lecture 3-4: exergy, heating and cooling, solar thermal

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Neil Greenham [email protected] Exergy

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Page 1: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Neil Greenham

[email protected]

Exergy

Page 2: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Exergy

The following systems all “store” about 1 kW hr of energy

• 36,000 C of charge at a potential of 100 V

• 3600 kg of water at a height of 100 m

• 1/7 litre of petrol

• 3000 m3 of air at 1°C above room temperature

Which of these would you pay the most money for?

Page 3: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Energy is conserved!

So, why do we have an “energy crisis”?

When we “use” energy, we convert it from a more useful form to a less useful form

How to quantify?

Page 4: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Exergy p, V, S, T

p0, T0

A = U + p0 V – T0 S

Often defined relative to “dead state”, where system is in equilibrium with surroundings

A = (U - U0) + p0 (V - V0) – T0 (S – S0)

Can also include (macroscopic) kinetic and potential energy terms

Where chemical species can be exchanged with environment, add chemical potential terms, µ0N

Thermodynamics: An Engineering Approach; Y. A. Cengel, M. A. Boles Fundamental of Engineering Thermodynamics; M. J. Moran, H. N. Shapiro

(also known as “availability”)

Page 5: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Example

dS = dQ/T = c dT/T S = c ln(T/T0)

Page 6: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal
Page 7: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Heat engines

W

TH

TL

QH

QL

Coefficient of performance, η = W/QH

p, V

TH

TL

QH

QL

Page 8: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Carnot cycle

1-2 Isothermal expansion 2-3 Adiabatic expansion 3-4 Isothermal compression 4-1 Adiabatic compression

Maximum efficiency (reversible)

H

Lrev T

T−= 1η

Page 9: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Heat pump

Refrigerator

W

TH

TL

QH

QL

Coefficient of performance, η = QH/W

LH

Hrev TT

T−

W

TH

TL

QH

QL

Coefficient of performance, η = QL/W

LH

Lrev TT

T−

Page 10: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Exergy

Proof:

dU = δQ + δW = δQ – p dV = δQ – (p – p0) dV – p0 dV = δQ – δWuseful,done – p0 dV

System with U, S, p, T Surroundings at p0, T0

Remove heat –δQ, and increase volume by dV

δWuseful,done = - dU – p0 dV + δQ

−δQ used to run heat engine operating between T and T0, doing work δWHE

δWHE = - (1 - T0/T) δQ = - δQ + T0/T δQ = - δQ + T0 dS For reversible change

(maximum work) Total useful work done, δWu = δWuseful,done + δWHE = - dU – p0 dV + δQ – δQ + T0 dS = - dU – p0 dV + T0 dS

Available work = = (U – U0) + p0 (V – V0) - T0 (S – S0) = exergy ∫dead

initial

udW

Page 11: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Exergetic efficiency

“Second law efficiency”

revex CoP

CoP=η = 1 for ideal, reversible system

E.g. for engine

usedexergydonework

ex =η

coefficient of performance

Page 12: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Is setting fire to fuel to make heat a good thing?

Page 13: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Neil Greenham

[email protected]

Heating and Cooling

Engines

Page 14: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Efficiency for heating

• Reduce temperature difference • Turn the thermostat down

• Reduce heat loss • Increase CoP of heat creation

Leakiness 8 kWhr / day / °C

Heat loss = leakiness × Average temperature difference

kWhr/day

kWhr / day / °C °C

Power required = heat loss / CoP

Page 15: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Reduce leakiness

New leakiness 6 kWh / day / °C

Old leakiness 8 kWh / day / °C

Page 16: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Increase coefficient of performance - use heat pumps

http://www.ecosystem-japan.com/

EcoCute water heater CoP = 4.9

Page 17: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Heating without fossil fuels

Heat pumps, powered by electricity

Ground-source heat pumps

Air-source heat pumps

4 times more efficient than ordinary electric heating

Page 18: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal
Page 19: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Ideal heat pump performance

Page 20: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Combined heat and power?

