                                         100            Industry
                                                                                                                                                              2050 Goal
                                                                                                                                                            Executive order
Slide:                                     0
                                               1990
                                                      1993
                                                             1996
                                                                    1999
                                                                           2002
                                                                                  2005
                                                                                         2008
                                                                                                 2011
                                                                                                        2014
                                                                                                               2017
                                                                                                                      2020
                                                                                                                             2023
                                                                                                                                    2026
                                                                                                                                           2029
                                                                                                                                                  2032
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                                                                                                                                                                2038
                                                                                                                                                                       2041
                                                                                                                                                                              2044
                                                                                                                                                                                     2047
                                                                                                                                                                                            2050
Snuller Price
American Heritage Dictionary, 10th ed.
Physical Meaning of Energy:


Energy = the ability to do work




                                                       Force




                                          distance

                                  Work = Force · distance
Energy = the ability to do work


Potential energy = mgh
(mass, gravitational acceleration, height)




                                             velocity
 Kinetic energy = ½ mv2
 (mass, velocity)
Examples of Energy


Natural gas in the pipeline            (chemical)
Gas flame on my kitchen stove          (chemical to thermal)
Hot water in the kettle                (thermal)
Electricity in the wall outlet         (electrical)
Spinning blade of the coffee grinder   (mechanical kinetic)
Pancakes & maple syrup                 (chemical)
Vase sitting on top shelf              (mechanical potential)
Vase falling down to floor             (mechanical kinetic)
Radioactivity                          (nuclear to radiant)
Sunshine                               (radiant to thermal)
Wind                                   (mechanical kinetic)
Because a measurable quantity of energy is conserved
during any conversion of one form to another,

it makes sense to give a single name to that quantity.
Matter and Energy Resources


“High Quality” means            High quality energy:
        concentrated            mechanical, electrical, radiant
        pure
        easy to use
        in an orderly state
                                Medium quality energy:
                                nuclear, chemical
“Low Quality” means
        dispersed
        impure
        more difficult to use   Low quality energy:

        disordered              thermal (heat)
2nd Law requires:
Some of the chemical fuel energy will be degraded into heat.
The amount of mechanical work or electricity produced will be less
than the fuel input.
Basic lesson:
Use energy sources matched in quality with end use needs.
Units of energy:              Units of power:

calories                      calories per hour
kilocalories
joules                        joules per second = watts
kilowatt-hours (kWh)          kilowatts (kW)
British Thermal Units (BTU)   BTU per hour
therms (105 BTU)
quads (1015 BTU)

                         Power = energy per unit time
Electric usage    232 kWh        $0.11/kWh
Gas usage         52 therms      $0.71/therm


Conversion factors:       1 therm = 100,000 Btu = 105 Btu
                          1 kWh = 3,413 Btu


Questions:
• Which is my greater energy consumption – electricity or gas?
• Which is more expensive per unit energy – electricity or gas?
Electric usage        232 kWh          $0.11/kWh
Gas usage             52 therms        $0.71/therm


Conversion factors:            1 therm = 100,000 Btu = 105 Btu
                               1 kWh = 3,413 Btu


Convert 232 kWh into therms by multiplying
by the conversion factors (3,413 Btu / kWh) and (1 therm / 105 Btu):


232 kWh x (3,413 Btu / kWh) x (1 therm / 105 Btu) = 7.9 therms
     → I use 7.9 therms worth of electricity
$ 0.115 / kWh




PG&E electric rates have stayed about the same
over the past five years
$ 1.04 / therm



                              $ 0.92 / therm




PG&E gas rates have gone up from $0.70 / therm
Electric rate       $ 0.115 / kWh
Gas rate            $ 0.92 – 1.04 / therm
Which is more expensive, gas or electricity?
Conversion factors:         1 therm = 100,000 Btu = 105 Btu
                            1 kWh = 3,412 Btu


$0.115/kWh x (1 kWh/3,412 Btu) x (105 Btu/therm)

                                      = $3.37/therm

→ electricity is over three times as expensive as natural gas
Time for a break, maybe?
Basic Passive Solar Design Problem:
Get solar heat when you want it, not when you don’t.


Careful:
Windows can be net gain or loss.
The Environmental Technology Center at Sonoma State University
Passive Solar Design Principle #1:
Think about where the sun is going to be.
from Miller, Living in the Environment
Note different scales for power radiated!
Thermal IR
Passive Solar Design Principle #2:
Remember conduction, convection and radiative heat transfer.
Q = m c ∆T

Q is amount of heat stored
m is mass
c is specific heat
∆T is temperature difference before/after
Outside and Inside Temperatures
                     100

                      90
Degrees Fahrenheit




                      80

                      70

                      60

                      50

                      40

                      30
                                                                                                                                             TEMP OUSTIDE

                      20                                                                                                                     TEMP INSIDE
                      10

                       0
                       12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM
                        AM            PM            AM            PM            AM            PM            AM            PM            AM


                                            06/27/01                                to                         07/01/01
Passive Solar Design Principle #3:
Store warmth or coolth in thermal mass.
R-value: thermal resistance
U-value: thermal conductance, R = 1/U
Heat flow example:

R-20 wall
U = 0.05 Btu/h-ft2-oF
Area = 100 ft2
∆T = 30oF

What is the rate of heat loss?

