Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime...

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Chilton and Colburn J-factor analogy The equation for heat transfer in the turbulent re Sieder-Tate Equation = 0.023 0.8 1/ 3 = ( ) 0.14 (for forced convection/ turbulent, Re > 10000 & 0.5 < Pr < 100) If we divide this by =0.023 ( ) 0.8 ( ) 1 3 ( 1 ) 0.14

Transcript of Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime...

Page 1: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

Recall: The equation for heat transfer in the turbulent regime

Sieder-Tate Equation 𝑁𝑒=0.023𝑅𝑒0.8 π‘ƒπ‘Ÿ 1 /3πœ™π‘£

πœ™π‘£=( πœ‡πœ‡π‘€)

0.14(for forced convection/ turbulent, Re > 10000 & 0.5 < Pr < 100)

If we divide this by

𝑁𝑁𝑒

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

=0.023

(𝑁𝑅𝑒 )0.8 (𝑁 π‘ƒπ‘Ÿ )13 ( πœ‡πœ‡1

)0.14

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

Page 2: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Dimensionless Groups

Dim. Group Ratio Equation

Prandtl, Pr molecular diffusivity of momentum / molecular diffusivity of heat

Schmidt, Sc momentum diffusivity/ mass diffusivity

Lewis, Le thermal diffusivity/ mass diffusivity

Stanton, St heat transferred/ thermal capacity

Nusselt, Nu convective / conductive heat transfer across the boundary

Page 3: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

This can be rearranged as

𝑁𝑁𝑒

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

=0.023

(𝑁𝑅𝑒 )0.8 (𝑁 π‘ƒπ‘Ÿ )13 ( πœ‡πœ‡1

)0.14

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

𝑁 π‘†π‘‘π‘π‘ƒπ‘Ÿ

23 ( πœ‡πœ‡1

)βˆ’ 0.14

=0.023π‘π‘…π‘’βˆ’ 0.2

𝑓2

=0.023π‘π‘…π‘’βˆ’0.2

For the turbulent flow region, an empirical equation relating f and Re

Page 4: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

𝑓2

=𝑁 𝑆𝑑𝑁 π‘ƒπ‘Ÿ

23 ( πœ‡πœ‡1

)0.14

=0.023π‘π‘…π‘’βˆ’0.2

} rsub { } 𝑱 𝑯 ΒΏ

This is called as the J-factor for heat transfer

Page 5: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

In a similar manner, we can relate the mass transfer and momentum transfer using

π‘˜π‘β€² π·π·π‘Žπ‘

=0.023 (𝑁𝑅𝑒 )0.83 (𝑁𝑆𝑐 )0.33

the equation for mass transfer of all liquids and gases

If we divide this by

π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 ) (𝑁𝑅𝑒 )0.03=0.023𝑁𝑅𝑒

βˆ’ 0.2

Page 6: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

T

π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 )=0.023 𝑁𝑅𝑒

βˆ’0.2

π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 ) (𝑁𝑅𝑒 )0.03=0.023𝑁𝑅𝑒

βˆ’ 0.2

π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 )= 𝑓

2

Page 7: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

𝑓2

=π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 )=0.023𝑁𝑅𝑒

βˆ’0.2

This is called as the J-factor for mass transfer

} rsub { } 𝑱 𝑫 ΒΏ

Page 8: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

Extends the Reynolds analogy to liquids

f2= hc p𝜌 𝑣

=π‘˜π‘β€²

𝑣

f2= hc p𝜌 𝑣

(𝑁 π‘ƒπ‘Ÿ

23 )( πœ‡πœ‡1

)0.14

=π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 )

Page 9: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Chilton and Colburn J-factor analogy

If we let

f2= hc p𝜌 𝑣

(𝑁 π‘ƒπ‘Ÿ

23 )=

π‘˜π‘β€²

𝑣(𝑁 𝑆𝑐

23 )

} rsub { } 𝑱 𝑯 ΒΏ } rsub { } 𝑱 𝑫 ΒΏ

𝑓2

= 𝐽 𝐻=J D

Applies to the following ranges:For heat transfer:10,000 < Re < 300,0000.6 < Pr < 100For mass transfer: 2,000 < Re < 300,0000.6 < Sc < 2,500

( πœ‡πœ‡1)

0.14

=1

Page 10: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Reynolds Analogy demonstrates similarity of mechanism (the gradients are assumed equal) Pr = 1 and Sc = 1

