Simplifying the Natural Convection Heat Transfer Correlation

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SUMMARY

The forum discussion focuses on simplifying the natural convection heat transfer correlation for a horizontal pipe, specifically the equation Nu=0.53Gr^0.25 Pr^0.25. The Grashof number (Gr) and Prandtl number (Pr) are defined with specific parameters, leading to the simplified heat transfer coefficient equation h ≈ 1.34((T_s-T_f)/d)^0.25 Wm^(-2) K^(-1). Participants discussed the steps to manipulate the original equation, emphasizing the distribution of exponents and the arrangement of terms to achieve the final simplified form.

PREREQUISITES
  • Understanding of heat transfer principles, specifically natural convection.
  • Familiarity with the Grashof number (Gr) and Prandtl number (Pr).
  • Basic algebraic manipulation skills for equations and exponents.
  • Knowledge of thermodynamic properties of air, including thermal conductivity and specific heat capacity.
NEXT STEPS
  • Study the derivation of the Grashof number and its significance in natural convection.
  • Learn about the Prandtl number and its role in heat transfer analysis.
  • Explore the application of the simplified heat transfer coefficient in practical engineering problems.
  • Investigate numerical methods for solving heat transfer equations in fluid dynamics.
USEFUL FOR

Engineers, thermodynamics students, and researchers focused on heat transfer analysis and natural convection processes will benefit from this discussion.

Tiberious
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Homework Statement



An appropriate correlation for heat transfer by natural convection from a horizontal pipe to the atmosphere is Nu=0.53Gr^0.25 Pr^0.25

Where,

Gr= (αp^2 d^3 (T_1-T_f )g)/μ^2

And

Pr⁡〖= (C_p μ)/k〗

Show the above correlation can be simplified to

h ≈1.34((T_s-T_f)/d)^0.25 Wm^(-2) K^(-1)

When air has the values listed below

α=3.077∙10^(-3 ) K^(-1)
p=1.086 kg m^(-3)
C_p=1.0063 kj kg^(-1) K^(-1)
k=2.816∙10^(-5) kWm^(-1) K^(-1)
μ=1.962∙10^(-5) kg m^(-1) s^(-1)

The Attempt at a Solution

Inputting the Grashof and Prandtl number equations:

Nu=0.53〖(αp^2 d^3 (T_1-T_f )g)/μ^2 〗^0.25 〖(C_p μ)/k〗^0.25

As,

N_u= hd/k

Replacing this into our equation,

hd/k=0.53〖(αp^2 d^3 (T_1-T_f )g)/μ^2 〗^0.25 〖(C_p μ)/k〗^0.25
Rearranging,

h=k/d 0.53〖(αp^2 d^3 (T_1-T_f )g)/μ^2 〗^0.25 〖(C_p μ)/k〗^0.25

Distributing through the exponents,

Struggling to figure this one out. Any assistance is appreciated.

I know I have to Distribute though the terms. Just a little unsure in what order to carry our the operations.
 
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Tiberious said:
Just a little unsure in what order to carry our the operations
Shouldn't matter ! So, please continue!
 
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Thank-you for your hasty reply.

So, do I multiply each term by the power of 0.25. Apologies, I've been staring at this for ages and am at a loss.
 
You have ##\Delta T^{0.25}## already. ##(d^3)^{0.25}## and ## 1/d ## give you the expected power of ##d##. The remainder is numerical.
 
Does this seem correct as the next stage ? Or, do we multiply each term ?

h= (2.816∙10^(-5))/d 0.53〖(〖3.077∙10^(-3 )∙1.086〗^2 d^3 (T_s-T_f )9.81)/〖1.962∙10^(-5)〗^2 〗^0.25 〖(1.0063∙1.962∙10^(-5))/(2.816∙10^(-5) )〗^0.25
 
Try it and see where it takes you;
the end of the tunnel is that you want to end up at 1.34
 
Okay - I've found my way to the below. Now I'm stuck.

0.0044h= (2.816∙10^(-5))/d 0.53((0.2355)∙(1.042) d^0.75 (T_s-T_f )^0.25 1.7698)(0.915)
 
What is the problem ?
Lump all the numbers in one and I do hope you know what ##d^{0.75}/d## is ?
 
BvU - Thanks.

I got to the below eventually..

h=1.34 (T_s-T_f )^0.25/d^0.25

From this we can derive that,

h ≈1.34((T_s-T_f)/d)^0.25
 

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