Q = U A ∆T
  = (0.05 Btu/h-ft2-oF) × (100 ft2) × (30 oF)
  = 150 Btu/h
Note:
U-value is weighted average of framing and area between framing.

Any air gap between insulation & framing ruins the insulating effect.
Ballpark value for residential building envelope:
UA = 500 Btu/h-oF

How much heating energy does it take?


Convenient characterization of heating climate:

“Degree-days” DD
              actually oF-d or ∆T-days
443 Degree-Days
in San Francisco for the
month of January
3001 Degree-Days
for the whole year

For example:
300 days of ∆T = 10oF
UA = 500 Btu/h-oF

How much heating energy does it take?

San Francisco heating climate: 3001 DD




Q = U A ∆T-days × hours/day
   = (500 Btu/h-oF) × (3001 oF-d) × (24 h/d)
   = 36 million Btu
        = 360 therms
Passive Solar Design Principle #4:
Insulate well.
SHGC: fraction of solar gain admitted
through window

Performance trade-off with U-value
for solar heating


U-value: thermal conductance

U = 1/R

0.35 Btu/hr-ft2-oF ≈ R-3
Passive Solar Design Principle #5:
Be smart about windows.
Passive Solar Design Principle #1:
Think about where the sun is going to be.

#2
Remember conduction, convection and radiative heat transfer.

#3
Store warmth or coolth in thermal mass.

#4
Insulate well.

#5
Be smart about windows.
Heat loss by conduction,
                                      convection and
                                      infrared radiation


Heat gain by
solar radiation




                  Building envelope
Heat gain by conduction,
                  convection and
                  infrared radiation


Heat gain by
solar radiation
Heat loss by conduction,
                         convection and
                         infrared radiation




Heat gain from natural
gas via hydronic floor
Question: Should I turn the heater off            Heat loss by conduction,
while I’m gone?                                   convection and
                                                  infrared radiation

  YES!
                           Driven by temperature difference
                           between inside and outside




                       Replaces heat lost through envelope




                      Heat gain from natural
                      gas via hydronic floor
Basic principle for smart energy use in any building:
Think of heat flow through the envelope.
Solar collectors for domestic hot water
Focusing with a parabolic mirror
If you use solar energy, your
children will be well-
groomed, polite and gladly
help with chores.
Solar Thermal Power at Kramer Junction, CA   Photo: PG&E
Photo: Pacific Gas & Electric
Vestas 1.8 MW 260’ height, 135’ radius   www.tva.gov
Interesting constraints:

Transmission infrastructure
Resource location, cooling water
Energy storage capacity
Temporal coordination
Drastic reductions of carbon emissions

Three investment strategies:

Energy efficiency

plus

• carbon capture
                         All three are expensive, so cost
• nuclear energy         alone is not a decisive factor.
• renewables
Image: IPCC
South Texas Project, Photo: www.nielsen-wurster.com
CCS:     Carbon Capture and Storage or
         Carbon Capture and Sequestration


Problematic issues:

•   sheer quantity of carbon
•   no inherent performance incentive
•   verification
•   permanence of disposal
Nuclear energy

Problematic issues:

• “vulnerability to human frailty, incl. stupidity and malice”
    (John Holdren)


• slow, committing infrastructure investment

• ethical concerns
Portfolio of renewable energy resources

Problematic issues:

• spatial and temporal constraints on energy availability

• requires sophisticated, integrated planning



In my opinion, these are the most readily solvable problems.
Pacific Gas & Electric, 1989
Exclusion zone radius 18 km, area 109 m2


Incident solar radiation 1000 W/m2
at conversion efficiency 0.1
could generate 108 kW or 100 GW of solar power
at capacity factor 0.2 would produce 5% of U.S. electric energy

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Energy in green building and the carbon imperative