Chilton-Colburn J-factor Analogy demonstrates numerical similarity(implies that the correlation equations are not faithful statements of the mechanism, but useful in predicting numerical values of coefficients wider range of Pr and Sc

Page 11: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Martinelli Analogy (heat and momentum transfer) applicable to the entire range of Pr number

Assumptions:1. The T driving forces between the wall and the fluid is small

enough so that ΞΌ/ΞΌ1 = 12. Well-developed turbulent flow exists within the test section3. Heat flux across the tube wall is constant along the test

section4. Both stress and heat flux are zero at the center of the tube

and increases linearly with radius to a maximum at the wall5. At any point Ξ΅q = Ρτ

Page 12: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Assumptions:

6. The velocity profile distribution given by Figure 12.5 is valid

Page 13: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

π‘žπ΄ ( π‘Ÿπ‘Ÿ1

)=βˆ’ (𝛼+𝛼 𝑑 ) (𝑑 (πœŒπ‘π‘π‘‡ )π‘‘π‘Ÿ )

𝜏 𝑦( π‘Ÿπ‘Ÿ1)=βˆ’(πœ‡πœŒ+πœ€π‘‘)( 𝑑 (𝑣 𝜌 )

π‘‘π‘Ÿ )

Both equal to zero;For cylindrical geometry

Page 14: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

π‘žπ΄ ( π‘Ÿπ‘Ÿ1

)=βˆ’ (𝛼+𝛼 𝑑 ) (𝑑 (πœŒπ‘π‘π‘‡ )π‘‘π‘Ÿ )

𝜏 𝑦( π‘Ÿπ‘Ÿ1)=βˆ’(πœ‡πœŒ+πœ€π‘‘)( 𝑑 (𝑣 𝜌 )

π‘‘π‘Ÿ )

Both equal to zero;For cylindrical geometry

Integrated and expressed as function of position

Converted in the form

Page 15: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Page 16: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Martinelli Analogy (heat and momentum transfer) applicable to the entire range of Pr number

predicts Nu for liquid metals contributes to understanding of the mechanism of heat and momentum transfer

Page 17: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Martinelli Analogy

Martinelli Analogy (heat and momentum transfer) applicable to the entire range of Pr number

predicts Nu for liquid metals contributes to understanding of the mechanism of heat and momentum transfer

Page 18: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Analogies

EXAMPLECompare the value of the Nusselt number, given by the appropriate empirical equation, to that predicted by the Reynolds, Colburn and Martinelli analogies for each of the following substances at Re= 100,000 and f = 0.0046. Consider all substances at 1000F, subject to heating with the tube wall at 1500F.

Page 19: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Example

Sample CalculationFor air,

𝑁𝑁𝑒=0.023 (𝑁𝑅𝑒 )0.8 (𝑁 π‘ƒπ‘Ÿ )13 ( πœ‡πœ‡1

)0.14

𝑁𝑁𝑒=0.023 (100,000 )0.8 (0.71 )13 ( 0.018

0.02 )0.14

𝑁𝑁𝑒=202(π‘šπ‘œπ‘ π‘‘π‘Žπ‘π‘π‘’π‘Ÿπ‘Žπ‘‘π‘’π‘£π‘Žπ‘™π‘’π‘’)

Page 20: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Example

Sample CalculationFor air, by Reynolds analogy

𝑁 𝑆𝑑=𝑁 𝑁𝑒

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

= f2

𝑁𝑁𝑒=f2𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ=( 0.0046

2 ) (105 )(0.71)

𝑁𝑁𝑒=16 3.3

Page 21: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Example

Sample CalculationFor air, by Colburn analogy

𝑁 𝑆𝑑=𝑁 𝑁𝑒

𝑁𝑅𝑒𝑁 π‘ƒπ‘Ÿ

f2=𝑁 𝑆𝑑 (𝑁 π‘ƒπ‘Ÿ

23 )( πœ‡πœ‡1

)0.14

𝑁𝑁𝑒=𝑁𝑅𝑒 (𝑁 π‘ƒπ‘Ÿ )13 ( 𝑓2 )( πœ‡πœ‡1

)0.14

𝑁𝑁𝑒=105 (0.71 )13 ( 0.0046

2 )( 0.0180.02 )

0.14

𝑁𝑁𝑒=202

Page 22: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

Example

Sample CalculationFor air, by Martinelli analogy

𝑁𝑁𝑒=170

Page 23: Chilton and Colburn J-factor analogy Recall: The equation for heat transfer in the turbulent regime Sieder-Tate Equation (for forced convection/ turbulent,

FIN