“Microgeneration”, “Decentralisation”

Page 21: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

(combined heat and power) (cogeneration) Carbon Trust on Micro-CHP

"Micro-CHP is an emerging set of technologies with the potential to provide carbon savings in both commercial and domestic environments."

Page 22: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Efficiency of CHP

Page 23: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

EcoCute water heater - CoP = 4.9

Can we do better than CHP? - Heat pumps

Page 24: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Engines

From Cengel & Boles, Thermodynamics

Page 25: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Engine efficiency

Air standard Otto cycle

Carnot efficiency

E.g. r = 8, 800 kJ/kg heat supplied, T1 = 290 K, k = 1.4

T3 = 1575 K, T4 = 701 K, T2 = 666 K

Actual efficiencies only ~20%

123

14 111 −−=−−

−= kth rTTTTη

r = compression ratio = V3/V4 = V2/V1

k = cp/cv

%8213

1 =−=TT

revη

%56=thη

(If heat supplied at T3 and extracted at T1)

From Cengel & Boles, Thermodynamics

Page 26: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Can Carnot efficiencies be achieved?

Stirling engine

1-2 Isothermal expansion 2-3 Cool at constant volume 3-4 Isothermal compression 4-1 Heat at constant volume

Transfer heat to “regenerator”

Recover heat from “regenerator”

Regenerator must be at same temperature as gas ⇒ Reversible

From Cengel & Boles, Thermodynamics

Page 27: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

```````

`

```````

Ideal Stirling Cycle

Hot gas expands Work out Heat in Transfer gas to

cold cylinder Heat transferred to regenerator

Cold gas contracts Work in Heat out

Transfer gas to hot cylinder Heat transferred from regenerator

From Cengel & Boles, Thermodynamics

Page 28: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

More complex than the ideal cycle!

Alpha Stirling Engine

```````

`

```````

Page 29: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Beta Stirling Engine

• Single piston for compression/expansion

• Move (insulated, loose fitting) displacer piston to “move” gas from hot to cold region and vice versa

Practical points

• Real efficiencies ≤ 50% • External combustion less easy to regulate • More expensive than diesel engines

Page 30: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

The Sun

Roughly a black body

• Temperature ~5800K • Distance 1.5×1011 m • Diameter 1.4×109 m

Stefan’s law

4TbodyblackbyemittedareaunitperPower σ=

42832

45

KmW1075152 −−−×== .

hckπσ

( )1

5

2

12−

=

kThchcTB

λλλ exp

Page 31: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Making things hot

Total power radiated by sun 24 4 sunrT πσ

Intensity (W m-2) at distance s 2

24

srT sun

sunσ

Power absorbed by object, radius r 22

24 r

srT sun

sun πσ

In equilibrium, power absorbed = power radiated 242

2

24 4 rTr

srT objectsun

sun πσπσ =

24

41

=

s

rT

T sun

sun

object

For sun, at earth, data from previous slide give ~1400 W m-2

Actual average value at noon, at equator, beyond atmosphere = 1366 W m-2

s radius rsun

radius r

Tobject = 280 K for searth-sun 256 K if 30% reflecting

Page 32: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Making things hotter

• Heat engines run better from high-temperature sources

• But, at high temperatures • Re-radiation increases • Things melt

Solar concentrator

• To increase temperature • Use a greenhouse • Increase the range of angles from which radiation is incident

See website for derivation of optimum temperature

Page 33: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Stirling Energy Systems 14 W/m2

Page 34: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Andasol, Spain

10 W/m2

Photo: ABB

Photo: IEA SolarPACES

Page 35: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Cover every south-facing roof

110 W/m2

10 m2 per person Assume 50% efficient

Solar Thermal

13 kWh per day per person

Page 36: Lecture 3-4: Exergy, Heating and Cooling, Solar Thermal

Real data

3 m2

3.8 kWh/d average

13 kWh/d for 10 m2