  • 1. Energy in Green Building: The Carbon Imperative and the Ruby Slippers Dr. Alexandra “Sascha” von Meier Professor, Dept. of Environmental Studies & Planning Sonoma State University www.sonoma.edu/ensp
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  • 3. Natural carbon cycle ≈ 50 GtC/y CO2 emissions ≈ 7 GtC/y 1 GtC/y = 1 billion tons of carbon per year, which may be bound in CO2 or other compounds
  • 4. CO2 removal from atmosphere ≈ 3 GtC/y CO2 emissions ≈ 7 GtC/y
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  • 11. Burning fossil fuel means combustion of hydrocarbons: CXHY + O2 → CO2 + H2O hydrocarbon + oxygen → carbon dioxide + water where the proportions of CO2 and H2O depend on X and Y
  • 12. GISS analysis of global surface temperature; 2008 point is 11-month mean. Source: Jim Hansen, 2008
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  • 15. Five Stages of Receiving Catastrophic News Denial Anger Bargaining Depression Acceptance
  • 16. Source: Arctic Council and International Arctic Science Committee, www.acia.uaf.edu
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  • 20. Climate stabilization (at 450 ppm CO2) requires global emissions to peak by 2015 and to fall to ~80% below 2000 levels by 2050 Slide: Jim Williams Source: Intergovernmental Panel on Climate Change, Climate Change 2007: Synthesis Report
  • 21. California’s Big Step Forward: Assembly Bill 32 600 Historical Emissions Inventory 2008 Estimate 500 2020 Goal under AB32 Million metric tonnes CO2e 400 Electricity 300 Transportation 200 2050 Target (EO 03-05) 100 Industry 2050 Goal Executive order Slide: 0 1990 1993 1996 1999 2002 2005 2008 2011 2014 2017 2020 2023 2026 2029 2032 2035 2038 2041 2044 2047 2050 Snuller Price
  • 23. Physical Meaning of Energy: Energy = the ability to do work Force distance Work = Force · distance
  • 24. Energy = the ability to do work Potential energy = mgh (mass, gravitational acceleration, height) velocity Kinetic energy = ½ mv2 (mass, velocity)
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  • 26. Examples of Energy Natural gas in the pipeline (chemical) Gas flame on my kitchen stove (chemical to thermal) Hot water in the kettle (thermal) Electricity in the wall outlet (electrical) Spinning blade of the coffee grinder (mechanical kinetic) Pancakes & maple syrup (chemical) Vase sitting on top shelf (mechanical potential) Vase falling down to floor (mechanical kinetic) Radioactivity (nuclear to radiant) Sunshine (radiant to thermal) Wind (mechanical kinetic)
  • 27. Because a measurable quantity of energy is conserved during any conversion of one form to another, it makes sense to give a single name to that quantity.
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  • 33. Matter and Energy Resources “High Quality” means High quality energy: concentrated mechanical, electrical, radiant pure easy to use in an orderly state Medium quality energy: nuclear, chemical “Low Quality” means dispersed impure more difficult to use Low quality energy: disordered thermal (heat)
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  • 41. 2nd Law requires: Some of the chemical fuel energy will be degraded into heat. The amount of mechanical work or electricity produced will be less than the fuel input.
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  • 43. Basic lesson: Use energy sources matched in quality with end use needs.
  • 44. Units of energy: Units of power: calories calories per hour kilocalories joules joules per second = watts kilowatt-hours (kWh) kilowatts (kW) British Thermal Units (BTU) BTU per hour therms (105 BTU) quads (1015 BTU) Power = energy per unit time
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  • 47. Electric usage 232 kWh $0.11/kWh Gas usage 52 therms $0.71/therm Conversion factors: 1 therm = 100,000 Btu = 105 Btu 1 kWh = 3,413 Btu Questions: • Which is my greater energy consumption – electricity or gas? • Which is more expensive per unit energy – electricity or gas?
  • 48. Electric usage 232 kWh $0.11/kWh Gas usage 52 therms $0.71/therm Conversion factors: 1 therm = 100,000 Btu = 105 Btu 1 kWh = 3,413 Btu Convert 232 kWh into therms by multiplying by the conversion factors (3,413 Btu / kWh) and (1 therm / 105 Btu): 232 kWh x (3,413 Btu / kWh) x (1 therm / 105 Btu) = 7.9 therms → I use 7.9 therms worth of electricity
  • 49. $ 0.115 / kWh PG&E electric rates have stayed about the same over the past five years
  • 50. $ 1.04 / therm $ 0.92 / therm PG&E gas rates have gone up from $0.70 / therm
  • 51. Electric rate $ 0.115 / kWh Gas rate $ 0.92 – 1.04 / therm Which is more expensive, gas or electricity? Conversion factors: 1 therm = 100,000 Btu = 105 Btu 1 kWh = 3,412 Btu $0.115/kWh x (1 kWh/3,412 Btu) x (105 Btu/therm) = $3.37/therm → electricity is over three times as expensive as natural gas
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  • 53. Time for a break, maybe?
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  • 55. Basic Passive Solar Design Problem: Get solar heat when you want it, not when you don’t. Careful: Windows can be net gain or loss.
  • 56. The Environmental Technology Center at Sonoma State University
