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MEGR 324 Lec1(Notes) Part 2 of 2

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Page 1: MEGR 324 Lec1(Notes) Part 2 of 2

Lec 1: Physical Origins and

Rate Equations

Page 2: MEGR 324 Lec1(Notes) Part 2 of 2

• What is heat transfer?

Heat transfer is thermal energy in transit due to a temperaturedifference.

• What is thermal energy?Thermal energy is associated with the translation, rotation,vibration and electronic states of the atoms and moleculesthat comprise matter. It represents the cumulative effect ofmicroscopic activities and is directly linked to the temperatureof matter.

Page 3: MEGR 324 Lec1(Notes) Part 2 of 2

Quantity Meaning Symbol Units

Thermal Energy+ Energy associated with microscopic behavior of matter

Temperature A means of indirectly assessing the amount of thermal energy stored in matter

Heat Transfer Thermal energy transport due to temperature gradients

Heat Amount of thermal energy transferred over a time interval U t ! 0

Heat Rate Thermal energy transfer per unit time

Heat Flux Thermal energy transfer per unit time and surface area

or U u J or J/kg

T K or °C

Q J

q W

qcc 2W/m

+ Thermal energy of system Thermal energy per unit mass of system

Uuoo

DO NOT confuse or interchange the meanings of Thermal Energy, Temperature and Heat Transfer

Page 4: MEGR 324 Lec1(Notes) Part 2 of 2

Conduction: Heat transfer in a solid or a stationary fluid (gas or liquid) due to the random motion of its constituent atoms, molecules and /or electrons.

Convection: Heat transfer due to the combined influence of bulk and random motion for fluid flow over a surface.

Radiation: Energy that is emitted by matter due to changes in the electron configurations of its atoms or molecules and is transported as

electromagnetic waves (or photons).

• Conduction and convection require the presence of temperature variations in a materialmedium.

• Although radiation originates from matter, its transport does not require a materialmedium and occurs most efficiently in a vacuum.

Modes of Heat Transfer

Page 5: MEGR 324 Lec1(Notes) Part 2 of 2

2 1x

T TdTq k kdx L

�cc � �

1 2x

T Tq k

L�cc (1.2)

Heat rate (W): x xq q Acc �

Application to one-dimensional, steady conduction across aplane wall of constant thermal conductivity:

Conduction:

General (vector) form of Fourier’s Law:

Heat flux

q k Tcc � �

Thermal conductivity Temperature gradient2W/m W/m K� °C/m or K/m

Heat Transfer Rates

Page 6: MEGR 324 Lec1(Notes) Part 2 of 2

Convection

Relation of convection to flow over a surface and developmentof velocity and thermal boundary layers:

Newton’s law of cooling:

� �h sq T Tfcc � (1.3a)

2Convection heat transfer coefficih : (W/ment K)�

Heat Transfer Rates

Page 7: MEGR 324 Lec1(Notes) Part 2 of 2

Radiation Heat transfer at a gas/surface interface involves radiation emission from the surface and may also involve theabsorption of radiation incident from the surroundings(irradiation, ), as well as convection � �if .sT Tfz

Energy outflow due to emission:4

b sE E TH HV (1.5)

� � emissiv: Surface 0ity 1H Hd dblackbody: Emissive power of a (the perfect emit r ) tebE

� �2Emissive powe: r W/mE

� �-8 2 4: Stefan-Boltzmann constant 5.67×10 W/m KV �

Energy absorption due to irradiation:absG GD

2: incident Absorbed radiatio (W )n /mabsG

� �absorpti: Surfa vityce 0 1D Dd d� �2Irradiation: W/mG

G

Heat Transfer Rates

Page 8: MEGR 324 Lec1(Notes) Part 2 of 2

Irradiation: Special case of surface exposed to largesurroundings of uniform temperature, surT

4sur surG G TV

� � � �4 4

If , the from the surface due to exchange with the surroundings is

net radiation heat flux:

rad b s s surq E T G T T

D H

H D HV

cc � � (1.7)

Heat Transfer Rates