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  • 62. Passive Solar Design Principle #1: Think about where the sun is going to be.
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  • 65. from Miller, Living in the Environment
  • 66. Note different scales for power radiated!
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  • 73. Passive Solar Design Principle #2: Remember conduction, convection and radiative heat transfer.
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  • 75. Q = m c ∆T Q is amount of heat stored m is mass c is specific heat ∆T is temperature difference before/after
  • 76. Outside and Inside Temperatures 100 90 Degrees Fahrenheit 80 70 60 50 40 30 TEMP OUSTIDE 20 TEMP INSIDE 10 0 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM 12:00 6:00 PM 12:00 6:00 AM AM PM AM PM AM PM AM PM AM 06/27/01 to 07/01/01
  • 77. Passive Solar Design Principle #3: Store warmth or coolth in thermal mass.
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  • 79. R-value: thermal resistance U-value: thermal conductance, R = 1/U
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  • 81. Heat flow example: R-20 wall U = 0.05 Btu/h-ft2-oF Area = 100 ft2 ∆T = 30oF What is the rate of heat loss? Q = U A ∆T = (0.05 Btu/h-ft2-oF) × (100 ft2) × (30 oF) = 150 Btu/h
  • 82. Note: U-value is weighted average of framing and area between framing. Any air gap between insulation & framing ruins the insulating effect.
  • 83. Ballpark value for residential building envelope: UA = 500 Btu/h-oF How much heating energy does it take? Convenient characterization of heating climate: “Degree-days” DD actually oF-d or ∆T-days
  • 84. 443 Degree-Days in San Francisco for the month of January 3001 Degree-Days for the whole year For example: 300 days of ∆T = 10oF
  • 85. UA = 500 Btu/h-oF How much heating energy does it take? San Francisco heating climate: 3001 DD Q = U A ∆T-days × hours/day = (500 Btu/h-oF) × (3001 oF-d) × (24 h/d) = 36 million Btu = 360 therms
  • 86. Passive Solar Design Principle #4: Insulate well.
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  • 88. SHGC: fraction of solar gain admitted through window Performance trade-off with U-value for solar heating U-value: thermal conductance U = 1/R 0.35 Btu/hr-ft2-oF ≈ R-3
  • 89. Passive Solar Design Principle #5: Be smart about windows.
  • 90. Passive Solar Design Principle #1: Think about where the sun is going to be. #2 Remember conduction, convection and radiative heat transfer. #3 Store warmth or coolth in thermal mass. #4 Insulate well. #5 Be smart about windows.
  • 91. Heat loss by conduction, convection and infrared radiation Heat gain by solar radiation Building envelope
  • 92. Heat gain by conduction, convection and infrared radiation Heat gain by solar radiation
  • 93. Heat loss by conduction, convection and infrared radiation Heat gain from natural gas via hydronic floor
  • 94. Question: Should I turn the heater off Heat loss by conduction, while I’m gone? convection and infrared radiation YES! Driven by temperature difference between inside and outside Replaces heat lost through envelope Heat gain from natural gas via hydronic floor
  • 95. Basic principle for smart energy use in any building: Think of heat flow through the envelope.
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  • 97. Solar collectors for domestic hot water
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  • 99. Focusing with a parabolic mirror
  • 100. If you use solar energy, your children will be well- groomed, polite and gladly help with chores.
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  • 103. Solar Thermal Power at Kramer Junction, CA Photo: PG&E
  • 104. Photo: Pacific Gas & Electric
  • 105. Vestas 1.8 MW 260’ height, 135’ radius www.tva.gov
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  • 107. Interesting constraints: Transmission infrastructure Resource location, cooling water Energy storage capacity Temporal coordination
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  • 110. Drastic reductions of carbon emissions Three investment strategies: Energy efficiency plus • carbon capture All three are expensive, so cost • nuclear energy alone is not a decisive factor. • renewables
  • 112. South Texas Project, Photo: www.nielsen-wurster.com
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  • 114. CCS: Carbon Capture and Storage or Carbon Capture and Sequestration Problematic issues: • sheer quantity of carbon • no inherent performance incentive • verification • permanence of disposal
  • 115. Nuclear energy Problematic issues: • “vulnerability to human frailty, incl. stupidity and malice” (John Holdren) • slow, committing infrastructure investment • ethical concerns
  • 116. Portfolio of renewable energy resources Problematic issues: • spatial and temporal constraints on energy availability • requires sophisticated, integrated planning In my opinion, these are the most readily solvable problems.
  • 117. Pacific Gas & Electric, 1989
  • 118. Exclusion zone radius 18 km, area 109 m2 Incident solar radiation 1000 W/m2 at conversion efficiency 0.1 could generate 108 kW or 100 GW of solar power at capacity factor 0.2 would produce 5% of U.S. electric energy